Initial revision

This commit is contained in:
curt
2000-02-09 19:27:02 +00:00
249 changed files with 27389 additions and 22577 deletions
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lib_LIBRARIES = libsgbucket.a
include_HEADERS = newbucket.hxx
libsgbucket_a_SOURCES = newbucket.cxx
# noinst_PROGRAMS = testbucket
# testbucket_SOURCES = testbucket.cxx
# testbucket_LDADD = \
# $(top_builddir)/bucket/libsgbucket.a \
# $(top_builddir)/misc/libsgmisc.a
INCLUDES += -I$(top_builddir)
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# Makefile.in generated automatically by automake 1.3 from Makefile.am
# Copyright (C) 1994, 1995, 1996, 1997, 1998 Free Software Foundation, Inc.
# This Makefile.in is free software; the Free Software Foundation
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# noinst_PROGRAMS = testbucket
# testbucket_SOURCES = testbucket.cxx
# testbucket_LDADD = \
# $(top_builddir)/bucket/libsgbucket.a \
# $(top_builddir)/misc/libsgmisc.a
INCLUDES += -I$(top_builddir)
# Tell versions [3.59,3.63) of GNU make to not export all variables.
# Otherwise a system limit (for SysV at least) may be exceeded.
.NOEXPORT:
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/**************************************************************************
* newbucket.hxx -- new bucket routines for better world modeling
*
* Written by Curtis L. Olson, started February 1999.
*
* Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <math.h>
#include <simgear/fgpath.hxx>
#include "newbucket.hxx"
// Build the path name for this bucket
string FGBucket::gen_base_path() const {
// long int index;
int top_lon, top_lat, main_lon, main_lat;
char hem, pole;
char raw_path[256];
top_lon = lon / 10;
main_lon = lon;
if ( (lon < 0) && (top_lon * 10 != lon) ) {
top_lon -= 1;
}
top_lon *= 10;
if ( top_lon >= 0 ) {
hem = 'e';
} else {
hem = 'w';
top_lon *= -1;
}
if ( main_lon < 0 ) {
main_lon *= -1;
}
top_lat = lat / 10;
main_lat = lat;
if ( (lat < 0) && (top_lat * 10 != lat) ) {
top_lat -= 1;
}
top_lat *= 10;
if ( top_lat >= 0 ) {
pole = 'n';
} else {
pole = 's';
top_lat *= -1;
}
if ( main_lat < 0 ) {
main_lat *= -1;
}
sprintf(raw_path, "%c%03d%c%02d/%c%03d%c%02d",
hem, top_lon, pole, top_lat,
hem, main_lon, pole, main_lat);
FGPath path( raw_path );
return path.str();
}
// find the bucket which is offset by the specified tile units in the
// X & Y direction. We need the current lon and lat to resolve
// ambiguities when going from a wider tile to a narrower one above or
// below. This assumes that we are feeding in
FGBucket fgBucketOffset( double dlon, double dlat, int dx, int dy ) {
FGBucket result( dlon, dlat );
double clat = result.get_center_lat() + dy * FG_BUCKET_SPAN;
// walk dy units in the lat direction
result.set_bucket( dlon, clat );
// find the lon span for the new latitude
double span = bucket_span( clat );
// walk dx units in the lon direction
double tmp = dlon + dx * span;
while ( tmp < -180.0 ) {
tmp += 360.0;
}
while ( tmp >= 180.0 ) {
tmp -= 360.0;
}
result.set_bucket( tmp, clat );
return result;
}
// calculate the offset between two buckets
void fgBucketDiff( const FGBucket& b1, const FGBucket& b2, int *dx, int *dy ) {
// Latitude difference
double c1_lat = b1.get_center_lat();
double c2_lat = b2.get_center_lat();
double diff_lat = c2_lat - c1_lat;
#ifdef HAVE_RINT
*dy = (int)rint( diff_lat / FG_BUCKET_SPAN );
#else
if ( diff_lat > 0 ) {
*dy = (int)( diff_lat / FG_BUCKET_SPAN + 0.5 );
} else {
*dy = (int)( diff_lat / FG_BUCKET_SPAN - 0.5 );
}
#endif
// longitude difference
double c1_lon = b1.get_center_lon();
double c2_lon = b2.get_center_lon();
double diff_lon = c2_lon - c1_lon;
double span;
if ( bucket_span(c1_lat) <= bucket_span(c2_lat) ) {
span = bucket_span(c1_lat);
} else {
span = bucket_span(c2_lat);
}
#ifdef HAVE_RINT
*dx = (int)rint( diff_lon / span );
#else
if ( diff_lon > 0 ) {
*dx = (int)( diff_lon / span + 0.5 );
} else {
*dx = (int)( diff_lon / span - 0.5 );
}
#endif
}
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/**************************************************************************
* newbucket.hxx -- new bucket routines for better world modeling
*
* Written by Curtis L. Olson, started February 1999.
*
* Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _NEWBUCKET_HXX
#define _NEWBUCKET_HXX
#include <simgear/compiler.h>
#include <simgear/constants.h>
#ifdef FG_HAVE_STD_INCLUDES
# include <cmath>
# include <cstdio> // sprintf()
# include <iostream>
#else
# include <math.h>
# include <stdio.h> // sprintf()
# include <iostream.h>
#endif
// I don't understand ... <math.h> or <cmath> should be included
// already depending on how you defined FG_HAVE_STD_INCLUDES, but I
// can go ahead and add this -- CLO
#ifdef __MWERKS__
# include <math.h> // needed fabs()
#endif
#include STL_STRING
FG_USING_STD(string);
#if ! defined( FG_HAVE_NATIVE_SGI_COMPILERS )
FG_USING_STD(ostream);
#endif
#define FG_BUCKET_SPAN 0.125 // 1/8 of a degree
#define FG_HALF_BUCKET_SPAN 0.0625 // 1/2 of 1/8 of a degree = 1/16 = 0.0625
class FGBucket;
ostream& operator<< ( ostream&, const FGBucket& );
bool operator== ( const FGBucket&, const FGBucket& );
class FGBucket {
private:
double cx, cy; // centerpoint (lon, lat) in degrees of bucket
int lon; // longitude index (-180 to 179)
int lat; // latitude index (-90 to 89)
int x; // x subdivision (0 to 7)
int y; // y subdivision (0 to 7)
public:
// default constructor
FGBucket();
// create a bucket which would contain the specified lon/lat
FGBucket(const double lon, const double lat);
// create a bucket based on "long int" index
FGBucket(const long int bindex);
// create an impossible bucket if false
FGBucket(const bool is_good);
~FGBucket();
// Set the bucket params for the specified lat and lon
void set_bucket( double dlon, double dlat );
void make_bad ( void );
// Generate the unique scenery tile index for this bucket
long int gen_index();
string gen_index_str() const;
// Build the path name for this bucket
string gen_base_path() const;
// return the center lon of a tile
double get_center_lon() const;
// return width of the tile
double get_width() const;
// return the center lat of a tile
double get_center_lat() const;
// return height of the tile
double get_height() const;
// Informational methods
inline int get_lon() const { return lon; }
inline int get_lat() const { return lat; }
inline int get_x() const { return x; }
inline int get_y() const { return y; }
// friends
friend ostream& operator<< ( ostream&, const FGBucket& );
friend bool operator== ( const FGBucket&, const FGBucket& );
};
// return the horizontal tile span factor based on latitude
inline double bucket_span( double l ) {
if ( l >= 89.0 ) {
return 360.0;
} else if ( l >= 88.0 ) {
return 8.0;
} else if ( l >= 86.0 ) {
return 4.0;
} else if ( l >= 83.0 ) {
return 2.0;
} else if ( l >= 76.0 ) {
return 1.0;
} else if ( l >= 62.0 ) {
return 0.5;
} else if ( l >= 22.0 ) {
return 0.25;
} else if ( l >= -22.0 ) {
return 0.125;
} else if ( l >= -62.0 ) {
return 0.25;
} else if ( l >= -76.0 ) {
return 0.5;
} else if ( l >= -83.0 ) {
return 1.0;
} else if ( l >= -86.0 ) {
return 2.0;
} else if ( l >= -88.0 ) {
return 4.0;
} else if ( l >= -89.0 ) {
return 8.0;
} else {
return 360.0;
}
}
// Set the bucket params for the specified lat and lon
inline void FGBucket::set_bucket( double dlon, double dlat ) {
//
// latitude first
//
double span = bucket_span( dlat );
double diff = dlon - (double)(int)dlon;
// cout << "diff = " << diff << " span = " << span << endl;
if ( (dlon >= 0) || (fabs(diff) < FG_EPSILON) ) {
lon = (int)dlon;
} else {
lon = (int)dlon - 1;
}
// find subdivision or super lon if needed
if ( span < FG_EPSILON ) {
// polar cap
lon = 0;
x = 0;
} else if ( span <= 1.0 ) {
x = (int)((dlon - lon) / span);
} else {
if ( (dlon >= 0) || (fabs(diff) < FG_EPSILON) ) {
lon = (int)( (int)(lon / span) * span);
} else {
// cout << " lon = " << lon
// << " tmp = " << (int)((lon-1) / span) << endl;
lon = (int)( (int)((lon + 1) / span) * span - span);
if ( lon < -180 ) {
lon = -180;
}
}
x = 0;
}
//
// then latitude
//
diff = dlat - (double)(int)dlat;
if ( (dlat >= 0) || (fabs(diff) < FG_EPSILON) ) {
lat = (int)dlat;
} else {
lat = (int)dlat - 1;
}
y = (int)((dlat - lat) * 8);
}
// default constructor
inline FGBucket::FGBucket() {}
// constructor for specified location
inline FGBucket::FGBucket(const double dlon, const double dlat) {
set_bucket(dlon, dlat);
}
// create an impossible bucket if false
inline FGBucket::FGBucket(const bool is_good) {
set_bucket(0.0, 0.0);
if ( !is_good ) {
lon = -1000;
}
}
// Parse a unique scenery tile index and find the lon, lat, x, and y
inline FGBucket::FGBucket(const long int bindex) {
long int index = bindex;
lon = index >> 14;
index -= lon << 14;
lon -= 180;
lat = index >> 6;
index -= lat << 6;
lat -= 90;
y = index >> 3;
index -= y << 3;
x = index;
}
// default destructor
inline FGBucket::~FGBucket() {}
// Generate the unique scenery tile index for this bucket
//
// The index is constructed as follows:
//
// 9 bits - to represent 360 degrees of longitude (-180 to 179)
// 8 bits - to represent 180 degrees of latitude (-90 to 89)
//
// Each 1 degree by 1 degree tile is further broken down into an 8x8
// grid. So we also need:
//
// 3 bits - to represent x (0 to 7)
// 3 bits - to represent y (0 to 7)
inline long int FGBucket::gen_index() {
return ((lon + 180) << 14) + ((lat + 90) << 6) + (y << 3) + x;
}
inline string FGBucket::gen_index_str() const {
char tmp[20];
sprintf(tmp, "%ld",
(((long)lon + 180) << 14) + ((lat + 90) << 6) + (y << 3) + x);
return (string)tmp;
}
// return the center lon of a tile
inline double FGBucket::get_center_lon() const {
double span = bucket_span( lat + y / 8.0 + FG_HALF_BUCKET_SPAN );
if ( span >= 1.0 ) {
return lon + span / 2.0;
} else {
return lon + x * span + span / 2.0;
}
}
// return the center lat of a tile
inline double FGBucket::get_center_lat() const {
return lat + y / 8.0 + FG_HALF_BUCKET_SPAN;
}
// return width of the tile
inline double FGBucket::get_width() const {
return bucket_span( get_center_lat() );
}
// return height of the tile
inline double FGBucket::get_height() const {
return FG_BUCKET_SPAN;
}
// create an impossible bucket
inline void FGBucket::make_bad( void ) {
set_bucket(0.0, 0.0);
lon = -1000;
}
// offset a bucket struct by the specified tile units in the X & Y
// direction
FGBucket fgBucketOffset( double dlon, double dlat, int x, int y );
// calculate the offset between two buckets
void fgBucketDiff( const FGBucket& b1, const FGBucket& b2, int *dx, int *dy );
/*
// Given a lat/lon, fill in the local tile index array
void fgBucketGenIdxArray(fgBUCKET *p1, fgBUCKET *tiles, int width, int height);
*/
inline ostream&
operator<< ( ostream& out, const FGBucket& b )
{
return out << b.lon << ":" << b.x << ", " << b.lat << ":" << b.y;
}
inline bool
operator== ( const FGBucket& b1, const FGBucket& b2 )
{
return ( b1.lon == b2.lon &&
b1.lat == b2.lat &&
b1.x == b2.x &&
b1.y == b2.y );
}
#endif // _NEWBUCKET_HXX
+9
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@@ -0,0 +1,9 @@
EXTRA_DIST = logtest.cxx
lib_LIBRARIES = libsgdebug.a
include_HEADERS = debug_types.h logstream.hxx
libsgdebug_a_SOURCES = logstream.cxx
INCLUDES += -I$(top_builddir)
+338
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@@ -0,0 +1,338 @@
# Makefile.in generated automatically by automake 1.3 from Makefile.am
# Copyright (C) 1994, 1995, 1996, 1997, 1998 Free Software Foundation, Inc.
# This Makefile.in is free software; the Free Software Foundation
# gives unlimited permission to copy and/or distribute it,
# with or without modifications, as long as this notice is preserved.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY, to the extent permitted by law; without
# even the implied warranty of MERCHANTABILITY or FITNESS FOR A
# PARTICULAR PURPOSE.
SHELL = /bin/sh
srcdir = @srcdir@
top_srcdir = @top_srcdir@
VPATH = @srcdir@
prefix = @prefix@
exec_prefix = @exec_prefix@
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sbindir = @sbindir@
libexecdir = @libexecdir@
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sysconfdir = @sysconfdir@
sharedstatedir = @sharedstatedir@
localstatedir = @localstatedir@
libdir = @libdir@
infodir = @infodir@
mandir = @mandir@
includedir = @includedir@
oldincludedir = /usr/include
DISTDIR =
pkgdatadir = $(datadir)/@PACKAGE@
pkglibdir = $(libdir)/@PACKAGE@
pkgincludedir = $(includedir)/@PACKAGE@
top_builddir = ..
ACLOCAL = @ACLOCAL@
AUTOCONF = @AUTOCONF@
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AUTOHEADER = @AUTOHEADER@
INSTALL = @INSTALL@
INSTALL_PROGRAM = @INSTALL_PROGRAM@
INSTALL_DATA = @INSTALL_DATA@
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transform = @program_transform_name@
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PRE_INSTALL = :
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CC = @CC@
CXX = @CXX@
LN_S = @LN_S@
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PACKAGE = @PACKAGE@
RANLIB = @RANLIB@
VERSION = @VERSION@
base_LIBS = @base_LIBS@
opengl_LIBS = @opengl_LIBS@
EXTRA_DIST = logtest.cxx
lib_LIBRARIES = libsgdebug.a
include_HEADERS = debug_types.h logstream.hxx
libsgdebug_a_SOURCES = logstream.cxx
mkinstalldirs = $(SHELL) $(top_srcdir)/mkinstalldirs
CONFIG_HEADER = ../include/config.h
CONFIG_CLEAN_FILES =
LIBRARIES = $(lib_LIBRARIES)
DEFS = @DEFS@ -I. -I$(srcdir) -I../include
CPPFLAGS = @CPPFLAGS@
LDFLAGS = @LDFLAGS@
LIBS = @LIBS@
X_CFLAGS = @X_CFLAGS@
X_LIBS = @X_LIBS@
X_EXTRA_LIBS = @X_EXTRA_LIBS@
X_PRE_LIBS = @X_PRE_LIBS@
libsgdebug_a_LIBADD =
libsgdebug_a_OBJECTS = logstream.o
AR = ar
CXXFLAGS = @CXXFLAGS@
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CXXLINK = $(CXX) $(CXXFLAGS) $(LDFLAGS) -o $@
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echo " $(RANLIB) $(DESTDIR)$(libdir)/$$p"; \
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$(COMPILE) -c $<
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done
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done
tags: TAGS
ID: $(HEADERS) $(SOURCES) $(LISP)
here=`pwd` && cd $(srcdir) \
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TAGS: $(HEADERS) $(SOURCES) $(TAGS_DEPENDENCIES) $(LISP)
tags=; \
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unique=`for i in $$list; do echo $$i; done | \
awk ' { files[$$0] = 1; } \
END { for (i in files) print i; }'`; \
test -z "$(ETAGS_ARGS)$$unique$(LISP)$$tags" \
|| (cd $(srcdir) && etags $(ETAGS_ARGS) $$tags $$unique $(LISP) -o $$here/TAGS)
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subdir = debug
distdir: $(DISTFILES)
here=`cd $(top_builddir) && pwd`; \
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distdir=`cd $(distdir) && pwd`; \
cd $(top_srcdir) \
&& $(AUTOMAKE) --include-deps --build-dir=$$here --srcdir-name=$(top_srcdir) --output-dir=$$top_distdir --gnu debug/Makefile
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test -f $(distdir)/$$file \
|| ln $$d/$$file $(distdir)/$$file 2> /dev/null \
|| cp -p $$d/$$file $(distdir)/$$file; \
done
DEPS_MAGIC := $(shell mkdir .deps > /dev/null 2>&1 || :)
-include $(DEP_FILES)
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$(COMPILE) -Wp,-MD,.deps/$(*F).P -c $<
%.lo: %.c
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$(LTCOMPILE) -Wp,-MD,.deps/$(*F).p -c $<
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< .deps/$(*F).p > .deps/$(*F).P
@-rm -f .deps/$(*F).p
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@echo '$(CXXCOMPILE) -c $<'; \
$(CXXCOMPILE) -Wp,-MD,.deps/$(*F).P -c $<
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$(mkinstalldirs) $(DATADIR)$(libdir) $(DATADIR)$(includedir)
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clean-generic:
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distclean-generic:
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maintainer-clean-generic:
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mostlyclean: mostlyclean-libLIBRARIES mostlyclean-compile \
mostlyclean-tags mostlyclean-depend mostlyclean-generic
clean: clean-libLIBRARIES clean-compile clean-tags clean-depend \
clean-generic mostlyclean
distclean: distclean-libLIBRARIES distclean-compile distclean-tags \
distclean-depend distclean-generic clean
-rm -f config.status
maintainer-clean: maintainer-clean-libLIBRARIES \
maintainer-clean-compile maintainer-clean-tags \
maintainer-clean-depend maintainer-clean-generic \
distclean
@echo "This command is intended for maintainers to use;"
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clean-libLIBRARIES maintainer-clean-libLIBRARIES uninstall-libLIBRARIES \
install-libLIBRARIES mostlyclean-compile distclean-compile \
clean-compile maintainer-clean-compile uninstall-includeHEADERS \
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INCLUDES += -I$(top_builddir)
# Tell versions [3.59,3.63) of GNU make to not export all variables.
# Otherwise a system limit (for SysV at least) may be exceeded.
.NOEXPORT:
+38
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@@ -0,0 +1,38 @@
// NB: To add a dbg_class, add it here, and add it to the structure in
// fg_debug.c
typedef enum {
FG_NONE = 0x00000000,
FG_TERRAIN = 0x00000001,
FG_ASTRO = 0x00000002,
FG_FLIGHT = 0x00000004,
FG_INPUT = 0x00000008,
FG_GL = 0x00000010,
FG_VIEW = 0x00000020,
FG_COCKPIT = 0x00000040,
FG_GENERAL = 0x00000080,
FG_MATH = 0x00000100,
FG_EVENT = 0x00000200,
FG_AIRCRAFT = 0x00000400,
FG_AUTOPILOT = 0x00000800,
FG_IO = 0x00001000,
FG_CLIPPER = 0x00002000,
FG_NETWORK = 0x00004000,
FG_UNDEFD = 0x00008000, // For range checking
FG_ALL = 0xFFFFFFFF
} fgDebugClass;
// NB: To add a priority, add it here.
typedef enum {
FG_BULK, // For frequent messages
FG_DEBUG, // Less frequent debug type messages
FG_INFO, // Informatory messages
FG_WARN, // Possible impending problem
FG_ALERT // Very possible impending problem
// FG_EXIT, // Problem (no core)
// FG_ABORT // Abandon ship (core)
} fgDebugPriority;
+63
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@@ -0,0 +1,63 @@
// Stream based logging mechanism.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include "logstream.hxx"
bool logbuf::logging_enabled = true;
fgDebugClass logbuf::logClass = FG_NONE;
fgDebugPriority logbuf::logPriority = FG_INFO;
streambuf* logbuf::sbuf = NULL;
logbuf::logbuf()
{
// if ( sbuf == NULL )
// sbuf = cerr.rdbuf();
}
logbuf::~logbuf()
{
if ( sbuf )
sync();
}
void
logbuf::set_sb( streambuf* sb )
{
if ( sbuf )
sync();
sbuf = sb;
}
void
logbuf::set_log_level( fgDebugClass c, fgDebugPriority p )
{
logClass = c;
logPriority = p;
}
void
logstream::setLogLevels( fgDebugClass c, fgDebugPriority p )
{
logbuf::set_log_level( c, p );
}
+220
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@@ -0,0 +1,220 @@
// Stream based logging mechanism.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _LOGSTREAM_H
#define _LOGSTREAM_H
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <simgear/compiler.h>
#ifdef FG_HAVE_STD_INCLUDES
# include <streambuf>
# include <iostream>
#else
# include <iostream.h>
# include <simgear/fg_traits.hxx>
#endif
#include <simgear/debug_types.h>
#ifndef FG_HAVE_NATIVE_SGI_COMPILERS
FG_USING_STD(streambuf);
FG_USING_STD(ostream);
FG_USING_STD(cerr);
FG_USING_STD(endl);
#endif
#ifdef __MWERKS__
# define cerr std::cerr
# define endl std::endl
FG_USING_STD(iostream);
#endif
//
// TODO:
//
// 1. Change output destination. Done.
// 2. Make logbuf thread safe.
// 3. Read environment for default debugClass and debugPriority.
//
//-----------------------------------------------------------------------------
//
// logbuf is an output-only streambuf with the ability to disable sets of
// messages at runtime. Only messages with priority >= logbuf::logPriority
// and debugClass == logbuf::logClass are output.
//
class logbuf : public streambuf
{
public:
#ifndef FG_HAVE_STD_INCLUDES
typedef char_traits<char> traits_type;
typedef char_traits<char>::int_type int_type;
typedef char_traits<char>::pos_type pos_type;
typedef char_traits<char>::off_type off_type;
#endif
// logbuf( streambuf* sb ) : sbuf(sb) {}
logbuf();
~logbuf();
// Is logging enabled?
bool enabled() { return logging_enabled; }
// Set the logging level of subsequent messages.
void set_log_state( fgDebugClass c, fgDebugPriority p );
// Set the global logging level.
static void set_log_level( fgDebugClass c, fgDebugPriority p );
//
void set_sb( streambuf* sb );
protected:
inline virtual int sync();
int_type overflow( int ch );
// int xsputn( const char* s, istreamsize n );
private:
// The streambuf used for actual output. Defaults to cerr.rdbuf().
static streambuf* sbuf;
static bool logging_enabled;
static fgDebugClass logClass;
static fgDebugPriority logPriority;
private:
// Not defined.
logbuf( const logbuf& );
void operator= ( const logbuf& );
};
inline int
logbuf::sync()
{
#ifdef FG_HAVE_STD_INCLUDES
return sbuf->pubsync();
#else
return sbuf->sync();
#endif
}
inline void
logbuf::set_log_state( fgDebugClass c, fgDebugPriority p )
{
logging_enabled = ((c & logClass) != 0 && p >= logPriority);
}
inline logbuf::int_type
logbuf::overflow( int c )
{
return logging_enabled ? sbuf->sputc(c) : (EOF == 0 ? 1: 0);
}
//-----------------------------------------------------------------------------
//
// logstream manipulator for setting the log level of a message.
//
struct loglevel
{
loglevel( fgDebugClass c, fgDebugPriority p )
: logClass(c), logPriority(p) {}
fgDebugClass logClass;
fgDebugPriority logPriority;
};
//-----------------------------------------------------------------------------
//
// A helper class that ensures a streambuf and ostream are constructed and
// destroyed in the correct order. The streambuf must be created before the
// ostream but bases are constructed before members. Thus, making this class
// a private base of logstream, declared to the left of ostream, we ensure the
// correct order of construction and destruction.
//
struct logstream_base
{
// logstream_base( streambuf* sb ) : lbuf(sb) {}
logstream_base() {}
logbuf lbuf;
};
//-----------------------------------------------------------------------------
//
//
//
class logstream : private logstream_base, public ostream
{
public:
// The default is to send messages to cerr.
logstream( ostream& out )
// : logstream_base(out.rdbuf()),
: logstream_base(),
ostream(&lbuf) { lbuf.set_sb(out.rdbuf());}
void set_output( ostream& out ) { lbuf.set_sb( out.rdbuf() ); }
// Set the global log class and priority level.
void setLogLevels( fgDebugClass c, fgDebugPriority p );
// Output operator to capture the debug level and priority of a message.
inline ostream& operator<< ( const loglevel& l );
};
inline ostream&
logstream::operator<< ( const loglevel& l )
{
lbuf.set_log_state( l.logClass, l.logPriority );
return *this;
}
//-----------------------------------------------------------------------------
//
// Return the one and only logstream instance.
// We use a function instead of a global object so we are assured that cerr
// has been initialised.
//
inline logstream&
fglog()
{
static logstream logstrm( cerr );
return logstrm;
}
#ifdef FG_NDEBUG
# define FG_LOG(C,P,M)
#elif defined( __MWERKS__ )
# define FG_LOG(C,P,M) ::fglog() << ::loglevel(C,P) << M << std::endl
#else
# define FG_LOG(C,P,M) fglog() << loglevel(C,P) << M << endl
#endif
#endif // _LOGSTREAM_H
+34
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@@ -0,0 +1,34 @@
#include <string>
#include "Debug/logstream.hxx"
int
main( int argc, char* argv[] )
{
fglog().setLogLevels( FG_ALL, FG_INFO );
FG_LOG( FG_TERRAIN, FG_BULK, "terrain::bulk" ); // shouldnt appear
FG_LOG( FG_TERRAIN, FG_DEBUG, "terrain::debug" ); // shouldnt appear
FG_LOG( FG_TERRAIN, FG_INFO, "terrain::info" );
FG_LOG( FG_TERRAIN, FG_WARN, "terrain::warn" );
FG_LOG( FG_TERRAIN, FG_ALERT, "terrain::alert" );
int i = 12345;
long l = 54321L;
double d = 3.14159;
string s = "Hello world!";
FG_LOG( FG_EVENT, FG_INFO, "event::info "
<< "i=" << i
<< ", l=" << l
<< ", d=" << d
<< ", d*l=" << d*l
<< ", s=\"" << s << "\"" );
// This shouldn't appear in log output:
FG_LOG( FG_EVENT, FG_DEBUG, "event::debug "
<< "- this should be seen - "
<< "d=" << d
<< ", s=\"" << s << "\"" );
return 0;
}
+19
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@@ -0,0 +1,19 @@
noinst_LIBRARIES = libAstro.a
libAstro_a_SOURCES = \
celestialBody.cxx celestialBody.hxx \
jupiter.cxx jupiter.hxx \
mars.cxx mars.hxx \
mercury.cxx mercury.hxx \
moon.cxx moon.hxx \
neptune.cxx neptune.hxx \
pluto.hxx \
saturn.cxx saturn.hxx \
sky.cxx sky.hxx \
solarsystem.cxx solarsystem.hxx \
star.cxx star.hxx \
stars.cxx stars.hxx \
uranus.cxx uranus.hxx \
venus.cxx venus.hxx
INCLUDES += -I$(top_builddir) -I$(top_builddir)/Lib -I$(top_builddir)/Simulator
+178
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@@ -0,0 +1,178 @@
/**************************************************************************
* celestialBody.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#include <Debug/logstream.hxx>
#ifdef FG_MATH_EXCEPTION_CLASH
# define exception c_exception
#endif
#include <math.h>
#include "celestialBody.hxx"
#include "star.hxx"
/**************************************************************************
* void CelestialBody::updatePosition(fgTIME *t, Star *ourSun)
*
* Basically, this member function provides a general interface for
* calculating the right ascension and declinaion. This function is
* used for calculating the planetary positions. For the planets, an
* overloaded member function is provided to additionally calculate the
* planet's magnitude.
* The sun and moon have their own overloaded updatePosition member, as their
* position is calculated an a slightly different manner.
*
* arguments:
* fgTIME t: provides the current time.
* Star *ourSun: the sun's position is needed to convert heliocentric
* coordinates into geocentric coordinates.
*
* return value: none
*
*************************************************************************/
void CelestialBody::updatePosition(FGTime *t, Star *ourSun)
{
double eccAnom, v, ecl, actTime,
xv, yv, xh, yh, zh, xg, yg, zg, xe, ye, ze;
updateOrbElements(t);
actTime = fgCalcActTime(t);
// calcualate the angle bewteen ecliptic and equatorial coordinate system
ecl = DEG_TO_RAD * (23.4393 - 3.563E-7 *actTime);
eccAnom = fgCalcEccAnom(M, e); //calculate the eccentric anomaly
xv = a * (cos(eccAnom) - e);
yv = a * (sqrt (1.0 - e*e) * sin(eccAnom));
v = atan2(yv, xv); // the planet's true anomaly
r = sqrt (xv*xv + yv*yv); // the planet's distance
// calculate the planet's position in 3D space
xh = r * (cos(N) * cos(v+w) - sin(N) * sin(v+w) * cos(i));
yh = r * (sin(N) * cos(v+w) + cos(N) * sin(v+w) * cos(i));
zh = r * (sin(v+w) * sin(i));
// calculate the ecliptic longitude and latitude
xg = xh + ourSun->getxs();
yg = yh + ourSun->getys();
zg = zh;
lonEcl = atan2(yh, xh);
latEcl = atan2(zh, sqrt(xh*xh+yh*yh));
xe = xg;
ye = yg * cos(ecl) - zg * sin(ecl);
ze = yg * sin(ecl) + zg * cos(ecl);
rightAscension = atan2(ye, xe);
declination = atan2(ze, sqrt(xe*xe + ye*ye));
FG_LOG(FG_GENERAL, FG_INFO, "Planet found at : "
<< rightAscension << " (ra), " << declination << " (dec)" );
//calculate some variables specific to calculating the magnitude
//of the planet
R = sqrt (xg*xg + yg*yg + zg*zg);
s = ourSun->getDistance();
// It is possible from these calculations for the argument to acos
// to exceed the valid range for acos(). So we do a little extra
// checking.
double tmp = (r*r + R*R - s*s) / (2*r*R);
if ( tmp > 1.0) {
tmp = 1.0;
} else if ( tmp < -1.0) {
tmp = -1.0;
}
FV = RAD_TO_DEG * acos( tmp );
};
/****************************************************************************
* double CelestialBody::fgCalcEccAnom(double M, double e)
* this private member calculates the eccentric anomaly of a celestial body,
* given its mean anomaly and eccentricity.
*
* -Mean anomaly: the approximate angle between the perihelion and the current
* position. this angle increases uniformly with time.
*
* True anomaly: the actual angle between perihelion and current position.
*
* Eccentric anomaly: this is an auxilary angle, used in calculating the true
* anomaly from the mean anomaly.
*
* -eccentricity. Indicates the amount in which the orbit deviates from a
* circle (0 = circle, 0-1, is ellipse, 1 = parabola, > 1 = hyperbola).
*
* This function is also known as solveKeplersEquation()
*
* arguments:
* M: the mean anomaly
* e: the eccentricity
*
* return value:
* the eccentric anomaly
*
****************************************************************************/
double CelestialBody::fgCalcEccAnom(double M, double e)
{
double
eccAnom, E0, E1, diff;
eccAnom = M + e * sin(M) * (1.0 + e * cos (M));
// iterate to achieve a greater precision for larger eccentricities
if (e > 0.05)
{
E0 = eccAnom;
do
{
E1 = E0 - (E0 - e * sin(E0) - M) / (1 - e *cos(E0));
diff = fabs(E0 - E1);
E0 = E1;
}
while (diff > (DEG_TO_RAD * 0.001));
return E0;
}
return eccAnom;
}
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/**************************************************************************
* celestialBody.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _CELESTIALBODY_H_
#define _CELESTIALBODY_H_
#ifndef __cplusplus
# error This library requires C++
#endif
#include <Time/fg_time.hxx>
#include <Include/fg_constants.h>
class Star;
class CelestialBody
{
protected: // make the data protected, in order to give the inherited
// classes direct access to the data
double NFirst; /* longitude of the ascending node first part */
double NSec; /* longitude of the ascending node second part */
double iFirst; /* inclination to the ecliptic first part */
double iSec; /* inclination to the ecliptic second part */
double wFirst; /* first part of argument of perihelion */
double wSec; /* second part of argument of perihelion */
double aFirst; /* semimayor axis first part*/
double aSec; /* semimayor axis second part */
double eFirst; /* eccentricity first part */
double eSec; /* eccentricity second part */
double MFirst; /* Mean anomaly first part */
double MSec; /* Mean anomaly second part */
double N, i, w, a, e, M; /* the resulting orbital elements, obtained from the former */
double rightAscension, declination;
double r, R, s, FV;
double magnitude;
double lonEcl, latEcl;
double fgCalcEccAnom(double M, double e);
double fgCalcActTime(FGTime *t);
void updateOrbElements(FGTime *t);
public:
CelestialBody(double Nf, double Ns,
double If, double Is,
double wf, double ws,
double af, double as,
double ef, double es,
double Mf, double Ms, FGTime *t);
void getPos(double *ra, double *dec);
void getPos(double *ra, double *dec, double *magnitude);
double getLon();
double getLat();
void updatePosition(FGTime *t, Star *ourSun);
};
/*****************************************************************************
* inline CelestialBody::CelestialBody
* public constructor for a generic celestialBody object.
* initializes the 6 primary orbital elements. The elements are:
* N: longitude of the ascending node
* i: inclination to the ecliptic
* w: argument of perihelion
* a: semi-major axis, or mean distance from the sun
* e: eccenticity
* M: mean anomaly
* Each orbital element consists of a constant part and a variable part that
* gradually changes over time.
*
* Argumetns:
* the 13 arguments to the constructor constitute the first, constant
* ([NiwaeM]f) and the second variable ([NiwaeM]s) part of the orbital
* elements. The 13th argument is the current time. Note that the inclination
* is written with a capital (If, Is), because 'if' is a reserved word in the
* C/C++ programming language.
***************************************************************************/
inline CelestialBody::CelestialBody(double Nf, double Ns,
double If, double Is,
double wf, double ws,
double af, double as,
double ef, double es,
double Mf, double Ms, FGTime *t)
{
NFirst = Nf; NSec = Ns;
iFirst = If; iSec = Is;
wFirst = wf; wSec = ws;
aFirst = af; aSec = as;
eFirst = ef; eSec = es;
MFirst = Mf; MSec = Ms;
updateOrbElements(t);
};
/****************************************************************************
* inline void CelestialBody::updateOrbElements(FGTime *t)
* given the current time, this private member calculates the actual
* orbital elements
*
* Arguments: FGTime *t: the current time:
*
* return value: none
***************************************************************************/
inline void CelestialBody::updateOrbElements(FGTime *t)
{
double actTime = fgCalcActTime(t);
M = DEG_TO_RAD * (MFirst + (MSec * actTime));
w = DEG_TO_RAD * (wFirst + (wSec * actTime));
N = DEG_TO_RAD * (NFirst + (NSec * actTime));
i = DEG_TO_RAD * (iFirst + (iSec * actTime));
e = eFirst + (eSec * actTime);
a = aFirst + (aSec * actTime);
}
/*****************************************************************************
* inline double CelestialBody::fgCalcActTime(FGTime *t)
* this private member function returns the offset in days from the epoch for
* wich the orbital elements are calculated (Jan, 1st, 2000).
*
* Argument: the current time
*
* return value: the (fractional) number of days until Jan 1, 2000.
****************************************************************************/
inline double CelestialBody::fgCalcActTime(FGTime *t)
{
return (t->getMjd() - 36523.5);
}
/*****************************************************************************
* inline void CelestialBody::getPos(double* ra, double* dec)
* gives public access to Right Ascension and declination
*
****************************************************************************/
inline void CelestialBody::getPos(double* ra, double* dec)
{
*ra = rightAscension;
*dec = declination;
}
/*****************************************************************************
* inline void CelestialBody::getPos(double* ra, double* dec, double* magnitude
* gives public acces to the current Right ascension, declination, and
* magnitude
****************************************************************************/
inline void CelestialBody::getPos(double* ra, double* dec, double* magn)
{
*ra = rightAscension;
*dec = declination;
*magn = magnitude;
}
inline double CelestialBody::getLon()
{
return lonEcl;
}
inline double CelestialBody::getLat()
{
return latEcl;
}
#endif // _CELESTIALBODY_H_
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/**************************************************************************
* jupiter.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "jupiter.hxx"
/*************************************************************************
* Jupiter::Jupiter(FGTime *t)
* Public constructor for class Jupiter
* Argument: The current time.
* the hard coded orbital elements for Jupiter are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Jupiter::Jupiter(FGTime *t) :
CelestialBody(100.4542, 2.7685400E-5,
1.3030, -1.557E-7,
273.8777, 1.6450500E-5,
5.2025600, 0.000000,
0.048498, 4.469E-9,
19.89500, 0.08308530010, t)
{
}
/*************************************************************************
* void Jupiter::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Jupiter, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Jupiter specific equation
*************************************************************************/
void Jupiter::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -9.25 + 5*log10( r*R ) + 0.014 * FV;
}
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/**************************************************************************
* jupiter.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _JUPITER_HXX_
#define _JUPITER_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Jupiter : public CelestialBody
{
public:
Jupiter (FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _JUPITER_HXX_
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/**************************************************************************
* mars.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "mars.hxx"
/*************************************************************************
* Mars::Mars(FGTime *t)
* Public constructor for class Mars
* Argument: The current time.
* the hard coded orbital elements for Mars are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Mars::Mars(FGTime *t) :
CelestialBody(49.55740, 2.1108100E-5,
1.8497, -1.78E-8,
286.5016, 2.9296100E-5,
1.5236880, 0.000000,
0.093405, 2.516E-9,
18.60210, 0.52402077660, t)
{
}
/*************************************************************************
* void Mars::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Mars, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Mars specific equation
*************************************************************************/
void Mars::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -1.51 + 5*log10( r*R ) + 0.016 * FV;
}
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/**************************************************************************
* mars.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _MARS_HXX_
#define _MARS_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Mars : public CelestialBody
{
public:
Mars ( FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _MARS_HXX_
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/**************************************************************************
* mercury.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "mercury.hxx"
/*************************************************************************
* Mercury::Mercury(FGTime *t)
* Public constructor for class Mercury
* Argument: The current time.
* the hard coded orbital elements for Mercury are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Mercury::Mercury(FGTime *t) :
CelestialBody (48.33130, 3.2458700E-5,
7.0047, 5.00E-8,
29.12410, 1.0144400E-5,
0.3870980, 0.000000,
0.205635, 5.59E-10,
168.6562, 4.09233443680, t)
{
}
/*************************************************************************
* void Mercury::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Mercury, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Mercury specific equation
*************************************************************************/
void Mercury::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -0.36 + 5*log10( r*R ) + 0.027 * FV + 2.2E-13 * pow(FV, 6);
}
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/**************************************************************************
* mercury.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _MERCURY_HXX_
#define _MERCURY_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Mercury : public CelestialBody
{
public:
Mercury ( FGTime *t);
void updatePosition(FGTime *t, Star* ourSun);
};
#endif // _MERURY_HXX_
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/**************************************************************************
* moon.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#include <string.h>
#include <Debug/logstream.hxx>
#include <Main/options.hxx>
#include <Misc/fgpath.hxx>
#include <Objects/texload.h>
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include <FDM/flight.hxx>
#include "moon.hxx"
/*************************************************************************
* Moon::Moon(FGTime *t)
* Public constructor for class Moon. Initializes the orbital elements and
* sets up the moon texture.
* Argument: The current time.
* the hard coded orbital elements for Moon are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Moon::Moon(FGTime *t) :
CelestialBody(125.1228, -0.0529538083,
5.1454, 0.00000,
318.0634, 0.1643573223,
60.266600, 0.000000,
0.054900, 0.000000,
115.3654, 13.0649929509, t)
{
int width, height;
FG_LOG( FG_GENERAL, FG_INFO, "Initializing Moon Texture");
#ifdef GL_VERSION_1_1
xglGenTextures(1, &moon_texid);
xglBindTexture(GL_TEXTURE_2D, moon_texid);
#elif GL_EXT_texture_object
xglGenTexturesEXT(1, &moon_texid);
xglBindTextureEXT(GL_TEXTURE_2D, moon_texid);
#else
# error port me
#endif
glPixelStorei(GL_UNPACK_ALIGNMENT, 1);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MIN_FILTER, GL_LINEAR);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MAG_FILTER, GL_LINEAR);
// load in the texture data
FGPath tpath( current_options.get_fg_root() );
tpath.append( "Textures" );
tpath.append( "moon.rgb" );
if ( (moon_texbuf = read_rgb_texture(tpath.c_str(), &width, &height))
== NULL )
{
// Try compressed
FGPath fg_tpath = tpath;
fg_tpath.append( ".gz" );
if ( (moon_texbuf = read_rgb_texture(fg_tpath.c_str(), &width, &height))
== NULL )
{
FG_LOG( FG_GENERAL, FG_ALERT,
"Error in loading moon texture " << tpath.str() );
exit(-1);
}
}
glTexImage2D( GL_TEXTURE_2D,
0,
GL_RGB,
256, 256,
0,
GL_RGB, GL_UNSIGNED_BYTE,
moon_texbuf);
// setup the halo texture
FG_LOG( FG_GENERAL, FG_INFO, "Initializing Moon Texture");
#ifdef GL_VERSION_1_1
xglGenTextures(1, &moon_halotexid);
xglBindTexture(GL_TEXTURE_2D, moon_halotexid);
#elif GL_EXT_texture_object
xglGenTexturesEXT(1, &moon_halotexid);
xglBindTextureEXT(GL_TEXTURE_2D, moon_halotexid);
#else
# error port me
#endif
glPixelStorei(GL_UNPACK_ALIGNMENT, 1);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MIN_FILTER, GL_LINEAR);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MAG_FILTER, GL_LINEAR);
setHalo();
glTexImage2D( GL_TEXTURE_2D,
0,
GL_RGBA,
256, 256,
0,
GL_RGBA, GL_UNSIGNED_BYTE,
moon_halotexbuf);
moonObject = gluNewQuadric();
}
Moon::~Moon()
{
//delete moonObject;
delete moon_texbuf;
delete moon_halotexbuf;
}
static int texWidth = 256; /* 64x64 is plenty */
void Moon::setHalo()
{
int texSize;
//void *textureBuf;
GLubyte *p;
int i,j;
double radius;
texSize = texWidth*texWidth;
moon_halotexbuf = new GLubyte[texSize*4];
if (!moon_halotexbuf)
return; // Ugly!
p = moon_halotexbuf;
radius = (double)(texWidth / 2);
for (i=0; i < texWidth; i++) {
for (j=0; j < texWidth; j++) {
double x, y, d;
*p = 0xff;
*(p+1) = 0xff;
*(p+2) = 0xff;
x = fabs((double)(i - (texWidth / 2)));
y = fabs((double)(j - (texWidth / 2)));
d = sqrt((x * x) + (y * y));
if (d < radius) {
double t = 1.0 - (d / radius); // t is 1.0 at center, 0.0 at edge */
// inverse square looks nice
*(p+3) = (int)((double) 0x20 * (t*t));
} else {
*(p+3) = 0x00;
}
p += 4;
}
}
//gluBuild2DMipmaps(GL_TEXTURE_2D, 1, texWidth, texWidth,
// GL_LUMINANCE,
// GL_UNSIGNED_BYTE, textureBuf);
//free(textureBuf);
}
/*****************************************************************************
* void Moon::updatePosition(FGTime *t, Star *ourSun)
* this member function calculates the actual topocentric position (i.e.)
* the position of the moon as seen from the current position on the surface
* of the moon.
****************************************************************************/
void Moon::updatePosition(FGTime *t, Star *ourSun)
{
double
eccAnom, ecl, actTime,
xv, yv, v, r, xh, yh, zh, xg, yg, zg, xe, ye, ze,
Ls, Lm, D, F, mpar, gclat, rho, HA, g,
geoRa, geoDec;
fgAIRCRAFT *air;
FGInterface *f;
air = &current_aircraft;
f = air->fdm_state;
updateOrbElements(t);
actTime = fgCalcActTime(t);
// calculate the angle between ecliptic and equatorial coordinate system
// in Radians
ecl = ((DEG_TO_RAD * 23.4393) - (DEG_TO_RAD * 3.563E-7) * actTime);
eccAnom = fgCalcEccAnom(M, e); // Calculate the eccentric anomaly
xv = a * (cos(eccAnom) - e);
yv = a * (sqrt(1.0 - e*e) * sin(eccAnom));
v = atan2(yv, xv); // the moon's true anomaly
r = sqrt (xv*xv + yv*yv); // and its distance
// estimate the geocentric rectangular coordinates here
xh = r * (cos(N) * cos (v+w) - sin (N) * sin(v+w) * cos(i));
yh = r * (sin(N) * cos (v+w) + cos (N) * sin(v+w) * cos(i));
zh = r * (sin(v+w) * sin(i));
// calculate the ecliptic latitude and longitude here
lonEcl = atan2 (yh, xh);
latEcl = atan2(zh, sqrt(xh*xh + yh*yh));
/* Calculate a number of perturbatioin, i.e. disturbances caused by the
* gravitational infuence of the sun and the other major planets.
* The largest of these even have a name */
Ls = ourSun->getM() + ourSun->getw();
Lm = M + w + N;
D = Lm - Ls;
F = Lm - N;
lonEcl += DEG_TO_RAD * (-1.274 * sin (M - 2*D)
+0.658 * sin (2*D)
-0.186 * sin(ourSun->getM())
-0.059 * sin(2*M - 2*D)
-0.057 * sin(M - 2*D + ourSun->getM())
+0.053 * sin(M + 2*D)
+0.046 * sin(2*D - ourSun->getM())
+0.041 * sin(M - ourSun->getM())
-0.035 * sin(D)
-0.031 * sin(M + ourSun->getM())
-0.015 * sin(2*F - 2*D)
+0.011 * sin(M - 4*D)
);
latEcl += DEG_TO_RAD * (-0.173 * sin(F-2*D)
-0.055 * sin(M - F - 2*D)
-0.046 * sin(M + F - 2*D)
+0.033 * sin(F + 2*D)
+0.017 * sin(2*M + F)
);
r += (-0.58 * cos(M - 2*D)
-0.46 * cos(2*D)
);
FG_LOG(FG_GENERAL, FG_INFO, "Running moon update");
xg = r * cos(lonEcl) * cos(latEcl);
yg = r * sin(lonEcl) * cos(latEcl);
zg = r * sin(latEcl);
xe = xg;
ye = yg * cos(ecl) -zg * sin(ecl);
ze = yg * sin(ecl) +zg * cos(ecl);
geoRa = atan2(ye, xe);
geoDec = atan2(ze, sqrt(xe*xe + ye*ye));
/* FG_LOG( FG_GENERAL, FG_INFO,
"(geocentric) geoRa = (" << (RAD_TO_DEG * geoRa)
<< "), geoDec= (" << (RAD_TO_DEG * geoDec) << ")" ); */
// Given the moon's geocentric ra and dec, calculate its
// topocentric ra and dec. i.e. the position as seen from the
// surface of the earth, instead of the center of the earth
// First calculate the moon's parrallax, that is, the apparent size of the
// (equatorial) radius of the earth, as seen from the moon
mpar = asin ( 1 / r);
// FG_LOG( FG_GENERAL, FG_INFO, "r = " << r << " mpar = " << mpar );
// FG_LOG( FG_GENERAL, FG_INFO, "lat = " << f->get_Latitude() );
gclat = f->get_Latitude() - 0.003358 *
sin (2 * DEG_TO_RAD * f->get_Latitude() );
// FG_LOG( FG_GENERAL, FG_INFO, "gclat = " << gclat );
rho = 0.99883 + 0.00167 * cos(2 * DEG_TO_RAD * f->get_Latitude());
// FG_LOG( FG_GENERAL, FG_INFO, "rho = " << rho );
if (geoRa < 0)
geoRa += (2*FG_PI);
HA = t->getLst() - (3.8197186 * geoRa);
/* FG_LOG( FG_GENERAL, FG_INFO, "t->getLst() = " << t->getLst()
<< " HA = " << HA ); */
g = atan (tan(gclat) / cos ((HA / 3.8197186)));
// FG_LOG( FG_GENERAL, FG_INFO, "g = " << g );
rightAscension = geoRa - mpar * rho * cos(gclat) * sin(HA) / cos (geoDec);
declination = geoDec - mpar * rho * sin (gclat) * sin (g - geoDec) / sin(g);
/* FG_LOG( FG_GENERAL, FG_INFO,
"Ra = (" << (RAD_TO_DEG *rightAscension)
<< "), Dec= (" << (RAD_TO_DEG *declination) << ")" ); */
}
/************************************************************************
* void Moon::newImage()
*
* This function regenerates a new visual image of the moon, which is added to
* solarSystem display list.
*
* Arguments: Right Ascension and declination
*
* return value: none
**************************************************************************/
void Moon::newImage()
{
fgLIGHT *l = &cur_light_params;
float moon_angle = l->moon_angle;
/*double x_2, x_4, x_8, x_10;
GLfloat ambient;
GLfloat amb[4];*/
int moonSize = 550;
GLfloat moonColor[4] = {0.85, 0.75, 0.35, 1.0};
GLfloat black[4] = {0.0, 0.0, 0.0, 1.0};
GLfloat white[4] = {1.0, 1.0, 1.0, 0.0};
if( moon_angle*RAD_TO_DEG < 100 )
{
FG_LOG( FG_ASTRO, FG_INFO, "Generating Moon Image" );
xglPushMatrix();
{
xglRotatef(((RAD_TO_DEG * rightAscension)- 90.0), 0.0, 0.0, 1.0);
xglRotatef((RAD_TO_DEG * declination), 1.0, 0.0, 0.0);
FG_LOG( FG_GENERAL, FG_INFO,
"Ra = (" << (RAD_TO_DEG *rightAscension)
<< "), Dec= (" << (RAD_TO_DEG *declination) << ")" );
xglTranslatef(0.0, 60000.0, 0.0);
glEnable(GL_BLEND); // BLEND ENABLED
// Draw the halo...
if (current_options.get_textures())
{
// glBlendFunc(GL_SRC_ALPHA, GL_ONE);
glBlendFunc ( GL_SRC_ALPHA, GL_ONE_MINUS_SRC_ALPHA ) ;
glEnable(GL_TEXTURE_2D); // TEXTURE ENABLED
glTexEnvf(GL_TEXTURE_ENV, GL_TEXTURE_ENV_MODE, GL_MODULATE);
glBindTexture(GL_TEXTURE_2D, moon_halotexid);
glBegin(GL_QUADS);
glTexCoord2f(0.0f, 0.0f); glVertex3f(-5000, 0.0, -5000);
glTexCoord2f(1.0f, 0.0f); glVertex3f( 5000, 0.0, -5000);
glTexCoord2f(1.0f, 1.0f); glVertex3f( 5000, 0.0, 5000);
glTexCoord2f(0.0f, 1.0f); glVertex3f(-5000, 0.0, 5000);
glEnd();
}
xglEnable(GL_LIGHTING); // LIGHTING ENABLED
xglEnable( GL_LIGHT0 );
// set lighting parameters
xglLightfv(GL_LIGHT0, GL_AMBIENT, white );
xglLightfv(GL_LIGHT0, GL_DIFFUSE, white );
// Enable( GL_CULL_FACE );
xglMaterialfv(GL_FRONT, GL_AMBIENT, black);
xglMaterialfv(GL_FRONT, GL_DIFFUSE, moonColor);
//glEnable(GL_TEXTURE_2D);
glBlendFunc(GL_ONE, GL_ONE);
//glTexEnvf(GL_TEXTURE_ENV, GL_TEXTURE_ENV_MODE, GL_MODULATE);
// Draw the moon-proper
if (current_options.get_textures())
{
glBindTexture(GL_TEXTURE_2D, moon_texid);
gluQuadricTexture(moonObject, GL_TRUE );
}
gluSphere(moonObject, moonSize, 12, 12 );
glDisable(GL_TEXTURE_2D); // TEXTURE DISABLED
glDisable(GL_BLEND); // BLEND DISABLED
}
xglPopMatrix();
glDisable(GL_LIGHTING); // Lighting Disabled.
}
else
{
}
}
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/**************************************************************************
* moon.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _MOON_HXX_
#define _MOON_HXX_
#include <Aircraft/aircraft.hxx>
#include <Include/fg_constants.h>
#include <Main/views.hxx>
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Moon : public CelestialBody
{
private:
void TexInit(); // This should move to the constructor eventually.
GLUquadricObj *moonObject;
GLuint Sphere;
GLuint moon_texid;
GLuint moon_halotexid;
GLubyte *moon_texbuf;
GLubyte *moon_halotexbuf;
void setHalo();
public:
Moon ( FGTime *t);
~Moon();
void updatePosition(FGTime *t, Star *ourSun);
void newImage();
};
#endif // _MOON_HXX_
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/**************************************************************************
* neptune.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "neptune.hxx"
/*************************************************************************
* Neptune::Neptune(FGTime *t)
* Public constructor for class Neptune
* Argument: The current time.
* the hard coded orbital elements for Neptune are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Neptune::Neptune(FGTime *t) :
CelestialBody(131.7806, 3.0173000E-5,
1.7700, -2.550E-7,
272.8461, -6.027000E-6,
30.058260, 3.313E-8,
0.008606, 2.150E-9,
260.2471, 0.00599514700, t)
{
}
/*************************************************************************
* void Neptune::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Neptune, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Neptune specific equation
*************************************************************************/
void Neptune::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -6.90 + 5*log10 (r*R) + 0.001 *FV;
}
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/**************************************************************************
* neptune.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _NEPTUNE_HXX_
#define _NEPTUNE_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Neptune : public CelestialBody
{
public:
Neptune ( FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _NEPTUNE_HXX_
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/**************************************************************************
* pluto.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _PLUTO_HXX_
#define _PLUTO_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
class Pluto : public CelestialBody
{
public:
Pluto ( FGTime t);
};
#endif // _PLUTO_HXX_
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/**************************************************************************
* saturn.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "saturn.hxx"
/*************************************************************************
* Saturn::Saturn(FGTime *t)
* Public constructor for class Saturn
* Argument: The current time.
* the hard coded orbital elements for Saturn are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Saturn::Saturn(FGTime *t) :
CelestialBody(113.6634, 2.3898000E-5,
2.4886, -1.081E-7,
339.3939, 2.9766100E-5,
9.5547500, 0.000000,
0.055546, -9.499E-9,
316.9670, 0.03344422820, t)
{
}
/*************************************************************************
* void Saturn::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Saturn, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Saturn specific equation
*************************************************************************/
void Saturn::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
double actTime = fgCalcActTime(t);
double ir = 0.4897394;
double Nr = 2.9585076 + 6.6672E-7*actTime;
double B = asin (sin(declination) * cos(ir) -
cos(declination) * sin(ir) *
sin(rightAscension - Nr));
double ring_magn = -2.6 * sin(fabs(B)) + 1.2 * pow(sin(B), 2);
magnitude = -9.0 + 5*log10(r*R) + 0.044 * FV + ring_magn;
}
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/**************************************************************************
* saturn.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _SATURN_HXX_
#define _SATURN_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Saturn : public CelestialBody
{
public:
Saturn ( FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _SATURN_HXX_
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// sky.cxx -- model sky with an upside down "bowl"
//
// Written by Curtis Olson, started December 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#ifdef HAVE_WINDOWS_H
# include <windows.h>
#endif
#include <math.h>
#include <GL/glut.h>
#include <XGL/xgl.h>
#include <Aircraft/aircraft.hxx>
#include <Debug/logstream.hxx>
#include <FDM/flight.hxx>
#include <Include/fg_constants.h>
#include <Main/views.hxx>
#include <Math/fg_random.h>
#include <Time/event.hxx>
#include <Time/fg_time.hxx>
#include "sky.hxx"
#ifdef __MWERKS__
# pragma global_optimizer off
#endif
// in meters of course
#define CENTER_ELEV 25000.0
#define INNER_RADIUS 50000.0
#define INNER_ELEV 20000.0
#define MIDDLE_RADIUS 70000.0
#define MIDDLE_ELEV 8000.0
#define OUTER_RADIUS 80000.0
#define OUTER_ELEV 0.0
#define BOTTOM_RADIUS 50000.0
#define BOTTOM_ELEV -2000.0
static float inner_vertex[12][3];
static float middle_vertex[12][3];
static float outer_vertex[12][3];
static float bottom_vertex[12][3];
static GLubyte inner_color[12][4];
static GLubyte middle_color[12][4];
static GLubyte outer_color[12][4];
// Calculate the sky structure vertices
void fgSkyVerticesInit( void ) {
float theta;
int i;
FG_LOG(FG_ASTRO, FG_INFO, " Generating the sky dome vertices.");
for ( i = 0; i < 12; i++ ) {
theta = (i * 30.0) * DEG_TO_RAD;
inner_vertex[i][0] = cos(theta) * INNER_RADIUS;
inner_vertex[i][1] = sin(theta) * INNER_RADIUS;
inner_vertex[i][2] = INNER_ELEV;
// printf(" %.2f %.2f\n", cos(theta) * INNER_RADIUS,
// sin(theta) * INNER_RADIUS);
middle_vertex[i][0] = cos((double)theta) * MIDDLE_RADIUS;
middle_vertex[i][1] = sin((double)theta) * MIDDLE_RADIUS;
middle_vertex[i][2] = MIDDLE_ELEV;
outer_vertex[i][0] = cos((double)theta) * OUTER_RADIUS;
outer_vertex[i][1] = sin((double)theta) * OUTER_RADIUS;
outer_vertex[i][2] = OUTER_ELEV;
bottom_vertex[i][0] = cos((double)theta) * BOTTOM_RADIUS;
bottom_vertex[i][1] = sin((double)theta) * BOTTOM_RADIUS;
bottom_vertex[i][2] = BOTTOM_ELEV;
}
}
// (Re)calculate the sky colors at each vertex
void fgSkyColorsInit( void ) {
fgLIGHT *l;
double sun_angle, diff;
double outer_param[3], outer_amt[3], outer_diff[3];
double middle_param[3], middle_amt[3], middle_diff[3];
int i, j;
l = &cur_light_params;
FG_LOG( FG_ASTRO, FG_INFO,
" Generating the sky colors for each vertex." );
// setup for the possibility of sunset effects
sun_angle = l->sun_angle * RAD_TO_DEG;
// fgPrintf( FG_ASTRO, FG_INFO,
// " Sun angle in degrees = %.2f\n", sun_angle);
if ( (sun_angle > 80.0) && (sun_angle < 100.0) ) {
// 0.0 - 0.4
outer_param[0] = (10.0 - fabs(90.0 - sun_angle)) / 20.0;
outer_param[1] = (10.0 - fabs(90.0 - sun_angle)) / 40.0;
outer_param[2] = -(10.0 - fabs(90.0 - sun_angle)) / 30.0;
// outer_param[2] = 0.0;
middle_param[0] = (10.0 - fabs(90.0 - sun_angle)) / 40.0;
middle_param[1] = (10.0 - fabs(90.0 - sun_angle)) / 80.0;
middle_param[2] = 0.0;
outer_diff[0] = outer_param[0] / 6.0;
outer_diff[1] = outer_param[1] / 6.0;
outer_diff[2] = outer_param[2] / 6.0;
middle_diff[0] = middle_param[0] / 6.0;
middle_diff[1] = middle_param[1] / 6.0;
middle_diff[2] = middle_param[2] / 6.0;
} else {
outer_param[0] = outer_param[1] = outer_param[2] = 0.0;
middle_param[0] = middle_param[1] = middle_param[2] = 0.0;
outer_diff[0] = outer_diff[1] = outer_diff[2] = 0.0;
middle_diff[0] = middle_diff[1] = middle_diff[2] = 0.0;
}
// printf(" outer_red_param = %.2f outer_red_diff = %.2f\n",
// outer_red_param, outer_red_diff);
// calculate transition colors between sky and fog
for ( j = 0; j < 3; j++ ) {
outer_amt[j] = outer_param[j];
middle_amt[j] = middle_param[j];
}
for ( i = 0; i < 6; i++ ) {
for ( j = 0; j < 3; j++ ) {
diff = l->sky_color[j] - l->fog_color[j];
// printf("sky = %.2f fog = %.2f diff = %.2f\n",
// l->sky_color[j], l->fog_color[j], diff);
inner_color[i][j] = (GLubyte)((l->sky_color[j] - diff * 0.3) * 255);
middle_color[i][j] = (GLubyte)((l->sky_color[j] - diff * 0.9
+ middle_amt[j]) * 255);
outer_color[i][j] = (GLubyte)((l->fog_color[j] + outer_amt[j])
* 255);
if ( inner_color[i][j] > 255 ) { inner_color[i][j] = 255; }
if ( inner_color[i][j] < 25 ) { inner_color[i][j] = 25; }
if ( middle_color[i][j] > 255 ) { middle_color[i][j] = 255; }
if ( middle_color[i][j] < 25 ) { middle_color[i][j] = 25; }
if ( outer_color[i][j] > 255 ) { outer_color[i][j] = 255; }
if ( outer_color[i][j] < 25 ) { outer_color[i][j] = 25; }
}
inner_color[i][3] = middle_color[i][3] = outer_color[i][3] =
(GLubyte)(l->sky_color[3] * 255);
for ( j = 0; j < 3; j++ ) {
outer_amt[j] -= outer_diff[j];
middle_amt[j] -= middle_diff[j];
}
/*
printf("inner_color[%d] = %.2f %.2f %.2f %.2f\n", i, inner_color[i][0],
inner_color[i][1], inner_color[i][2], inner_color[i][3]);
printf("middle_color[%d] = %.2f %.2f %.2f %.2f\n", i,
middle_color[i][0], middle_color[i][1], middle_color[i][2],
middle_color[i][3]);
printf("outer_color[%d] = %.2f %.2f %.2f %.2f\n", i,
outer_color[i][0], outer_color[i][1], outer_color[i][2],
outer_color[i][3]);
*/
}
for ( j = 0; j < 3; j++ ) {
outer_amt[j] = 0.0;
middle_amt[j] = 0.0;
}
for ( i = 6; i < 12; i++ ) {
for ( j = 0; j < 3; j++ ) {
diff = l->sky_color[j] - l->fog_color[j];
// printf("sky = %.2f fog = %.2f diff = %.2f\n",
// l->sky_color[j], l->fog_color[j], diff);
inner_color[i][j] = (GLubyte)((l->sky_color[j] - diff * 0.3) * 255);
middle_color[i][j] = (GLubyte)((l->sky_color[j] - diff * 0.9
+ middle_amt[j]) * 255);
outer_color[i][j] = (GLubyte)((l->fog_color[j] + outer_amt[j])
* 255);
if ( inner_color[i][j] > 255 ) { inner_color[i][j] = 255; }
if ( inner_color[i][j] < 25 ) { inner_color[i][j] = 25; }
if ( middle_color[i][j] > 255 ) { middle_color[i][j] = 255; }
if ( middle_color[i][j] < 25 ) { middle_color[i][j] = 25; }
if ( outer_color[i][j] > 255 ) { outer_color[i][j] = 255; }
if ( outer_color[i][j] < 35 ) { outer_color[i][j] = 35; }
}
inner_color[i][3] = middle_color[i][3] = outer_color[i][3] =
(GLubyte)(l->sky_color[3] * 255);
for ( j = 0; j < 3; j++ ) {
outer_amt[j] += outer_diff[j];
middle_amt[j] += middle_diff[j];
}
/*
printf("inner_color[%d] = %.2f %.2f %.2f %.2f\n", i, inner_color[i][0],
inner_color[i][1], inner_color[i][2], inner_color[i][3]);
printf("middle_color[%d] = %.2f %.2f %.2f %.2f\n", i,
middle_color[i][0], middle_color[i][1], middle_color[i][2],
middle_color[i][3]);
printf("outer_color[%d] = %.2f %.2f %.2f %.2f\n", i,
outer_color[i][0], outer_color[i][1], outer_color[i][2],
outer_color[i][3]);
*/
}
}
// Initialize the sky structure and colors
void fgSkyInit( void ) {
FG_LOG( FG_ASTRO, FG_INFO, "Initializing the sky" );
fgSkyVerticesInit();
// regester fgSkyColorsInit() as an event to be run periodically
global_events.Register( "fgSkyColorsInit()", fgSkyColorsInit,
fgEVENT::FG_EVENT_READY, 30000);
}
// Draw the Sky
void fgSkyRender( void ) {
FGInterface *f;
fgLIGHT *l;
GLubyte sky_color[4];
GLubyte inner_color[4];
GLubyte middle_color[4];
GLubyte outer_color[4];
double diff;
int i;
f = current_aircraft.fdm_state;
l = &cur_light_params;
// printf("Rendering the sky.\n");
// calculate the proper colors
for ( i = 0; i < 3; i++ ) {
diff = l->sky_color[i] - l->adj_fog_color[i];
// printf("sky = %.2f fog = %.2f diff = %.2f\n",
// l->sky_color[j], l->adj_fog_color[j], diff);
inner_color[i] = (GLubyte)((l->sky_color[i] - diff * 0.3) * 255);
middle_color[i] = (GLubyte)((l->sky_color[i] - diff * 0.9) * 255);
outer_color[i] = (GLubyte)(l->adj_fog_color[i] * 255);
}
inner_color[3] = middle_color[3] = outer_color[3] =
(GLubyte)(l->adj_fog_color[3] * 255);
xglPushMatrix();
// Translate to view position
Point3D zero_elev = current_view.get_cur_zero_elev();
xglTranslatef( zero_elev.x(), zero_elev.y(), zero_elev.z() );
// printf(" Translated to %.2f %.2f %.2f\n",
// zero_elev.x, zero_elev.y, zero_elev.z );
// Rotate to proper orientation
// printf(" lon = %.2f lat = %.2f\n", FG_Longitude * RAD_TO_DEG,
// FG_Latitude * RAD_TO_DEG);
xglRotatef( f->get_Longitude() * RAD_TO_DEG, 0.0, 0.0, 1.0 );
xglRotatef( 90.0 - f->get_Latitude() * RAD_TO_DEG, 0.0, 1.0, 0.0 );
xglRotatef( l->sun_rotation * RAD_TO_DEG, 0.0, 0.0, 1.0 );
// Draw inner/center section of sky*/
xglBegin( GL_TRIANGLE_FAN );
for ( i = 0; i < 4; i++ ) {
sky_color[i] = (GLubyte)(l->sky_color[i] * 255);
}
xglColor4fv(l->sky_color);
xglVertex3f(0.0, 0.0, CENTER_ELEV);
for ( i = 11; i >= 0; i-- ) {
xglColor4ubv( inner_color );
xglVertex3fv( inner_vertex[i] );
}
xglColor4ubv( inner_color );
xglVertex3fv( inner_vertex[11] );
xglEnd();
// Draw the middle ring
xglBegin( GL_TRIANGLE_STRIP );
for ( i = 0; i < 12; i++ ) {
xglColor4ubv( middle_color );
// printf("middle_color[%d] = %.2f %.2f %.2f %.2f\n", i,
// middle_color[i][0], middle_color[i][1], middle_color[i][2],
// middle_color[i][3]);
// xglColor4f(1.0, 0.0, 0.0, 1.0);
xglVertex3fv( middle_vertex[i] );
xglColor4ubv( inner_color );
// printf("inner_color[%d] = %.2f %.2f %.2f %.2f\n", i,
// inner_color[i][0], inner_color[i][1], inner_color[i][2],
// inner_color[i][3]);
// xglColor4f(0.0, 0.0, 1.0, 1.0);
xglVertex3fv( inner_vertex[i] );
}
xglColor4ubv( middle_color );
// xglColor4f(1.0, 0.0, 0.0, 1.0);
xglVertex3fv( middle_vertex[0] );
xglColor4ubv( inner_color );
// xglColor4f(0.0, 0.0, 1.0, 1.0);
xglVertex3fv( inner_vertex[0] );
xglEnd();
// Draw the outer ring
xglBegin( GL_TRIANGLE_STRIP );
for ( i = 0; i < 12; i++ ) {
xglColor4ubv( outer_color );
xglVertex3fv( outer_vertex[i] );
xglColor4ubv( middle_color );
xglVertex3fv( middle_vertex[i] );
}
xglColor4ubv( outer_color );
xglVertex3fv( outer_vertex[0] );
xglColor4ubv( middle_color );
xglVertex3fv( middle_vertex[0] );
xglEnd();
// Draw the bottom skirt
xglBegin( GL_TRIANGLE_STRIP );
xglColor4ubv( outer_color );
for ( i = 0; i < 12; i++ ) {
xglVertex3fv( bottom_vertex[i] );
xglVertex3fv( outer_vertex[i] );
}
xglVertex3fv( bottom_vertex[0] );
xglVertex3fv( outer_vertex[0] );
xglEnd();
xglPopMatrix();
}
+53
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// sky.hxx -- model sky with an upside down "bowl"
//
// Written by Curtis Olson, started December 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _SKY_HXX
#define _SKY_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <plib/ssg.h> // plib include
class fgSky : ssgLeaf
{
};
// (Re)generate the display list
void fgSkyInit( void );
// (Re)calculate the sky colors at each vertex
void fgSkyColorsInit( void );
// Draw the Sky
void fgSkyRender( void );
#endif // _SKY_HXX
+215
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/**************************************************************************
* solarsystem.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#ifdef HAVE_WINDOWS_H
# include <windows.h>
#endif
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include <GL/glut.h>
#include <XGL/xgl.h>
#include <Debug/logstream.hxx>
#include <Time/sunpos.hxx>
#include <Time/moonpos.hxx>
#include "solarsystem.hxx"
/***************************************************************************
* default constructor for class SolarSystem:
* or course there can only be one way to create an entire solar system -:) )
* the FGTime argument is needed to properly initialize the the current orbital
* elements
*************************************************************************/
SolarSystem::SolarSystem(FGTime *t)
{
if (theSolarSystem)
{
FG_LOG( FG_GENERAL, FG_ALERT, "Error: only one solarsystem allowed" );
exit(-1);
}
theSolarSystem = this;
ourSun = new Star(t);
earthsMoon = new Moon(t);
mercury = new Mercury(t);
venus = new Venus(t);
mars = new Mars(t);
jupiter = new Jupiter(t);
saturn = new Saturn(t);
uranus = new Uranus(t);
neptune = new Neptune(t);
displayList = 0;
};
/**************************************************************************
* the destructor for class SolarSystem;
**************************************************************************/
SolarSystem::~SolarSystem()
{
delete ourSun;
delete earthsMoon;
delete mercury;
delete venus;
delete mars;
delete jupiter;
delete saturn;
delete uranus;
delete neptune;
}
/****************************************************************************
* void SolarSystem::rebuild()
*
* this member function updates the positions for the sun, moon, and planets,
* and then rebuilds the display list.
*
* arguments: none
* return value: none
***************************************************************************/
void SolarSystem::rebuild()
{
//fgLIGHT *l = &cur_light_params;
FGTime *t = FGTime::cur_time_params;
//float x, y, z;
//double sun_angle;
double ra, dec;
//double x_2, x_4, x_8, x_10;*/
double magnitude;
//GLfloat ambient;
//GLfloat amb[4];
glDisable(GL_LIGHTING);
// Step 1: update all the positions
ourSun->updatePosition(t);
earthsMoon->updatePosition(t, ourSun);
mercury->updatePosition(t, ourSun);
venus->updatePosition(t, ourSun);
mars->updatePosition(t, ourSun);
jupiter->updatePosition(t, ourSun);
saturn->updatePosition(t, ourSun);
uranus->updatePosition(t, ourSun);
neptune->updatePosition(t, ourSun);
fgUpdateSunPos(); // get the right sun angle (especially important when
// running for the first time).
fgUpdateMoonPos();
if (displayList)
xglDeleteLists(displayList, 1);
displayList = xglGenLists(1);
FG_LOG( FG_ASTRO, FG_INFO, "Rebuilding astro display list" );
// Step 2: rebuild the display list
xglNewList( displayList, GL_COMPILE);
{
// Step 2a: Add the moon...
// Not that it is preferred to draw the moon first, and the sun next, in order to mime a
// solar eclipse. This is yet untested though...
// Euhh, actually the ecplise doesn't work...
earthsMoon->newImage();
// Step 2b: Add the sun
ourSun->newImage();
// Step 2c: Add the planets
xglBegin(GL_POINTS);
mercury->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
venus ->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
mars ->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
jupiter->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
saturn ->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
uranus ->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
neptune->getPos(&ra, &dec, &magnitude);addPlanetToList(ra, dec, magnitude);
xglEnd();
xglEnable(GL_LIGHTING);
}
xglEndList();
}
/*****************************************************************************
* double SolarSystem::scaleMagnitude(double magn)
* This private member function rescales the original magnitude, as used in the
* astronomical sense of the word, into a value used by OpenGL to draw a
* convincing Star or planet
*
* Argument: the astronomical magnitude
*
* return value: the rescaled magnitude
****************************************************************************/
double SolarSystem::scaleMagnitude(double magn)
{
double magnitude = (0.0 - magn) / 5.0 + 1.0;
magnitude = magnitude * 0.7 + (3 * 0.1);
if (magnitude > 1.0) magnitude = 1.0;
if (magnitude < 0.0) magnitude = 0.0;
return magnitude;
}
/***************************************************************************
* void SolarSytem::addPlanetToList(double ra, double dec, double magn);
*
* This private member function first causes the magnitude to be properly
* rescaled, and then adds the planet to the display list.
*
* arguments: Right Ascension, declination, and magnitude
*
* return value: none
**************************************************************************/
void SolarSystem::addPlanetToList(double ra, double dec, double magn)
{
double
magnitude = scaleMagnitude ( magn );
fgLIGHT *l = &cur_light_params;
if ((double) (l->sun_angle - FG_PI_2) >
((magnitude - 1.0) * - 20 * DEG_TO_RAD))
{
xglColor3f (magnitude, magnitude, magnitude);
xglVertex3f( 50000.0 * cos (ra) * cos (dec),
50000.0 * sin (ra) * cos (dec),
50000.0 * sin (dec));
}
}
SolarSystem* SolarSystem::theSolarSystem = 0;
/******************************************************************************
* void solarSystemRebuild()
* this a just a wrapper function, provided for use as an interface to the
* event manager
*****************************************************************************/
void solarSystemRebuild()
{
SolarSystem::theSolarSystem->rebuild();
}
+91
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/**************************************************************************
* solarsystem.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _SOLARSYSTEM_H_
#define _SOLARSYSTEM_H_
#include <Time/light.hxx>
#include <Time/fg_time.hxx>
#include <Main/views.hxx>
#include "star.hxx"
#include "moon.hxx"
#include "mercury.hxx"
#include "venus.hxx"
#include "mars.hxx"
#include "jupiter.hxx"
#include "saturn.hxx"
#include "uranus.hxx"
#include "neptune.hxx"
#include "pluto.hxx"
class SolarSystem
{
private:
Star* ourSun;
Moon* earthsMoon;
Mercury* mercury;
Venus* venus;
Mars* mars;
Jupiter* jupiter;
Saturn* saturn;
Uranus* uranus;
Neptune* neptune;
//Pluto* pluto;
GLint displayList;
double scaleMagnitude(double magn);
void addPlanetToList(double ra, double dec, double magn);
public:
SolarSystem(FGTime *t);
CelestialBody *getSun();
CelestialBody *getMoon();
~SolarSystem();
static SolarSystem *theSolarSystem; // thanks to Bernie Bright!
void rebuild();
friend void solarSystemRebuild();
void draw();
};
inline CelestialBody* SolarSystem::getSun()
{
return ourSun;
}
inline CelestialBody* SolarSystem::getMoon()
{
return earthsMoon;
}
inline void SolarSystem::draw()
{
xglCallList(displayList);
}
extern void solarSystemRebuild();
#endif // _SOLARSYSTEM_H_
+267
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/**************************************************************************
* star.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include <Time/sunpos.hxx>
#include <Debug/logstream.hxx>
#include <Time/light.hxx>
#include <Main/options.hxx>
#include "star.hxx"
/*************************************************************************
* Star::Star(FGTime *t)
* Public constructor for class Star
* Argument: The current time.
* the hard coded orbital elements our sun are passed to
* CelestialBody::CelestialBody();
* note that the word sun is avoided, in order to prevent some compilation
* problems on sun systems
************************************************************************/
Star::Star(FGTime *t) :
CelestialBody (0.000000, 0.0000000000,
0.0000, 0.00000,
282.9404, 4.7093500E-5,
1.0000000, 0.000000,
0.016709, -1.151E-9,
356.0470, 0.98560025850, t)
{
FG_LOG( FG_GENERAL, FG_INFO, "Initializing Sun Texture");
#ifdef GL_VERSION_1_1
xglGenTextures(1, &sun_texid);
xglBindTexture(GL_TEXTURE_2D, sun_texid);
#elif GL_EXT_texture_object
xglGenTexturesEXT(1, &sun_texid);
xglBindTextureEXT(GL_TEXTURE_2D, sun_texid);
#else
# error port me
#endif
glPixelStorei(GL_UNPACK_ALIGNMENT, 1);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MIN_FILTER, GL_LINEAR);
glTexParameteri(GL_TEXTURE_2D, GL_TEXTURE_MAG_FILTER, GL_LINEAR);
setTexture();
glTexImage2D( GL_TEXTURE_2D,
0,
GL_RGBA,
256, 256,
0,
GL_RGBA, GL_UNSIGNED_BYTE,
sun_texbuf);
SunObject = gluNewQuadric();
if(SunObject == NULL)
{
printf("gluNewQuadric(SunObject) failed !\n");
exit(0);
}
//SunList = 0;
distance = 0.0;
}
Star::~Star()
{
//delete SunObject;
delete [] sun_texbuf;
}
static int texWidth = 256; /* 64x64 is plenty */
void Star::setTexture()
{
int texSize;
//void *textureBuf;
GLubyte *p;
int i,j;
double radius;
texSize = texWidth*texWidth;
sun_texbuf = new GLubyte[texSize*4];
if (!sun_texbuf)
return; // Ugly!
p = sun_texbuf;
radius = (double)(texWidth / 2);
for (i=0; i < texWidth; i++) {
for (j=0; j < texWidth; j++) {
double x, y, d;
*p = 0xff;
*(p+1) = 0xff;
*(p+2) = 0xff;
x = fabs((double)(i - (texWidth / 2)));
y = fabs((double)(j - (texWidth / 2)));
d = sqrt((x * x) + (y * y));
if (d < radius) {
double t = 1.0 - (d / radius); // t is 1.0 at center, 0.0 at edge */
// inverse square looks nice
*(p+3) = (int)((double) 0xff * (t*t));
} else {
*(p+3) = 0x00;
}
p += 4;
}
}
//gluBuild2DMipmaps(GL_TEXTURE_2D, 1, texWidth, texWidth,
// GL_LUMINANCE,
// GL_UNSIGNED_BYTE, textureBuf);
//free(textureBuf);
}
/*************************************************************************
* void Jupiter::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of our sun.
*************************************************************************/
void Star::updatePosition(FGTime *t)
{
double
actTime, eccAnom,
xv, yv, v, r,
xe, ye, ze, ecl;
updateOrbElements(t);
actTime = fgCalcActTime(t);
ecl = DEG_TO_RAD * (23.4393 - 3.563E-7 * actTime); // Angle in Radians
eccAnom = fgCalcEccAnom(M, e); // Calculate the eccentric Anomaly (also known as solving Kepler's equation)
xv = cos(eccAnom) - e;
yv = sqrt (1.0 - e*e) * sin(eccAnom);
v = atan2 (yv, xv); // the sun's true anomaly
distance = r = sqrt (xv*xv + yv*yv); // and its distance
lonEcl = v + w; // the sun's true longitude
latEcl = 0;
// convert the sun's true longitude to ecliptic rectangular
// geocentric coordinates (xs, ys)
xs = r * cos (lonEcl);
ys = r * sin (lonEcl);
// convert ecliptic coordinates to equatorial rectangular
// geocentric coordinates
xe = xs;
ye = ys * cos (ecl);
ze = ys * sin (ecl);
// And finally, calculate right ascension and declination
rightAscension = atan2 (ye, xe);
declination = atan2 (ze, sqrt (xe*xe + ye*ye));
}
void Star::newImage(void)
{
/*static float stars[3];
stars[0] = 0.0;
stars[1] = 0.0;
stars[2] = 1.0;*/
fgLIGHT *l = &cur_light_params;
float sun_angle = l->sun_angle;
if( sun_angle*RAD_TO_DEG < 100 ) { // else no need to draw sun
double x_2, x_4, x_8, x_10;
GLfloat ambient;
GLfloat amb[4];
int sun_size = 550;
// daily variation sun gets larger near horizon
/*if(sun_angle*RAD_TO_DEG > 84.0 && sun_angle*RAD_TO_DEG < 95)
{
double sun_grow = 9*fabs(94-sun_angle*RAD_TO_DEG);
sun_size = (int)(sun_size + sun_size * cos(sun_grow*DEG_TO_RAD));
}*/
x_2 = sun_angle * sun_angle;
x_4 = x_2 * x_2;
x_8 = x_4 * x_4;
x_10 = x_8 * x_2;
ambient = (float)(0.4 * pow (1.1, - x_10 / 30.0));
if (ambient < 0.3) ambient = 0.3;
if (ambient > 1.0) ambient = 1.0;
amb[0] = ((ambient * 6.0) - 1.0); // minimum value = 0.8
amb[1] = ((ambient * 11.0) - 3.0); // minimum value = 0.3
amb[2] = ((ambient * 12.0) - 3.6); // minimum value = 0.0
amb[3] = 1.00;
if (amb[0] > 1.0) amb[0] = 1.0;
if (amb[1] > 1.0) amb[1] = 1.0;
if (amb[2] > 1.0) amb[2] = 1.0;
xglColor3fv(amb);
glPushMatrix();
{
xglRotatef(((RAD_TO_DEG * rightAscension)- 90.0), 0.0, 0.0, 1.0);
xglRotatef((RAD_TO_DEG * declination), 1.0, 0.0, 0.0);
xglTranslatef(0,60000,0);
if (current_options.get_textures())
{
glEnable(GL_TEXTURE_2D); // TEXTURE ENABLED
glEnable(GL_BLEND); // BLEND ENABLED
// glBlendFunc(GL_ONE, GL_ONE_MINUS_SRC_ALPHA);
glBlendFunc ( GL_SRC_ALPHA, GL_ONE_MINUS_SRC_ALPHA ) ;
glTexEnvf(GL_TEXTURE_ENV, GL_TEXTURE_ENV_MODE, GL_MODULATE);
glBindTexture(GL_TEXTURE_2D, sun_texid);
glBegin(GL_QUADS);
glTexCoord2f(0.0f, 0.0f); glVertex3f(-5000, 0.0, -5000);
glTexCoord2f(1.0f, 0.0f); glVertex3f( 5000, 0.0, -5000);
glTexCoord2f(1.0f, 1.0f); glVertex3f( 5000, 0.0, 5000);
glTexCoord2f(0.0f, 1.0f); glVertex3f(-5000, 0.0, 5000);
glEnd();
}
xglDisable(GL_TEXTURE_2D); // TEXTURE DISABLED
xglDisable(GL_BLEND); // BLEND DISABLED
}
glPopMatrix();
glDisable(GL_LIGHTING); // LIGHTING DISABLED
glDisable(GL_BLEND); // BLEND DISABLED
glPushMatrix();
{
xglRotatef(((RAD_TO_DEG * rightAscension)- 90.0), 0.0, 0.0, 1.0);
xglRotatef((RAD_TO_DEG * declination), 1.0, 0.0, 0.0);
xglColor4fv(amb);
xglTranslatef(0,60000,0);
gluSphere( SunObject, sun_size, 10, 10 );
}
glPopMatrix();
glDisable(GL_TEXTURE_2D); // TEXTURE DISABLED
glDisable(GL_BLEND); // BLEND DISABLED
}
}
+98
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/**************************************************************************
* star.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _STAR_HXX_
#define _STAR_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
class Star : public CelestialBody
{
private:
//double longitude; // the sun's true longitude - this is depreciated by
// CelestialBody::lonEcl
double xs, ys; // the sun's rectangular geocentric coordinates
double distance; // the sun's distance to the earth
GLUquadricObj *SunObject;
GLuint sun_texid;
GLubyte *sun_texbuf;
void setTexture();
public:
Star (FGTime *t);
~Star();
void updatePosition(FGTime *t);
double getM();
double getw();
//double getLon();
double getxs();
double getys();
double getDistance();
void newImage();
};
inline double Star::getM()
{
return M;
}
inline double Star::getw()
{
return w;
}
inline double Star::getxs()
{
return xs;
}
inline double Star::getys()
{
return ys;
}
inline double Star::getDistance()
{
return distance;
}
#endif // _STAR_HXX_
+267
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// stars.cxx -- data structures and routines for managing and rendering stars.
//
// Written by Curtis Olson, started August 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@me.umn.edu
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
//*************************************************************************/
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#ifdef HAVE_WINDOWS_H
# include <windows.h>
#endif
#include "Include/compiler.h"
#ifdef FG_HAVE_STD_INCLUDES
# include <cmath>
# include <cstdio>
# include <cstring>
# include <ctime>
#else
# include <math.h>
# include <stdio.h>
# include <string.h>
# include <time.h>
#endif
#include <string>
#include <GL/glut.h>
#include <XGL/xgl.h>
#include <Aircraft/aircraft.hxx>
#include <Debug/logstream.hxx>
#include <Include/fg_constants.h>
#include <Misc/fgpath.hxx>
#include <Misc/fgstream.hxx>
#include <Misc/stopwatch.hxx>
#include <Main/options.hxx>
#include <Main/views.hxx>
#include <Time/fg_time.hxx>
#include "Misc/stopwatch.hxx"
#include "stars.hxx"
// FG_USING_STD(getline);
#define EpochStart (631065600)
#define DaysSinceEpoch(secs) (((secs)-EpochStart)*(1.0/(24*3600)))
#define FG_MAX_STARS 3500
// Define four structures, each with varying amounts of stars
static GLint stars[FG_STAR_LEVELS];
// Initialize the Star Management Subsystem
int fgStarsInit( void ) {
// -dw- avoid local data > 32k error by dynamic allocation of the
// array, problem for some compilers
Point3D *starlist = new Point3D[FG_MAX_STARS];
// struct CelestialCoord pltPos;
double right_ascension, declination, magnitude;
double min_magnitude[FG_STAR_LEVELS];
// double ra_save, decl_save;
// double ra_save1, decl_save1;
int i, j, starcount, count;
FG_LOG( FG_ASTRO, FG_INFO, "Initializing stars" );
if ( FG_STAR_LEVELS < 4 ) {
FG_LOG( FG_ASTRO, FG_ALERT, "Big whups in stars.cxx" );
exit(-1);
}
// build the full path name to the stars data base file
FGPath path ( current_options.get_fg_root() );
path.append( "Astro/stars" );
FG_LOG( FG_ASTRO, FG_INFO, " Loading stars from " << path.str() );
fg_gzifstream in( path.str() );
if ( ! in ) {
FG_LOG( FG_ASTRO, FG_ALERT, "Cannot open star file: " << path.str() );
exit(-1);
}
starcount = 0;
StopWatch timer;
timer.start();
// read in each line of the file
while ( ! in.eof() && starcount < FG_MAX_STARS )
{
in >> skipcomment;
string name;
getline( in, name, ',' );
in >> starlist[starcount];
++starcount;
}
timer.stop();
FG_LOG( FG_ASTRO, FG_INFO,
"Loaded " << starcount << " stars in "
<< timer.elapsedSeconds() << " seconds" );
min_magnitude[0] = 4.2;
min_magnitude[1] = 3.6;
min_magnitude[2] = 3.0;
min_magnitude[3] = 2.4;
min_magnitude[4] = 1.8;
min_magnitude[5] = 1.2;
min_magnitude[6] = 0.6;
min_magnitude[7] = 0.0;
// build the various star display lists
for ( i = 0; i < FG_STAR_LEVELS; i++ ) {
stars[i] = xglGenLists(1);
xglNewList( stars[i], GL_COMPILE );
xglBegin( GL_POINTS );
count = 0;
for ( j = 0; j < starcount; j++ ) {
magnitude = starlist[j].z();
// printf("magnitude = %.2f\n", magnitude);
if ( magnitude < min_magnitude[i] ) {
right_ascension = starlist[j].x();
declination = starlist[j].y();
count++;
// scale magnitudes to (0.0 - 1.0)
magnitude = (0.0 - magnitude) / 5.0 + 1.0;
// scale magnitudes again so they look ok
if ( magnitude > 1.0 ) { magnitude = 1.0; }
if ( magnitude < 0.0 ) { magnitude = 0.0; }
// magnitude =
// magnitude * 0.7 + (((FG_STAR_LEVELS - 1) - i) * 0.042);
magnitude = magnitude * 0.9 +
(((FG_STAR_LEVELS - 1) - i) * 0.014);
// printf(" Found star: %d %s, %.3f %.3f %.3f\n", count,
// name, right_ascension, declination, magnitude);
xglColor3f( magnitude, magnitude, magnitude );
//xglColor3f(0,0,0);*/
xglVertex3f( 50000.0*cos(right_ascension)*cos(declination),
50000.0*sin(right_ascension)*cos(declination),
50000.0*sin(declination) );
}
} // while
xglEnd();
/*
xglBegin(GL_LINE_LOOP);
xglColor3f(1.0, 0.0, 0.0);
xglVertex3f( 50000.0 * cos(ra_save-0.2) * cos(decl_save-0.2),
50000.0 * sin(ra_save-0.2) * cos(decl_save-0.2),
50000.0 * sin(decl_save-0.2) );
xglVertex3f( 50000.0 * cos(ra_save+0.2) * cos(decl_save-0.2),
50000.0 * sin(ra_save+0.2) * cos(decl_save-0.2),
50000.0 * sin(decl_save-0.2) );
xglVertex3f( 50000.0 * cos(ra_save+0.2) * cos(decl_save+0.2),
50000.0 * sin(ra_save+0.2) * cos(decl_save+0.2),
50000.0 * sin(decl_save+0.2) );
xglVertex3f( 50000.0 * cos(ra_save-0.2) * cos(decl_save+0.2),
50000.0 * sin(ra_save-0.2) * cos(decl_save+0.2),
50000.0 * sin(decl_save+0.2) );
xglEnd();
*/
/*
xglBegin(GL_LINE_LOOP);
xglColor3f(0.0, 1.0, 0.0);
xglVertex3f( 50000.0 * cos(ra_save1-0.2) * cos(decl_save1-0.2),
50000.0 * sin(ra_save1-0.2) * cos(decl_save1-0.2),
50000.0 * sin(decl_save1-0.2) );
xglVertex3f( 50000.0 * cos(ra_save1+0.2) * cos(decl_save1-0.2),
50000.0 * sin(ra_save1+0.2) * cos(decl_save1-0.2),
50000.0 * sin(decl_save1-0.2) );
xglVertex3f( 50000.0 * cos(ra_save1+0.2) * cos(decl_save1+0.2),
50000.0 * sin(ra_save1+0.2) * cos(decl_save1+0.2),
50000.0 * sin(decl_save1+0.2) );
xglVertex3f( 50000.0 * cos(ra_save1-0.2) * cos(decl_save1+0.2),
50000.0 * sin(ra_save1-0.2) * cos(decl_save1+0.2),
50000.0 * sin(decl_save1+0.2) );
xglEnd();
*/
xglEndList();
FG_LOG( FG_ASTRO, FG_INFO,
" Loading " << count << " stars brighter than "
<< min_magnitude[i] );
}
return 1; // OK, we got here because initialization worked.
}
// Draw the Stars
void fgStarsRender( void ) {
FGInterface *f;
fgLIGHT *l;
FGTime *t;
int i;
f = current_aircraft.fdm_state;
l = &cur_light_params;
t = FGTime::cur_time_params;
// FG_PI_2 + 0.1 is about 6 degrees after sundown and before sunrise
// t->sun_angle = 3.0; // to force stars to be drawn (for testing)
// render the stars
if ( l->sun_angle > (FG_PI_2 + 5 * DEG_TO_RAD ) ) {
// determine which star structure to draw
if ( l->sun_angle > (FG_PI_2 + 10.0 * DEG_TO_RAD ) ) {
i = 0;
} else if ( l->sun_angle > (FG_PI_2 + 8.8 * DEG_TO_RAD ) ) {
i = 1;
} else if ( l->sun_angle > (FG_PI_2 + 7.5 * DEG_TO_RAD ) ) {
i = 2;
} else if ( l->sun_angle > (FG_PI_2 + 7.0 * DEG_TO_RAD ) ) {
i = 3;
} else if ( l->sun_angle > (FG_PI_2 + 6.5 * DEG_TO_RAD ) ) {
i = 4;
} else if ( l->sun_angle > (FG_PI_2 + 6.0 * DEG_TO_RAD ) ) {
i = 5;
} else if ( l->sun_angle > (FG_PI_2 + 5.5 * DEG_TO_RAD ) ) {
i = 6;
} else {
i = 7;
}
// printf("RENDERING STARS = %d (night)\n", i);
xglCallList(stars[i]);
} else {
// printf("not RENDERING STARS (day)\n");
}
}
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// stars.hxx -- data structures and routines for managing and rendering stars.
//
// Written by Curtis Olson, started August 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@me.umn.edu
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _STARS_HXX
#define _STARS_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <Time/fg_time.hxx>
#define FG_STAR_LEVELS 8 // how many star transitions
// Initialize the Star Management Subsystem
int fgStarsInit( void );
// Draw the Stars
void fgStarsRender( void );
// [no longer used?] extern FGTime cur_time_params;
#endif // _STARS_HXX
+60
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/**************************************************************************
* uranus.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "uranus.hxx"
/*************************************************************************
* Uranus::Uranus(FGTime *t)
* Public constructor for class Uranus
* Argument: The current time.
* the hard coded orbital elements for Uranus are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Uranus::Uranus(FGTime *t) :
CelestialBody(74.00050, 1.3978000E-5,
0.7733, 1.900E-8,
96.66120, 3.0565000E-5,
19.181710, -1.55E-8,
0.047318, 7.450E-9,
142.5905, 0.01172580600, t)
{
}
/*************************************************************************
* void Uranus::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Uranus, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Uranus specific equation
*************************************************************************/
void Uranus::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -7.15 + 5*log10( r*R) + 0.001 * FV;
}
+38
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/**************************************************************************
* uranus.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _URANUS_HXX_
#define _URANUS_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Uranus : public CelestialBody
{
public:
Uranus ( FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _URANUS_HXX_
+60
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/**************************************************************************
* venus.cxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifdef __BORLANDC__
# define exception c_exception
#endif
#include <math.h>
#include "venus.hxx"
/*************************************************************************
* Venus::Venus(FGTime *t)
* Public constructor for class Venus
* Argument: The current time.
* the hard coded orbital elements for Venus are passed to
* CelestialBody::CelestialBody();
************************************************************************/
Venus::Venus(FGTime *t) :
CelestialBody(76.67990, 2.4659000E-5,
3.3946, 2.75E-8,
54.89100, 1.3837400E-5,
0.7233300, 0.000000,
0.006773, -1.302E-9,
48.00520, 1.60213022440, t)
{
}
/*************************************************************************
* void Venus::updatePosition(FGTime *t, Star *ourSun)
*
* calculates the current position of Venus, by calling the base class,
* CelestialBody::updatePosition(); The current magnitude is calculated using
* a Venus specific equation
*************************************************************************/
void Venus::updatePosition(FGTime *t, Star *ourSun)
{
CelestialBody::updatePosition(t, ourSun);
magnitude = -4.34 + 5*log10( r*R ) + 0.013 * FV + 4.2E-07 * pow(FV,3);
}
+38
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/**************************************************************************
* venus.hxx
* Written by Durk Talsma. Originally started October 1997, for distribution
* with the FlightGear project. Version 2 was written in August and
* September 1998. This code is based upon algorithms and data kindly
* provided by Mr. Paul Schlyter. (pausch@saaf.se).
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License as
* published by the Free Software Foundation; either version 2 of the
* License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful, but
* WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
*
* $Id$
**************************************************************************/
#ifndef _VENUS_HXX_
#define _VENUS_HXX_
#include <Time/fg_time.hxx>
#include "celestialBody.hxx"
#include "star.hxx"
class Venus : public CelestialBody
{
public:
Venus ( FGTime *t);
void updatePosition(FGTime *t, Star *ourSun);
};
#endif // _VENUS_HXX_
+168
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/* #include "HEADERS.h" */
/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
/* --------------------------------------------------------------------------
* This file contains routines that perform geometry-related operations
* on matrices.
* -------------------------------------------------------------------------*/
#include "mat3defs.h"
/* -------------------------- Static Routines ---------------------------- */
/* ------------------------- Internal Routines --------------------------- */
/* -------------------------- Public Routines ---------------------------- */
/*
* This takes a matrix used to transform points, and returns a corresponding
* matrix that can be used to transform direction vectors (between points).
*/
void
MAT3direction_matrix(register double (*result_mat)[4], register double (*mat)[4])
{
register int i;
MAT3copy(result_mat, mat);
for (i = 0; i < 4; i++) result_mat[i][3] = result_mat[3][i] = 0.0;
result_mat[3][3] = 1.0;
}
/*
* This takes a matrix used to transform points, and returns a corresponding
* matrix that can be used to transform vectors that must remain perpendicular
* to planes defined by the points. It is useful when you are transforming
* some object that has both points and normals in its definition, and you
* only have the transformation matrix for the points. This routine returns
* FALSE if the normal matrix is uncomputable. Otherwise, it returns TRUE.
*
* Spike sez: "This is the adjoint for the non-homogeneous part of the
* transformation."
*/
int
MAT3normal_matrix(register double (*result_mat)[4], register double (*mat)[4])
{
register int ret;
MAT3mat tmp_mat;
MAT3direction_matrix(result_mat, mat);
if ( (ret = MAT3invert(tmp_mat, tmp_mat)) ) {
MAT3transpose(result_mat, tmp_mat);
}
return(ret);
}
/*
* Sets the given matrix to be a scale matrix for the given vector of
* scale values.
*/
void
MAT3scale(double (*result_mat)[4], double *scale)
{
MAT3identity(result_mat);
result_mat[0][0] = scale[0];
result_mat[1][1] = scale[1];
result_mat[2][2] = scale[2];
}
/*
* Sets up a matrix for a rotation about an axis given by the line from
* (0,0,0) to axis, through an angle (in radians).
* Looking along the axis toward the origin, the rotation is counter-clockwise.
*/
#define SELECT .7071 /* selection constant (roughly .5*sqrt(2) */
void
MAT3rotate(double (*result_mat)[4], double *axis, double angle_in_radians)
{
MAT3vec naxis, /* Axis of rotation, normalized */
base2, /* 2nd unit basis vec, perp to axis */
base3; /* 3rd unit basis vec, perp to axis & base2 */
double dot;
MAT3mat base_mat, /* Change-of-basis matrix */
base_mat_trans; /* Inverse of c-o-b matrix */
register int i;
/* Step 1: extend { axis } to a basis for 3-space: { axis, base2, base3 }
* which is orthonormal (all three have unit length, and all three are
* mutually orthogonal). Also should be oriented, i.e. axis cross base2 =
* base3, rather than -base3.
*
* Method: Find a vector linearly independent from axis. For this we
* either use the y-axis, or, if that is too close to axis, the
* z-axis. 'Too close' means that the dot product is too near to 1.
*/
MAT3_COPY_VEC(naxis, axis);
MAT3_NORMALIZE_VEC(naxis, dot);
if (dot == 0.0) {
/* ERR_ERROR(MAT3_errid, ERR_SEVERE,
(ERR_S, "Zero-length axis vector given to MAT3rotate")); */
return;
}
MAT3perp_vec(base2, naxis, TRUE);
MAT3cross_product(base3, naxis, base2);
/* Set up the change-of-basis matrix, and its inverse */
MAT3identity(base_mat);
MAT3identity(base_mat_trans);
MAT3identity(result_mat);
for (i = 0; i < 3; i++){
base_mat_trans[i][0] = base_mat[0][i] = naxis[i];
base_mat_trans[i][1] = base_mat[1][i] = base2[i];
base_mat_trans[i][2] = base_mat[2][i] = base3[i];
}
/* If T(u) = uR, where R is base_mat, then T(x-axis) = naxis,
* T(y-axis) = base2, and T(z-axis) = base3. The inverse of base_mat is
* its transpose. OK?
*/
result_mat[1][1] = result_mat[2][2] = cos(angle_in_radians);
result_mat[2][1] = -(result_mat[1][2] = sin(angle_in_radians));
MAT3mult(result_mat, base_mat_trans, result_mat);
MAT3mult(result_mat, result_mat, base_mat);
}
/*
* Sets the given matrix to be a translation matrix for the given vector of
* translation values.
*/
void
MAT3translate(double (*result_mat)[4], double *trans)
{
MAT3identity(result_mat);
result_mat[3][0] = trans[0];
result_mat[3][1] = trans[1];
result_mat[3][2] = trans[2];
}
/*
* Sets the given matrix to be a shear matrix for the given x and y shear
* values.
*/
void
MAT3shear(double (*result_mat)[4], double xshear, double yshear)
{
MAT3identity(result_mat);
result_mat[2][0] = xshear;
result_mat[2][1] = yshear;
}
+311
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/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
/* --------------------------------------------------------------------------
* This file contains routines that operate solely on matrices.
* -------------------------------------------------------------------------*/
#include "mat3defs.h"
/* -------------------------- Static Routines ---------------------------- */
#define SMALL 1e-20 /* Small enough to be considered zero */
/*
* Shuffles rows in inverse of 3x3. See comment in MAT3_inv3_second_col().
*/
static void
MAT3_inv3_swap( register double inv[3][3], int row0, int row1, int row2)
{
register int i, tempi;
double temp;
#define SWAP_ROWS(a, b) \
for (i = 0; i < 3; i++) SWAP(inv[a][i], inv[b][i], temp); \
SWAP(a, b, tempi)
if (row0 != 0){
if (row1 == 0) {
SWAP_ROWS(row0, row1);
}
else {
SWAP_ROWS(row0, row2);
}
}
if (row1 != 1) {
SWAP_ROWS(row1, row2);
}
}
/*
* Does Gaussian elimination on second column.
*/
static int
MAT3_inv3_second_col (register double source[3][3], register double inv[3][3], int row0)
{
register int row1, row2, i1, i2, i;
double temp;
double a, b;
/* Find which row to use */
if (row0 == 0) i1 = 1, i2 = 2;
else if (row0 == 1) i1 = 0, i2 = 2;
else i1 = 0, i2 = 1;
/* Find which is larger in abs. val.:the entry in [i1][1] or [i2][1] */
/* and use that value for pivoting. */
a = source[i1][1]; if (a < 0) a = -a;
b = source[i2][1]; if (b < 0) b = -b;
if (a > b) row1 = i1;
else row1 = i2;
row2 = (row1 == i1 ? i2 : i1);
/* Scale row1 in source */
if ((source[row1][1] < SMALL) && (source[row1][1] > -SMALL)) return(FALSE);
temp = 1.0 / source[row1][1];
source[row1][1] = 1.0;
source[row1][2] *= temp; /* source[row1][0] is zero already */
/* Scale row1 in inv */
inv[row1][row1] = temp; /* it used to be a 1.0 */
inv[row1][row0] *= temp;
/* Clear column one, source, and make corresponding changes in inv */
for (i = 0; i < 3; i++) if (i != row1) { /* for i = all rows but row1 */
temp = -source[i][1];
source[i][1] = 0.0;
source[i][2] += temp * source[row1][2];
inv[i][row1] = temp * inv[row1][row1];
inv[i][row0] += temp * inv[row1][row0];
}
/* Scale row2 in source */
if ((source[row2][2] < SMALL) && (source[row2][2] > -SMALL)) return(FALSE);
temp = 1.0 / source[row2][2];
source[row2][2] = 1.0; /* source[row2][*] is zero already */
/* Scale row2 in inv */
inv[row2][row2] = temp; /* it used to be a 1.0 */
inv[row2][row0] *= temp;
inv[row2][row1] *= temp;
/* Clear column one, source, and make corresponding changes in inv */
for (i = 0; i < 3; i++) if (i != row2) { /* for i = all rows but row2 */
temp = -source[i][2];
source[i][2] = 0.0;
inv[i][row0] += temp * inv[row2][row0];
inv[i][row1] += temp * inv[row2][row1];
inv[i][row2] += temp * inv[row2][row2];
}
/*
* Now all is done except that the inverse needs to have its rows shuffled.
* row0 needs to be moved to inv[0][*], row1 to inv[1][*], etc.
*
* We *didn't* do the swapping before the elimination so that we could more
* easily keep track of what ops are needed to be done in the inverse.
*/
MAT3_inv3_swap(inv, row0, row1, row2);
return(TRUE);
}
/*
* Fast inversion routine for 3 x 3 matrices. - Written by jfh.
*
* This takes 30 multiplies/divides, as opposed to 39 for Cramer's Rule.
* The algorithm consists of performing fast gaussian elimination, by never
* doing any operations where the result is guaranteed to be zero, or where
* one operand is guaranteed to be zero. This is done at the cost of clarity,
* alas.
*
* Returns 1 if the inverse was successful, 0 if it failed.
*/
static int
MAT3_invert3 (register double source[3][3], register double inv[3][3])
{
register int i, row0;
double temp;
double a, b, c;
inv[0][0] = inv[1][1] = inv[2][2] = 1.0;
inv[0][1] = inv[0][2] = inv[1][0] = inv[1][2] = inv[2][0] = inv[2][1] = 0.0;
/* attempt to find the largest entry in first column to use as pivot */
a = source[0][0]; if (a < 0) a = -a;
b = source[1][0]; if (b < 0) b = -b;
c = source[2][0]; if (c < 0) c = -c;
if (a > b) {
if (a > c) row0 = 0;
else row0 = 2;
}
else {
if (b > c) row0 = 1;
else row0 = 2;
}
/* Scale row0 of source */
if ((source[row0][0] < SMALL) && (source[row0][0] > -SMALL)) return(FALSE);
temp = 1.0 / source[row0][0];
source[row0][0] = 1.0;
source[row0][1] *= temp;
source[row0][2] *= temp;
/* Scale row0 of inverse */
inv[row0][row0] = temp; /* other entries are zero -- no effort */
/* Clear column zero of source, and make corresponding changes in inverse */
for (i = 0; i < 3; i++) if (i != row0) { /* for i = all rows but row0 */
temp = -source[i][0];
source[i][0] = 0.0;
source[i][1] += temp * source[row0][1];
source[i][2] += temp * source[row0][2];
inv[i][row0] = temp * inv[row0][row0];
}
/*
* We've now done gaussian elimination so that the source and
* inverse look like this:
*
* 1 * * * 0 0
* 0 * * * 1 0
* 0 * * * 0 1
*
* We now proceed to do elimination on the second column.
*/
if (! MAT3_inv3_second_col(source, inv, row0)) return(FALSE);
return(TRUE);
}
/*
* Finds a new pivot for a non-simple 4x4. See comments in MAT3invert().
*/
static int
MAT3_inv4_pivot (register MAT3mat src, MAT3vec r, double *s, int *swap)
{
register int i, j;
double temp, max;
*swap = -1;
if (MAT3_IS_ZERO(src[3][3])) {
/* Look for a different pivot element: one with largest abs value */
max = 0.0;
for (i = 0; i < 4; i++) {
if (src[i][3] > max) max = src[*swap = i][3];
else if (src[i][3] < -max) max = -src[*swap = i][3];
}
/* No pivot element available ! */
if (*swap < 0) return(FALSE);
else for (j = 0; j < 4; j++) SWAP(src[*swap][j], src[3][j], temp);
}
MAT3_SET_VEC (r, -src[0][3], -src[1][3], -src[2][3]);
*s = 1.0 / src[3][3];
src[0][3] = src[1][3] = src[2][3] = 0.0;
src[3][3] = 1.0;
MAT3_SCALE_VEC(src[3], src[3], *s);
for (i = 0; i < 3; i++) {
src[0][i] += r[0] * src[3][i];
src[1][i] += r[1] * src[3][i];
src[2][i] += r[2] * src[3][i];
}
return(TRUE);
}
/* ------------------------- Internal Routines --------------------------- */
/* -------------------------- Public Routines ---------------------------- */
/*
* This returns the inverse of the given matrix. The result matrix
* may be the same as the one to invert.
*
* Fast inversion routine for 4 x 4 matrices, written by jfh.
*
* Returns 1 if the inverse was successful, 0 if it failed.
*
* This routine has been specially tweaked to notice the following:
* If the matrix has the form
* * * * 0
* * * * 0
* * * * 0
* * * * 1
*
* (as do many matrices in graphics), then we compute the inverse of
* the upper left 3x3 matrix and use this to find the general inverse.
*
* In the event that the right column is not 0-0-0-1, we do gaussian
* elimination to make it so, then use the 3x3 inverse, and then do
* our gaussian elimination.
*/
int
MAT3invert(double (*result_mat)[4], double (*mat)[4])
{
MAT3mat src, inv;
register int i, j, simple;
double m[3][3], inv3[3][3], s, temp;
MAT3vec r, t;
int swap;
MAT3copy(src, mat);
MAT3identity(inv);
/* If last column is not (0,0,0,1), use special code */
simple = (mat[0][3] == 0.0 && mat[1][3] == 0.0 &&
mat[2][3] == 0.0 && mat[3][3] == 1.0);
if (! simple && ! MAT3_inv4_pivot(src, r, &s, &swap)) return(FALSE);
MAT3_COPY_VEC(t, src[3]); /* Translation vector */
/* Copy upper-left 3x3 matrix */
for (i = 0; i < 3; i++) for (j = 0; j < 3; j++) m[i][j] = src[i][j];
if (! MAT3_invert3(m, inv3)) return(FALSE);
for (i = 0; i < 3; i++) for (j = 0; j < 3; j++) inv[i][j] = inv3[i][j];
for (i = 0; i < 3; i++) for (j = 0; j < 3; j++)
inv[3][i] -= t[j] * inv3[j][i];
if (! simple) {
/* We still have to undo our gaussian elimination from earlier on */
/* add r0 * first col to last col */
/* add r1 * 2nd col to last col */
/* add r2 * 3rd col to last col */
for (i = 0; i < 4; i++) {
inv[i][3] += r[0] * inv[i][0] + r[1] * inv[i][1] + r[2] * inv[i][2];
inv[i][3] *= s;
}
if (swap >= 0)
for (i = 0; i < 4; i++) SWAP(inv[i][swap], inv[i][3], temp);
}
MAT3copy(result_mat, inv);
return(TRUE);
}
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/* #include "HEADERS.h" */
/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
/* --------------------------------------------------------------------------
* This file contains routines that operate solely on matrices.
* -------------------------------------------------------------------------*/
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#ifdef WIN32
# ifndef HAVE_STL_SGI_PORT
# ifdef __BORLANDC__
# include <mem.h>
# else
# include <memory.h> /* required for memset() and memcpy() */
# endif
# endif
#endif
#include <string.h>
#include "mat3defs.h"
MAT3mat identityMatrix = {
{ 1.0, 0.0, 0.0, 0.0 },
{ 0.0, 1.0, 0.0, 0.0 },
{ 0.0, 0.0, 1.0, 0.0 },
{ 0.0, 0.0, 0.0, 1.0 }
};
/* #include "macros.h" */
/* -------------------------- Static Routines ---------------------------- */
/* ------------------------- Internal Routines --------------------------- */
/* -------------------------- Public Routines ---------------------------- */
#if !defined( USE_XTRA_MAT3_INLINES )
/*
* This multiplies two matrices, producing a third, which may the same as
* either of the first two.
*/
void
MAT3mult (double (*result_mat)[4], register double (*mat1)[4], register double (*mat2)[4])
{
register int i, j;
MAT3mat tmp_mat;
for (i = 0; i < 4; i++)
for (j = 0; j < 4; j++)
tmp_mat[i][j] = (mat1[i][0] * mat2[0][j] +
mat1[i][1] * mat2[1][j] +
mat1[i][2] * mat2[2][j] +
mat1[i][3] * mat2[3][j]);
MAT3copy (result_mat, tmp_mat);
}
#endif // !defined( USE_XTRA_MAT3_INLINES )
/*
* This returns the transpose of a matrix. The result matrix may be
* the same as the one to transpose.
*/
void
MAT3transpose (double (*result_mat)[4], register double (*mat)[4])
{
register int i, j;
MAT3mat tmp_mat;
for (i = 0; i < 4; i++)
for (j = 0; j < 4; j++)
tmp_mat[i][j] = mat[j][i];
MAT3copy (result_mat, tmp_mat);
}
/*
* This prints the given matrix to the given file pointer.
*/
void
MAT3print(double (*mat)[4], FILE *fp)
{
MAT3print_formatted(mat, fp, CNULL, CNULL, CNULL, CNULL);
}
/*
* This prints the given matrix to the given file pointer.
* use the format string to pass to fprintf. head and tail
* are printed at the beginning and end of each line.
*/
void
MAT3print_formatted(double (*mat)[4], FILE *fp, char *title, char *head, char *format, char *tail)
{
register int i, j;
/* This is to allow this to be called easily from a debugger */
if (fp == NULL) fp = stderr;
if (title == NULL) title = "MAT3 matrix:\n";
if (head == NULL) head = " ";
if (format == NULL) format = "%#8.4lf ";
if (tail == NULL) tail = "\n";
(void) fprintf(fp, title);
for (i = 0; i < 4; i++) {
(void) fprintf(fp, head);
for (j = 0; j < 4; j++) (void) fprintf(fp, format, mat[i][j]);
(void) fprintf(fp, tail);
}
}
+154
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/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
/* --------------------------------------------------------------------------
* This file contains routines that operate on matrices and vectors, or
* vectors and vectors.
* -------------------------------------------------------------------------*/
/* #include "sphigslocal.h" */
/* -------------------------- Static Routines ---------------------------- */
/* ------------------------- Internal Routines --------------------------- */
/* -------------------------- Public Routines ---------------------------- */
/*
* Multiplies a vector by a matrix, setting the result vector.
* It assumes all homogeneous coordinates are 1.
* The two vectors involved may be the same.
*/
#include "mat3.h"
#ifndef TRUE
# define TRUE 1
#endif
#ifndef FALSE
# define FALSE 0
#endif
#if !defined( USE_XTRA_MAT3_INLINES )
void
MAT3mult_vec(double *result_vec, register double *vec, register double (*mat)[4])
{
MAT3vec tempvec;
register double *temp = tempvec;
temp[0] = vec[0] * mat[0][0] + vec[1] * mat[1][0] +
vec[2] * mat[2][0] + mat[3][0];
temp[1] = vec[0] * mat[0][1] + vec[1] * mat[1][1] +
vec[2] * mat[2][1] + mat[3][1];
temp[2] = vec[0] * mat[0][2] + vec[1] * mat[1][2] +
vec[2] * mat[2][2] + mat[3][2];
MAT3_COPY_VEC(result_vec, temp);
}
#endif // !defined( USE_XTRA_MAT3_INLINES )
/*
* Multiplies a vector of size 4 by a matrix, setting the result vector.
* The fourth element of the vector is the homogeneous coordinate, which
* may or may not be 1. If the "normalize" parameter is TRUE, then the
* result vector will be normalized so that the homogeneous coordinate is 1.
* The two vectors involved may be the same.
* This returns zero if the vector was to be normalized, but couldn't be.
*/
int
MAT3mult_hvec(double *result_vec, register double *vec, register double (*mat)[4], int normalize)
{
MAT3hvec tempvec;
double norm_fac;
register double *temp = tempvec;
register int ret = TRUE;
temp[0] = vec[0] * mat[0][0] + vec[1] * mat[1][0] +
vec[2] * mat[2][0] + vec[3] * mat[3][0];
temp[1] = vec[0] * mat[0][1] + vec[1] * mat[1][1] +
vec[2] * mat[2][1] + vec[3] * mat[3][1];
temp[2] = vec[0] * mat[0][2] + vec[1] * mat[1][2] +
vec[2] * mat[2][2] + vec[3] * mat[3][2];
temp[3] = vec[0] * mat[0][3] + vec[1] * mat[1][3] +
vec[2] * mat[2][3] + vec[3] * mat[3][3];
/* Normalize if asked for, possible, and necessary */
if (normalize) {
if (MAT3_IS_ZERO(temp[3])) {
#ifndef THINK_C
fprintf (stderr,
"Can't normalize vector: homogeneous coordinate is 0");
#endif
ret = FALSE;
}
else {
norm_fac = 1.0 / temp[3];
MAT3_SCALE_VEC(result_vec, temp, norm_fac);
result_vec[3] = 1.0;
}
}
else MAT3_COPY_HVEC(result_vec, temp);
return(ret);
}
#if !defined( USE_XTRA_MAT3_INLINES )
/*
* Sets the first vector to be the cross-product of the last two vectors.
*/
void
MAT3cross_product(double *result_vec, register double *vec1, register double *vec2)
{
MAT3vec tempvec;
register double *temp = tempvec;
temp[0] = vec1[1] * vec2[2] - vec1[2] * vec2[1];
temp[1] = vec1[2] * vec2[0] - vec1[0] * vec2[2];
temp[2] = vec1[0] * vec2[1] - vec1[1] * vec2[0];
MAT3_COPY_VEC(result_vec, temp);
}
#endif // !defined( USE_XTRA_MAT3_INLINES )
/*
* Finds a vector perpendicular to vec and stores it in result_vec.
* Method: take any vector (we use <0,1,0>) and subtract the
* portion of it pointing in the vec direction. This doesn't
* work if vec IS <0,1,0> or is very near it. So if this is
* the case, use <0,0,1> instead.
* If "is_unit" is TRUE, the given vector is assumed to be unit length.
*/
#define SELECT .7071 /* selection constant (roughly .5*sqrt(2) */
void
MAT3perp_vec(double *result_vec, double *vec, int is_unit)
{
MAT3vec norm;
double dot;
MAT3_SET_VEC(result_vec, 0.0, 1.0, 0.0);
MAT3_COPY_VEC(norm, vec);
if (! is_unit) MAT3_NORMALIZE_VEC(norm, dot);
/* See if vector is too close to <0,1,0>. If so, use <0,0,1> */
if ((dot = MAT3_DOT_PRODUCT(norm, result_vec)) > SELECT || dot < -SELECT) {
result_vec[1] = 0.0;
result_vec[2] = 1.0;
dot = MAT3_DOT_PRODUCT(norm, result_vec);
}
/* Subtract off non-perpendicular part */
result_vec[0] -= dot * norm[0];
result_vec[1] -= dot * norm[1];
result_vec[2] -= dot * norm[2];
/* Make result unit length */
MAT3_NORMALIZE_VEC(result_vec, dot);
}
+30
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@@ -0,0 +1,30 @@
lib_LIBRARIES = libsgmath.a
include_HEADERS = \
fg_geodesy.hxx \
fg_memory.h \
fg_random.h \
fg_types.hxx \
interpolater.hxx \
leastsqs.hxx \
mat3.h \
point3d.hxx \
polar3d.hxx \
vector.hxx
EXTRA_DIST = linintp2.h linintp2.inl sphrintp.h sphrintp.inl
libsgmath_a_SOURCES = \
MAT3geom.c \
MAT3inv.c \
MAT3mat.c \
MAT3vec.c \
fg_geodesy.cxx \
fg_random.c \
interpolater.cxx \
leastsqs.cxx \
mat3defs.h mat3err.h \
polar3d.cxx \
vector.cxx
INCLUDES += -I$(top_builddir)
+365
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@@ -0,0 +1,365 @@
# Makefile.in generated automatically by automake 1.3 from Makefile.am
# Copyright (C) 1994, 1995, 1996, 1997, 1998 Free Software Foundation, Inc.
# This Makefile.in is free software; the Free Software Foundation
# gives unlimited permission to copy and/or distribute it,
# with or without modifications, as long as this notice is preserved.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY, to the extent permitted by law; without
# even the implied warranty of MERCHANTABILITY or FITNESS FOR A
# PARTICULAR PURPOSE.
SHELL = /bin/sh
srcdir = @srcdir@
top_srcdir = @top_srcdir@
VPATH = @srcdir@
prefix = @prefix@
exec_prefix = @exec_prefix@
bindir = @bindir@
sbindir = @sbindir@
libexecdir = @libexecdir@
datadir = @datadir@
sysconfdir = @sysconfdir@
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INSTALL_DATA = @INSTALL_DATA@
INSTALL_SCRIPT = @INSTALL_SCRIPT@
transform = @program_transform_name@
NORMAL_INSTALL = :
PRE_INSTALL = :
POST_INSTALL = :
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CC = @CC@
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MAKEINFO = @MAKEINFO@
PACKAGE = @PACKAGE@
RANLIB = @RANLIB@
VERSION = @VERSION@
base_LIBS = @base_LIBS@
opengl_LIBS = @opengl_LIBS@
lib_LIBRARIES = libsgmath.a
include_HEADERS = \
fg_geodesy.hxx \
fg_memory.h \
fg_random.h \
fg_types.hxx \
interpolater.hxx \
leastsqs.hxx \
mat3.h \
point3d.hxx \
polar3d.hxx \
vector.hxx
EXTRA_DIST = linintp2.h linintp2.inl sphrintp.h sphrintp.inl
libsgmath_a_SOURCES = \
MAT3geom.c \
MAT3inv.c \
MAT3mat.c \
MAT3vec.c \
fg_geodesy.cxx \
fg_random.c \
interpolater.cxx \
leastsqs.cxx \
mat3defs.h mat3err.h \
polar3d.cxx \
vector.cxx
mkinstalldirs = $(SHELL) $(top_srcdir)/mkinstalldirs
CONFIG_HEADER = ../include/config.h
CONFIG_CLEAN_FILES =
LIBRARIES = $(lib_LIBRARIES)
DEFS = @DEFS@ -I. -I$(srcdir) -I../include
CPPFLAGS = @CPPFLAGS@
LDFLAGS = @LDFLAGS@
LIBS = @LIBS@
X_CFLAGS = @X_CFLAGS@
X_LIBS = @X_LIBS@
X_EXTRA_LIBS = @X_EXTRA_LIBS@
X_PRE_LIBS = @X_PRE_LIBS@
libsgmath_a_LIBADD =
libsgmath_a_OBJECTS = MAT3geom.o MAT3inv.o MAT3mat.o MAT3vec.o \
fg_geodesy.o fg_random.o interpolater.o leastsqs.o polar3d.o vector.o
AR = ar
CXXFLAGS = @CXXFLAGS@
CXXCOMPILE = $(CXX) $(DEFS) $(INCLUDES) $(CPPFLAGS) $(CXXFLAGS)
CXXLINK = $(CXX) $(CXXFLAGS) $(LDFLAGS) -o $@
CFLAGS = @CFLAGS@
COMPILE = $(CC) $(DEFS) $(INCLUDES) $(CPPFLAGS) $(CFLAGS)
LINK = $(CC) $(CFLAGS) $(LDFLAGS) -o $@
HEADERS = $(include_HEADERS)
DIST_COMMON = Makefile.am Makefile.in
DISTFILES = $(DIST_COMMON) $(SOURCES) $(HEADERS) $(TEXINFOS) $(EXTRA_DIST)
TAR = tar
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// fg_geodesy.cxx -- routines to convert between geodetic and geocentric
// coordinate systems.
//
// Copied and adapted directly from LaRCsim/ls_geodesy.c
//
// See below for the complete original LaRCsim comments.
//
// $Id$
#include <simgear/compiler.h>
#ifdef FG_HAVE_STD_INCLUDES
# include <cmath>
# include <cerrno>
#else
# include <math.h>
# include <errno.h>
#endif
#include <simgear/logstream.hxx>
#include <simgear/constants.h>
#include "point3d.hxx"
#include "fg_geodesy.hxx"
#ifndef FG_HAVE_NATIVE_SGI_COMPILERS
FG_USING_STD(cout);
#endif
// ONE_SECOND is pi/180/60/60, or about 100 feet at earths' equator
#define ONE_SECOND 4.848136811E-6
// fgGeocToGeod(lat_geoc, radius, *lat_geod, *alt, *sea_level_r)
// INPUTS:
// lat_geoc Geocentric latitude, radians, + = North
// radius C.G. radius to earth center (meters)
//
// OUTPUTS:
// lat_geod Geodetic latitude, radians, + = North
// alt C.G. altitude above mean sea level (meters)
// sea_level_r radius from earth center to sea level at
// local vertical (surface normal) of C.G. (meters)
void fgGeocToGeod( double lat_geoc, double radius, double
*lat_geod, double *alt, double *sea_level_r )
{
double t_lat, x_alpha, mu_alpha, delt_mu, r_alpha, l_point, rho_alpha;
double sin_mu_a, denom,delt_lambda, lambda_sl, sin_lambda_sl;
if( ( (FG_PI_2 - lat_geoc) < ONE_SECOND ) // near North pole
|| ( (FG_PI_2 + lat_geoc) < ONE_SECOND ) ) // near South pole
{
*lat_geod = lat_geoc;
*sea_level_r = EQUATORIAL_RADIUS_M*E;
*alt = radius - *sea_level_r;
} else {
t_lat = tan(lat_geoc);
x_alpha = E*EQUATORIAL_RADIUS_M/sqrt(t_lat*t_lat + E*E);
double tmp = RESQ_M - x_alpha * x_alpha;
if ( tmp < 0.0 ) { tmp = 0.0; }
mu_alpha = atan2(sqrt(tmp),E*x_alpha);
if (lat_geoc < 0) mu_alpha = - mu_alpha;
sin_mu_a = sin(mu_alpha);
delt_lambda = mu_alpha - lat_geoc;
r_alpha = x_alpha/cos(lat_geoc);
l_point = radius - r_alpha;
*alt = l_point*cos(delt_lambda);
// check for domain error
if ( errno == EDOM ) {
FG_LOG( FG_GENERAL, FG_ALERT, "Domain ERROR in fgGeocToGeod!!!!" );
*alt = 0.0;
}
denom = sqrt(1-EPS*EPS*sin_mu_a*sin_mu_a);
rho_alpha = EQUATORIAL_RADIUS_M*(1-EPS)/
(denom*denom*denom);
delt_mu = atan2(l_point*sin(delt_lambda),rho_alpha + *alt);
*lat_geod = mu_alpha - delt_mu;
lambda_sl = atan( E*E * tan(*lat_geod) ); // SL geoc. latitude
sin_lambda_sl = sin( lambda_sl );
*sea_level_r =
sqrt(RESQ_M / (1 + ((1/(E*E))-1)*sin_lambda_sl*sin_lambda_sl));
// check for domain error
if ( errno == EDOM ) {
FG_LOG( FG_GENERAL, FG_ALERT, "Domain ERROR in fgGeocToGeod!!!!" );
*sea_level_r = 0.0;
}
}
}
// fgGeodToGeoc( lat_geod, alt, *sl_radius, *lat_geoc )
// INPUTS:
// lat_geod Geodetic latitude, radians, + = North
// alt C.G. altitude above mean sea level (meters)
//
// OUTPUTS:
// sl_radius SEA LEVEL radius to earth center (meters)
// (add Altitude to get true distance from earth center.
// lat_geoc Geocentric latitude, radians, + = North
//
void fgGeodToGeoc( double lat_geod, double alt, double *sl_radius,
double *lat_geoc )
{
double lambda_sl, sin_lambda_sl, cos_lambda_sl, sin_mu, cos_mu, px, py;
lambda_sl = atan( E*E * tan(lat_geod) ); // sea level geocentric latitude
sin_lambda_sl = sin( lambda_sl );
cos_lambda_sl = cos( lambda_sl );
sin_mu = sin(lat_geod); // Geodetic (map makers') latitude
cos_mu = cos(lat_geod);
*sl_radius =
sqrt(RESQ_M / (1 + ((1/(E*E))-1)*sin_lambda_sl*sin_lambda_sl));
py = *sl_radius*sin_lambda_sl + alt*sin_mu;
px = *sl_radius*cos_lambda_sl + alt*cos_mu;
*lat_geoc = atan2( py, px );
}
// Direct and inverse distance functions
//
// Proceedings of the 7th International Symposium on Geodetic
// Computations, 1985
//
// "The Nested Coefficient Method for Accurate Solutions of Direct and
// Inverse Geodetic Problems With Any Length"
//
// Zhang Xue-Lian
// pp 747-763
//
// modified for FlightGear to use WGS84 only -- Norman Vine
#define GEOD_INV_PI FG_PI
// s == distance
// az = azimuth
// for WGS_84 a = 6378137.000, rf = 298.257223563;
static double M0( double e2 ) {
//double e4 = e2*e2;
return GEOD_INV_PI*(1.0 - e2*( 1.0/4.0 + e2*( 3.0/64.0 +
e2*(5.0/256.0) )))/2.0;
}
// given, alt, lat1, lon1, az1 and distance (s), calculate lat2, lon2
// and az2. Lat, lon, and azimuth are in degrees. distance in meters
int geo_direct_wgs_84 ( double alt, double lat1, double lon1, double az1,
double s, double *lat2, double *lon2, double *az2 )
{
double a = 6378137.000, rf = 298.257223563;
double RADDEG = (GEOD_INV_PI)/180.0, testv = 1.0E-10;
double f = ( rf > 0.0 ? 1.0/rf : 0.0 );
double b = a*(1.0-f);
double e2 = f*(2.0-f);
double phi1 = lat1*RADDEG, lam1 = lon1*RADDEG;
double sinphi1 = sin(phi1), cosphi1 = cos(phi1);
double azm1 = az1*RADDEG;
double sinaz1 = sin(azm1), cosaz1 = cos(azm1);
if( fabs(s) < 0.01 ) { // distance < centimeter => congruency
*lat2 = lat1;
*lon2 = lon1;
*az2 = 180.0 + az1;
if( *az2 > 360.0 ) *az2 -= 360.0;
return 0;
} else if( cosphi1 ) { // non-polar origin
// u1 is reduced latitude
double tanu1 = sqrt(1.0-e2)*sinphi1/cosphi1;
double sig1 = atan2(tanu1,cosaz1);
double cosu1 = 1.0/sqrt( 1.0 + tanu1*tanu1 ), sinu1 = tanu1*cosu1;
double sinaz = cosu1*sinaz1, cos2saz = 1.0-sinaz*sinaz;
double us = cos2saz*e2/(1.0-e2);
// Terms
double ta = 1.0+us*(4096.0+us*(-768.0+us*(320.0-175.0*us)))/16384.0,
tb = us*(256.0+us*(-128.0+us*(74.0-47.0*us)))/1024.0,
tc = 0;
// FIRST ESTIMATE OF SIGMA (SIG)
double first = s/(b*ta); // !!
double sig = first;
double c2sigm, sinsig,cossig, temp,denom,rnumer, dlams, dlam;
do {
c2sigm = cos(2.0*sig1+sig);
sinsig = sin(sig); cossig = cos(sig);
temp = sig;
sig = first +
tb*sinsig*(c2sigm+tb*(cossig*(-1.0+2.0*c2sigm*c2sigm) -
tb*c2sigm*(-3.0+4.0*sinsig*sinsig)
*(-3.0+4.0*c2sigm*c2sigm)/6.0)
/4.0);
} while( fabs(sig-temp) > testv);
// LATITUDE OF POINT 2
// DENOMINATOR IN 2 PARTS (TEMP ALSO USED LATER)
temp = sinu1*sinsig-cosu1*cossig*cosaz1;
denom = (1.0-f)*sqrt(sinaz*sinaz+temp*temp);
// NUMERATOR
rnumer = sinu1*cossig+cosu1*sinsig*cosaz1;
*lat2 = atan2(rnumer,denom)/RADDEG;
// DIFFERENCE IN LONGITUDE ON AUXILARY SPHERE (DLAMS )
rnumer = sinsig*sinaz1;
denom = cosu1*cossig-sinu1*sinsig*cosaz1;
dlams = atan2(rnumer,denom);
// TERM C
tc = f*cos2saz*(4.0+f*(4.0-3.0*cos2saz))/16.0;
// DIFFERENCE IN LONGITUDE
dlam = dlams-(1.0-tc)*f*sinaz*(sig+tc*sinsig*
(c2sigm+
tc*cossig*(-1.0+2.0*
c2sigm*c2sigm)));
*lon2 = (lam1+dlam)/RADDEG;
if (*lon2 > 180.0 ) *lon2 -= 360.0;
if (*lon2 < -180.0 ) *lon2 += 360.0;
// AZIMUTH - FROM NORTH
*az2 = atan2(-sinaz,temp)/RADDEG;
if ( fabs(*az2) < testv ) *az2 = 0.0;
if( *az2 < 0.0) *az2 += 360.0;
return 0;
} else { // phi1 == 90 degrees, polar origin
double dM = a*M0(e2) - s;
double paz = ( phi1 < 0.0 ? 180.0 : 0.0 );
return geo_direct_wgs_84( alt, 0.0, lon1, paz, dM,lat2,lon2,az2 );
}
}
// given alt, lat1, lon1, lat2, lon2, calculate starting and ending
// az1, az2 and distance (s). Lat, lon, and azimuth are in degrees.
// distance in meters
int geo_inverse_wgs_84( double alt, double lat1, double lon1, double lat2,
double lon2, double *az1, double *az2, double *s )
{
double a = 6378137.000, rf = 298.257223563;
int iter=0;
double RADDEG = (GEOD_INV_PI)/180.0, testv = 1.0E-10;
double f = ( rf > 0.0 ? 1.0/rf : 0.0 );
double b = a*(1.0-f);
// double e2 = f*(2.0-f); // unused in this routine
double phi1 = lat1*RADDEG, lam1 = lon1*RADDEG;
double sinphi1 = sin(phi1), cosphi1 = cos(phi1);
double phi2 = lat2*RADDEG, lam2 = lon2*RADDEG;
double sinphi2 = sin(phi2), cosphi2 = cos(phi2);
if( (fabs(lat1-lat2) < testv &&
( fabs(lon1-lon2) < testv) || fabs(lat1-90.0) < testv ) )
{
// TWO STATIONS ARE IDENTICAL : SET DISTANCE & AZIMUTHS TO ZERO */
*az1 = 0.0; *az2 = 0.0; *s = 0.0;
return 0;
} else if( fabs(cosphi1) < testv ) {
// initial point is polar
int k = geo_inverse_wgs_84( alt, lat2,lon2,lat1,lon1, az1,az2,s );
k = k; // avoid compiler error since return result is unused
b = *az1; *az1 = *az2; *az2 = b;
return 0;
} else if( fabs(cosphi2) < testv ) {
// terminal point is polar
int k = geo_inverse_wgs_84( alt, lat1,lon1,lat1,lon1+180.0,
az1,az2,s );
k = k; // avoid compiler error since return result is unused
*s /= 2.0;
*az2 = *az1 + 180.0;
if( *az2 > 360.0 ) *az2 -= 360.0;
return 0;
} else if( (fabs( fabs(lon1-lon2) - 180 ) < testv) &&
(fabs(lat1+lat2) < testv) )
{
// Geodesic passes through the pole (antipodal)
double s1,s2;
geo_inverse_wgs_84( alt, lat1,lon1, lat1,lon2, az1,az2, &s1 );
geo_inverse_wgs_84( alt, lat2,lon2, lat1,lon2, az1,az2, &s2 );
*az2 = *az1;
*s = s1 + s2;
return 0;
} else {
// antipodal and polar points don't get here
double dlam = lam2 - lam1, dlams = dlam;
double sdlams,cdlams, sig,sinsig,cossig, sinaz,
cos2saz, c2sigm;
double tc,temp, us,rnumer,denom, ta,tb;
double cosu1,sinu1, sinu2,cosu2;
// Reduced latitudes
temp = (1.0-f)*sinphi1/cosphi1;
cosu1 = 1.0/sqrt(1.0+temp*temp);
sinu1 = temp*cosu1;
temp = (1.0-f)*sinphi2/cosphi2;
cosu2 = 1.0/sqrt(1.0+temp*temp);
sinu2 = temp*cosu2;
do {
sdlams = sin(dlams), cdlams = cos(dlams);
sinsig = sqrt(cosu2*cosu2*sdlams*sdlams+
(cosu1*sinu2-sinu1*cosu2*cdlams)*
(cosu1*sinu2-sinu1*cosu2*cdlams));
cossig = sinu1*sinu2+cosu1*cosu2*cdlams;
sig = atan2(sinsig,cossig);
sinaz = cosu1*cosu2*sdlams/sinsig;
cos2saz = 1.0-sinaz*sinaz;
c2sigm = (sinu1 == 0.0 || sinu2 == 0.0 ? cossig :
cossig-2.0*sinu1*sinu2/cos2saz);
tc = f*cos2saz*(4.0+f*(4.0-3.0*cos2saz))/16.0;
temp = dlams;
dlams = dlam+(1.0-tc)*f*sinaz*
(sig+tc*sinsig*
(c2sigm+tc*cossig*(-1.0+2.0*c2sigm*c2sigm)));
if (fabs(dlams) > GEOD_INV_PI && iter++ > 50) {
return iter;
}
} while ( fabs(temp-dlams) > testv);
us = cos2saz*(a*a-b*b)/(b*b); // !!
// BACK AZIMUTH FROM NORTH
rnumer = -(cosu1*sdlams);
denom = sinu1*cosu2-cosu1*sinu2*cdlams;
*az2 = atan2(rnumer,denom)/RADDEG;
if( fabs(*az2) < testv ) *az2 = 0.0;
if(*az2 < 0.0) *az2 += 360.0;
// FORWARD AZIMUTH FROM NORTH
rnumer = cosu2*sdlams;
denom = cosu1*sinu2-sinu1*cosu2*cdlams;
*az1 = atan2(rnumer,denom)/RADDEG;
if( fabs(*az1) < testv ) *az1 = 0.0;
if(*az1 < 0.0) *az1 += 360.0;
// Terms a & b
ta = 1.0+us*(4096.0+us*(-768.0+us*(320.0-175.0*us)))/
16384.0;
tb = us*(256.0+us*(-128.0+us*(74.0-47.0*us)))/1024.0;
// GEODETIC DISTANCE
*s = b*ta*(sig-tb*sinsig*
(c2sigm+tb*(cossig*(-1.0+2.0*c2sigm*c2sigm)-tb*
c2sigm*(-3.0+4.0*sinsig*sinsig)*
(-3.0+4.0*c2sigm*c2sigm)/6.0)/
4.0));
return 0;
}
}
/***************************************************************************
TITLE: ls_geodesy
----------------------------------------------------------------------------
FUNCTION: Converts geocentric coordinates to geodetic positions
----------------------------------------------------------------------------
MODULE STATUS: developmental
----------------------------------------------------------------------------
GENEALOGY: Written as part of LaRCSim project by E. B. Jackson
----------------------------------------------------------------------------
DESIGNED BY: E. B. Jackson
CODED BY: E. B. Jackson
MAINTAINED BY: E. B. Jackson
----------------------------------------------------------------------------
MODIFICATION HISTORY:
DATE PURPOSE BY
930208 Modified to avoid singularity near polar region. EBJ
930602 Moved backwards calcs here from ls_step. EBJ
931214 Changed erroneous Latitude and Altitude variables to
*lat_geod and *alt in routine ls_geoc_to_geod. EBJ
940111 Changed header files from old ls_eom.h style to ls_types,
and ls_constants. Also replaced old DATA type with new
SCALAR type. EBJ
CURRENT RCS HEADER:
$Header$
* Revision 1.5 1994/01/11 18:47:05 bjax
* Changed include files to use types and constants, not ls_eom.h
* Also changed DATA type to SCALAR type.
*
* Revision 1.4 1993/12/14 21:06:47 bjax
* Removed global variable references Altitude and Latitude. EBJ
*
* Revision 1.3 1993/06/02 15:03:40 bjax
* Made new subroutine for calculating geodetic to geocentric; changed name
* of forward conversion routine from ls_geodesy to ls_geoc_to_geod.
*
----------------------------------------------------------------------------
REFERENCES:
[ 1] Stevens, Brian L.; and Lewis, Frank L.: "Aircraft
Control and Simulation", Wiley and Sons, 1992.
ISBN 0-471-61397-5
----------------------------------------------------------------------------
CALLED BY: ls_aux
----------------------------------------------------------------------------
CALLS TO:
----------------------------------------------------------------------------
INPUTS:
lat_geoc Geocentric latitude, radians, + = North
radius C.G. radius to earth center, ft
----------------------------------------------------------------------------
OUTPUTS:
lat_geod Geodetic latitude, radians, + = North
alt C.G. altitude above mean sea level, ft
sea_level_r radius from earth center to sea level at
local vertical (surface normal) of C.G.
--------------------------------------------------------------------------*/
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// fg_geodesy.hxx -- routines to convert between geodetic and geocentric
// coordinate systems.
//
// Copied and adapted directly from LaRCsim/ls_geodesy.c
//
// See below for the complete original LaRCsim comments.
//
// $Id$
#ifndef _FG_GEODESY_HXX
#define _FG_GEODESY_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/point3d.hxx>
#include <simgear/polar3d.hxx>
// fgGeocToGeod(lat_geoc, radius, *lat_geod, *alt, *sea_level_r)
// INPUTS:
// lat_geoc Geocentric latitude, radians, + = North
// radius C.G. radius to earth center (meters)
//
// OUTPUTS:
// lat_geod Geodetic latitude, radians, + = North
// alt C.G. altitude above mean sea level (meters)
// sea_level_r radius from earth center to sea level at
// local vertical (surface normal) of C.G. (meters)
void fgGeocToGeod( double lat_geoc, double radius, double
*lat_geod, double *alt, double *sea_level_r );
// fgGeodToGeoc( lat_geod, alt, *sl_radius, *lat_geoc )
// INPUTS:
// lat_geod Geodetic latitude, radians, + = North
// alt C.G. altitude above mean sea level (meters)
//
// OUTPUTS:
// sl_radius SEA LEVEL radius to earth center (meters)
// (add Altitude to get true distance from earth center.
// lat_geoc Geocentric latitude, radians, + = North
//
void fgGeodToGeoc( double lat_geod, double alt, double *sl_radius,
double *lat_geoc );
// convert a geodetic point lon(radians), lat(radians), elev(meter) to
// a cartesian point
inline Point3D fgGeodToCart(const Point3D& geod) {
double gc_lon, gc_lat, sl_radius;
// printf("A geodetic point is (%.2f, %.2f, %.2f)\n",
// geod[0], geod[1], geod[2]);
gc_lon = geod.lon();
fgGeodToGeoc(geod.lat(), geod.radius(), &sl_radius, &gc_lat);
// printf("A geocentric point is (%.2f, %.2f, %.2f)\n", gc_lon,
// gc_lat, sl_radius+geod[2]);
Point3D pp = Point3D( gc_lon, gc_lat, sl_radius + geod.radius());
return fgPolarToCart3d(pp);
}
// given, alt, lat1, lon1, az1 and distance (s), calculate lat2, lon2
// and az2. Lat, lon, and azimuth are in degrees. distance in meters
int geo_direct_wgs_84 ( double alt, double lat1, double lon1, double az1,
double s, double *lat2, double *lon2, double *az2 );
// given alt, lat1, lon1, lat2, lon2, calculate starting and ending
// az1, az2 and distance (s). Lat, lon, and azimuth are in degrees.
// distance in meters
int geo_inverse_wgs_84( double alt, double lat1, double lon1, double lat2,
double lon2, double *az1, double *az2, double *s );
/***************************************************************************
TITLE: ls_geodesy
----------------------------------------------------------------------------
FUNCTION: Converts geocentric coordinates to geodetic positions
----------------------------------------------------------------------------
MODULE STATUS: developmental
----------------------------------------------------------------------------
GENEALOGY: Written as part of LaRCSim project by E. B. Jackson
----------------------------------------------------------------------------
DESIGNED BY: E. B. Jackson
CODED BY: E. B. Jackson
MAINTAINED BY: E. B. Jackson
----------------------------------------------------------------------------
MODIFICATION HISTORY:
DATE PURPOSE BY
930208 Modified to avoid singularity near polar region. EBJ
930602 Moved backwards calcs here from ls_step. EBJ
931214 Changed erroneous Latitude and Altitude variables to
*lat_geod and *alt in routine ls_geoc_to_geod. EBJ
940111 Changed header files from old ls_eom.h style to ls_types,
and ls_constants. Also replaced old DATA type with new
SCALAR type. EBJ
CURRENT RCS HEADER:
$Header$
* Revision 1.5 1994/01/11 18:47:05 bjax
* Changed include files to use types and constants, not ls_eom.h
* Also changed DATA type to SCALAR type.
*
* Revision 1.4 1993/12/14 21:06:47 bjax
* Removed global variable references Altitude and Latitude. EBJ
*
* Revision 1.3 1993/06/02 15:03:40 bjax
* Made new subroutine for calculating geodetic to geocentric; changed name
* of forward conversion routine from ls_geodesy to ls_geoc_to_geod.
*
----------------------------------------------------------------------------
REFERENCES:
[ 1] Stevens, Brian L.; and Lewis, Frank L.: "Aircraft
Control and Simulation", Wiley and Sons, 1992.
ISBN 0-471-61397-5
----------------------------------------------------------------------------
CALLED BY: ls_aux
----------------------------------------------------------------------------
CALLS TO:
----------------------------------------------------------------------------
INPUTS:
lat_geoc Geocentric latitude, radians, + = North
radius C.G. radius to earth center, ft
----------------------------------------------------------------------------
OUTPUTS:
lat_geod Geodetic latitude, radians, + = North
alt C.G. altitude above mean sea level, ft
sea_level_r radius from earth center to sea level at
local vertical (surface normal) of C.G.
--------------------------------------------------------------------------*/
#endif // _FG_GEODESY_HXX
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// fg_memory.h -- memcpy/bcopy portability declarations
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _FG_MEMORY_H
#define _FG_MEMORY_H
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#ifdef HAVE_MEMCPY
# ifdef HAVE_MEMORY_H
# include <memory.h>
# endif
# define fgmemcmp memcmp
# define fgmemcpy memcpy
# define fgmemzero(dest,len) memset(dest,0,len)
#elif defined(HAVE_BCOPY)
# define fgmemcmp bcmp
# define fgmemcpy(dest,src,n) bcopy(src,dest,n)
# define fgmemzero bzero
#else
/*
* Neither memcpy() or bcopy() available.
* Use substitutes provided be zlib.
*/
# include <zutil.h>
# define fgmemcmp zmemcmp
# define fgmemcpy zmemcpy
# define fgmemzero zmemzero
#endif
#endif // _FG_MEMORY_H
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// fg_random.c -- routines to handle random number generation
//
// Written by Curtis Olson, started July 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <stdio.h>
#include <stdlib.h> // for random(), srandom()
#include <time.h> // for time() to seed srandom()
#include "fg_random.h"
#ifndef HAVE_RAND
# ifdef sgi
# undef RAND_MAX
# define RAND_MAX 2147483647
# endif
#endif
#ifdef __SUNPRO_CC
extern "C" {
long int random(void);
void srandom(unsigned int seed);
}
#endif
// Seed the random number generater with time() so we don't see the
// same sequence every time
void fg_srandom(void) {
// fgPrintf( FG_MATH, FG_INFO, "Seeding random number generater\n");
#ifdef HAVE_RAND
srand(time(NULL));
#else
srandom(time(NULL));
#endif
}
// return a random number between [0.0, 1.0)
double fg_random(void) {
#ifdef HAVE_RAND
return(rand() / (double)RAND_MAX);
#else
return(random() / (double)RAND_MAX);
#endif
}
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// fg_random.h -- routines to handle random number generation
//
// Written by Curtis Olson, started July 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _FG_RANDOM_H
#define _FG_RANDOM_H
#ifdef __cplusplus
extern "C" {
#endif
// Seed the random number generater with time() so we don't see the
// same sequence every time
void fg_srandom(void);
// return a random number between [0.0, 1.0)
double fg_random(void);
#ifdef __cplusplus
}
#endif
#endif // _FG_RANDOM_H
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// fg_types.hxx -- commonly used types I don't want to have to keep redefining
//
// Written by Curtis Olson, started March 1999.
//
// Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _FG_TYPES_HXX
#define _FG_TYPES_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/compiler.h>
#include STL_STRING
#include <vector>
#include <simgear/point3d.hxx>
FG_USING_STD(vector);
FG_USING_STD(string);
typedef vector < int > int_list;
typedef int_list::iterator int_list_iterator;
typedef int_list::const_iterator const_int_list_iterator;
typedef vector < Point3D > point_list;
typedef point_list::iterator point_list_iterator;
typedef point_list::const_iterator const_point_list_iterator;
typedef vector < string > string_list;
typedef string_list::iterator string_list_iterator;
typedef string_list::const_iterator const_string_list_iterator;
class point2d {
public:
union {
double x;
double dist;
double lon;
};
union {
double y;
double theta;
double lat;
};
};
#endif // _FG_TYPES_HXX
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//
// interpolater.cxx -- routines to handle linear interpolation from a table of
// x,y The table must be sorted by "x" in ascending order
//
// Written by Curtis Olson, started April 1998.
//
// Copyright (C) 1998 Curtis L. Olson - curt@me.umn.edu
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include <simgear/compiler.h>
#ifdef __MWERKS__
#include <stdlib.h> // for exit()
#endif
#include STL_STRING
#include <simgear/logstream.hxx>
#include <simgear/fg_zlib.h>
#include <simgear/fgstream.hxx>
#include "interpolater.hxx"
// Constructor -- loads the interpolation table from the specified
// file
fgINTERPTABLE::fgINTERPTABLE( const string& file ) {
FG_LOG( FG_MATH, FG_INFO, "Initializing Interpolator for " << file );
fg_gzifstream in( file );
if ( !in ) {
FG_LOG( FG_GENERAL, FG_ALERT, "Cannot open file: " << file );
exit(-1);
}
size = 0;
in >> skipcomment;
while ( in ) {
if ( size < MAX_TABLE_SIZE ) {
in >> table[size][0] >> table[size][1];
size++;
} else {
FG_LOG( FG_MATH, FG_ALERT,
"fgInterpolateInit(): Exceed max table size = "
<< MAX_TABLE_SIZE );
exit(-1);
}
}
}
// Given an x value, linearly interpolate the y value from the table
double fgINTERPTABLE::interpolate(double x) {
int i;
double y;
i = 0;
while ( (x > table[i][0]) && (i < size) ) {
i++;
}
// printf ("i = %d ", i);
if ( (i == 0) && (x < table[0][0]) ) {
FG_LOG( FG_MATH, FG_ALERT,
"fgInterpolateInit(): lookup error, x to small = " << x );
return(0.0);
}
if ( x > table[i][0] ) {
FG_LOG( FG_MATH, FG_ALERT,
"fgInterpolateInit(): lookup error, x to big = " << x );
return(0.0);
}
// y = y1 + (y0 - y1)(x - x1) / (x0 - x1)
y = table[i][1] +
( (table[i-1][1] - table[i][1]) *
(x - table[i][0]) ) /
(table[i-1][0] - table[i][0]);
return(y);
}
// Destructor
fgINTERPTABLE::~fgINTERPTABLE( void ) {
}
+62
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//
// interpolater.hxx -- routines to handle linear interpolation from a table of
// x,y The table must be sorted by "x" in ascending order
//
// Written by Curtis Olson, started April 1998.
//
// Copyright (C) 1998 Curtis L. Olson - curt@me.umn.edu
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _INTERPOLATER_H
#define _INTERPOLATER_H
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/compiler.h>
#include STL_STRING
FG_USING_STD(string);
#define MAX_TABLE_SIZE 32
class fgINTERPTABLE {
int size;
double table[MAX_TABLE_SIZE][2];
public:
// Constructor -- loads the interpolation table from the specified
// file
fgINTERPTABLE( const string& file );
// Given an x value, linearly interpolate the y value from the table
double interpolate(double x);
// Destructor
~fgINTERPTABLE( void );
};
#endif // _INTERPOLATER_H
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// leastsqs.c -- Implements a simple linear least squares best fit routine
//
// Written by Curtis Olson, started September 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or modify
// it under the terms of the GNU General Public License as published by
// the Free Software Foundation; either version 2 of the License, or
// (at your option) any later version.
//
// This program is distributed in the hope that it will be useful,
// but WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
// GNU General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
//
#include <stdio.h>
#include "leastsqs.hxx"
/*
Least squares fit:
y = b0 + b1x
n*sum(xi*yi) - (sum(xi)*sum(yi))
b1 = --------------------------------
n*sum(xi^2) - (sum(xi))^2
b0 = sum(yi)/n - b1*(sum(xi)/n)
*/
double sum_xi, sum_yi, sum_xi_2, sum_xi_yi;
int sum_n;
void least_squares(double *x, double *y, int n, double *m, double *b) {
int i;
sum_xi = sum_yi = sum_xi_2 = sum_xi_yi = 0.0;
sum_n = n;
for ( i = 0; i < n; i++ ) {
sum_xi += x[i];
sum_yi += y[i];
sum_xi_2 += x[i] * x[i];
sum_xi_yi += x[i] * y[i];
}
/* printf("sum(xi)=%.2f sum(yi)=%.2f sum(xi^2)=%.2f sum(xi*yi)=%.2f\n",
sum_xi, sum_yi, sum_xi_2, sum_xi_yi); */
*m = ( (double)sum_n * sum_xi_yi - sum_xi * sum_yi ) /
( (double)sum_n * sum_xi_2 - sum_xi * sum_xi );
*b = (sum_yi / (double)sum_n) - (*m) * (sum_xi / (double)sum_n);
/* printf("slope = %.2f intercept = %.2f\n", *m, *b); */
}
/* incrimentally update existing values with a new data point */
void least_squares_update(double x, double y, double *m, double *b) {
++sum_n;
sum_xi += x;
sum_yi += y;
sum_xi_2 += x * x;
sum_xi_yi += x * y;
/* printf("sum(xi)=%.2f sum(yi)=%.2f sum(xi^2)=%.2f sum(xi*yi)=%.2f\n",
sum_xi, sum_yi, sum_xi_2, sum_xi_yi); */
*m = ( (double)sum_n * sum_xi_yi - sum_xi * sum_yi ) /
( (double)sum_n * sum_xi_2 - sum_xi * sum_xi );
*b = (sum_yi / (double)sum_n) - (*m) * (sum_xi / (double)sum_n);
/* printf("slope = %.2f intercept = %.2f\n", *m, *b); */
}
/*
return the least squares error:
(y[i] - y_hat[i])^2
-------------------
n
*/
double least_squares_error(double *x, double *y, int n, double m, double b) {
int i;
double error, sum;
sum = 0.0;
for ( i = 0; i < n; i++ ) {
error = y[i] - (m * x[i] + b);
sum += error * error;
// printf("%.2f %.2f\n", error, sum);
}
return ( sum / (double)n );
}
/*
return the maximum least squares error:
(y[i] - y_hat[i])^2
*/
double least_squares_max_error(double *x, double *y, int n, double m, double b){
int i;
double error, max_error;
max_error = 0.0;
for ( i = 0; i < n; i++ ) {
error = y[i] - (m * x[i] + b);
error = error * error;
if ( error > max_error ) {
max_error = error;
}
}
return ( max_error );
}
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// leastsqs.h -- Implements a simple linear least squares best fit routine
//
// Written by Curtis Olson, started September 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or modify
// it under the terms of the GNU General Public License as published by
// the Free Software Foundation; either version 2 of the License, or
// (at your option) any later version.
//
// This program is distributed in the hope that it will be useful,
// but WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
// GNU General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
///
#ifndef _LEASTSQS_H
#define _LEASTSQS_H
#ifndef __cplusplus
# error This library requires C++
#endif
/*
Least squares fit:
y = b0 + b1x
n*sum(xi*yi) - (sum(xi)*sum(yi))
b1 = --------------------------------
n*sum(xi^2) - (sum(xi))^2
b0 = sum(yi)/n - b1*(sum(xi)/n)
*/
void least_squares(double *x, double *y, int n, double *m, double *b);
/* incrimentally update existing values with a new data point */
void least_squares_update(double x, double y, double *m, double *b);
/*
return the least squares error:
(y[i] - y_hat[i])^2
-------------------
n
*/
double least_squares_error(double *x, double *y, int n, double m, double b);
/*
return the maximum least squares error:
(y[i] - y_hat[i])^2
*/
double least_squares_max_error(double *x, double *y, int n, double m, double b);
#endif // _LEASTSQS_H
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/*
WARNING - Do not remove this header.
This code is a templated version of the 'magic-software' spherical
interpolation code by Dave Eberly. The original (un-hacked) code can be
obtained from here: http://www.magic-software.com/gr_appr.htm
This code is derived from linintp2.h/cpp and sphrintp.h/cpp.
Dave Eberly says that the conditions for use are:
* You may distribute the original source code to others at no charge.
* You may modify the original source code and distribute it to others at
no charge. The modified code must be documented to indicate that it is
not part of the original package.
* You may use this code for non-commercial purposes. You may also
incorporate this code into commercial packages. However, you may not
sell any of your source code which contains my original and/or modified
source code. In such a case, you need to factor out my code and freely
distribute it.
* The original code comes with absolutely no warranty and no guarantee is
made that the code is bug-free.
This does not seem incompatible with GPL - so this modified version
is hereby placed under GPL along with the rest of FlightGear.
Christian Mayer
*/
#ifndef LININTP2_H
#define LININTP2_H
template<class T>
class mgcLinInterp2D
{
public:
mgcLinInterp2D (int _numPoints, double* x, double* y, T* _f);
~mgcLinInterp2D ();
double XMin () { return xmin; }
double XMax () { return xmax; }
double XRange () { return xmax-xmin; }
double YMin () { return ymin; }
double YMax () { return ymax; }
double YRange () { return ymax-ymin; }
int PointCount () { return numPoints; }
void GetPoint (int i, double& x, double& y);
int EdgeCount () { return numEdges; }
void GetEdge (int i, double& x0, double& y0, double& x1, double& y1);
int TriangleCount () { return numTriangles; }
void GetTriangle (int i, double& x0, double& y0, double& x1, double& y1,
double& x2, double& y2);
int Evaluate (double x, double y, T& F);
private:
typedef struct
{
double x, y;
}
Vertex;
typedef struct
{
int vertex[3]; // listed in counterclockwise order
int adj[3];
// adj[0] points to triangle sharing edge (vertex[0],vertex[1])
// adj[1] points to triangle sharing edge (vertex[1],vertex[2])
// adj[2] points to triangle sharing edge (vertex[2],vertex[0])
}
Triangle;
typedef struct
{
int vertex[2];
int triangle[2];
int index[2];
}
Edge;
int numPoints;
double** point;
double** tmppoint;
T* f;
double xmin, xmax, ymin, ymax;
int numEdges;
Edge* edge;
int numTriangles;
Triangle* triangle;
int Delaunay2D ();
void ComputeBarycenter (Vertex& v0, Vertex& v1, Vertex& v2, Vertex& ver,
double c[3]);
int InTriangle (Vertex& v0, Vertex& v1, Vertex& v2, Vertex& test);
};
#include "linintp2.inl"
#endif
+540
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@@ -0,0 +1,540 @@
/*
WARNING - Do not remove this header.
This code is a templated version of the 'magic-software' spherical
interpolation code by Dave Eberly. The original (un-hacked) code can be
obtained from here: http://www.magic-software.com/gr_appr.htm
This code is derived from linintp2.h/cpp and sphrintp.h/cpp.
Dave Eberly says that the conditions for use are:
* You may distribute the original source code to others at no charge.
* You may modify the original source code and distribute it to others at
no charge. The modified code must be documented to indicate that it is
not part of the original package.
* You may use this code for non-commercial purposes. You may also
incorporate this code into commercial packages. However, you may not
sell any of your source code which contains my original and/or modified
source code. In such a case, you need to factor out my code and freely
distribute it.
* The original code comes with absolutely no warranty and no guarantee is
made that the code is bug-free.
This does not seem incompatible with GPL - so this modified version
is hereby placed under GPL along with the rest of FlightGear.
Christian Mayer
*/
#include <float.h>
#include <math.h>
#include <stdlib.h>
#include "linintp2.h"
//---------------------------------------------------------------------------
template<class T>
mgcLinInterp2D<T>::mgcLinInterp2D (int _numPoints, double* x, double* y,
T* _f)
{
if ( (numPoints = _numPoints) < 3 )
{
point = 0;
edge = 0;
triangle = 0;
numTriangles = 0;
return;
}
cout << "[ 20%] allocating memory \r";
point = new double*[numPoints];
tmppoint = new double*[numPoints+3];
f = new T[numPoints];
int i;
for (i = 0; i < numPoints; i++)
point[i] = new double[2];
for (i = 0; i < numPoints+3; i++)
tmppoint[i] = new double[2];
for (i = 0; i < numPoints; i++)
{
point[i][0] = tmppoint[i][0] = x[i];
point[i][1] = tmppoint[i][1] = y[i];
f[i] = _f[i];
}
cout << "[ 30%] creating delaunay diagram \r";
Delaunay2D();
}
//---------------------------------------------------------------------------
template<class T>
mgcLinInterp2D<T>::~mgcLinInterp2D ()
{
if ( numPoints < 3 )
return;
int i;
if ( point )
{
for (i = 0; i < numPoints; i++)
delete[] point[i];
delete[] point;
}
if ( tmppoint )
{
for (i = 0; i < numPoints+3; i++)
delete[] tmppoint[i];
delete[] tmppoint;
}
delete[] f;
delete[] edge;
delete[] triangle;
}
//---------------------------------------------------------------------------
template<class T>
void mgcLinInterp2D<T>::ComputeBarycenter (Vertex& v0, Vertex& v1, Vertex& v2,
Vertex& ver, double c[3])
{
double A0 = v0.x-v2.x, B0 = v0.y-v2.y;
double A1 = v1.x-v2.x, B1 = v1.y-v2.y;
double A2 = ver.x-v2.x, B2 = ver.y-v2.y;
double m00 = A0*A0+B0*B0, m01 = A0*A1+B0*B1, m11 = A1*A1+B1*B1;
double r0 = A2*A0+B2*B0, r1 = A2*A1+B2*B1;
double det = m00*m11-m01*m01;
c[0] = (m11*r0-m01*r1)/det;
c[1] = (m00*r1-m01*r0)/det;
c[2] = 1-c[0]-c[1];
}
//---------------------------------------------------------------------------
template<class T>
int mgcLinInterp2D<T>::InTriangle (Vertex& v0, Vertex& v1, Vertex& v2,
Vertex& test)
{
const double eps = 1e-08;
double tx, ty, nx, ny;
// test against normal to first edge
tx = test.x - v0.x;
ty = test.y - v0.y;
nx = v0.y - v1.y;
ny = v1.x - v0.x;
if ( tx*nx + ty*ny < -eps )
return 0;
// test against normal to second edge
tx = test.x - v1.x;
ty = test.y - v1.y;
nx = v1.y - v2.y;
ny = v2.x - v1.x;
if ( tx*nx + ty*ny < -eps )
return 0;
// test against normal to third edge
tx = test.x - v2.x;
ty = test.y - v2.y;
nx = v2.y - v0.y;
ny = v0.x - v2.x;
if ( tx*nx + ty*ny < -eps )
return 0;
return 1;
}
//---------------------------------------------------------------------------
template<class T>
int mgcLinInterp2D<T>::Evaluate (double x, double y, T& F)
{
Vertex ver = { x, y };
// determine which triangle contains the target point
int i;
Vertex v0, v1, v2;
for (i = 0; i < numTriangles; i++)
{
Triangle& t = triangle[i];
v0.x = point[t.vertex[0]][0];
v0.y = point[t.vertex[0]][1];
v1.x = point[t.vertex[1]][0];
v1.y = point[t.vertex[1]][1];
v2.x = point[t.vertex[2]][0];
v2.y = point[t.vertex[2]][1];
if ( InTriangle(v0,v1,v2,ver) )
break;
}
if ( i == numTriangles ) // point is outside interpolation region
{
return 0;
}
Triangle& t = triangle[i]; // (x,y) is in this triangle
// compute barycentric coordinates with respect to subtriangle
double bary[3];
ComputeBarycenter(v0,v1,v2,ver,bary);
// compute barycentric combination of function values at vertices
F = bary[0]*f[t.vertex[0]]+bary[1]*f[t.vertex[1]]+bary[2]*f[t.vertex[2]];
return 1;
}
//---------------------------------------------------------------------------
template<class T>
int mgcLinInterp2D<T>::Delaunay2D ()
{
int result;
const double EPSILON = 1e-12;
const int TSIZE = 75;
const double RANGE = 10.0;
xmin = tmppoint[0][0];
xmax = xmin;
ymin = tmppoint[0][1];
ymax = ymin;
int i;
for (i = 0; i < numPoints; i++)
{
double value = tmppoint[i][0];
if ( xmax < value )
xmax = value;
if ( xmin > value )
xmin = value;
value = tmppoint[i][1];
if ( ymax < value )
ymax = value;
if ( ymin > value )
ymin = value;
}
double xrange = xmax-xmin, yrange = ymax-ymin;
double maxrange = xrange;
if ( maxrange < yrange )
maxrange = yrange;
// need to scale the data later to do a correct triangle count
double maxrange2 = maxrange*maxrange;
// tweak the points by very small random numbers
double bgs = EPSILON*maxrange;
srand(367);
for (i = 0; i < numPoints; i++)
{
tmppoint[i][0] += bgs*(0.5 - rand()/double(RAND_MAX));
tmppoint[i][1] += bgs*(0.5 - rand()/double(RAND_MAX));
}
double wrk[2][3] =
{
{ 5*RANGE, -RANGE, -RANGE },
{ -RANGE, 5*RANGE, -RANGE }
};
for (i = 0; i < 3; i++)
{
tmppoint[numPoints+i][0] = xmin+xrange*wrk[0][i];
tmppoint[numPoints+i][1] = ymin+yrange*wrk[1][i];
}
int i0, i1, i2, i3, i4, i5, i6, i7, i8, i9, i11;
int nts, ii[3];
double xx;
int tsz = 2*TSIZE;
int** tmp = new int*[tsz+1];
tmp[0] = new int[2*(tsz+1)];
for (i0 = 1; i0 < tsz+1; i0++)
tmp[i0] = tmp[0] + 2*i0;
i1 = 2*(numPoints + 2);
int* id = new int[i1];
for (i0 = 0; i0 < i1; i0++)
id[i0] = i0;
int** a3s = new int*[i1];
a3s[0] = new int[3*i1];
for (i0 = 1; i0 < i1; i0++)
a3s[i0] = a3s[0] + 3*i0;
a3s[0][0] = numPoints;
a3s[0][1] = numPoints+1;
a3s[0][2] = numPoints+2;
double** ccr = new double*[i1]; // circumscribed centers and radii
ccr[0] = new double[3*i1];
for (i0 = 1; i0 < i1; i0++)
ccr[i0] = ccr[0] + 3*i0;
ccr[0][0] = 0.0;
ccr[0][1] = 0.0;
ccr[0][2] = FLT_MAX;
nts = 1; // number of triangles
i4 = 1;
cout << "[ 40%] create triangulation \r";
// compute triangulation
for (i0 = 0; i0 < numPoints; i0++)
{
i1 = i7 = -1;
i9 = 0;
for (i11 = 0; i11 < nts; i11++)
{
i1++;
while ( a3s[i1][0] < 0 )
i1++;
xx = ccr[i1][2];
for (i2 = 0; i2 < 2; i2++)
{
double z = tmppoint[i0][i2]-ccr[i1][i2];
xx -= z*z;
if ( xx < 0 )
goto Corner3;
}
i9--;
i4--;
id[i4] = i1;
for (i2 = 0; i2 < 3; i2++)
{
ii[0] = 0;
if (ii[0] == i2)
ii[0]++;
for (i3 = 1; i3 < 2; i3++)
{
ii[i3] = ii[i3-1] + 1;
if (ii[i3] == i2)
ii[i3]++;
}
if ( i7 > 1 )
{
i8 = i7;
for (i3 = 0; i3 <= i8; i3++)
{
for (i5 = 0; i5 < 2; i5++)
if ( a3s[i1][ii[i5]] != tmp[i3][i5] )
goto Corner1;
for (i6 = 0; i6 < 2; i6++)
tmp[i3][i6] = tmp[i8][i6];
i7--;
goto Corner2;
Corner1:;
}
}
if ( ++i7 > tsz )
{
// temporary storage exceeded, increase TSIZE
result = 0;
goto ExitDelaunay;
}
for (i3 = 0; i3 < 2; i3++)
tmp[i7][i3] = a3s[i1][ii[i3]];
Corner2:;
}
a3s[i1][0] = -1;
Corner3:;
}
for (i1 = 0; i1 <= i7; i1++)
{
for (i2 = 0; i2 < 2; i2++)
for (wrk[i2][2] = 0, i3 = 0; i3 < 2; i3++)
{
wrk[i2][i3] = tmppoint[tmp[i1][i2]][i3]-tmppoint[i0][i3];
wrk[i2][2] +=
0.5*wrk[i2][i3]*(tmppoint[tmp[i1][i2]][i3]+
tmppoint[i0][i3]);
}
xx = wrk[0][0]*wrk[1][1]-wrk[1][0]*wrk[0][1];
ccr[id[i4]][0] = (wrk[0][2]*wrk[1][1]-wrk[1][2]*wrk[0][1])/xx;
ccr[id[i4]][1] = (wrk[0][0]*wrk[1][2]-wrk[1][0]*wrk[0][2])/xx;
for (ccr[id[i4]][2] = 0, i2 = 0; i2 < 2; i2++)
{
double z = tmppoint[i0][i2]-ccr[id[i4]][i2];
ccr[id[i4]][2] += z*z;
a3s[id[i4]][i2] = tmp[i1][i2];
}
a3s[id[i4]][2] = i0;
i4++;
i9++;
}
nts += i9;
}
// count the number of triangles
cout << "[ 50%] count the number of triangles \r";
numTriangles = 0;
i0 = -1;
for (i11 = 0; i11 < nts; i11++)
{
i0++;
while ( a3s[i0][0] < 0 )
i0++;
if ( a3s[i0][0] < numPoints )
{
for (i1 = 0; i1 < 2; i1++)
for (i2 = 0; i2 < 2; i2++)
wrk[i1][i2] =
tmppoint[a3s[i0][i1]][i2]-tmppoint[a3s[i0][2]][i2];
if ( fabs(wrk[0][0]*wrk[1][1]-wrk[0][1]*wrk[1][0]) > EPSILON*maxrange2 )
numTriangles++;
}
}
// create the triangles
cout << "[ 60%] create the triangles \r";
triangle = new Triangle[numTriangles];
numTriangles = 0;
i0 = -1;
for (i11 = 0; i11 < nts; i11++)
{
i0++;
while ( a3s[i0][0] < 0 )
i0++;
if ( a3s[i0][0] < numPoints )
{
for (i1 = 0; i1 < 2; i1++)
for (i2 = 0; i2 < 2; i2++)
wrk[i1][i2] =
tmppoint[a3s[i0][i1]][i2]-tmppoint[a3s[i0][2]][i2];
xx = wrk[0][0]*wrk[1][1]-wrk[0][1]*wrk[1][0];
if ( fabs(xx) > EPSILON*maxrange2 )
{
int delta = xx < 0 ? 1 : 0;
Triangle& tri = triangle[numTriangles];
tri.vertex[0] = a3s[i0][0];
tri.vertex[1] = a3s[i0][1+delta];
tri.vertex[2] = a3s[i0][2-delta];
tri.adj[0] = -1;
tri.adj[1] = -1;
tri.adj[2] = -1;
numTriangles++;
}
}
}
// build edge table
cout << "[ 70%] build the edge table \r";
numEdges = 0;
edge = new Edge[3*numTriangles];
int j, j0, j1;
for (i = 0; i < numTriangles; i++)
{
if ( (i%500) == 0)
cout << "[ 7" << 10*i/numTriangles << "%] build the edge table \r";
Triangle& t = triangle[i];
for (j0 = 0, j1 = 1; j0 < 3; j0++, j1 = (j1+1)%3)
{
for (j = 0; j < numEdges; j++)
{
Edge& e = edge[j];
if ( (t.vertex[j0] == e.vertex[0]
&& t.vertex[j1] == e.vertex[1])
|| (t.vertex[j0] == e.vertex[1]
&& t.vertex[j1] == e.vertex[0]) )
break;
}
if ( j == numEdges ) // add edge to table
{
edge[j].vertex[0] = t.vertex[j0];
edge[j].vertex[1] = t.vertex[j1];
edge[j].triangle[0] = i;
edge[j].index[0] = j0;
edge[j].triangle[1] = -1;
numEdges++;
}
else // edge already exists, add triangle to table
{
edge[j].triangle[1] = i;
edge[j].index[1] = j0;
}
}
}
// establish links between adjacent triangles
cout << "[ 80%] establishing links between adjacent triangles \r";
for (i = 0; i < numEdges; i++)
{
if ( edge[i].triangle[1] != -1 )
{
j0 = edge[i].triangle[0];
j1 = edge[i].triangle[1];
triangle[j0].adj[edge[i].index[0]] = j1;
triangle[j1].adj[edge[i].index[1]] = j0;
}
}
result = 1;
ExitDelaunay:;
delete[] tmp[0];
delete[] tmp;
delete[] id;
delete[] a3s[0];
delete[] a3s;
delete[] ccr[0];
delete[] ccr;
cout << "[ 90%] finsishes delauney triangulation \r";
return result;
}
//---------------------------------------------------------------------------
template<class T>
void mgcLinInterp2D<T>::GetPoint (int i, double& x, double& y)
{
// assumes i is valid [can use PointCount() before passing i]
x = point[i][0];
y = point[i][1];
}
//---------------------------------------------------------------------------
template<class T>
void mgcLinInterp2D<T>::GetEdge (int i, double& x0, double& y0, double& x1,
double& y1)
{
// assumes i is valid [can use EdgeCount() before passing i]
int v0 = edge[i].vertex[0], v1 = edge[i].vertex[1];
x0 = point[v0][0];
y0 = point[v0][1];
x1 = point[v1][0];
y1 = point[v1][1];
}
//---------------------------------------------------------------------------
template<class T>
void mgcLinInterp2D<T>::GetTriangle (int i, double& x0, double& y0, double& x1,
double& y1, double& x2, double& y2)
{
// assumes i is valid [can use TriangleCount() before passing i]
int v0 = triangle[i].vertex[0];
int v1 = triangle[i].vertex[1];
int v2 = triangle[i].vertex[2];
x0 = point[v0][0];
y0 = point[v0][1];
x1 = point[v1][0];
y1 = point[v1][1];
x2 = point[v2][0];
y2 = point[v2][1];
}
//---------------------------------------------------------------------------
+233
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@@ -0,0 +1,233 @@
/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
/* -------------------------------------------------------------------------
Public MAT3 include file
------------------------------------------------------------------------- */
#ifndef MAT3_HAS_BEEN_INCLUDED
#define MAT3_HAS_BEEN_INCLUDED
/* ----------------------------- Constants ------------------------------ */
/*
* Make sure the math library .h file is included, in case it wasn't.
*/
#ifndef HUGE
#include <math.h>
#endif
#include <stdio.h>
#include <string.h>
#include <simgear/fg_memory.h>
#ifdef __cplusplus
extern "C" {
#endif
#define MAT3_DET0 -1 /* Indicates singular mat */
#define MAT3_EPSILON 1e-12 /* Close enough to zero */
#ifdef M_PI
# define MAT3_PI M_PI
#else
# define MAT3_PI 3.14159265358979323846
#endif
#define USE_XTRA_MAT3_INLINES
#if defined(i386)
#define USE_X86_ASM
#endif
#if defined(USE_X86_ASM)
static __inline__ int FloatToInt(float f)
{
int r;
__asm__ ("fistpl %0" : "=m" (r) : "t" (f) : "st");
return r;
}
#elif defined(__MSC__) && defined(__WIN32__)
static __inline int FloatToInt(float f)
{
int r;
_asm {
fld f
fistp r
}
return r;
}
#else
#define FloatToInt(F) ((int) ((F) < 0.0f ? (F)-0.5f : (F)+0.5f))
#endif
/* ------------------------------ Types --------------------------------- */
typedef double MAT3mat[4][4]; /* 4x4 matrix */
typedef double MAT3vec[3]; /* Vector */
typedef double MAT3hvec[4]; /* Vector with homogeneous coord */
/* ------------------------------ Macros -------------------------------- */
extern MAT3mat identityMatrix;
/* Tests if a number is within EPSILON of zero */
#define MAT3_IS_ZERO(N) ((N) < MAT3_EPSILON && (N) > -MAT3_EPSILON)
/* Sets a vector to the three given values */
#define MAT3_SET_VEC(V,X,Y,Z) ((V)[0]=(X), (V)[1]=(Y), (V)[2]=(Z))
/* Tests a vector for all components close to zero */
#define MAT3_IS_ZERO_VEC(V) (MAT3_IS_ZERO((V)[0]) && \
MAT3_IS_ZERO((V)[1]) && \
MAT3_IS_ZERO((V)[2]))
/* Dot product of two vectors */
#define MAT3_DOT_PRODUCT(V1,V2) \
((V1)[0]*(V2)[0] + (V1)[1]*(V2)[1] + (V1)[2]*(V2)[2])
/* Copy one vector to other */
#define MAT3_COPY_VEC(TO,FROM) ((TO)[0] = (FROM)[0], \
(TO)[1] = (FROM)[1], \
(TO)[2] = (FROM)[2])
/* Normalize vector to unit length, using TEMP as temporary variable.
* TEMP will be zero if vector has zero length */
#define MAT3_NORMALIZE_VEC(V,TEMP) \
if ((TEMP = sqrt(MAT3_DOT_PRODUCT(V,V))) > MAT3_EPSILON) { \
TEMP = 1.0 / TEMP; \
MAT3_SCALE_VEC(V,V,TEMP); \
} else TEMP = 0.0
/* Scale vector by given factor, storing result vector in RESULT_V */
#define MAT3_SCALE_VEC(RESULT_V,V,SCALE) \
MAT3_SET_VEC(RESULT_V, (V)[0]*(SCALE), (V)[1]*(SCALE), (V)[2]*(SCALE))
/* Adds vectors V1 and V2, storing result in RESULT_V */
#define MAT3_ADD_VEC(RESULT_V,V1,V2) \
MAT3_SET_VEC(RESULT_V, (V1)[0]+(V2)[0], (V1)[1]+(V2)[1], \
(V1)[2]+(V2)[2])
/* Subtracts vector V2 from V1, storing result in RESULT_V */
#define MAT3_SUB_VEC(RESULT_V,V1,V2) \
MAT3_SET_VEC(RESULT_V, (V1)[0]-(V2)[0], (V1)[1]-(V2)[1], \
(V1)[2]-(V2)[2])
/* Multiplies vectors V1 and V2, storing result in RESULT_V */
#define MAT3_MULT_VEC(RESULT_V,V1,V2) \
MAT3_SET_VEC(RESULT_V, (V1)[0]*(V2)[0], (V1)[1]*(V2)[1], \
(V1)[2]*(V2)[2])
/* Sets RESULT_V to the linear combination of V1 and V2, scaled by
* SCALE1 and SCALE2, respectively */
#define MAT3_LINEAR_COMB(RESULT_V,SCALE1,V1,SCALE2,V2) \
MAT3_SET_VEC(RESULT_V, (SCALE1)*(V1)[0] + (SCALE2)*(V2)[0], \
(SCALE1)*(V1)[1] + (SCALE2)*(V2)[1], \
(SCALE1)*(V1)[2] + (SCALE2)*(V2)[2])
/* Several of the vector macros are useful for homogeneous-coord vectors */
#define MAT3_SET_HVEC(V,X,Y,Z,W) ((V)[0]=(X), (V)[1]=(Y), \
(V)[2]=(Z), (V)[3]=(W))
#define MAT3_COPY_HVEC(TO,FROM) ((TO)[0] = (FROM)[0], \
(TO)[1] = (FROM)[1], \
(TO)[2] = (FROM)[2], \
(TO)[3] = (FROM)[3])
#define MAT3_SCALE_HVEC(RESULT_V,V,SCALE) \
MAT3_SET_HVEC(RESULT_V, (V)[0]*(SCALE), (V)[1]*(SCALE), \
(V)[2]*(SCALE), (V)[3]*(SCALE))
#define MAT3_ADD_HVEC(RESULT_V,V1,V2) \
MAT3_SET_HVEC(RESULT_V, (V1)[0]+(V2)[0], (V1)[1]+(V2)[1], \
(V1)[2]+(V2)[2], (V1)[3]+(V2)[3])
#define MAT3_SUB_HVEC(RESULT_V,V1,V2) \
MAT3_SET_HVEC(RESULT_V, (V1)[0]-(V2)[0], (V1)[1]-(V2)[1], \
(V1)[2]-(V2)[2], (V1)[3]-(V2)[3])
#define MAT3_MULT_HVEC(RESULT_V,V1,V2) \
MAT3_SET_HVEC(RESULT_V, (V1)[0]*(V2)[0], (V1)[1]*(V2)[1], \
(V1)[2]*(V2)[2], (V1)[3]*(V2)[3])
/* ------------------------------ Entries ------------------------------- */
#define MAT3identity(mat) fgmemcpy( mat, identityMatrix, sizeof(MAT3mat) )
#define MAT3zero(mat) fgmemzero( mat, sizeof(MAT3mat) )
#define MAT3copy(to, from) fgmemcpy( to, from, sizeof(MAT3mat) )
#if defined( USE_XTRA_MAT3_INLINES )
# define MAT3mult_vec( result_vec, vec, mat) { \
MAT3vec tempvec; \
tempvec[0]=vec[0]*mat[0][0]+vec[1]*mat[1][0]+vec[2]*mat[2][0]+mat[3][0]; \
tempvec[1]=vec[0]*mat[0][1]+vec[1]*mat[1][1]+vec[2]*mat[2][1]+mat[3][1]; \
tempvec[2]=vec[0]*mat[0][2]+vec[1]*mat[1][2]+vec[2]*mat[2][2]+mat[3][2]; \
result_vec[0] = tempvec[0]; \
result_vec[1] = tempvec[1]; \
result_vec[2] = tempvec[2]; \
}
# define MAT3cross_product(result_vec, vec1, vec2) { \
MAT3vec tempvec; \
tempvec[0] = vec1[1] * vec2[2] - vec1[2] * vec2[1]; \
tempvec[1] = vec1[2] * vec2[0] - vec1[0] * vec2[2]; \
tempvec[2] = vec1[0] * vec2[1] - vec1[1] * vec2[0]; \
result_vec[0] = tempvec[0]; \
result_vec[1] = tempvec[1]; \
result_vec[2] = tempvec[2]; \
}
# define MAT3mult( result_mat, mat1, mat2) { \
register int i, j; \
MAT3mat tmp_mat; \
for (i = 0; i < 4; i++) \
for (j = 0; j < 4; j++) \
tmp_mat[i][j] = (mat1[i][0] * mat2[0][j] + \
mat1[i][1] * mat2[1][j] + \
mat1[i][2] * mat2[2][j] + \
mat1[i][3] * mat2[3][j]); \
fgmemcpy(result_mat, tmp_mat, sizeof(MAT3mat)); \
}
#else // !defined( USE_XTRA_MAT3_INLINES )
/* In MAT3mat.c */
void MAT3mult(MAT3mat result, MAT3mat, MAT3mat);
void MAT3mult_vec(MAT3vec result_vec, MAT3vec vec, MAT3mat mat);
void MAT3cross_product(MAT3vec result,MAT3vec,MAT3vec);
#endif // defined( USE_XTRA_MAT3_INLINES )
/* In MAT3geom.c */
void MAT3direction_matrix (MAT3mat result_mat, MAT3mat mat);
int MAT3normal_matrix (MAT3mat result_mat, MAT3mat mat);
void MAT3rotate (MAT3mat result_mat, MAT3vec axis, double angle_in_radians);
void MAT3translate (MAT3mat result_mat, MAT3vec trans);
void MAT3scale (MAT3mat result_mat, MAT3vec scale);
void MAT3shear(MAT3mat result_mat, double xshear, double yshear);
void MAT3transpose (MAT3mat result, MAT3mat);
int MAT3invert (MAT3mat result, MAT3mat);
void MAT3print (MAT3mat, FILE *fp);
void MAT3print_formatted (MAT3mat, FILE *fp,
char *title, char *head, char *format, char *tail);
int MAT3equal( void );
double MAT3trace( void );
int MAT3power( void );
int MAT3column_reduce( void );
int MAT3kernel_basis( void );
/* In MAT3vec.c */
int MAT3mult_hvec (MAT3hvec result_vec, MAT3hvec vec, MAT3mat mat, int normalize);
void MAT3perp_vec(MAT3vec result_vec, MAT3vec vec, int is_unit);
#ifdef __cplusplus
}
#endif
#endif /* MAT3_HAS_BEEN_INCLUDED */
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/* Copyright 1988, Brown Computer Graphics Group. All Rights Reserved. */
#ifndef _MAT3DEFS_H
#define _MAT3DEFS_H
#ifdef __cplusplus
extern "C" {
#endif
#include <stdio.h>
/* #include <Math/mat3err.h> */
#include "mat3.h"
/* ----------------------------- Constants ------------------------------ */
#define FALSE 0
#define TRUE 1
#define CNULL ((char *) NULL)
/* ------------------------------ Macros -------------------------------- */
#define ALLOCN(P,T,N,M) \
if ((P = (T *) malloc((unsigned) (N) * sizeof(T))) == NULL) \
ERR_ERROR(MAT3_errid, ERR_FATAL, (ERR_ALLOC1, M)); \
else
#define FREE(P) free((char *) (P))
#define ABS(A) ((A) > 0 ? (A) : -(A))
#define MIN(A,B) ((A) < (B) ? (A) : (B))
#define MAX(A,B) ((A) > (B) ? (A) : (B))
#define SWAP(A,B,T) (T = A, A = B, B = T)
/* Is N within EPS of zero ? */
#define IS_ZERO(N,EPS) ((N) < EPS && (N) > -EPS)
/* Macros for lu routines */
#define LU_PERMUTE(p,i,j) { int LU_T; LU_T = p[i]; p[i] = p[j]; p[j] = LU_T; }
/* ------------------------- Internal Entries ---------------------------- */
/* ------------------------- Global Variables ---------------------------- */
/* extern ERRid *MAT3_errid; */
#ifdef __cplusplus
}
#endif
#endif /* _MAT3DEFS_H */
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#ifndef _MAT3ERR_H
#define _MAT3ERR_H
#ifdef __cplusplus
extern "C" {
#endif
#include "sph_errtypes.h"
#ifdef THINK_C
/* We hide this from gnu's compiler, which doesn't understand it. */
void SPH__error (int errtype, ...);
#endif
#define ERR_ERROR(A,B,C) \
if (1) {char cstr[256]; sprintf C; SPH__error(ERR_MAT3_PACKAGE, cstr); } else
#define ERR_S cstr,"%s\n"
#define ERR_SI cstr,"%s: %d\n"
#define ERR_SS cstr,"%s: %s\n"
#define ERR_SEVERE 0
#define ERR_FATAL 0
#define ERR_ALLOC1 0
typedef int ERRid;
#define ERRregister_package(S) 100
#ifdef __cplusplus
}
#endif
#endif /* _MAT3ERR_H */
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// point3d.hxx -- a 3d point class.
//
// Adapted from algebra3 by Jean-Francois Doue, started October 1998.
//
// Copyright (C) 1998 Curtis L. Olson - curt@me.umn.edu
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _POINT3D_HXX
#define _POINT3D_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/compiler.h>
#ifdef FG_MATH_EXCEPTION_CLASH
# define exception c_exception
#endif
#ifdef FG_HAVE_STD_INCLUDES
# include <iostream>
# include <cassert>
# include <cmath>
#else
# include <iostream.h>
# include <assert.h>
# include <math.h>
#endif
// I don't understand ... <math.h> or <cmath> should be included
// already depending on how you defined FG_HAVE_STD_INCLUDES, but I
// can go ahead and add this -- CLO
#ifdef __MWERKS__
FG_USING_NAMESPACE(std);
#endif
#ifndef FG_HAVE_NATIVE_SGI_COMPILERS
FG_USING_STD(ostream);
FG_USING_STD(istream);
#endif
const double fgPoint3_Epsilon = 0.0000001;
enum {PX, PY, PZ}; // axes
// Kludge for msvc++ 6.0 - requires forward decls of friend functions.
class Point3D;
istream& operator>> ( istream&, Point3D& );
ostream& operator<< ( ostream&, const Point3D& );
Point3D operator- (const Point3D& p); // -p1
bool operator== (const Point3D& a, const Point3D& b); // p1 == p2?
///////////////////////////
//
// 3D Point
//
///////////////////////////
class Point3D {
protected:
double n[3];
public:
// Constructors
Point3D();
Point3D(const double x, const double y, const double z);
explicit Point3D(const double d);
Point3D(const Point3D &p);
// Assignment operators
Point3D& operator = ( const Point3D& p ); // assignment of a Point3D
Point3D& operator += ( const Point3D& p ); // incrementation by a Point3D
Point3D& operator -= ( const Point3D& p ); // decrementation by a Point3D
Point3D& operator *= ( const double d ); // multiplication by a constant
Point3D& operator /= ( const double d ); // division by a constant
void setx(const double x);
void sety(const double y);
void setz(const double z);
// Queries
double& operator [] ( int i); // indexing
double operator[] (int i) const; // read-only indexing
inline const double *get_n() const { return n; };
double x() const; // cartesian x
double y() const; // cartesian y
double z() const; // cartesian z
double lon() const; // polar longitude
double lat() const; // polar latitude
double radius() const; // polar radius
double elev() const; // geodetic elevation (if specifying a surface point)
// friends
friend Point3D operator - (const Point3D& p); // -p1
friend bool operator == (const Point3D& a, const Point3D& b); // p1 == p2?
friend istream& operator>> ( istream&, Point3D& );
friend ostream& operator<< ( ostream&, const Point3D& );
// Special functions
double distance3D(const Point3D& a) const; // distance between
double distance3Dsquared(const Point3D& a) const; // distance between ^ 2
};
// input from stream
inline istream&
operator >> ( istream& in, Point3D& p)
{
char c;
in >> p.n[PX];
// read past optional comma
while ( in.get(c) ) {
if ( (c != ' ') && (c != ',') ) {
// push back on the stream
in.putback(c);
break;
}
}
in >> p.n[PY];
// read past optional comma
while ( in.get(c) ) {
if ( (c != ' ') && (c != ',') ) {
// push back on the stream
in.putback(c);
break;
}
}
in >> p.n[PZ];
return in;
}
inline ostream&
operator<< ( ostream& out, const Point3D& p )
{
return out << p.n[PX] << ", " << p.n[PY] << ", " << p.n[PZ];
}
///////////////////////////
//
// Point3D Member functions
//
///////////////////////////
// CONSTRUCTORS
inline Point3D::Point3D() {}
inline Point3D::Point3D(const double x, const double y, const double z)
{
n[PX] = x; n[PY] = y; n[PZ] = z;
}
inline Point3D::Point3D(const double d)
{
n[PX] = n[PY] = n[PZ] = d;
}
inline Point3D::Point3D(const Point3D& p)
{
n[PX] = p.n[PX]; n[PY] = p.n[PY]; n[PZ] = p.n[PZ];
}
// ASSIGNMENT OPERATORS
inline Point3D& Point3D::operator = (const Point3D& p)
{
n[PX] = p.n[PX]; n[PY] = p.n[PY]; n[PZ] = p.n[PZ]; return *this;
}
inline Point3D& Point3D::operator += ( const Point3D& p )
{
n[PX] += p.n[PX]; n[PY] += p.n[PY]; n[PZ] += p.n[PZ]; return *this;
}
inline Point3D& Point3D::operator -= ( const Point3D& p )
{
n[PX] -= p.n[PX]; n[PY] -= p.n[PY]; n[PZ] -= p.n[PZ]; return *this;
}
inline Point3D& Point3D::operator *= ( const double d )
{
n[PX] *= d; n[PY] *= d; n[PZ] *= d; return *this;
}
inline Point3D& Point3D::operator /= ( const double d )
{
double d_inv = 1./d; n[PX] *= d_inv; n[PY] *= d_inv; n[PZ] *= d_inv;
return *this;
}
inline void Point3D::setx(const double x) {
n[PX] = x;
}
inline void Point3D::sety(const double y) {
n[PY] = y;
}
inline void Point3D::setz(const double z) {
n[PZ] = z;
}
// QUERIES
inline double& Point3D::operator [] ( int i)
{
assert(! (i < PX || i > PZ));
return n[i];
}
inline double Point3D::operator [] ( int i) const {
assert(! (i < PX || i > PZ));
return n[i];
}
inline double Point3D::x() const { return n[PX]; }
inline double Point3D::y() const { return n[PY]; }
inline double Point3D::z() const { return n[PZ]; }
inline double Point3D::lon() const { return n[PX]; }
inline double Point3D::lat() const { return n[PY]; }
inline double Point3D::radius() const { return n[PZ]; }
inline double Point3D::elev() const { return n[PZ]; }
// FRIENDS
inline Point3D operator - (const Point3D& a)
{
return Point3D(-a.n[PX],-a.n[PY],-a.n[PZ]);
}
inline Point3D operator + (const Point3D& a, const Point3D& b)
{
return Point3D(a) += b;
}
inline Point3D operator - (const Point3D& a, const Point3D& b)
{
return Point3D(a) -= b;
}
inline Point3D operator * (const Point3D& a, const double d)
{
return Point3D(a) *= d;
}
inline Point3D operator * (const double d, const Point3D& a)
{
return a*d;
}
inline Point3D operator / (const Point3D& a, const double d)
{
return Point3D(a) *= (1.0 / d );
}
inline bool operator == (const Point3D& a, const Point3D& b)
{
return
fabs(a.n[PX] - b.n[PX]) < fgPoint3_Epsilon &&
fabs(a.n[PY] - b.n[PY]) < fgPoint3_Epsilon &&
fabs(a.n[PZ] - b.n[PZ]) < fgPoint3_Epsilon;
}
inline bool operator != (const Point3D& a, const Point3D& b)
{
return !(a == b);
}
// Special functions
inline double
Point3D::distance3D(const Point3D& a ) const
{
double x, y, z;
x = n[PX] - a.n[PX];
y = n[PY] - a.n[PY];
z = n[PZ] - a.n[PZ];
return sqrt(x*x + y*y + z*z);
}
inline double
Point3D::distance3Dsquared(const Point3D& a ) const
{
double x, y, z;
x = n[PX] - a.n[PX];
y = n[PY] - a.n[PY];
z = n[PZ] - a.n[PZ];
return(x*x + y*y + z*z);
}
#endif // _POINT3D_HXX
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// polar.cxx -- routines to deal with polar math and transformations
//
// Written by Curtis Olson, started June 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include <math.h>
#include <stdio.h>
#include <simgear/constants.h>
#include "polar3d.hxx"
// Find the Altitude above the Ellipsoid (WGS84) given the Earth
// Centered Cartesian coordinate vector Distances are specified in
// meters.
double fgGeodAltFromCart(const Point3D& cp)
{
double t_lat, x_alpha, mu_alpha;
double lat_geoc, radius;
double result;
lat_geoc = FG_PI_2 - atan2( sqrt(cp.x()*cp.x() + cp.y()*cp.y()), cp.z() );
radius = sqrt( cp.x()*cp.x() + cp.y()*cp.y() + cp.z()*cp.z() );
if( ( (FG_PI_2 - lat_geoc) < ONE_SECOND ) // near North pole
|| ( (FG_PI_2 + lat_geoc) < ONE_SECOND ) ) // near South pole
{
result = radius - EQUATORIAL_RADIUS_M*E;
} else {
t_lat = tan(lat_geoc);
x_alpha = E*EQUATORIAL_RADIUS_M/sqrt(t_lat*t_lat + E*E);
mu_alpha = atan2(sqrt(RESQ_M - x_alpha*x_alpha),E*x_alpha);
if (lat_geoc < 0) {
mu_alpha = - mu_alpha;
}
result = (radius - x_alpha/cos(lat_geoc))*cos(mu_alpha - lat_geoc);
}
return(result);
}
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// polar.hxx -- routines to deal with polar math and transformations
//
// Written by Curtis Olson, started June 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _POLAR_HXX
#define _POLAR_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/constants.h>
#include <simgear/point3d.hxx>
// Find the Altitude above the Ellipsoid (WGS84) given the Earth
// Centered Cartesian coordinate vector Distances are specified in
// meters.
double fgGeodAltFromCart(const Point3D& cp);
// Convert a polar coordinate to a cartesian coordinate. Lon and Lat
// must be specified in radians. The FG convention is for distances
// to be specified in meters
inline Point3D fgPolarToCart3d(const Point3D& p) {
double tmp = cos( p.lat() ) * p.radius();
return Point3D( cos( p.lon() ) * tmp,
sin( p.lon() ) * tmp,
sin( p.lat() ) * p.radius() );
}
// Convert a cartesian coordinate to polar coordinates (lon/lat
// specified in radians. Distances are specified in meters.
inline Point3D fgCartToPolar3d(const Point3D& cp) {
return Point3D( atan2( cp.y(), cp.x() ),
FG_PI_2 -
atan2( sqrt(cp.x()*cp.x() + cp.y()*cp.y()), cp.z() ),
sqrt(cp.x()*cp.x() + cp.y()*cp.y() + cp.z()*cp.z()) );
}
// calc new lon/lat given starting lon/lat, and offset radial, and
// distance. NOTE: starting point is specifed in radians, distance is
// specified in meters (and converted internally to radians)
// ... assumes a spherical world
inline Point3D calc_lon_lat( const Point3D& orig, double course, double dist ) {
Point3D result;
// lat=asin(sin(lat1)*cos(d)+cos(lat1)*sin(d)*cos(tc))
// IF (cos(lat)=0)
// lon=lon1 // endpoint a pole
// ELSE
// lon=mod(lon1-asin(sin(tc)*sin(d)/cos(lat))+pi,2*pi)-pi
// ENDIF
// printf("calc_lon_lat() offset.theta = %.2f offset.dist = %.2f\n",
// offset.theta, offset.dist);
dist *= METER_TO_NM * NM_TO_RAD;
result.sety( asin( sin(orig.y()) * cos(dist) +
cos(orig.y()) * sin(dist) * cos(course) ) );
if ( cos(result.y()) < FG_EPSILON ) {
result.setx( orig.x() ); // endpoint a pole
} else {
result.setx(
fmod(orig.x() - asin( sin(course) * sin(dist) /
cos(result.y()) ) + FG_PI, FG_2PI) - FG_PI );
}
return result;
}
#endif // _POLAR_HXX
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/*
WARNING - Do not remove this header.
This code is a templated version of the 'magic-software' spherical
interpolation code by Dave Eberly. The original (un-hacked) code can be
obtained from here: http://www.magic-software.com/gr_appr.htm
This code is derived from linintp2.h/cpp and sphrintp.h/cpp.
Dave Eberly says that the conditions for use are:
* You may distribute the original source code to others at no charge.
* You may modify the original source code and distribute it to others at
no charge. The modified code must be documented to indicate that it is
not part of the original package.
* You may use this code for non-commercial purposes. You may also
incorporate this code into commercial packages. However, you may not
sell any of your source code which contains my original and/or modified
source code. In such a case, you need to factor out my code and freely
distribute it.
* The original code comes with absolutely no warranty and no guarantee is
made that the code is bug-free.
This does not seem incompatible with GPL - so this modified version
is hereby placed under GPL along with the rest of FlightGear.
Christian Mayer
*/
#ifndef SPHRINTP_H
#define SPHRINTP_H
#include "linintp2.h"
#include <plib/sg.h>
template<class T>
class SphereInterpolate
{
public:
SphereInterpolate (int n, const double* x, const double* y,
const double* z, const T* f);
SphereInterpolate (int n, const sgVec2* p, const T* f);
~SphereInterpolate ();
void GetSphericalCoords (const double x, const double y, const double z,
double& thetaAngle, double& phiAngle) const;
int Evaluate (const double x, const double y, const double z, T& f) const;
int Evaluate (const double thetaAngle, const double phiAngle, T& f) const;
T Evaluate(const sgVec2& p) const
{
T retval;
Evaluate(p[1], p[0], retval);
return retval;
}
T Evaluate(const sgVec3& p) const
{
T retval;
Evaluate(p[1], p[0], retval);
return retval;
}
protected:
int numPoints;
double* theta;
double* phi;
T* func;
mgcLinInterp2D<T>* pInterp;
};
#include "sphrintp.inl"
#endif
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/*
WARNING - Do not remove this header.
This code is a templated version of the 'magic-software' spherical
interpolation code by Dave Eberly. The original (un-hacked) code can be
obtained from here: http://www.magic-software.com/gr_appr.htm
This code is derived from linintp2.h/cpp and sphrintp.h/cpp.
Dave Eberly says that the conditions for use are:
* You may distribute the original source code to others at no charge.
* You may modify the original source code and distribute it to others at
no charge. The modified code must be documented to indicate that it is
not part of the original package.
* You may use this code for non-commercial purposes. You may also
incorporate this code into commercial packages. However, you may not
sell any of your source code which contains my original and/or modified
source code. In such a case, you need to factor out my code and freely
distribute it.
* The original code comes with absolutely no warranty and no guarantee is
made that the code is bug-free.
This does not seem incompatible with GPL - so this modified version
is hereby placed under GPL along with the rest of FlightGear.
Christian Mayer
*/
#include <math.h>
#include "sphrintp.h"
static const double PI = 4.0*atan(1.0);
static const double TWOPI = 2.0*PI;
//---------------------------------------------------------------------------
template<class T>
SphereInterpolate<T>::SphereInterpolate (int n, const double* x,
const double* y, const double* z,
const T* f)
{
// Assumes (x[i],y[i],z[i]) is unit length for all 0 <= i < n.
// For complete spherical coverage, include the two antipodal points
// (0,0,1,f(0,0,1)) and (0,0,-1,f(0,0,-1)) in the data set.
cout << "Initialising spherical interpolator.\n";
cout << "[ 0%] Allocating memory \r";
theta = new double[3*n];
phi = new double[3*n];
func = new T[3*n];
// convert data to spherical coordinates
int i;
T empty;
for (i = 0; i < n; i++)
{
GetSphericalCoords(x[i],y[i],z[i],theta[i],phi[i]);
func[i] = f[i];
}
// use periodicity to get wrap-around in the Delaunay triangulation
cout << "[ 10%] copying vertices for wrap-around\r";
int j, k;
for (i = 0, j = n, k = 2*n; i < n; i++, j++, k++)
{
theta[j] = theta[i]+TWOPI;
theta[k] = theta[i]-TWOPI;
phi[j] = phi[i];
phi[k] = phi[i];
func[j] = func[i];
func[k] = func[i];
}
pInterp = new mgcLinInterp2D<T>(3*n,theta,phi,func);
cout << "[100%] Finished initialising spherical interpolator. \n";
}
template<class T>
SphereInterpolate<T>::SphereInterpolate (int n, const sgVec2* p, const T* f)
{
// Assumes (x[i],y[i],z[i]) is unit length for all 0 <= i < n.
// For complete spherical coverage, include the two antipodal points
// (0,0,1,f(0,0,1)) and (0,0,-1,f(0,0,-1)) in the data set.
cout << "Initialising spherical interpolator.\n";
cout << "[ 0%] Allocating memory \r";
theta = new double[3*n];
phi = new double[3*n];
func = new T[3*n];
// convert data to spherical coordinates
cout << "[ 10%] copying vertices for wrap-around \r";
int i, j, k;
for (i = 0, j = n, k = 2*n; i < n; i++, j++, k++)
{
phi[i] = p[i][0];
theta[i] = p[i][1];
func[i] = f[i];
// use periodicity to get wrap-around in the Delaunay triangulation
phi[j] = phi[i];
phi[k] = phi[i];
theta[j] = theta[i]+TWOPI;
theta[k] = theta[i]-TWOPI;
func[j] = func[i];
func[k] = func[i];
}
pInterp = new mgcLinInterp2D<T>(3*n,theta,phi,func);
cout << "[100%] Finished initialising spherical interpolator. \n";
}
//---------------------------------------------------------------------------
template<class T>
SphereInterpolate<T>::~SphereInterpolate ()
{
delete pInterp;
delete[] theta;
delete[] phi;
delete[] func;
}
//---------------------------------------------------------------------------
template<class T>
void SphereInterpolate<T>::GetSphericalCoords (const double x, const double y, const double z,
double& thetaAngle,
double& phiAngle) const
{
// Assumes (x,y,z) is unit length. Returns -PI <= thetaAngle <= PI
// and 0 <= phiAngle <= PI.
if ( z < 1.0f )
{
if ( z > -1.0f )
{
thetaAngle = atan2(y,x);
phiAngle = acos(z);
}
else
{
thetaAngle = -PI;
phiAngle = PI;
}
}
else
{
thetaAngle = -PI;
phiAngle = 0.0f;
}
}
//---------------------------------------------------------------------------
template<class T>
int SphereInterpolate<T>::Evaluate (const double x, const double y, const double z, T& f) const
{
// assumes (x,y,z) is unit length
double thetaAngle, phiAngle;
GetSphericalCoords(x,y,z,thetaAngle,phiAngle);
return pInterp->Evaluate(thetaAngle,phiAngle,f);
}
//---------------------------------------------------------------------------
template<class T>
int SphereInterpolate<T>::Evaluate (const double thetaAngle, const double phiAngle, T& f) const
{
return pInterp->Evaluate(thetaAngle,phiAngle,f);
}
//---------------------------------------------------------------------------
+179
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@@ -0,0 +1,179 @@
// vector.cxx -- additional vector routines
//
// Written by Curtis Olson, started December 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include <math.h>
#include <stdio.h>
// #include <Include/fg_types.h>
#include "vector.hxx"
#include "mat3.h"
// Map a vector onto the plane specified by normal
void map_vec_onto_cur_surface_plane(MAT3vec normal, MAT3vec v0, MAT3vec vec,
MAT3vec result)
{
MAT3vec u1, v, tmp;
// calculate a vector "u1" representing the shortest distance from
// the plane specified by normal and v0 to a point specified by
// "vec". "u1" represents both the direction and magnitude of
// this desired distance.
// u1 = ( (normal <dot> vec) / (normal <dot> normal) ) * normal
MAT3_SCALE_VEC( u1,
normal,
( MAT3_DOT_PRODUCT(normal, vec) /
MAT3_DOT_PRODUCT(normal, normal)
)
);
// printf(" vec = %.2f, %.2f, %.2f\n", vec[0], vec[1], vec[2]);
// printf(" v0 = %.2f, %.2f, %.2f\n", v0[0], v0[1], v0[2]);
// printf(" u1 = %.2f, %.2f, %.2f\n", u1[0], u1[1], u1[2]);
// calculate the vector "v" which is the vector "vec" mapped onto
// the plane specified by "normal" and "v0".
// v = v0 + vec - u1
MAT3_ADD_VEC(tmp, v0, vec);
MAT3_SUB_VEC(v, tmp, u1);
// printf(" v = %.2f, %.2f, %.2f\n", v[0], v[1], v[2]);
// Calculate the vector "result" which is "v" - "v0" which is a
// directional vector pointing from v0 towards v
// result = v - v0
MAT3_SUB_VEC(result, v, v0);
// printf(" result = %.2f, %.2f, %.2f\n",
// result[0], result[1], result[2]);
}
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance from the point to the line
double fgPointLine(MAT3vec p, MAT3vec p0, MAT3vec d) {
MAT3vec u, u1, v;
double ud, dd, tmp;
// u = p - p0
MAT3_SUB_VEC(u, p, p0);
// calculate the projection, u1, of u along d.
// u1 = ( dot_prod(u, d) / dot_prod(d, d) ) * d;
ud = MAT3_DOT_PRODUCT(u, d);
dd = MAT3_DOT_PRODUCT(d, d);
tmp = ud / dd;
MAT3_SCALE_VEC(u1, d, tmp);;
// v = u - u1 = vector from closest point on line, p1, to the
// original point, p.
MAT3_SUB_VEC(v, u, u1);
return sqrt(MAT3_DOT_PRODUCT(v, v));
}
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double fgPointLineSquared(MAT3vec p, MAT3vec p0, MAT3vec d) {
MAT3vec u, u1, v;
double ud, dd, tmp;
// u = p - p0
MAT3_SUB_VEC(u, p, p0);
// calculate the projection, u1, of u along d.
// u1 = ( dot_prod(u, d) / dot_prod(d, d) ) * d;
ud = MAT3_DOT_PRODUCT(u, d);
dd = MAT3_DOT_PRODUCT(d, d);
tmp = ud / dd;
MAT3_SCALE_VEC(u1, d, tmp);;
// v = u - u1 = vector from closest point on line, p1, to the
// original point, p.
MAT3_SUB_VEC(v, u, u1);
return ( MAT3_DOT_PRODUCT(v, v) );
}
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double sgPointLineDistSquared( const sgVec3 p, const sgVec3 p0,
const sgVec3 d ) {
sgVec3 u, u1, v;
double ud, dd, tmp;
// u = p - p0
sgSubVec3(u, p, p0);
// calculate the projection, u1, of u along d.
// u1 = ( dot_prod(u, d) / dot_prod(d, d) ) * d;
ud = sgScalarProductVec3(u, d);
dd = sgScalarProductVec3(d, d);
tmp = ud / dd;
sgScaleVec3(u1, d, tmp);;
// v = u - u1 = vector from closest point on line, p1, to the
// original point, p.
sgSubVec3(v, u, u1);
return ( sgScalarProductVec3(v, v) );
}
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double sgdPointLineDistSquared( const sgdVec3 p, const sgdVec3 p0,
const sgdVec3 d ) {
sgdVec3 u, u1, v;
double ud, dd, tmp;
// u = p - p0
sgdSubVec3(u, p, p0);
// calculate the projection, u1, of u along d.
// u1 = ( dot_prod(u, d) / dot_prod(d, d) ) * d;
ud = sgdScalarProductVec3(u, d);
dd = sgdScalarProductVec3(d, d);
tmp = ud / dd;
sgdScaleVec3(u1, d, tmp);;
// v = u - u1 = vector from closest point on line, p1, to the
// original point, p.
sgdSubVec3(v, u, u1);
return ( sgdScalarProductVec3(v, v) );
}
+118
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@@ -0,0 +1,118 @@
// vector.hxx -- additional vector routines
//
// Written by Curtis Olson, started December 1997.
//
// Copyright (C) 1997 Curtis L. Olson - curt@infoplane.com
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _VECTOR_HXX
#define _VECTOR_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <simgear/compiler.h>
#include <plib/sg.h>
#include <simgear/mat3.h>
// Map a vector onto the plane specified by normal
void map_vec_onto_cur_surface_plane( MAT3vec normal,
MAT3vec v0,
MAT3vec vec,
MAT3vec result );
inline void sgmap_vec_onto_cur_surface_plane( sgVec3 normal,
sgVec3 v0,
sgVec3 vec,
sgVec3 result )
{
sgVec3 u1, v, tmp;
// calculate a vector "u1" representing the shortest distance from
// the plane specified by normal and v0 to a point specified by
// "vec". "u1" represents both the direction and magnitude of
// this desired distance.
// u1 = ( (normal <dot> vec) / (normal <dot> normal) ) * normal
sgScaleVec3( u1,
normal,
( sgScalarProductVec3(normal, vec) /
sgScalarProductVec3(normal, normal)
)
);
// printf(" vec = %.2f, %.2f, %.2f\n", vec[0], vec[1], vec[2]);
// printf(" v0 = %.2f, %.2f, %.2f\n", v0[0], v0[1], v0[2]);
// printf(" u1 = %.2f, %.2f, %.2f\n", u1[0], u1[1], u1[2]);
// calculate the vector "v" which is the vector "vec" mapped onto
// the plane specified by "normal" and "v0".
// v = v0 + vec - u1
sgAddVec3(tmp, v0, vec);
sgSubVec3(v, tmp, u1);
// printf(" v = %.2f, %.2f, %.2f\n", v[0], v[1], v[2]);
// Calculate the vector "result" which is "v" - "v0" which is a
// directional vector pointing from v0 towards v
// result = v - v0
sgSubVec3(result, v, v0);
// printf(" result = %.2f, %.2f, %.2f\n",
// result[0], result[1], result[2]);
}
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance from the point to the line
double fgPointLine(MAT3vec p, MAT3vec p0, MAT3vec d);
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double fgPointLineSquared(MAT3vec p, MAT3vec p0, MAT3vec d);
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double sgPointLineDistSquared( const sgVec3 p, const sgVec3 p0,
const sgVec3 d );
// Given a point p, and a line through p0 with direction vector d,
// find the shortest distance (squared) from the point to the line
double sgdPointLineDistSquared( const sgdVec3 p, const sgdVec3 p0,
const sgdVec3 d );
#endif // _VECTOR_HXX
+73
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@@ -0,0 +1,73 @@
#pragma comment(compiler)
#pragma comment(date)
#pragma comment(timestamp)
#include <stdlib.h>
#pragma title("antoi - char array to integer")
#pragma pagesize (80)
#pragma page(1)
/********************************************************************/
/* */
/* Title: antoi */
/* Date: Jan 28, 1991 */
/* Organization: W/OSO242 - Graphics and Display Section */
/* Programmer: Allan Darling */
/* Language: C/370 */
/* */
/* Abstract: This function will convert a character array */
/* (string) of length (len) into an integer. */
/* The integer is created via a call to the */
/* function atoi. This function extends the */
/* functionality of atoi by removing the */
/* requirement for a sentinal delimited string */
/* as input. */
/* */
/* Input: - Pointer to an array of characters. */
/* - Integer indicating the number of character to include */
/* in the conversion. */
/* */
/* Output:- An integer corresponding to the value in the character */
/* array or MAXNEG (-2147483648) if the function is */
/* unable to acquire system storage. */
/* */
/* Modification History: */
/* None */
/* */
/********************************************************************/
int antoi(char * string, int len)
{
/*******************/
/* local variables */
/*******************/
char * tmpstr;
int i,
retval;
/*****************/
/* function body */
/*****************/
tmpstr = (char *)malloc((len+1) * sizeof(char));
if (tmpstr == NULL) return (-2147483648);
for (i = 0; i < len; i++)
tmpstr[i] = string[i];
tmpstr[len] = '\0';
retval = atoi(tmpstr);
free(tmpstr);
return(retval);
} /* end antoi */
#pragma page(1)
+172
View File
@@ -0,0 +1,172 @@
#pragma comment (compiler)
//#pragma comment (date)
//#pragma comment (timestamp)
#pragma pagesize(80)
#include "Local.h" /* standard header file */
#pragma subtitle(" ")
#pragma page(1)
#pragma subtitle("charcmp - characters compare with patterns ")
/********************************************************************/
/* */
/* Title: charcmp */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 12 Dec 1995 */
/* Programmer: CINDY L. CHONG */
/* Language: C/370 */
/* */
/* Abstract: This function will compare each character in the */
/* string match with each character in the pattern */
/* which is made up of characters. The str can */
/* be longer than the pattern. */
/* */
/* External Functions Called: */
/* None. */
/* */
/* Input: str is a pointer to char */
/* pattern is a pointer to char */
/* */
/* Output: Return true if str matches pattern, */
/* otherwise, return false */
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
bool charcmp(char *str, char *pattern)
{
/**********************************************************/
/* Loop while str and pattern is not equal to null, then */
/* inscreases str and pattern by one */
/**********************************************************/
for (; *pattern != '\0'; pattern++)
{
if (*str == '\0')
return FALSE;
/************************************************************/
/* If pattern match str, then increase str and jump out the */
/* case and read next char of the str and pattern */
/************************************************************/
if ( isspace(*pattern) )
pattern = nxtalpha(pattern);
switch( *pattern )
{
case 'c':
if ( !isalnum(*str++) )
{
return FALSE;
}
break;
case 'a':
if ( !isalpha(*str) )
{
return FALSE;
}
str++;
break;
case 'n':
if ( !iscntrl(*str++) )
{
return FALSE;
}
break;
case 'd':
if ( !isdigit(*str) )
{
return FALSE;
}
str++;
break;
case 'g':
if ( !isgraph(*str++) )
{
return FALSE;
}
break;
case 'i':
if ( !islower(*str++) )
{
return FALSE;
}
break;
case 'p':
if ( !isprint(*str++) )
{
return FALSE;
}
break;
case 't':
if ( !ispunct(*str++) )
{
return FALSE;
}
break;
case 'w':
if ( !isspace(*str++) )
{
return FALSE;
}
break;
case 'u':
if ( !isupper(*str++) )
{
return FALSE;
}
break;
case 's':
if (*str++ != ' ')
{
return FALSE;
}
break;
case 'm':
if ( !isspace(*str) )
{
return FALSE;
}
else
{
while ( isspace(*str) )
str++;
}
break;
case '\'':
pattern++;
if (*pattern != *str)
{
return FALSE;
}
pattern++;
str++;
break;
default:
return FALSE;
} /* end switch */
} /* end for */
return (TRUE);
}
File diff suppressed because it is too large Load Diff
File diff suppressed because it is too large Load Diff
+544
View File
@@ -0,0 +1,544 @@
#include "Metar.h"
#pragma page(1)
#pragma subtitle(" ")
#pragma subtitle("subtitle - description ")
/********************************************************************/
/* */
/* Title: dRVMETAR */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 28 Oct 1994 */
/* Programmer: CARL MCCALLA */
/* Language: C/370 */
/* */
/* Abstract: DRVMETAR is a main routine that acts a driver */
/* for testing the METAR Decoder function. */
/* */
/* External Functions Called: */
/* None. */
/* DcdMETAR */
/* prtDcdMetar */
/* Sec0MTSm */
/* Sec1MTSm */
/* */
/* Input: None */
/* */
/* Output: None */
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
main()
{
char bltn_prefix[20];
static char *string[] =
{
"KAST 221156Z COR 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KAST COR 221156Z 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KAST COR 221156Z 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KP88 COR 221156 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KP88 COR 221156 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 6//// 70109 T00890084 10100 20089 55005",
NULL,
"EPIT 1755 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1/2V3/4",
"KFAR 181154Z 10003KT 1/4SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 10345 20226 T01610133 $",
"KFAR 181154Z 10003KT 1/SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 10345 20226 T01610133 $",
"RKSS 21009KT 1400 RP2000 // ////// 21/20 1006/2972 NOSIG",
"RKSS 1200 21009KT 1400 RP2000 // ////// 21/20 1006/2972 NOSIG",
"RKSS 1130Z 23011KT 1100 R14R/P1500N R14L/P1500N BR SCT010 BKN030 "
"BKN080 21/21 Q1006 NOSIG",
"RKSS 1130Z 23011KT 1100 R14R/P1500 R14L/P1500 BR SCT010 BKN030 "
"BKN080 21/21 Q1006 NOSIG",
NULL,
"KFAR 181154Z 10003KT 4SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 1//// 2//// T01610133 $",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE10 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE9 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE FZDZE10 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE FZDZE9 LO CLD SLP186",
"MKJP 1400Z 13011KT 9999 FEW022 30/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 M30/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/30 Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/M30 Q1015",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 BKN045 OVC090 "
"SCT120 FEW250 RMK OCNL LTGICCG OHD",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 07/01 Q1011 "
"RMK TEMPO 8000 -SHRA BKN015 FRQ LTG VC",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 07/01 Q1011 "
"RMK TEMPO 8000 -SHRA BKN015 LTG DSNT W",
"METAR KLAX 281156Z AUTO VRB100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT FC "
"+TS BLPY FEW/// SCT000 BKN050 SCT150 OVC250 3/M1 A2991 RMK "
"TORNADO B13E45 6 NE MOV E A02 PK WND 18515/45 "
"WSHFT 1350 FROPA TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"VIS 2 1/2 RY11 "
"DVR/1000V1600FT "
"OCNL LTG VCY STN "
"RAB1030E1145 FZDZE56 BLPYE57 CIG 1000V1500 CIG 020 RY11 "
"PRESFR PRESRR SLP013 FG FEW/// HZ SCT000 VIS NW 2 1/2 GR 3/4 "
"VIRGA SE -XRAFG3 CIGE005 BKN014 V OVC "
"FU BKN020 NOSPECI LAST 8/365 SNINCR 2/10 4/178 "
"933125 98096 P 0125 60225 70565 "
"T00261015 10369 21026 "
"404800360 52101 VISNO RY05 CHINO RY27 PNO RVRNO "
"PWINO FZRANO TSNO $",
"KBOS 251356Z 26011KT 10SM CLR 12/02 A2995 RMK AO2 SC VCNTY "
"STN SSE-NNW SCT CI ABV SLP141 T01220023",
"EFHK 36009KT 340V060 CAVOK 12/M02 Q1013 NOSIG",
"EGKK 24011KT 210V300 9999 SCT020 BKN045 12/06 Q1007 NOSIG",
"EGPD 31018KT 8000 RA FEW013 BKN021 OVC045 06/04 Q0994 NOSIG",
"EKCH 16012KT CAVOK 20/07 Q1006 NOSIG",
"ESKN 10014KT 9000 BR SCT100 14/04 Q1010",
"LOWW 231450Z 14017KT CAVOK 23/07 Q1010 NOSIG",
"METAR CYCH 171500Z CCA 30017KT 2SM -SN BKN006",
"METAR CYOW 171500Z CCA 30017KT 2SM -SN BKN006 OVC020 00/M02 "
"A2957 RMK S35F4NS1 /S01/ SNW WET SNW MELTG ON GRND CIG 5-7 "
"SLP018",
"KAST 221156Z AUTO 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005"
" TSB0159E30 TS SE MOV NE",
"KAST 221156Z AUTO 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005"
" TSE0159 TS SE",
"KHVR 1756Z 31007KT 5SM -SN SCT011 BKN024 OVC030 M05/M08 A3056 "
"RMK AOA 933004 "
"BKN V SCT TNO PCPN 000 $ SLP389 4/015 60002 "
"T10501077 11050 21078 51010",
"SPECI KGFI 041420Z AUTO 18030KT 3 1/2SM RVRNO TS -RA BKN008 OVC060 "
"26/22 A2991 RMK A02 RA15TSB20 PRESFR SLP 101 P 0000 T02640218",
"METAR KCLE 281156Z 170100G135KT 110V180 M1/4SM "
"R01L/P6000FT +TSSHRA VCFG "
"BKN025 SCT100 OVC200 M26/ A2991 RMK PK WND 18515/45 A02 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"CIG 1000V1500 PRESFR FRQ LTG CG NW "
"RAB1030E1145 FZDZE56 PRESRR SLP135 GS "
"T1263 "
"VIRGA NW 8/365 4/178 P 0125 60225 7//// 70565 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"CYQR 161700Z 15015KT 15SM SCT045 SCT090 BKN250 10/03 A2955 "
"RMK SC1AC2C11 OB TAKEN H+ 5 DUE AWOS FAILURE SLP027",
"KPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 199/182",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP701 P0254 199/182",
"KHLN 281156Z AUTO 27005KT 10SM OVC023 07/05 A3011 RMK AOA OVC V "
"BKN $ SLP202 60000 70001 T00670050 10122 20061 53003",
"KPHX 281156Z 12004KT 10SM CLR 15/05 A2996 RMK AOA SLP135 T01500050 "
"10250 20150 53006",
"KFCA 281156Z 30003KT 10SM CLR 06/02 A3009 RMK AO TNO $ SLP191 "
"T00610023 10167 20056 53003",
"KAST 281156Z 00000KT 10SM BKN095 09/08 A2997 RMK AOA SLP150 "
"T00940084 10161 20094 52005 ",
"KHVR 281156Z 03003KT 10SM OVC020 09/07 A3010 RMK AO TNO ZRNO "
"$ SLP194 T00940073 10156 20089 51005",
"KGGW 281156Z 35006KT 5SM BR OVC010 10/09 A3003 RMK AOA $ SLP177 "
"70003 T01000095 10156 20110 53008",
"KELY 1153Z AUTO 14004KT 10SM SCT075 01/M01 A3011 RMK AOA TNO ZRNO "
"SLP171 70001 T00061011 10139 21006 51005",
"KFLG 281156Z 29006KT 10SM CLR 04/M01 A3012 RMK AO TNO SLP147 "
"T00391011 21006 51004",
"KGTF 281156Z 27005KT 7SM BKN080 04/04 A3010 RMK AOA SLP205 "
"T00440045 10117 20039 51006",
"K13A 1918Z 20011KT 26/M06 RMK AO PKWND 020/RNO 644V264 T02611061",
"KP88 1919Z 09001KT 14/03 RMK AO / PKWND 002/RNO 158 Z T01440034",
"K40B 1924Z 29004KT 15/M07 RMK AO PKWND 011/RM MV263 T01501072",
"KGGW 1756Z 33018KT 10SM OVC015 M03/M06 A3041 RMK AOA SLP338 "
"4/007 60002 T10281055 11028 21072 51009",
"KPHX 1756Z 130004KT 10SM CLR 18/M03 A3001 RMK AOA SLP154 "
"T01781033 10178 20067 58007",
"KFCA 1756Z 29005KT 10SM CLR 05/M11 A3049 RMK AOA TNO SLP352 "
"T00501111 10050 21044 50004",
"KAST 1756Z 01006KT 10SM CLR 11/04 A3047 RMK AOA SLP316 "
"T01110045 10111 20000 50002",
"KELY 1753Z 34010KT 10SM CLR 01/M07 A3022 RMK AOA TNO ZRNO "
"SLP240 T00111066 10011 21078 58007",
"KFLG 1756Z 07006KT 10SM CLR 06/M12 A3009 RMK AO TNO ZRNO "
"SLP178 T00561122 10061 21100 58005",
"KGTF 1756Z 35010KT 1/2SM -SN FG VV09 M06/M08 A3051 RMK AOA "
"933004 SFC VSBY 3/4 "
"PCPN M SLP393 60010 T10611077 11044 21067 53013",
"KHLN 1756Z 35012KT 10SM SCT032 OVC060 M02/M09 A3048 RMK AOA "
"SLP369 60000 T10171094 11017 21061 53006",
"KAST 1756Z 01006KT 10SM CLR 11/04 A3047 RMK AOA SLP316 61104 "
"71235 T01110045 10111 20000 401720056 58002",
"METAR KLAX 04281156Z AUTO VRB100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT FC "
"+TS BLPY FEW000 BKN050 SCT150 OVC250 3/M1 A2991 RMK "
"TORNADO B13 DSNT NE A02 PK WND 18515/45 "
"WSHFT 1350 FROPA TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"VIS 2 1/2 RY11 OCNL LTG VCY STN "
"RAB1030E1145 FZDZE56 BLPYE57 CIG 1000V1500 CIG 020 RY11 "
"PRESFR PRESRR SLP013 FG FEW000 VIS NW2 1/2 GR 3/4 "
"VIRGA SE -XRAFG3 CIGE005 BKN014 V OVC "
"FU BKN020 NOSPECI LAST 8/365 SNINCR 2/10 4/178 "
"933125 98096 P 0125 60225 70565 "
"T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 17012KT 130V210 3 1/2SM R15L/0500FT -RA "
"SCT050 OVC110 26/18 A2991 RMK FUNNEL CLOUDS A02 RAB30 "
"SLP 101 GR M1/4 VIRGA SCT V BKN P 0010 T02640178",
"METAR KGFI 041356Z AUTO 05008KT 10SM R15L/P6000FT CLR A2991 "
"RMK WATERSPOUTS VCY STN NW A02 SLP 101 10288 20243 52021 $ ",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 OCNL LTG AP "
"RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 T01990182",
"KABE 281900Z NIL",
"METAR KPIT NIL",
"METAR KCLE 04281156Z 170100G135KT 110V180 M1/4SM "
"R01L/P6000FT +TSSHRA VCFG "
"BKN025 SCT100 OVC200 M26/ A2991 RMK PK WND 18515/45 A02 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"CIG 1000V1500 PRESFR FRQ LTG CG NW "
"RAB1030E1145 FZDZE56 PRESRR SLP135 GS "
"T1263 "
"VIRGA NW 8/365 4/178 P 0125 60225 7//// 70565 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KPHL 040256Z AUTO 170100G135KT 130V210 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 LTG DSNT "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP037 GR 2 3/4 "
"VIRGA E 8/365 4/178 P 0125 70565 21026 T0263 10369 60225 "
"404800360 52101 PWINO FZRANO TSNO $",
"SPECI KGFI 041420Z AUTO 18030KT 2 1/2SM RVRNO TS -RA BKN008 "
"OVC060 25/22 A2991 RMK A02 LTG DSNT W "
"RAB15TSB20 PRESFR SLP101 P 0000 "
"254/218",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR M1/4 "
"VIRGA SE 8/365 4/178 P 0125 6//// 60225 70565 T0263 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 6//// 60225 70565 T0263 10369 21026 "
"VIRGA 35 8/365 4/178 P 0125 21026 70565 10369 60225 T0263 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 3/M1 A2991 RMK A02 PK WND 18515/45 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 60225 70565 T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 3/M1 A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 60225 70565 T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO",
"METAR KGFI 041356Z AUTO 05008KT 10SM R15L/P6000FT CLR A2991 RMK "
"A02 SLP 101 10288 20243 52021",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 M199/M182",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 M199/182",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 199/M182",
"METAR APIT 171755Z AUTO 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 4/369 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 8/563 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 SLP875 SGB1213E1225",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK SLP056 "
"RAE0123",
"SPECI APIT 171755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 8/321 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 SLP875 FGB1713",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 SLP875",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 1/2 SLP875",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 1/2 SLP875",
"EGPF 1720Z 00000KT 9999 -SHRA STC014 SCT020CB BNK024 12/09 "
"Q1003 NOSIG",
"NZAA 1700Z 03010KT 30KM 03 5CU022 7SC035 11/07 Q1006.5 NOSIG",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK KAUKAU 30050KT",
"DGAA 1800Z 22012KT 9999 SCT009 BKN120 25/21 Q1015",
"DAAT 1830Z 30010KT CAVOK 29/06 Q1019",
"GQPP 1800Z 34023KT 3000 DRSA SKC 24/20 Q1011 NSG",
"DAAG 1830Z 06006KT 9999 SCT020 25/22 Q1015",
"DABB 1830Z 04010KT 9999 SCT030TCU SCT033CB 27/18 Q1017",
"DABC 1830Z 00000KT 9999 SCT026TCU SCT036CB 22/18 Q1020 RETS",
"NZAA 1700Z 03010KT 30KM 03 5CU022 7SC035 11/07 Q1006.5 NOSIG",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK K",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK KAUKAU 30050KT",
"DGAA 1800Z 22012KT 9999 SCT009 BKN120 25/21 Q1015",
"GFLL 1900Z NIL",
"GOOY 1800Z 03006G17KT 340V080 6000 TSRA BKN016 BKN030CB "
"BKN133 26/23 Q1013 NOSIG",
"GCXO 1930Z 32018KT 8000 SCT003 SCT007 18/16 Q1019",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2",
"BPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2",
"CPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 1/2",
"DPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 1/2",
"FPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 3/4V2 1/2",
"GPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 3/4V3",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB MM/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB MM/16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/MM A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/MM A2992",
NULL};
/***************************/
/* DECLARE LOCAL VARIABLES */
/***************************/
Decoded_METAR Metar;
Decoded_METAR *Mptr = &Metar;
int j,
ErReturn;
static char *synopRTRN = NULL;
/***************************************************/
/* START BODY OF MAIN ROUTINE FOR CALLING DcdMETAR */
/***************************************************/
j = 0;
while( string[j] != NULL)
{
/*-- PRINT INPUT METAR REPORT ----------------------------*/
printf("INPUT METAR REPORT: %s\n",string[j] );
/*-- DECODE INPUT REPORT ---------------------------------*/
if ( (ErReturn = DcdMETAR( string[ j ], Mptr )) != 0 )
printf("DcdMETAR: Error Return Number: %d\n",ErReturn);
/*-- PRINT DECODED METAR REPORT ELEMENTS -----------------*/
prtDMETR( Mptr );
j++;
}
}
+63
View File
@@ -0,0 +1,63 @@
#include "Local.h" /* standard header file */
#include "Metar.h"
#pragma subtitle(" ")
#pragma page(1)
#pragma subtitle("subtitle - description ")
/********************************************************************/
/* */
/* Title: fracPart */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 13 Jun 1995 */
/* Programmer: CARL MCCALLA */
/* Language: C/370 */
/* */
/* Abstract: Convert a character string fraction into a */
/* decimal (floating point) number. */
/* */
/* External Functions Called: */
/* None. */
/* */
/* Input: string - a pointer to a character string frac- */
/* tion. */
/* Output: A decimal (floating point) number. */
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
float fracPart( char *string )
{
/***************************/
/* DECLARE LOCAL VARIABLES */
/***************************/
char buf[ 6 ],
*slash;
float numerator,
denominator;
/*************************/
/* START BODY OF ROUTINE */
/*************************/
slash = strchr(string, '/');
memset(buf , '\0', 6);
strncpy( buf, string, slash-string);
numerator = (float) atoi(buf);
memset(buf , '\0', 6);
strcpy( buf, slash+1);
denominator = (float) atoi(buf);
return (numerator/denominator);
}
File diff suppressed because it is too large Load Diff
+305
View File
@@ -0,0 +1,305 @@
# Generated automatically from Makefile.in by configure.
# Makefile.in generated automatically by automake 1.3 from Makefile.am
# Copyright (C) 1994, 1995, 1996, 1997, 1998 Free Software Foundation, Inc.
# This Makefile.in is free software; the Free Software Foundation
# gives unlimited permission to copy and/or distribute it,
# with or without modifications, as long as this notice is preserved.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY, to the extent permitted by law; without
# even the implied warranty of MERCHANTABILITY or FITNESS FOR A
# PARTICULAR PURPOSE.
SHELL = /bin/sh
srcdir = .
top_srcdir = ../..
prefix = /h/curt
exec_prefix = ${prefix}
bindir = /h/curt/bin/Linux
sbindir = ${exec_prefix}/sbin
libexecdir = ${exec_prefix}/libexec
datadir = ${prefix}/share
sysconfdir = ${prefix}/etc
sharedstatedir = ${prefix}/com
localstatedir = ${prefix}/var
libdir = ${exec_prefix}/lib
infodir = ${prefix}/info
mandir = ${prefix}/man
includedir = ${prefix}/include
oldincludedir = /usr/include
DISTDIR =
pkgdatadir = $(datadir)/FlightGear
pkglibdir = $(libdir)/FlightGear
pkgincludedir = $(includedir)/FlightGear
top_builddir = ../..
ACLOCAL = aclocal
AUTOCONF = autoconf
AUTOMAKE = automake
AUTOHEADER = autoheader
INSTALL = /usr/bin/install -c
INSTALL_PROGRAM = ${INSTALL}
INSTALL_DATA = ${INSTALL} -m 644
INSTALL_SCRIPT = ${INSTALL_PROGRAM}
transform = s,x,x,
NORMAL_INSTALL = :
PRE_INSTALL = :
POST_INSTALL = :
NORMAL_UNINSTALL = :
PRE_UNINSTALL = :
POST_UNINSTALL = :
CC = egcc
CXX = c++
LN_S = ln -s
MAKEINFO = /h/curt/projects/FlightGear-0.7/missing makeinfo
PACKAGE = FlightGear
RANLIB = ranlib
VERSION = 0.7.2
audio_LIBS = -lsl -lsm
base_LIBS = -lm
opengl_LIBS = -lglut -lMesaGLU -lMesaGL -lXmu -lXt -lSM -lICE -lXi -lXext -lX11 -lm
noinst_LIBRARIES = libMetar.a
libMetar_a_SOURCES = \
Antoi.cpp Charcmp.cpp Dcdmetar.cpp Dcdmtrmk.cpp Drvmetar.c \
Fracpart.cpp Local.h Metar.h \
MetarReport.cpp MetarReport.h \
MetarStation.cpp MetarStation.h \
Prtdmetr.cpp Stspack2.cpp Stspack3.cpp
mkinstalldirs = $(SHELL) $(top_srcdir)/mkinstalldirs
CONFIG_HEADER = ../../Include/config.h
CONFIG_CLEAN_FILES =
LIBRARIES = $(noinst_LIBRARIES)
DEFS = -DHAVE_CONFIG_H -I. -I$(srcdir) -I../../Include
CPPFLAGS = -I/usr/local/include -I/usr/local/plib/include -I/usr/X11R6/include
LDFLAGS = -L/h/curt/lib -L/usr/local/lib -L/usr/local/plib/lib -L/usr/X11R6/lib
LIBS = -lm
X_CFLAGS = -I/usr/X11R6/include
X_LIBS = -L/usr/X11R6/lib
X_EXTRA_LIBS =
X_PRE_LIBS = -lSM -lICE
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+265
View File
@@ -0,0 +1,265 @@
#ifndef METARX
#define METARX
/********************************************************************/
/* */
/* Title: METAR H */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 19 Jan 1996 */
/* Programmer: CARL MCCALLA */
/* Language: C/370 */
/* */
/* Abstract: METAR Decoder Header File. */
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#include "Local.h" /* standard header file */
/*********************************************/
/* */
/* RUNWAY VISUAL RANGE STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/*********************************************/
typedef struct runway_VisRange {
char runway_designator[6];
bool vrbl_visRange;
bool below_min_RVR;
bool above_max_RVR;
int visRange;
int Max_visRange;
int Min_visRange;
} Runway_VisRange;
/***********************************************/
/* */
/* DISPATCH VISUAL RANGE STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/***********************************************/
typedef struct dispatch_VisRange {
bool vrbl_visRange;
bool below_min_DVR;
bool above_max_DVR;
int visRange;
int Max_visRange;
int Min_visRange;
} Dispatch_VisRange;
/*****************************************/
/* */
/* CLOUD CONDITION STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/*****************************************/
typedef struct cloud_Conditions {
char cloud_type[5];
char cloud_hgt_char[4];
char other_cld_phenom[4];
int cloud_hgt_meters;
} Cloud_Conditions;
/*****************************************/
/* */
/* WIND GROUP DATA STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/*****************************************/
typedef struct windstruct {
char windUnits[ 4 ];
bool windVRB;
int windDir;
int windSpeed;
int windGust;
} WindStruct;
/*****************************************/
/* */
/* RECENT WX GROUP STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/*****************************************/
typedef struct recent_wx {
char Recent_weather[ 5 ];
int Bhh;
int Bmm;
int Ehh;
int Emm;
} Recent_Wx;
/***************************************/
/* */
/* DECODED METAR STRUCTURE DECLARATION */
/* AND VARIABLE TYPE DEFINITION */
/* */
/***************************************/
typedef struct decoded_METAR {
char synoptic_cloud_type[ 6 ];
char snow_depth_group[ 6 ];
char codeName[ 6 ];
char stnid[5];
char horiz_vsby[5];
char dir_min_horiz_vsby[3];
char vsby_Dir[ 3 ];
char WxObstruct[10][8];
char autoIndicator[5];
char VSBY_2ndSite_LOC[10];
char SKY_2ndSite_LOC[10];
char SKY_2ndSite[10];
char SectorVsby_Dir[ 3 ];
char ObscurAloft[ 12 ];
char ObscurAloftSkyCond[ 12 ];
char VrbSkyBelow[ 4 ];
char VrbSkyAbove[ 4 ];
char LTG_DIR[ 3 ];
char CloudLow;
char CloudMedium;
char CloudHigh;
char CIG_2ndSite_LOC[10];
char VIRGA_DIR[3];
char TornadicType[15];
char TornadicLOC[10];
char TornadicDIR[4];
char TornadicMovDir[3];
char CHINO_LOC[6];
char VISNO_LOC[6];
char PartialObscurationAmt[2][7];
char PartialObscurationPhenom[2][12];
char SfcObscuration[6][10];
char charPrevailVsby[12];
char charVertVsby[10];
char TS_LOC[3];
char TS_MOVMNT[3];
bool Indeterminant3_6HrPrecip;
bool CIGNO;
bool SLPNO;
bool ACFTMSHP;
bool NOSPECI;
bool FIRST;
bool LAST;
bool SunSensorOut;
bool AUTO;
bool COR;
bool NIL_rpt;
bool CAVOK;
bool RVRNO;
bool A_altstng;
bool Q_altstng;
bool VIRGA;
bool VOLCASH;
bool GR;
bool CHINO;
bool VISNO;
bool PNO;
bool PWINO;
bool FZRANO;
bool TSNO;
bool DollarSign;
bool PRESRR;
bool PRESFR;
bool Wshft_FROPA;
bool OCNL_LTG;
bool FRQ_LTG;
bool CNS_LTG;
bool CG_LTG;
bool IC_LTG;
bool CC_LTG;
bool CA_LTG;
bool DSNT_LTG;
bool AP_LTG;
bool VcyStn_LTG;
bool OVHD_LTG;
bool LightningVCTS;
bool LightningTS;
int TornadicDistance;
int ob_hour;
int ob_minute;
int ob_date;
int minWnDir;
int maxWnDir;
int VertVsby;
int temp;
int dew_pt_temp;
int QFE;
int hectoPasc_altstng;
int char_prestndcy;
int minCeiling;
int maxCeiling;
int WshfTime_hour;
int WshfTime_minute;
int min_vrbl_wind_dir;
int max_vrbl_wind_dir;
int PKWND_dir;
int PKWND_speed;
int PKWND_hour;
int PKWND_minute;
int SKY_2ndSite_Meters;
int Ceiling;
int Estimated_Ceiling;
int SNINCR;
int SNINCR_TotalDepth;
int SunshineDur;
int ObscurAloftHgt;
int VrbSkyLayerHgt;
int Num8thsSkyObscured;
int CIG_2ndSite_Meters;
int snow_depth;
int BTornadicHour;
int BTornadicMinute;
int ETornadicHour;
int ETornadicMinute;
float SectorVsby;
float WaterEquivSnow;
float VSBY_2ndSite;
float prevail_vsbySM;
float prevail_vsbyM;
float prevail_vsbyKM;
float prestndcy;
float precip_amt;
float precip_24_amt;
float maxtemp;
float mintemp;
float max24temp;
float min24temp;
float minVsby;
float maxVsby;
float hourlyPrecip;
float TWR_VSBY;
float SFC_VSBY;
float Temp_2_tenths;
float DP_Temp_2_tenths;
float SLP;
float GR_Size;
double inches_altstng;
Runway_VisRange RRVR[12];
Dispatch_VisRange DVR;
Recent_Wx ReWx[3];
WindStruct winData;
Cloud_Conditions cldTypHgt[6];
} Decoded_METAR;
#define MAXWXSYMBOLS 10 /*-- NOT TO EXCEED 10 PRES. WX GRPS --*/
#define MAXTOKENS 500 /*-- RPT NOT TO EXCEED 500 GRPS --*/
void prtDMETR( Decoded_METAR *Mptr );
int DcdMETAR( char *string, Decoded_METAR *Mptr );
#endif
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// Metar report implementation class code
#include "MetarReport.h"
#include "Metar.h"
CMetarReport::CMetarReport(
char *s ) :
m_DecodedReport( 0 )
{
m_DecodedReport = new Decoded_METAR;
DcdMETAR( s, (Decoded_METAR *)m_DecodedReport );
}
CMetarReport::~CMetarReport()
{
}
static int DecodeDirChars( char* c )
{
int r = 0;
if ( c[0] )
{
if ( c[0] == 'E' ) r = 90;
else if ( c[0] == 'S' ) r = 180;
else if ( c[0] == 'W' ) r = 270;
if ( r == 0 )
{
if ( c[1] == 'E' ) r = 45;
else if ( c[1] == 'W' ) r = 315;
}
else if ( r = 180 )
{
if ( c[1] == 'E' ) r = 135;
else if ( c[1] == 'W' ) r = 225;
}
}
return r;
}
char *CMetarReport::StationID()
{
return ((Decoded_METAR *)m_DecodedReport)->stnid;
}
int CMetarReport::WindDirection()
{
return ((Decoded_METAR *)m_DecodedReport)->winData.windDir;
}
int CMetarReport::WindSpeed()
{
return ((Decoded_METAR *)m_DecodedReport)->winData.windSpeed;
}
int CMetarReport::WindGustSpeed()
{
return ((Decoded_METAR *)m_DecodedReport)->winData.windGust;
}
int CMetarReport::LightningDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->LTG_DIR );
}
char CMetarReport::CloudLow()
{
return ((Decoded_METAR *)m_DecodedReport)->CloudLow;
}
char CMetarReport::CloudMedium()
{
return ((Decoded_METAR *)m_DecodedReport)->CloudMedium;
}
char CMetarReport::CloudHigh()
{
return ((Decoded_METAR *)m_DecodedReport)->CloudHigh;
}
int CMetarReport::VirgaDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->VIRGA_DIR );
}
int CMetarReport::TornadicDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->TornadicDIR );
}
int CMetarReport::TornadicMovementDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->TornadicMovDir );
}
int CMetarReport::ThunderStormDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->TS_LOC );
}
int CMetarReport::ThunderStormMovementDirection()
{
return DecodeDirChars( ((Decoded_METAR *)m_DecodedReport)->TS_MOVMNT );
}
bool CMetarReport::Virga()
{
return ((Decoded_METAR *)m_DecodedReport)->VIRGA;
}
bool CMetarReport::VolcanicAsh()
{
return ((Decoded_METAR *)m_DecodedReport)->VOLCASH;
}
bool CMetarReport::Hail()
{
return ((Decoded_METAR *)m_DecodedReport)->GR;
}
bool CMetarReport::OccationalLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->OCNL_LTG;
}
bool CMetarReport::FrequentLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->FRQ_LTG;
}
bool CMetarReport::ContinuousLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->CNS_LTG;
}
bool CMetarReport::CloudToGroundLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->CG_LTG;
}
bool CMetarReport::InterCloudLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->IC_LTG;
}
bool CMetarReport::CloudToCloudLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->CC_LTG;
}
bool CMetarReport::CloudToAirLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->CA_LTG;
}
bool CMetarReport::DistantLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->DSNT_LTG;
}
bool CMetarReport::AirportLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->AP_LTG;
}
bool CMetarReport::VicinityLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->VcyStn_LTG;
}
bool CMetarReport::OverheadLightning()
{
return ((Decoded_METAR *)m_DecodedReport)->OVHD_LTG;
}
int CMetarReport::Temperature()
{
return ((Decoded_METAR *)m_DecodedReport)->temp;
}
int CMetarReport::DewpointTemperature()
{
return ((Decoded_METAR *)m_DecodedReport)->dew_pt_temp;
}
int CMetarReport::VerticalVisibility() // Meters
{
return ((Decoded_METAR *)m_DecodedReport)->VertVsby;
}
int CMetarReport::Ceiling()
{
return FEET_TO_METER * ((Decoded_METAR *)m_DecodedReport)->Ceiling;
}
int CMetarReport::EstimatedCeiling()
{
return FEET_TO_METER * ((Decoded_METAR *)m_DecodedReport)->Estimated_Ceiling;
}
int CMetarReport::VariableSkyLayerHeight()
{
return FEET_TO_METER * ((Decoded_METAR *)m_DecodedReport)->VrbSkyLayerHgt;
}
int CMetarReport::SnowDepthInches()
{
return ((Decoded_METAR *)m_DecodedReport)->snow_depth;
}
std::ostream&
operator << ( ostream& out, CMetarReport& p )
{
return out
<< "StationID " << p.StationID()
<< " WindDirection " << p.WindDirection()
<< " WindSpeed " << p.WindSpeed()
<< " WindGustSpeed " << p.WindGustSpeed() << std::endl
<< "CloudLow " << p.CloudLow()
<< " CloudMedium " << p.CloudMedium()
<< " CloudHigh " << p.CloudHigh() << std::endl
<< "TornadicDirection " << p.TornadicDirection()
<< " TornadicMovementDirection " << p.TornadicMovementDirection() << std::endl
<< "ThunderStormDirection " << p.ThunderStormDirection()
<< " ThunderStormMovementDirection " << p.ThunderStormMovementDirection() << std::endl
<< "Virga " << p.Virga()
<< " VirgaDirection " << p.VirgaDirection() << std::endl
<< "VolcanicAsh " << p.VolcanicAsh() << std::endl
<< "Hail " << p.Hail() << std::endl
<< "LightningDirection " << p.LightningDirection()
<< " OccationalLightning " << p.OccationalLightning()
<< " FrequentLightning " << p.FrequentLightning()
<< " ContinuousLightning " << p.ContinuousLightning() << std::endl
<< "CloudToGroundLightning " << p.CloudToGroundLightning()
<< " InterCloudLightning " << p.InterCloudLightning()
<< " CloudToCloudLightning " << p.CloudToCloudLightning()
<< " CloudToAirLightning " << p.CloudToAirLightning() << std::endl
<< "DistantLightning " << p.DistantLightning()
<< " AirportLightning " << p.AirportLightning()
<< " VicinityLightning " << p.VicinityLightning()
<< " OverheadLightning " << p.OverheadLightning() << std::endl
<< "VerticalVisibility " << p.VerticalVisibility() << std::endl // Meters
<< "Temperature " << p.Temperature()
<< " DewpointTemperature " << p.DewpointTemperature() << std::endl
<< "Ceiling " << p.Ceiling()
<< " EstimatedCeiling " << p.EstimatedCeiling()
<< " VariableSkyLayerHeight " << p.VariableSkyLayerHeight() << std::endl
<< "SnowDepthInches " << p.SnowDepthInches() << std::endl
;
}
void CMetarReport::dump()
{
prtDMETR( (Decoded_METAR *)m_DecodedReport );
}
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// Class encapulating the metar report information
//
// Individual METAR reports are found in this directory:
// ftp://weather.noaa.gov/data/observations/metar/stations
//
#ifndef _MetarReport_
#define _MetarReport_
#include <iostream>
#include <string>
#include <vector>
#include <Math/point3d.hxx>
#include <Math/polar3d.hxx>
class CMetarReport
{
// Typedefs, enumerations
// Attributes
private:
void *m_DecodedReport;
// A void pointer which is cast to the correct type in the cpp file.
// I don't want the ugly metar structure and header files dragged into
// every report user program file.
// Probably should be a smart pointer if copy constructor and assignment
// is allowed.
// Operations
public:
CMetarReport(
char *s );
// Constructor
~CMetarReport();
// Destructor
char *StationID();
// Directions in degrees
// Speed in knots
// Altitude in meters
// Temperature in centigrade
int WindDirection();
int WindSpeed();
int WindGustSpeed();
// Add cloud more cloud info...
// Cloud code characters...
char CloudLow();
char CloudMedium();
char CloudHigh();
bool Virga();
int VirgaDirection();
int TornadicDirection();
int TornadicMovementDirection();
int ThunderStormDirection();
int ThunderStormMovementDirection();
bool VolcanicAsh();
bool Hail();
int LightningDirection();
bool OccationalLightning();
bool FrequentLightning();
bool ContinuousLightning();
bool Lightning()
{
return OccationalLightning() || FrequentLightning() || ContinuousLightning();
}
bool CloudToGroundLightning();
bool InterCloudLightning();
bool CloudToCloudLightning();
bool CloudToAirLightning();
bool DistantLightning();
bool AirportLightning();
bool OverheadLightning();
bool VicinityLightning();
int Temperature();
int DewpointTemperature();
int VerticalVisibility();
int Ceiling();
int EstimatedCeiling();
int VariableSkyLayerHeight();
int SnowDepthInches();
void dump();
private:
CMetarReport(
const CMetarReport &rNewObj );
// Copy constructor. Not implemented.
CMetarReport &operator =(
const CMetarReport &rObj );
// Assignment operator. Not implemented.
};
std::ostream& operator << ( std::ostream&, CMetarReport& );
#endif
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// Metar station implementation code
#include <stdio.h>
#include "MetarStation.h"
#include <algorithm>
#define TESTPROG
#ifndef TESTPROG
// options is too tightly integrated into FlightGear to use in a test program
#include <Main/options.hxx>
#endif
#include <Misc/fgpath.hxx>
std::vector< CMetarStation *> METAR_Stations;
int CMetarStation::initialized( CMetarStation::initialize() );
std::string CMetarStation::tempName;
double CMetarStation::decodeDMS( char *b )
{
double r = 0;
double m = 0;
double s = 0;
if ( *b )
{
// Degrees
r = (*b - '0') * 10.0; b++;
r += (*b - '0'); b++;
if ( *b != '-' )
{
r *= 10;
r += (*b - '0'); b++;
}
b++;
// Minutes
m = (*b - '0') * 10.0; b++;
m += (*b - '0'); b++;
r += m/60.0;
if ( *b == '-' )
{
// Seconds
b++;
s = (*b - '0') * 10.0; b++;
s += (*b - '0'); b++;
}
r += s/3600.0;
// Direction (E W N S)
if ( *b == 'W' || *b == 'S' ) r = -r;
}
return r * DEG_TO_RAD;
}
CMetarStation::CMetarStation(
char *s )
{
char *t;
t = strchr( s, ';' ); *t = 0; t++;
m_ID = s;
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_number = atoi( s ) * 1000;
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_number += atoi( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_name = s;
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_state = s;
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_country = s;
s = t; t = strchr( s, ';' ); *t = 0; t++;
m_region = atoi( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
double latitude = decodeDMS( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
double longitude = decodeDMS( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
double ulatitude = decodeDMS( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
double ulongitude = decodeDMS( s );
s = t; t = strchr( s, ';' ); *t = 0; t++;
double altitude = atoi( s ) * FEET_TO_METER;
s = t; t = strchr( s, ';' ); *t = 0; t++;
double ualtitude = atoi( s ) * FEET_TO_METER;
Point3D p( longitude, latitude, altitude+EQUATORIAL_RADIUS_M );
m_locationPolar = p;
m_locationCart = fgPolarToCart3d( p );
Point3D up( ulongitude, ulatitude, ualtitude+EQUATORIAL_RADIUS_M );
m_upperLocationPolar = up;
m_upperLocationCart = fgPolarToCart3d( up );
s = t;
m_pFlag = s[0];
}
// Constructor
// Decodes METAR station string of this format:
// KPUB;72;464;Pueblo, Pueblo Memorial Airport;CO;United States;4;38-17-24N;104-29-54W;38-17-03N;104-29-43W;1440;1420;P
int CMetarStation::initialize()
{
// Read the list of metar stations, decoding and adding to global list.
CMetarStation *m;
char buf[256];
// Goto the Flight Gear installation directory
#ifdef TESTPROG
FGPath weatherPath( "/mkv/Build/FlightGear" );
#else
FGPath weatherPath( current_options.get_fg_root() );
#endif
weatherPath.append( "Weather/MetarStations" );
// Open the metar station list
FILE *f = fopen( weatherPath.c_str(), "r" );
if ( f != NULL )
{
// Read each line, create an instance of a station, and add it to the vector
while ( fgets( buf, 256, f) != NULL && feof( f ) == 0 )
{
//std::cout << buf << std::endl;
m = new CMetarStation( buf );
//m->dump();
METAR_Stations.push_back( m );
}
// Close the list
fclose( f );
std::cout << METAR_Stations.size() << " Metar stations" << std::endl;
return 1;
}
else
{
std::cout << "Could not open MetarStations file " << std::endl;
return 0;
}
}
int CMetarStation::sameName( CMetarStation *m )
{
return m->m_ID == tempName;
}
CMetarStation *CMetarStation::find( std::string stationID )
{
tempName = stationID;
CMetarStation **m = std::find_if( METAR_Stations.begin(), METAR_Stations.end(), sameName );
if ( m != METAR_Stations.end() ) return *m;
return 0;
}
double bestDist;
CMetarStation *bestStation;
Point3D curLocation;
void findHelper( CMetarStation *s )
{
double dist = s->locationCart().distance3Dsquared( curLocation );
if (dist < bestDist )
{
bestDist = dist;
bestStation = s;
}
}
CMetarStation *CMetarStation::find( Point3D locationCart )
{
bestDist = 99999999;
bestStation = 0;
curLocation = locationCart;
for_each( findHelper );
return bestStation;
}
void CMetarStation::for_each( void f( CMetarStation *s ) )
{
std::for_each( METAR_Stations.begin(), METAR_Stations.end(), f );
}
void CMetarStation::dump()
{
std::cout << "ID:" << ID();
std::cout << std::endl;
std::cout << "number:" << number();
std::cout << std::endl;
std::cout << "name:" << name();
std::cout << std::endl;
std::cout << "state:" << state();
std::cout << std::endl;
std::cout << "country:" << country();
std::cout << std::endl;
std::cout << "region:" << region();
std::cout << std::endl;
std::cout << "Location (cart):" << locationCart();
std::cout << std::endl;
std::cout << "Location (polar):" << locationPolar();
std::cout << std::endl;
std::cout << "Upper Location (cart):" << upperLocationCart();
std::cout << std::endl;
std::cout << "Upper Location (polar):" << upperLocationPolar();
std::cout << std::endl;
std::cout << "P flag:" << pFlag();
std::cout << std::endl;
}
std::ostream&
operator << ( ostream& out, const CMetarStation& p )
{
return out
<< "ID:" << p.m_ID << std::endl
<< "number:" << p.m_number << std::endl
<< "name:" << p.m_name << std::endl
<< "state:" << p.m_state << std::endl
<< "country:" << p.m_country << std::endl
<< "region:" << p.m_region << std::endl
<< "Location (cart):" << p.m_locationCart << std::endl
<< "Location (polar):" << p.m_locationCart << std::endl
<< "Upper Location (cart):" << p.m_upperLocationCart << std::endl
<< "Upper Location (polar):" << p.m_upperLocationPolar << std::endl
<< "P flag:" << p.m_pFlag << std::endl;
}
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// Class encapulating the metar station information
//
// METAR station information is kept in this file:
// http://www.nws.noaa.gov/pub/stninfo/nsd_cccc.gz
// http://www.nws.noaa.gov/pub/stninfo/nsd_cccc.txt
// This class looks for the file FG_ROOT/Weather/MetarStations instread of nsd_cccc.
#ifndef _MetarStation_
#define _MetarStation_
#include <iostream>
#include <string>
#include <vector>
#include <Math/point3d.hxx>
#include <Math/polar3d.hxx>
//using namespace std;
class CMetarStation
{
// Attributes
private:
std::string m_ID;
unsigned long m_number;
std::string m_name;
std::string m_state;
std::string m_country;
int m_region;
Point3D m_locationPolar;
Point3D m_upperLocationPolar;
Point3D m_locationCart;
Point3D m_upperLocationCart;
int m_altitude;
int m_upperAltitude;
char m_pFlag;
static int initialized;
static std::string tempName;
// Operations
private:
double decodeDMS( char *b );
static int sameName( CMetarStation *m );
CMetarStation(
char *s );
// Constructor
~CMetarStation()
{
}
// Destructor
public:
std::string &ID() { return m_ID; }
unsigned long number() { return m_number; }
std::string &name() { return m_name; }
std::string &state() { return m_state; }
std::string &country() { return m_country; }
int region() { return m_region; }
Point3D &locationPolar() { return m_locationPolar; }
Point3D &upperLocationPolar() { return m_upperLocationPolar; }
Point3D &locationCart() { return m_locationCart; }
Point3D &upperLocationCart() { return m_upperLocationCart; }
char pFlag() { return m_pFlag; }
// Get attributes
friend std::ostream& operator << ( std::ostream&, const CMetarStation& );
void dump();
static CMetarStation *find( std::string stationID );
static CMetarStation *find( Point3D locationCart );
static void for_each( void f( CMetarStation *s ) );
private:
CMetarStation(
const CMetarStation &rNewObj );
// Copy constructor. Not implemented.
CMetarStation &operator =(
const CMetarStation &rObj );
// Assignment operator. Not implemented.
static int initialize();
};
#endif
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// Metar Library test
#include <iostream>
#include "../MetarReport.h"
#include "../MetarStation.h"
#include <GL/glut.h>
static char *report[] =
{
"KAST 221156Z COR 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KAST COR 221156Z 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KAST COR 221156Z 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KP88 COR 221156 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005",
"KP88 COR 221156 09005KT 1/SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 6//// 70109 T00890084 10100 20089 55005",
"EPIT 1755 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1/2V3/4",
"KFAR 181154Z 10003KT 1/4SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 10345 20226 T01610133 $",
"KFAR 181154Z 10003KT 1/SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 10345 20226 T01610133 $",
"RKSS 21009KT 1400 RP2000 // ////// 21/20 1006/2972 NOSIG",
"RKSS 1200 21009KT 1400 RP2000 // ////// 21/20 1006/2972 NOSIG",
"RKSS 1130Z 23011KT 1100 R14R/P1500N R14L/P1500N BR SCT010 BKN030 "
"BKN080 21/21 Q1006 NOSIG",
"RKSS 1130Z 23011KT 1100 R14R/P1500 R14L/P1500 BR SCT010 BKN030 "
"BKN080 21/21 Q1006 NOSIG",
"KFAR 181154Z 10003KT 4SM HZ CLR 16/13 A2988 RMK AO2 "
"SLP117 56012 1//// 2//// T01610133 $",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE10 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE DUE9 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE FZDZE10 LO CLD SLP186",
"CYYE 061300Z 3500KT 15SM BKN005 OVC040 08/08 A3004 RMK "
"SF6SC1 VSBY RDCE FZDZE9 LO CLD SLP186",
"MKJP 1400Z 13011KT 9999 FEW022 30/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 M30/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/XX Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/30 Q1015",
"MKJP 1400Z 13011KT 9999 FEW022 MM/M30 Q1015",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 BKN045 OVC090 "
"SCT120 FEW250 RMK OCNL LTGICCG OHD",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 07/01 Q1011 "
"RMK TEMPO 8000 -SHRA BKN015 FRQ LTG VC",
"EGPD 36016G26KT 320V030 9999 FEW015TCU SCT026 07/01 Q1011 "
"RMK TEMPO 8000 -SHRA BKN015 LTG DSNT W",
"METAR KLAX 281156Z AUTO VRB100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT FC "
"+TS BLPY FEW/// SCT000 BKN050 SCT150 OVC250 3/M1 A2991 RMK "
"TORNADO B13E45 6 NE MOV E A02 PK WND 18515/45 "
"WSHFT 1350 FROPA TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"VIS 2 1/2 RY11 "
"DVR/1000V1600FT "
"OCNL LTG VCY STN "
"RAB1030E1145 FZDZE56 BLPYE57 CIG 1000V1500 CIG 020 RY11 "
"PRESFR PRESRR SLP013 FG FEW/// HZ SCT000 VIS NW 2 1/2 GR 3/4 "
"VIRGA SE -XRAFG3 CIGE005 BKN014 V OVC "
"FU BKN020 NOSPECI LAST 8/365 SNINCR 2/10 4/178 "
"933125 98096 P 0125 60225 70565 "
"T00261015 10369 21026 "
"404800360 52101 VISNO RY05 CHINO RY27 PNO RVRNO "
"PWINO FZRANO TSNO $",
"KBOS 251356Z 26011KT 10SM CLR 12/02 A2995 RMK AO2 SC VCNTY "
"STN SSE-NNW SCT CI ABV SLP141 T01220023",
"EFHK 36009KT 340V060 CAVOK 12/M02 Q1013 NOSIG",
"EGKK 24011KT 210V300 9999 SCT020 BKN045 12/06 Q1007 NOSIG",
"EGPD 31018KT 8000 RA FEW013 BKN021 OVC045 06/04 Q0994 NOSIG",
"EKCH 16012KT CAVOK 20/07 Q1006 NOSIG",
"ESKN 10014KT 9000 BR SCT100 14/04 Q1010",
"LOWW 231450Z 14017KT CAVOK 23/07 Q1010 NOSIG",
"METAR CYCH 171500Z CCA 30017KT 2SM -SN BKN006",
"METAR CYOW 171500Z CCA 30017KT 2SM -SN BKN006 OVC020 00/M02 "
"A2957 RMK S35F4NS1 /S01/ SNW WET SNW MELTG ON GRND CIG 5-7 "
"SLP018",
"KAST 221156Z AUTO 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005"
" TSB0159E30 TS SE MOV NE",
"KAST 221156Z AUTO 09005KT 7SM -RA OVC026 09/08 A2996 RMK "
"AO2 TNO SLP143 P0007 60047 70109 T00890084 10100 20089 55005"
" TSE0159 TS SE",
"KHVR 1756Z 31007KT 5SM -SN SCT011 BKN024 OVC030 M05/M08 A3056 "
"RMK AOA 933004 "
"BKN V SCT TNO PCPN 000 $ SLP389 4/015 60002 "
"T10501077 11050 21078 51010",
"SPECI KGFI 041420Z AUTO 18030KT 3 1/2SM RVRNO TS -RA BKN008 OVC060 "
"26/22 A2991 RMK A02 RA15TSB20 PRESFR SLP 101 P 0000 T02640218",
"METAR KCLE 281156Z 170100G135KT 110V180 M1/4SM "
"R01L/P6000FT +TSSHRA VCFG "
"BKN025 SCT100 OVC200 M26/ A2991 RMK PK WND 18515/45 A02 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"CIG 1000V1500 PRESFR FRQ LTG CG NW "
"RAB1030E1145 FZDZE56 PRESRR SLP135 GS "
"T1263 "
"VIRGA NW 8/365 4/178 P 0125 60225 7//// 70565 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"CYQR 161700Z 15015KT 15SM SCT045 SCT090 BKN250 10/03 A2955 "
"RMK SC1AC2C11 OB TAKEN H+ 5 DUE AWOS FAILURE SLP027",
"KPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 199/182",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP701 P0254 199/182",
"KHLN 281156Z AUTO 27005KT 10SM OVC023 07/05 A3011 RMK AOA OVC V "
"BKN $ SLP202 60000 70001 T00670050 10122 20061 53003",
"KPHX 281156Z 12004KT 10SM CLR 15/05 A2996 RMK AOA SLP135 T01500050 "
"10250 20150 53006",
"KFCA 281156Z 30003KT 10SM CLR 06/02 A3009 RMK AO TNO $ SLP191 "
"T00610023 10167 20056 53003",
"KAST 281156Z 00000KT 10SM BKN095 09/08 A2997 RMK AOA SLP150 "
"T00940084 10161 20094 52005 ",
"KHVR 281156Z 03003KT 10SM OVC020 09/07 A3010 RMK AO TNO ZRNO "
"$ SLP194 T00940073 10156 20089 51005",
"KGGW 281156Z 35006KT 5SM BR OVC010 10/09 A3003 RMK AOA $ SLP177 "
"70003 T01000095 10156 20110 53008",
"KELY 1153Z AUTO 14004KT 10SM SCT075 01/M01 A3011 RMK AOA TNO ZRNO "
"SLP171 70001 T00061011 10139 21006 51005",
"KFLG 281156Z 29006KT 10SM CLR 04/M01 A3012 RMK AO TNO SLP147 "
"T00391011 21006 51004",
"KGTF 281156Z 27005KT 7SM BKN080 04/04 A3010 RMK AOA SLP205 "
"T00440045 10117 20039 51006",
"K13A 1918Z 20011KT 26/M06 RMK AO PKWND 020/RNO 644V264 T02611061",
"KP88 1919Z 09001KT 14/03 RMK AO / PKWND 002/RNO 158 Z T01440034",
"K40B 1924Z 29004KT 15/M07 RMK AO PKWND 011/RM MV263 T01501072",
"KGGW 1756Z 33018KT 10SM OVC015 M03/M06 A3041 RMK AOA SLP338 "
"4/007 60002 T10281055 11028 21072 51009",
"KPHX 1756Z 130004KT 10SM CLR 18/M03 A3001 RMK AOA SLP154 "
"T01781033 10178 20067 58007",
"KFCA 1756Z 29005KT 10SM CLR 05/M11 A3049 RMK AOA TNO SLP352 "
"T00501111 10050 21044 50004",
"KAST 1756Z 01006KT 10SM CLR 11/04 A3047 RMK AOA SLP316 "
"T01110045 10111 20000 50002",
"KELY 1753Z 34010KT 10SM CLR 01/M07 A3022 RMK AOA TNO ZRNO "
"SLP240 T00111066 10011 21078 58007",
"KFLG 1756Z 07006KT 10SM CLR 06/M12 A3009 RMK AO TNO ZRNO "
"SLP178 T00561122 10061 21100 58005",
"KGTF 1756Z 35010KT 1/2SM -SN FG VV09 M06/M08 A3051 RMK AOA "
"933004 SFC VSBY 3/4 "
"PCPN M SLP393 60010 T10611077 11044 21067 53013",
"KHLN 1756Z 35012KT 10SM SCT032 OVC060 M02/M09 A3048 RMK AOA "
"SLP369 60000 T10171094 11017 21061 53006",
"KAST 1756Z 01006KT 10SM CLR 11/04 A3047 RMK AOA SLP316 61104 "
"71235 T01110045 10111 20000 401720056 58002",
"METAR KLAX 04281156Z AUTO VRB100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT FC "
"+TS BLPY FEW000 BKN050 SCT150 OVC250 3/M1 A2991 RMK "
"TORNADO B13 DSNT NE A02 PK WND 18515/45 "
"WSHFT 1350 FROPA TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"VIS 2 1/2 RY11 OCNL LTG VCY STN "
"RAB1030E1145 FZDZE56 BLPYE57 CIG 1000V1500 CIG 020 RY11 "
"PRESFR PRESRR SLP013 FG FEW000 VIS NW2 1/2 GR 3/4 "
"VIRGA SE -XRAFG3 CIGE005 BKN014 V OVC "
"FU BKN020 NOSPECI LAST 8/365 SNINCR 2/10 4/178 "
"933125 98096 P 0125 60225 70565 "
"T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 17012KT 130V210 3 1/2SM R15L/0500FT -RA "
"SCT050 OVC110 26/18 A2991 RMK FUNNEL CLOUDS A02 RAB30 "
"SLP 101 GR M1/4 VIRGA SCT V BKN P 0010 T02640178",
"METAR KGFI 041356Z AUTO 05008KT 10SM R15L/P6000FT CLR A2991 "
"RMK WATERSPOUTS VCY STN NW A02 SLP 101 10288 20243 52021 $ ",
"SPECI KGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"A2900 RMK A02A PK WND 18056/28 OCNL LTG AP "
"RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 T01990182",
"KABE 281900Z NIL",
"METAR KPIT NIL",
"METAR KCLE 04281156Z 170100G135KT 110V180 M1/4SM "
"R01L/P6000FT +TSSHRA VCFG "
"BKN025 SCT100 OVC200 M26/ A2991 RMK PK WND 18515/45 A02 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"CIG 1000V1500 PRESFR FRQ LTG CG NW "
"RAB1030E1145 FZDZE56 PRESRR SLP135 GS "
"T1263 "
"VIRGA NW 8/365 4/178 P 0125 60225 7//// 70565 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KPHL 040256Z AUTO 170100G135KT 130V210 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 LTG DSNT "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP037 GR 2 3/4 "
"VIRGA E 8/365 4/178 P 0125 70565 21026 T0263 10369 60225 "
"404800360 52101 PWINO FZRANO TSNO $",
"SPECI KGFI 041420Z AUTO 18030KT 2 1/2SM RVRNO TS -RA BKN008 "
"OVC060 25/22 A2991 RMK A02 LTG DSNT W "
"RAB15TSB20 PRESFR SLP101 P 0000 "
"254/218",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR M1/4 "
"VIRGA SE 8/365 4/178 P 0125 6//// 60225 70565 T0263 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 M26/ A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 6//// 60225 70565 T0263 10369 21026 "
"VIRGA 35 8/365 4/178 P 0125 21026 70565 10369 60225 T0263 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 3/M1 A2991 RMK A02 PK WND 18515/45 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 60225 70565 T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO $",
"METAR KGFI 041356Z AUTO 170100G135KT 130V210 3 1/2SM "
"R15L/0500FT R22L/2700FT R16/1200FT R34/1000V1600FT R01L/P6000FT "
"FC +TS BKN050 SCT150 OVC250 3/M1 A2991 RMK A02 PK WND 185150/1345 "
"WSHFT 1350 TWR VIS 1 1/2 SFC VIS 1/4 VIS 1/4V1 1/4 "
"RAB1030E1145 FZDZE56 CIG 1000V1500 PRESFR PRESRR SLP997 GR 25 "
"VIRGA 35 8/365 4/178 P 0125 60225 70565 T00261015 10369 21026 "
"404800360 52101 PWINO FZRANO TSNO",
"METAR KGFI 041356Z AUTO 05008KT 10SM R15L/P6000FT CLR A2991 RMK "
"A02 SLP 101 10288 20243 52021",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 M199/M182",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 M199/182",
"SPECI DGFI 041430Z 18045G56KT M1/4SM R15/0200FT FC +TS VV010 20/18 "
"M20/M18 A2900 RMK A02A PK WND 18056/28 RAB15E25TSB20 FCB1430 PRESFR "
"SLP 701 P 0254 199/M182",
"METAR APIT 171755Z AUTO 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 4/369 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 8/563 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 SLP875 SGB1213E1225",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK SLP056 "
"RAE0123",
"SPECI APIT 171755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 8/321 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 SLP875 FGB1713",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 SLP875",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 1/2 SLP875",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 1/2 SLP875",
"EGPF 1720Z 00000KT 9999 -SHRA STC014 SCT020CB BNK024 12/09 "
"Q1003 NOSIG",
"NZAA 1700Z 03010KT 30KM 03 5CU022 7SC035 11/07 Q1006.5 NOSIG",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK KAUKAU 30050KT",
"DGAA 1800Z 22012KT 9999 SCT009 BKN120 25/21 Q1015",
"DAAT 1830Z 30010KT CAVOK 29/06 Q1019",
"GQPP 1800Z 34023KT 3000 DRSA SKC 24/20 Q1011 NSG",
"DAAG 1830Z 06006KT 9999 SCT020 25/22 Q1015",
"DABB 1830Z 04010KT 9999 SCT030TCU SCT033CB 27/18 Q1017",
"DABC 1830Z 00000KT 9999 SCT026TCU SCT036CB 22/18 Q1020 RETS",
"NZAA 1700Z 03010KT 30KM 03 5CU022 7SC035 11/07 Q1006.5 NOSIG",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK K",
"NZWN 1700Z 35030G49KT 320V030 20KM 02 5SC021 7SC046 12/08 "
" Q0994.2 TEMPO 6000 RA 5ST012 2CB015 RMK KAUKAU 30050KT",
"DGAA 1800Z 22012KT 9999 SCT009 BKN120 25/21 Q1015",
"GFLL 1900Z NIL",
"GOOY 1800Z 03006G17KT 340V080 6000 TSRA BKN016 BKN030CB "
"BKN133 26/23 Q1013 NOSIG",
"GCXO 1930Z 32018KT 8000 SCT003 SCT007 18/16 Q1019",
"APIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2",
"BPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2",
"CPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1V2 1/2",
"DPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 1 1/2V2 1/2",
"FPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 3/4V2 1/2",
"GPIT 1755Z 22015G25KT 1 3/4SM R22L/2700FT R16/1200FT "
"R34/1000V1600FT R01L/P6000FT R04RR/900FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/16 A2992 "
"RMK 58033 6003/ TWELVE 70125 10039 20029 410840112 "
"PCPN 0009 WSHFT 1715 PK WND 2032/1725 "
"CIG 20V25 WND 12V25 TWR VIS 2 1/2 "
"SFC VIS 1 1/2 VIS 3/4V3",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB MM/M16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB MM/16 A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB M18/MM A2992",
"KPIT 1935Z 22015G25KT 1 3/4SM R22L/2700FT "
"TSRA -DZ FG +SNPE SCT005 BKN010 OVC250CB 18/MM A2992",
NULL};
void dispMetarStation( CMetarStation *s )
{
glPointSize( 2.0 );
glColor3d(1.0,1.0,0.0);
glVertex3d( s->locationCart().x()/1000.0, s->locationCart().y()/1000.0, s->locationCart().z()/1000.0 );
}
static int ii = 0;
void
display(void)
{
glPushMatrix();
glClear(GL_COLOR_BUFFER_BIT | GL_DEPTH_BUFFER_BIT);
glRotatef((ii%360), 1.0, 0.0, 0.0);
glRotatef((ii%360), 0.0, 1.0, 0.0);
glRotatef((ii%360), 0.0, 0.0, 1.0);
glBegin( GL_POINTS );
CMetarStation::for_each( dispMetarStation );
glEnd();
glColor3d(0.0, 0.0, 1.0);
glutWireSphere(EARTH_RAD,32,16);
glutSwapBuffers();
ii++;
glPopMatrix();
}
void
idle(void)
{
// std::cout << "Idle" << std::endl;
glutPostRedisplay();
}
void
init(void)
{
glEnable(GL_DEPTH_TEST);
glMatrixMode(GL_PROJECTION);
gluPerspective( 50.0, 1.0, 1.0, 40000.0);
glMatrixMode(GL_MODELVIEW);
gluLookAt(0.0, -19000.0, 0.0,
0.0, 0.0, 0.0,
0.0, 0.0, 1.0);
}
void testMetarStation(int argc,
char **argv )
{
std::cout << "Display all Metar Stations" << std::endl;
glutInit(&argc, argv);
glutInitDisplayMode(GLUT_DOUBLE | GLUT_RGB | GLUT_DEPTH);
glutCreateWindow("Metar Stations");
glutDisplayFunc(display);
glutIdleFunc(idle);
init();
glutMainLoop();
}
void testMetarReport()
{
std::cout << "Decode some Metar reports" << std::endl;
int i = 0;
while ( report[i] )
{
std::cout << i << ": " << report[i] << std::endl;
CMetarReport dr( report[i] );
//dr.dump();
std::cout << dr << std::endl;
CMetarStation *ms = CMetarStation::find( dr.StationID() );
if ( ms )
{
std::cout << *ms << std::endl;
}
else
{
std::cout << "No corresponding METAR station found" << std::endl;
}
i++;
}
}
int
main(
int argc,
char **argv )
{
std::cout << "Metar subsystem test" << std::endl;
testMetarReport();
testMetarStation( argc, argv );
return 0;
}
+100
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Microsoft Developer Studio Workspace File, Format Version 6.00
# WARNING: DO NOT EDIT OR DELETE THIS WORKSPACE FILE!
###############################################################################
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Package=<5>
{{{
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Project_Dep_Name Metar
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+590
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#include "Local.h" /* standard header file */
#include "Metar.h"
#pragma page(1)
#pragma subtitle("subtitle - description ")
/********************************************************************/
/* */
/* Title: prtDMETR */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 15 Sep 1994 */
/* Programmer: CARL MCCALLA */
/* Language: C/370 */
/* */
/* Abstract: prtDMETR prints, in order of the ASOS METAR */
/* format, all non-initialized members of the structure */
/* addressed by the Decoded_METAR pointer. */
/* */
/* External Functions Called: */
/* None. */
/* */
/* Input: Mptr - ptr to a decoded_METAR structure. */
/* */
/* Output: NONE */
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
void prtDMETR( Decoded_METAR *Mptr )
{
/***************************/
/* DECLARE LOCAL VARIABLES */
/***************************/
int i;
/*************************/
/* START BODY OF ROUTINE */
/*************************/
printf("\n\n\n/*******************************************/\n");
printf("/* THE DECODED METAR REPORT FOLLOWS */\n");
printf("/*******************************************/\n\n");
if( Mptr->codeName[ 0 ] != '\0' )
printf("REPORT CODE NAME : %s\n",Mptr->codeName);
if( Mptr->stnid[ 0 ] != '\0' )
printf("STATION ID : %s\n",Mptr->stnid);
if( Mptr->ob_date != MAXINT )
printf("OBSERVATION DAY : %d\n",Mptr->ob_date);
if( Mptr->ob_hour != MAXINT )
printf("OBSERVATION HOUR : %d\n",Mptr->ob_hour);
if( Mptr->ob_minute != MAXINT )
printf("OBSERVATION MINUTE : %d\n",Mptr->ob_minute);
if( Mptr->NIL_rpt )
printf("NIL REPORT : TRUE\n");
if( Mptr->AUTO )
printf("AUTO REPORT : TRUE\n");
if( Mptr->COR )
printf("CORRECTED REPORT : TRUE\n");
if( Mptr->winData.windVRB )
printf("WIND DIRECTION VRB : TRUE\n");
if( Mptr->winData.windDir != MAXINT )
printf("WIND DIRECTION : %d\n",Mptr->winData.windDir);
if( Mptr->winData.windSpeed != MAXINT )
printf("WIND SPEED : %d\n",Mptr->winData.windSpeed);
if( Mptr->winData.windGust != MAXINT )
printf("WIND GUST : %d\n",Mptr->winData.windGust);
if( Mptr->winData.windUnits[ 0 ] != '\0' )
printf("WIND UNITS : %s\n",Mptr->winData.windUnits);
if( Mptr->minWnDir != MAXINT )
printf("MIN WIND DIRECTION : %d\n",Mptr->minWnDir);
if( Mptr->maxWnDir != MAXINT )
printf("MAX WIND DIRECTION : %d\n",Mptr->maxWnDir);
if( Mptr->prevail_vsbyM != (float) MAXINT )
printf("PREVAIL VSBY (M) : %f\n",Mptr->prevail_vsbyM);
if( Mptr->prevail_vsbyKM != (float) MAXINT )
printf("PREVAIL VSBY (KM) : %f\n",Mptr->prevail_vsbyKM);
if( Mptr->prevail_vsbySM != (float) MAXINT )
printf("PREVAIL VSBY (SM) : %.3f\n",Mptr->prevail_vsbySM);
if( Mptr->charPrevailVsby[0] != '\0' )
printf("PREVAIL VSBY (CHAR) : %s\n",Mptr->charPrevailVsby);
if( Mptr->vsby_Dir[ 0 ] != '\0' )
printf("VISIBILITY DIRECTION: %s\n",Mptr->vsby_Dir);
if( Mptr->RVRNO )
printf("RVRNO : TRUE\n");
for ( i = 0; i < 12; i++ )
{
if( Mptr->RRVR[i].runway_designator[0] != '\0' )
printf("RUNWAY DESIGNATOR : %s\n",
Mptr->RRVR[i].runway_designator);
if( Mptr->RRVR[i].visRange != MAXINT )
printf("R_WAY VIS RANGE (FT): %d\n",
Mptr->RRVR[i].visRange);
if( Mptr->RRVR[i].vrbl_visRange )
printf("VRBL VISUAL RANGE : TRUE\n");
if( Mptr->RRVR[i].below_min_RVR )
printf("BELOW MIN RVR : TRUE\n");
if( Mptr->RRVR[i].above_max_RVR )
printf("ABOVE MAX RVR : TRUE\n");
if( Mptr->RRVR[i].Max_visRange != MAXINT )
printf("MX R_WAY VISRNG (FT): %d\n",
Mptr->RRVR[i].Max_visRange);
if( Mptr->RRVR[i].Min_visRange != MAXINT )
printf("MN R_WAY VISRNG (FT): %d\n",
Mptr->RRVR[i].Min_visRange);
}
if( Mptr->DVR.visRange != MAXINT )
printf("DISPATCH VIS RANGE : %d\n",
Mptr->DVR.visRange);
if( Mptr->DVR.vrbl_visRange )
printf("VRBL DISPATCH VISRNG: TRUE\n");
if( Mptr->DVR.below_min_DVR )
printf("BELOW MIN DVR : TRUE\n");
if( Mptr->DVR.above_max_DVR )
printf("ABOVE MAX DVR : TRUE\n");
if( Mptr->DVR.Max_visRange != MAXINT )
printf("MX DSPAT VISRNG (FT): %d\n",
Mptr->DVR.Max_visRange);
if( Mptr->DVR.Min_visRange != MAXINT )
printf("MN DSPAT VISRNG (FT): %d\n",
Mptr->DVR.Min_visRange);
i = 0;
while ( Mptr->WxObstruct[i][0] != '\0' && i < MAXWXSYMBOLS )
{
printf("WX/OBSTRUCT VISION : %s\n",
Mptr->WxObstruct[i] );
i++;
}
if( Mptr->PartialObscurationAmt[0][0] != '\0' )
printf("OBSCURATION AMOUNT : %s\n",
&(Mptr->PartialObscurationAmt[0][0]));
if( Mptr->PartialObscurationPhenom[0][0] != '\0' )
printf("OBSCURATION PHENOM : %s\n",
&(Mptr->PartialObscurationPhenom[0][0]));
if( Mptr->PartialObscurationAmt[1][0] != '\0' )
printf("OBSCURATION AMOUNT : %s\n",
&(Mptr->PartialObscurationAmt[1][0]));
if( Mptr->PartialObscurationPhenom[1][0] != '\0' )
printf("OBSCURATION PHENOM : %s\n",
&(Mptr->PartialObscurationPhenom[1][0]));
i = 0;
while ( Mptr->cldTypHgt[ i ].cloud_type[0] != '\0' &&
i < 6 )
{
if( Mptr->cldTypHgt[ i ].cloud_type[0] != '\0' )
printf("CLOUD COVER : %s\n",
Mptr->cldTypHgt[ i ].cloud_type);
if( Mptr->cldTypHgt[ i ].cloud_hgt_char[0] != '\0' )
printf("CLOUD HGT (CHARAC.) : %s\n",
Mptr->cldTypHgt[ i ].cloud_hgt_char);
if( Mptr->cldTypHgt[ i ].cloud_hgt_meters != MAXINT)
printf("CLOUD HGT (METERS) : %d\n",
Mptr->cldTypHgt[ i ].cloud_hgt_meters);
if( Mptr->cldTypHgt[ i ].other_cld_phenom[0] != '\0' )
printf("OTHER CLOUD PHENOM : %s\n",
Mptr->cldTypHgt[ i ].other_cld_phenom);
i++;
}
if( Mptr->temp != MAXINT )
printf("TEMP. (CELSIUS) : %d\n", Mptr->temp);
if( Mptr->dew_pt_temp != MAXINT )
printf("D.P. TEMP. (CELSIUS): %d\n", Mptr->dew_pt_temp);
if( Mptr->A_altstng )
printf("ALTIMETER (INCHES) : %.2f\n",
Mptr->inches_altstng );
if( Mptr->Q_altstng )
printf("ALTIMETER (PASCALS) : %d\n",
Mptr->hectoPasc_altstng );
if( Mptr->TornadicType[0] != '\0' )
printf("TORNADIC ACTVTY TYPE: %s\n",
Mptr->TornadicType );
if( Mptr->BTornadicHour != MAXINT )
printf("TORN. ACTVTY BEGHOUR: %d\n",
Mptr->BTornadicHour );
if( Mptr->BTornadicMinute != MAXINT )
printf("TORN. ACTVTY BEGMIN : %d\n",
Mptr->BTornadicMinute );
if( Mptr->ETornadicHour != MAXINT )
printf("TORN. ACTVTY ENDHOUR: %d\n",
Mptr->ETornadicHour );
if( Mptr->ETornadicMinute != MAXINT )
printf("TORN. ACTVTY ENDMIN : %d\n",
Mptr->ETornadicMinute );
if( Mptr->TornadicDistance != MAXINT )
printf("TORN. DIST. FROM STN: %d\n",
Mptr->TornadicDistance );
if( Mptr->TornadicLOC[0] != '\0' )
printf("TORNADIC LOCATION : %s\n",
Mptr->TornadicLOC );
if( Mptr->TornadicDIR[0] != '\0' )
printf("TORNAD. DIR FROM STN: %s\n",
Mptr->TornadicDIR );
if( Mptr->TornadicMovDir[0] != '\0' )
printf("TORNADO DIR OF MOVM.: %s\n",
Mptr->TornadicMovDir );
if( Mptr->autoIndicator[0] != '\0' )
printf("AUTO INDICATOR : %s\n",
Mptr->autoIndicator);
if( Mptr->PKWND_dir != MAXINT )
printf("PEAK WIND DIRECTION : %d\n",Mptr->PKWND_dir);
if( Mptr->PKWND_speed != MAXINT )
printf("PEAK WIND SPEED : %d\n",Mptr->PKWND_speed);
if( Mptr->PKWND_hour != MAXINT )
printf("PEAK WIND HOUR : %d\n",Mptr->PKWND_hour);
if( Mptr->PKWND_minute != MAXINT )
printf("PEAK WIND MINUTE : %d\n",Mptr->PKWND_minute);
if( Mptr->WshfTime_hour != MAXINT )
printf("HOUR OF WIND SHIFT : %d\n",Mptr->WshfTime_hour);
if( Mptr->WshfTime_minute != MAXINT )
printf("MINUTE OF WIND SHIFT: %d\n",Mptr->WshfTime_minute);
if( Mptr->Wshft_FROPA != FALSE )
printf("FROPA ASSOC. W/WSHFT: TRUE\n");
if( Mptr->TWR_VSBY != (float) MAXINT )
printf("TOWER VISIBILITY : %.2f\n",Mptr->TWR_VSBY);
if( Mptr->SFC_VSBY != (float) MAXINT )
printf("SURFACE VISIBILITY : %.2f\n",Mptr->SFC_VSBY);
if( Mptr->minVsby != (float) MAXINT )
printf("MIN VRBL_VIS (SM) : %.4f\n",Mptr->minVsby);
if( Mptr->maxVsby != (float) MAXINT )
printf("MAX VRBL_VIS (SM) : %.4f\n",Mptr->maxVsby);
if( Mptr->VSBY_2ndSite != (float) MAXINT )
printf("VSBY_2ndSite (SM) : %.4f\n",Mptr->VSBY_2ndSite);
if( Mptr->VSBY_2ndSite_LOC[0] != '\0' )
printf("VSBY_2ndSite LOC. : %s\n",
Mptr->VSBY_2ndSite_LOC);
if( Mptr->OCNL_LTG )
printf("OCCASSIONAL LTG : TRUE\n");
if( Mptr->FRQ_LTG )
printf("FREQUENT LIGHTNING : TRUE\n");
if( Mptr->CNS_LTG )
printf("CONTINUOUS LTG : TRUE\n");
if( Mptr->CG_LTG )
printf("CLOUD-GROUND LTG : TRUE\n");
if( Mptr->IC_LTG )
printf("IN-CLOUD LIGHTNING : TRUE\n");
if( Mptr->CC_LTG )
printf("CLD-CLD LIGHTNING : TRUE\n");
if( Mptr->CA_LTG )
printf("CLOUD-AIR LIGHTNING : TRUE\n");
if( Mptr->AP_LTG )
printf("LIGHTNING AT AIRPORT: TRUE\n");
if( Mptr->OVHD_LTG )
printf("LIGHTNING OVERHEAD : TRUE\n");
if( Mptr->DSNT_LTG )
printf("DISTANT LIGHTNING : TRUE\n");
if( Mptr->LightningVCTS )
printf("L'NING W/I 5-10(ALP): TRUE\n");
if( Mptr->LightningTS )
printf("L'NING W/I 5 (ALP) : TRUE\n");
if( Mptr->VcyStn_LTG )
printf("VCY STN LIGHTNING : TRUE\n");
if( Mptr->LTG_DIR[0] != '\0' )
printf("DIREC. OF LIGHTNING : %s\n", Mptr->LTG_DIR);
i = 0;
while( i < 3 && Mptr->ReWx[ i ].Recent_weather[0] != '\0' )
{
printf("RECENT WEATHER : %s",
Mptr->ReWx[i].Recent_weather);
if( Mptr->ReWx[i].Bhh != MAXINT )
printf(" BEG_hh = %d",Mptr->ReWx[i].Bhh);
if( Mptr->ReWx[i].Bmm != MAXINT )
printf(" BEG_mm = %d",Mptr->ReWx[i].Bmm);
if( Mptr->ReWx[i].Ehh != MAXINT )
printf(" END_hh = %d",Mptr->ReWx[i].Ehh);
if( Mptr->ReWx[i].Emm != MAXINT )
printf(" END_mm = %d",Mptr->ReWx[i].Emm);
printf("\n");
i++;
}
if( Mptr->minCeiling != MAXINT )
printf("MIN VRBL_CIG (FT) : %d\n",Mptr->minCeiling);
if( Mptr->maxCeiling != MAXINT )
printf("MAX VRBL_CIG (FT)) : %d\n",Mptr->maxCeiling);
if( Mptr->CIG_2ndSite_Meters != MAXINT )
printf("CIG2ndSite (FT) : %d\n",Mptr->CIG_2ndSite_Meters);
if( Mptr->CIG_2ndSite_LOC[0] != '\0' )
printf("CIG @ 2nd Site LOC. : %s\n",Mptr->CIG_2ndSite_LOC);
if( Mptr->PRESFR )
printf("PRESFR : TRUE\n");
if( Mptr->PRESRR )
printf("PRESRR : TRUE\n");
if( Mptr->SLPNO )
printf("SLPNO : TRUE\n");
if( Mptr->SLP != (float) MAXINT )
printf("SLP (hPa) : %.1f\n", Mptr->SLP);
if( Mptr->SectorVsby != (float) MAXINT )
printf("SECTOR VSBY (MILES) : %.2f\n", Mptr->SectorVsby );
if( Mptr->SectorVsby_Dir[ 0 ] != '\0' )
printf("SECTOR VSBY OCTANT : %s\n", Mptr->SectorVsby_Dir );
if( Mptr->TS_LOC[ 0 ] != '\0' )
printf("THUNDERSTORM LOCAT. : %s\n", Mptr->TS_LOC );
if( Mptr->TS_MOVMNT[ 0 ] != '\0' )
printf("THUNDERSTORM MOVMNT.: %s\n", Mptr->TS_MOVMNT);
if( Mptr->GR )
printf("GR (HAILSTONES) : TRUE\n");
if( Mptr->GR_Size != (float) MAXINT )
printf("HLSTO SIZE (INCHES) : %.3f\n",Mptr->GR_Size);
if( Mptr->VIRGA )
printf("VIRGA : TRUE\n");
if( Mptr->VIRGA_DIR[0] != '\0' )
printf("DIR OF VIRGA FRM STN: %s\n", Mptr->VIRGA_DIR);
for( i = 0; i < 6; i++ ) {
if( Mptr->SfcObscuration[i][0] != '\0' )
printf("SfcObscuration : %s\n",
&(Mptr->SfcObscuration[i][0]) );
}
if( Mptr->Num8thsSkyObscured != MAXINT )
printf("8ths of SkyObscured : %d\n",Mptr->Num8thsSkyObscured);
if( Mptr->CIGNO )
printf("CIGNO : TRUE\n");
if( Mptr->Ceiling != MAXINT )
printf("Ceiling (ft) : %d\n",Mptr->Ceiling);
if( Mptr->Estimated_Ceiling != MAXINT )
printf("Estimated CIG (ft) : %d\n",Mptr->Estimated_Ceiling);
if( Mptr->VrbSkyBelow[0] != '\0' )
printf("VRB SKY COND BELOW : %s\n",Mptr->VrbSkyBelow);
if( Mptr->VrbSkyAbove[0] != '\0' )
printf("VRB SKY COND ABOVE : %s\n",Mptr->VrbSkyAbove);
if( Mptr->VrbSkyLayerHgt != MAXINT )
printf("VRBSKY COND HGT (FT): %d\n",Mptr->VrbSkyLayerHgt);
if( Mptr->ObscurAloftHgt != MAXINT )
printf("Hgt Obscur Aloft(ft): %d\n",Mptr->ObscurAloftHgt);
if( Mptr->ObscurAloft[0] != '\0' )
printf("Obscur Phenom Aloft : %s\n",Mptr->ObscurAloft);
if( Mptr->ObscurAloftSkyCond[0] != '\0' )
printf("Obscur ALOFT SKYCOND: %s\n",Mptr->ObscurAloftSkyCond);
if( Mptr->NOSPECI )
printf("NOSPECI : TRUE\n");
if( Mptr->LAST )
printf("LAST : TRUE\n");
if( Mptr->synoptic_cloud_type[ 0 ] != '\0' )
printf("SYNOPTIC CLOUD GROUP: %s\n",Mptr->synoptic_cloud_type);
if( Mptr->CloudLow != '\0' )
printf("LOW CLOUD CODE : %c\n",Mptr->CloudLow);
if( Mptr->CloudMedium != '\0' )
printf("MEDIUM CLOUD CODE : %c\n",Mptr->CloudMedium);
if( Mptr->CloudHigh != '\0' )
printf("HIGH CLOUD CODE : %c\n",Mptr->CloudHigh);
if( Mptr->SNINCR != MAXINT )
printf("SNINCR (INCHES) : %d\n",Mptr->SNINCR);
if( Mptr->SNINCR_TotalDepth != MAXINT )
printf("SNINCR(TOT. INCHES) : %d\n",Mptr->SNINCR_TotalDepth);
if( Mptr->snow_depth_group[ 0 ] != '\0' )
printf("SNOW DEPTH GROUP : %s\n",Mptr->snow_depth_group);
if( Mptr->snow_depth != MAXINT )
printf("SNOW DEPTH (INCHES) : %d\n",Mptr->snow_depth);
if( Mptr->WaterEquivSnow != (float) MAXINT )
printf("H2O EquivSno(inches): %.2f\n",Mptr->WaterEquivSnow);
if( Mptr->SunshineDur != MAXINT )
printf("SUNSHINE (MINUTES) : %d\n",Mptr->SunshineDur);
if( Mptr->SunSensorOut )
printf("SUN SENSOR OUT : TRUE\n");
if( Mptr->hourlyPrecip != (float) MAXINT )
printf("HRLY PRECIP (INCHES): %.2f\n",Mptr->hourlyPrecip);
if( Mptr->precip_amt != (float) MAXINT)
printf("3/6HR PRCIP (INCHES): %.2f\n",
Mptr->precip_amt);
if( Mptr->Indeterminant3_6HrPrecip )
printf("INDTRMN 3/6HR PRECIP: TRUE\n");
if( Mptr->precip_24_amt != (float) MAXINT)
printf("24HR PRECIP (INCHES): %.2f\n",
Mptr->precip_24_amt);
if( Mptr->Temp_2_tenths != (float) MAXINT )
printf("TMP2TENTHS (CELSIUS): %.1f\n",Mptr->Temp_2_tenths);
if( Mptr->DP_Temp_2_tenths != (float) MAXINT )
printf("DPT2TENTHS (CELSIUS): %.1f\n",Mptr->DP_Temp_2_tenths);
if( Mptr->maxtemp != (float) MAXINT)
printf("MAX TEMP (CELSIUS) : %.1f\n",
Mptr->maxtemp);
if( Mptr->mintemp != (float) MAXINT)
printf("MIN TEMP (CELSIUS) : %.1f\n",
Mptr->mintemp);
if( Mptr->max24temp != (float) MAXINT)
printf("24HrMAXTMP (CELSIUS): %.1f\n",
Mptr->max24temp);
if( Mptr->min24temp != (float) MAXINT)
printf("24HrMINTMP (CELSIUS): %.1f\n",
Mptr->min24temp);
if( Mptr->char_prestndcy != MAXINT)
printf("CHAR PRESS TENDENCY : %d\n",
Mptr->char_prestndcy );
if( Mptr->prestndcy != (float) MAXINT)
printf("PRES. TENDENCY (hPa): %.1f\n",
Mptr->prestndcy );
if( Mptr->PWINO )
printf("PWINO : TRUE\n");
if( Mptr->PNO )
printf("PNO : TRUE\n");
if( Mptr->CHINO )
printf("CHINO : TRUE\n");
if( Mptr->CHINO_LOC[0] != '\0' )
printf("CHINO_LOC : %s\n",Mptr->CHINO_LOC);
if( Mptr->VISNO )
printf("VISNO : TRUE\n");
if( Mptr->VISNO_LOC[0] != '\0' )
printf("VISNO_LOC : %s\n",Mptr->VISNO_LOC);
if( Mptr->FZRANO )
printf("FZRANO : TRUE\n");
if( Mptr->TSNO )
printf("TSNO : TRUE\n");
if( Mptr->DollarSign)
printf("DOLLAR $IGN INDCATR : TRUE\n");
if( Mptr->horiz_vsby[ 0 ] != '\0' )
printf("HORIZ VISIBILITY : %s\n",Mptr->horiz_vsby);
if( Mptr->dir_min_horiz_vsby[ 0 ] != '\0' )
printf("DIR MIN HORIZ VSBY : %s\n",Mptr->dir_min_horiz_vsby);
if( Mptr->CAVOK )
printf("CAVOK : TRUE\n");
if( Mptr->VertVsby != MAXINT )
printf("Vert. Vsby (meters) : %d\n",
Mptr->VertVsby );
if( Mptr->charVertVsby[0] != '\0' )
printf("Vert. Vsby (CHAR) : %s\n",
Mptr->charVertVsby );
if( Mptr->QFE != MAXINT )
printf("QFE : %d\n", Mptr->QFE);
if( Mptr->VOLCASH )
printf("VOLCANIC ASH : TRUE\n");
if( Mptr->min_vrbl_wind_dir != MAXINT )
printf("MIN VRBL WIND DIR : %d\n",Mptr->min_vrbl_wind_dir);
if( Mptr->max_vrbl_wind_dir != MAXINT )
printf("MAX VRBL WIND DIR : %d\n",Mptr->max_vrbl_wind_dir);
printf("\n\n\n");
return;
}
+69
View File
@@ -0,0 +1,69 @@
There are 2 classes: CMetarStation (MetarStation.h) and CMetarReport
(MetarReport.h). These classes provide mechanisms to get information
about meteorological data reporting stations and about the reports
themselves. These stations and reports are known as METAR. See
http://tgsv5.nws.noaa.gov/oso/oso1/oso12/metar.htm for information
from the USA perspective. Quoting from that site:
On 1 July 1996, the international standard code for hourly and special
surface weather observations, METAR/SPECI, took effect.
The METAR acronym roughly translates from the French as Aviation
Routine Weather Report . A special report, SPECI, is merely a METAR
formatted report which is issued on a non-routine basis as dictated by
changing meteorological conditions. The SPECI acronym roughly translates as
Aviation Selected Special Weather Report . Meanwhile, the international
standard code format for terminal forecasts issued for airports, TAF,
also took effect. The acronym translates to Aerodrome Forecast.
This implementation ignores the SPECI and TAF acronyms, calling the
entire system METAR.
The class CMetarStation is implemented by MetarStation.h and
MetarStation.cpp. It decodes a text file containing information about
individual METAR reporting stations and builds a static database of that
information during static construction of the class. There are static
member methods to find individual stations, and member functions to
extract individual station attributes. The information about METAR
stations probably has some overlap with FGFS airport information. That
needs to be investigated. The METAR station information is kept in this
file:
http://www.nws.noaa.gov/pub/stninfo/nsd_cccc.gz
http://www.nws.noaa.gov/pub/stninfo/nsd_cccc.txt
This class looks for the file FG_ROOT/Weather/MetarStations instead of
nsd_cccc.
The current implementation does not look for updates to this file on the
internet.
The class CMetarReport is implemented by MetarReport.h and MetarReport.cpp.
It encapsulates the decoding software written by Carl McCalla at -
NOAA/National Weather Service
1325 East-West Highway
SSMC2, W/OSO242, Station 5114
Silver Spring, Maryland 20910
Work: (301) 713-0882, Ext 115
FAX: (301) 608-0911
E-Mail Address: cmccalla@smtpgate.ssmc.noaa.gov
http://www.nws.noaa.gov/software/
This software generally sucks and the CMetarReport class attempts to clean
up some of that suckiness. A CMetarReport object is created with an ASCII
string as a construction parameter. The string contains a METAR report.
There
are member methods to extract selected information from a report by calling
the McCalla software. Additional information can be selected by adding new
member methods as needed. Certainly the methods currently implemented are
not sufficient. METAR reports are available via the internet. In the USA,
NOAA provides individual METAR reports in this directory:
ftp://weather.noaa.gov/data/observations/metar/stations
Other sources are available as well. The current implementation does not
look for reports on the internet.
There is a test program in the MetarTest subdirectory. It requires that a
#define be changed in the MetarStation.cpp file. Add #define TESTPROG to
the code or -D TESTPROG to the compilation. This is necessary because the
FGFS options class is coupled tightly to code that shouldn't be pulled into
the test program. The test program will decode many METAR reports and
display
them to the screen, then it will plot all the METAR reporting stations on a
tumbling globe.
+211
View File
@@ -0,0 +1,211 @@
#pragma comment (compiler)
//#pragma comment (date)
//#pragma comment (timestamp)
#pragma pagesize(80)
#include "Local.h" /* standard header file */
#pragma page(1)
#pragma subtitle(" ")
#pragma subtitle("stspack2 - Local string test functions ")
/********************************************************************/
/* */
/* Title: stspack2 */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 05 Oct 1992 */
/* Programmer: ALLAN DARLING */
/* Language: C/2 */
/* */
/* Abstract: The stspack2 package contains functions to */
/* perform the isalnum through isxdigit functions */
/* on strings. The functions come in four forms: */
/* those that test NULL delimited strings and are */
/* named in the form sxxxxxxx, those that test at */
/* most n characters and are named in the form */
/* nxxxxxxx, those that search forward in a string */
/* and are named in the form nxtyyyyy, and those */
/* that search backward in a string and are named */
/* in the form lstyyyyy. */
/* */
/* The xxxxxxx is the name of the test applied to */
/* each character in the string, such as isalpha, */
/* thus a function to test a NULL delimited string */
/* an return a nonzero value if all characters in */
/* the string are digits is named sisdigit. */
/* */
/* The yyyyy is the name of the test applied to */
/* characters in a string, minus the 'is' prefix. */
/* Thus a function to find the next digit in a NULL */
/* delimited string and return a pointer to it is */
/* named nxtdigit. */
/* */
/* The only exception to the naming rule is for the */
/* functions that test for hexadecimal digits. */
/* These are named sisxdigi, nisxdigi, nxtxdigi, */
/* and lstxdigi because of the eight character */
/* function name limitation. */
/* */
/* The nxxxxxxx class of functions will test up to */
/* n characters or the first NULL character */
/* encountered, whichever comes first. For all */
/* classes of functions, the string sentinal is */
/* not included in the test. */
/* */
/* External Functions Called: */
/* isalnum, isalpha, iscntrl, isdigit, isgraph, */
/* islower, isprint, ispunct, isspace, isupper, */
/* isxdigit. */
/* */
/* Input: For sxxxxxxx class functions, a pointer to a */
/* NULL delimited character string. */
/* */
/* For nxtyyyyy class functions, a pointer to a */
/* NULL delimited character string. */
/* */
/* for nxxxxxxx class functions, a pointer to a */
/* character array, and a positive, nonzero integer.*/
/* */
/* for lstyyyyy class functions, a pointer to a */
/* character array, and a positive, nonzero integer.*/
/* */
/* Output: A nonzero value if the test is true for all */
/* characters in the string, a zero value otherwise.*/
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
int nisalnum(char *s, int n) {
for (; *s && n; s++, n--)
if (!isalnum(*s))
return (0);
return (1);
} /* end nisalnum */
int nisalpha(char *s, int n) {
for (; *s && n; s++, n--)
if (!isalpha(*s))
return (0);
return (1);
} /* end nisalpha */
int niscntrl(char *s, int n) {
for (; *s && n; s++, n--)
if (!iscntrl(*s))
return (0);
return (1);
} /* end niscntrl */
int nisdigit(char *s, int n) {
for (; *s && n; s++, n--)
if (!isdigit(*s))
return (0);
return (1);
} /* end nisdigit */
int nisgraph(char *s, int n) {
for (; *s && n; s++, n--)
if (!isgraph(*s))
return (0);
return (1);
} /* end nisgraph */
int nislower(char *s, int n) {
for (; *s && n; s++, n--)
if (!islower(*s))
return (0);
return (1);
} /* end nislower */
int nisprint(char *s, int n) {
for (; *s && n; s++, n--)
if (!isprint(*s))
return (0);
return (1);
} /* end nisprint */
int nispunct(char *s, int n) {
for (; *s && n; s++, n--)
if (!ispunct(*s))
return (0);
return (1);
} /* end nispunct */
int nisspace(char *s, int n) {
for (; *s && n; s++, n--)
if (!isspace(*s))
return (0);
return (1);
} /* end nisspace */
int nisupper(char *s, int n) {
for (; *s && n; s++, n--)
if (!isupper(*s))
return (0);
return (1);
} /* end nisupper */
int nisxdigi(char *s, int n) {
for (; *s && n; s++, n--)
if (!isxdigit(*s))
return (0);
return (1);
} /* end nisxdigi */
#pragma page(1)
+211
View File
@@ -0,0 +1,211 @@
#pragma comment (compiler)
//#pragma comment (date)
//#pragma comment (timestamp)
#pragma pagesize(80)
#include "Local.h" /* standard header file */
#pragma page(1)
#pragma subtitle(" ")
#pragma subtitle("stspack3 - Local string test functions ")
/********************************************************************/
/* */
/* Title: stspack3 */
/* Organization: W/OSO242 - GRAPHICS AND DISPLAY SECTION */
/* Date: 05 Oct 1992 */
/* Programmer: ALLAN DARLING */
/* Language: C/2 */
/* */
/* Abstract: The stspack3 package contains functions to */
/* perform the isalnum through isxdigit functions */
/* on strings. The functions come in four forms: */
/* those that test NULL delimited strings and are */
/* named in the form sxxxxxxx, those that test at */
/* most n characters and are named in the form */
/* nxxxxxxx, those that search forward in a string */
/* and are named in the form nxtyyyyy, and those */
/* that search backward in a string and are named */
/* in the form lstyyyyy. */
/* */
/* The xxxxxxx is the name of the test applied to */
/* each character in the string, such as isalpha, */
/* thus a function to test a NULL delimited string */
/* an return a nonzero value if all characters in */
/* the string are digits is named sisdigit. */
/* */
/* The yyyyy is the name of the test applied to */
/* characters in a string, minus the 'is' prefix. */
/* Thus a function to find the next digit in a NULL */
/* delimited string and return a pointer to it is */
/* named nxtdigit. */
/* */
/* The only exception to the naming rule is for the */
/* functions that test for hexadecimal digits. */
/* These are named sisxdigi, nisxdigi, nxtxdigi, */
/* and lstxdigi because of the eight character */
/* function name limitation. */
/* */
/* The nxxxxxxx class of functions will test up to */
/* n characters or the first NULL character */
/* encountered, whichever comes first. For all */
/* classes of functions, the string sentinal is */
/* not included in the test. */
/* */
/* External Functions Called: */
/* isalnum, isalpha, iscntrl, isdigit, isgraph, */
/* islower, isprint, ispunct, isspace, isupper, */
/* isxdigit. */
/* */
/* Input: For sxxxxxxx class functions, a pointer to a */
/* NULL delimited character string. */
/* */
/* For nxtyyyyy class functions, a pointer to a */
/* NULL delimited character string. */
/* */
/* for nxxxxxxx class functions, a pointer to a */
/* character array, and a positive, nonzero integer.*/
/* */
/* for lstyyyyy class functions, a pointer to a */
/* character array, and a positive, nonzero integer.*/
/* */
/* Output: A nonzero value if the test is true for all */
/* characters in the string, a zero value otherwise.*/
/* */
/* Modification History: */
/* None. */
/* */
/********************************************************************/
#pragma page(1)
char *nxtalnum(char *s) {
for (; !isalnum(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtalnum */
char *nxtalpha(char *s) {
for (; !isalpha(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtalpha */
char *nxtcntrl(char *s) {
for (; !iscntrl(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtcntrl */
char *nxtdigit(char *s) {
for (; !isdigit(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtdigit */
char *nxtgraph(char *s) {
for (; !isgraph(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtgraph */
char *nxtlower(char *s) {
for (; !islower(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtlower */
char *nxtprint(char *s) {
for (; !isprint(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtprint */
char *nxtpunct(char *s) {
for (; !ispunct(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtpunct */
char *nxtspace(char *s) {
for (; !isspace(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtspace */
char *nxtupper(char *s) {
for (; !isupper(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtupper */
char *nxtxdigi(char *s) {
for (; !isxdigit(*s) && *s; s++) ;
if (*s)
return (s);
else
return (NULL);
} /* end nxtxdigi */
#pragma page(1)
+30
View File
@@ -0,0 +1,30 @@
## Process this file with automake to produce Makefile.in
if HAVE_ZLIB
ZLIB_INCL =
else
ZLIB_INCL = -I$(top_builddir)/zlib
endif
lib_LIBRARIES = libsgmisc.a
include_HEADERS = \
fgpath.hxx \
fgstream.hxx \
stopwatch.hxx \
strutils.hxx \
texcoord.hxx \
zfstream.hxx
libsgmisc_a_SOURCES = \
fgpath.cxx \
fgstream.cxx \
strutils.cxx \
texcoord.cxx \
zfstream.cxx
INCLUDES += \
-I$(top_builddir) \
-I$(top_builddir)/bucket \
-I$(top_builddir)/math \
$(ZLIB_INCL)
+356
View File
@@ -0,0 +1,356 @@
# Makefile.in generated automatically by automake 1.3 from Makefile.am
# Copyright (C) 1994, 1995, 1996, 1997, 1998 Free Software Foundation, Inc.
# This Makefile.in is free software; the Free Software Foundation
# gives unlimited permission to copy and/or distribute it,
# with or without modifications, as long as this notice is preserved.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY, to the extent permitted by law; without
# even the implied warranty of MERCHANTABILITY or FITNESS FOR A
# PARTICULAR PURPOSE.
SHELL = /bin/sh
srcdir = @srcdir@
top_srcdir = @top_srcdir@
VPATH = @srcdir@
prefix = @prefix@
exec_prefix = @exec_prefix@
bindir = @bindir@
sbindir = @sbindir@
libexecdir = @libexecdir@
datadir = @datadir@
sysconfdir = @sysconfdir@
sharedstatedir = @sharedstatedir@
localstatedir = @localstatedir@
libdir = @libdir@
infodir = @infodir@
mandir = @mandir@
includedir = @includedir@
oldincludedir = /usr/include
DISTDIR =
pkgdatadir = $(datadir)/@PACKAGE@
pkglibdir = $(libdir)/@PACKAGE@
pkgincludedir = $(includedir)/@PACKAGE@
top_builddir = ..
ACLOCAL = @ACLOCAL@
AUTOCONF = @AUTOCONF@
AUTOMAKE = @AUTOMAKE@
AUTOHEADER = @AUTOHEADER@
INSTALL = @INSTALL@
INSTALL_PROGRAM = @INSTALL_PROGRAM@
INSTALL_DATA = @INSTALL_DATA@
INSTALL_SCRIPT = @INSTALL_SCRIPT@
transform = @program_transform_name@
NORMAL_INSTALL = :
PRE_INSTALL = :
POST_INSTALL = :
NORMAL_UNINSTALL = :
PRE_UNINSTALL = :
POST_UNINSTALL = :
CC = @CC@
CXX = @CXX@
LN_S = @LN_S@
MAKEINFO = @MAKEINFO@
PACKAGE = @PACKAGE@
RANLIB = @RANLIB@
VERSION = @VERSION@
base_LIBS = @base_LIBS@
opengl_LIBS = @opengl_LIBS@
@HAVE_ZLIB_TRUE@ZLIB_INCL =
@HAVE_ZLIB_FALSE@ZLIB_INCL = -I$(top_builddir)/zlib
lib_LIBRARIES = libsgmisc.a
include_HEADERS = \
fgpath.hxx \
fgstream.hxx \
stopwatch.hxx \
strutils.hxx \
texcoord.hxx \
zfstream.hxx
libsgmisc_a_SOURCES = \
fgpath.cxx \
fgstream.cxx \
strutils.cxx \
texcoord.cxx \
zfstream.cxx
mkinstalldirs = $(SHELL) $(top_srcdir)/mkinstalldirs
CONFIG_HEADER = ../include/config.h
CONFIG_CLEAN_FILES =
LIBRARIES = $(lib_LIBRARIES)
DEFS = @DEFS@ -I. -I$(srcdir) -I../include
CPPFLAGS = @CPPFLAGS@
LDFLAGS = @LDFLAGS@
LIBS = @LIBS@
X_CFLAGS = @X_CFLAGS@
X_LIBS = @X_LIBS@
X_EXTRA_LIBS = @X_EXTRA_LIBS@
X_PRE_LIBS = @X_PRE_LIBS@
libsgmisc_a_LIBADD =
libsgmisc_a_OBJECTS = fgpath.o fgstream.o strutils.o texcoord.o \
zfstream.o
AR = ar
CXXFLAGS = @CXXFLAGS@
CXXCOMPILE = $(CXX) $(DEFS) $(INCLUDES) $(CPPFLAGS) $(CXXFLAGS)
CXXLINK = $(CXX) $(CXXFLAGS) $(LDFLAGS) -o $@
HEADERS = $(include_HEADERS)
DIST_COMMON = Makefile.am Makefile.in
DISTFILES = $(DIST_COMMON) $(SOURCES) $(HEADERS) $(TEXINFOS) $(EXTRA_DIST)
TAR = tar
GZIP = --best
DEP_FILES = .deps/fgpath.P .deps/fgstream.P .deps/strutils.P \
.deps/texcoord.P .deps/zfstream.P
CXXMKDEP = $(CXX) -M $(DEFS) $(INCLUDES) $(CPPFLAGS) $(CXXFLAGS)
SOURCES = $(libsgmisc_a_SOURCES)
OBJECTS = $(libsgmisc_a_OBJECTS)
all: Makefile $(LIBRARIES) $(HEADERS)
.SUFFIXES:
.SUFFIXES: .S .c .cxx .o .s
$(srcdir)/Makefile.in: Makefile.am $(top_srcdir)/configure.in $(ACLOCAL_M4)
cd $(top_srcdir) && $(AUTOMAKE) --gnu misc/Makefile
Makefile: $(srcdir)/Makefile.in $(top_builddir)/config.status $(BUILT_SOURCES)
cd $(top_builddir) \
&& CONFIG_FILES=$(subdir)/$@ CONFIG_HEADERS= $(SHELL) ./config.status
mostlyclean-libLIBRARIES:
clean-libLIBRARIES:
-test -z "$(lib_LIBRARIES)" || rm -f $(lib_LIBRARIES)
distclean-libLIBRARIES:
maintainer-clean-libLIBRARIES:
install-libLIBRARIES: $(lib_LIBRARIES)
@$(NORMAL_INSTALL)
$(mkinstalldirs) $(DESTDIR)$(libdir)
list='$(lib_LIBRARIES)'; for p in $$list; do \
if test -f $$p; then \
echo " $(INSTALL_DATA) $$p $(DESTDIR)$(libdir)/$$p"; \
$(INSTALL_DATA) $$p $(DESTDIR)$(libdir)/$$p; \
else :; fi; \
done
@$(POST_INSTALL)
@list='$(lib_LIBRARIES)'; for p in $$list; do \
if test -f $$p; then \
echo " $(RANLIB) $(DESTDIR)$(libdir)/$$p"; \
$(RANLIB) $(DESTDIR)$(libdir)/$$p; \
else :; fi; \
done
uninstall-libLIBRARIES:
@$(NORMAL_UNINSTALL)
list='$(lib_LIBRARIES)'; for p in $$list; do \
rm -f $(DESTDIR)$(libdir)/$$p; \
done
.s.o:
$(COMPILE) -c $<
.S.o:
$(COMPILE) -c $<
mostlyclean-compile:
-rm -f *.o core *.core
clean-compile:
distclean-compile:
-rm -f *.tab.c
maintainer-clean-compile:
libsgmisc.a: $(libsgmisc_a_OBJECTS) $(libsgmisc_a_DEPENDENCIES)
-rm -f libsgmisc.a
$(AR) cru libsgmisc.a $(libsgmisc_a_OBJECTS) $(libsgmisc_a_LIBADD)
$(RANLIB) libsgmisc.a
.cxx.o:
$(CXXCOMPILE) -c $<
install-includeHEADERS: $(include_HEADERS)
@$(NORMAL_INSTALL)
$(mkinstalldirs) $(DESTDIR)$(includedir)
@list='$(include_HEADERS)'; for p in $$list; do \
if test -f "$$p"; then d= ; else d="$(srcdir)/"; fi; \
echo " $(INSTALL_DATA) $$d$$p $(DESTDIR)$(includedir)/$$p"; \
$(INSTALL_DATA) $$d$$p $(DESTDIR)$(includedir)/$$p; \
done
uninstall-includeHEADERS:
@$(NORMAL_UNINSTALL)
list='$(include_HEADERS)'; for p in $$list; do \
rm -f $(DESTDIR)$(includedir)/$$p; \
done
tags: TAGS
ID: $(HEADERS) $(SOURCES) $(LISP)
here=`pwd` && cd $(srcdir) \
&& mkid -f$$here/ID $(SOURCES) $(HEADERS) $(LISP)
TAGS: $(HEADERS) $(SOURCES) $(TAGS_DEPENDENCIES) $(LISP)
tags=; \
here=`pwd`; \
list='$(SOURCES) $(HEADERS)'; \
unique=`for i in $$list; do echo $$i; done | \
awk ' { files[$$0] = 1; } \
END { for (i in files) print i; }'`; \
test -z "$(ETAGS_ARGS)$$unique$(LISP)$$tags" \
|| (cd $(srcdir) && etags $(ETAGS_ARGS) $$tags $$unique $(LISP) -o $$here/TAGS)
mostlyclean-tags:
clean-tags:
distclean-tags:
-rm -f TAGS ID
maintainer-clean-tags:
distdir = $(top_builddir)/$(PACKAGE)-$(VERSION)/$(subdir)
subdir = misc
distdir: $(DISTFILES)
here=`cd $(top_builddir) && pwd`; \
top_distdir=`cd $(top_distdir) && pwd`; \
distdir=`cd $(distdir) && pwd`; \
cd $(top_srcdir) \
&& $(AUTOMAKE) --include-deps --build-dir=$$here --srcdir-name=$(top_srcdir) --output-dir=$$top_distdir --gnu misc/Makefile
@for file in $(DISTFILES); do \
d=$(srcdir); \
test -f $(distdir)/$$file \
|| ln $$d/$$file $(distdir)/$$file 2> /dev/null \
|| cp -p $$d/$$file $(distdir)/$$file; \
done
DEPS_MAGIC := $(shell mkdir .deps > /dev/null 2>&1 || :)
-include $(DEP_FILES)
mostlyclean-depend:
clean-depend:
distclean-depend:
maintainer-clean-depend:
-rm -rf .deps
%.o: %.c
@echo '$(COMPILE) -c $<'; \
$(COMPILE) -Wp,-MD,.deps/$(*F).P -c $<
%.lo: %.c
@echo '$(LTCOMPILE) -c $<'; \
$(LTCOMPILE) -Wp,-MD,.deps/$(*F).p -c $<
@-sed -e 's/^\([^:]*\)\.o:/\1.lo \1.o:/' \
< .deps/$(*F).p > .deps/$(*F).P
@-rm -f .deps/$(*F).p
%.o: %.cxx
@echo '$(CXXCOMPILE) -c $<'; \
$(CXXCOMPILE) -Wp,-MD,.deps/$(*F).P -c $<
%.lo: %.cxx
@echo '$(LTCXXCOMPILE) -c $<'; \
$(LTCXXCOMPILE) -Wp,-MD,.deps/$(*F).p -c $<
@-sed -e 's/^\([^:]*\)\.o:/\1.lo \1.o:/' \
< .deps/$(*F).p > .deps/$(*F).P
@-rm -f .deps/$(*F).p
info:
dvi:
check: all
$(MAKE)
installcheck:
install-exec: install-libLIBRARIES
@$(NORMAL_INSTALL)
install-data: install-includeHEADERS
@$(NORMAL_INSTALL)
install: install-exec install-data all
@:
uninstall: uninstall-libLIBRARIES uninstall-includeHEADERS
install-strip:
$(MAKE) INSTALL_PROGRAM='$(INSTALL_PROGRAM) -s' INSTALL_SCRIPT='$(INSTALL_PROGRAM)' install
installdirs:
$(mkinstalldirs) $(DATADIR)$(libdir) $(DATADIR)$(includedir)
mostlyclean-generic:
-test -z "$(MOSTLYCLEANFILES)" || rm -f $(MOSTLYCLEANFILES)
clean-generic:
-test -z "$(CLEANFILES)" || rm -f $(CLEANFILES)
distclean-generic:
-rm -f Makefile $(DISTCLEANFILES)
-rm -f config.cache config.log stamp-h stamp-h[0-9]*
-test -z "$(CONFIG_CLEAN_FILES)" || rm -f $(CONFIG_CLEAN_FILES)
maintainer-clean-generic:
-test -z "$(MAINTAINERCLEANFILES)" || rm -f $(MAINTAINERCLEANFILES)
-test -z "$(BUILT_SOURCES)" || rm -f $(BUILT_SOURCES)
mostlyclean: mostlyclean-libLIBRARIES mostlyclean-compile \
mostlyclean-tags mostlyclean-depend mostlyclean-generic
clean: clean-libLIBRARIES clean-compile clean-tags clean-depend \
clean-generic mostlyclean
distclean: distclean-libLIBRARIES distclean-compile distclean-tags \
distclean-depend distclean-generic clean
-rm -f config.status
maintainer-clean: maintainer-clean-libLIBRARIES \
maintainer-clean-compile maintainer-clean-tags \
maintainer-clean-depend maintainer-clean-generic \
distclean
@echo "This command is intended for maintainers to use;"
@echo "it deletes files that may require special tools to rebuild."
.PHONY: mostlyclean-libLIBRARIES distclean-libLIBRARIES \
clean-libLIBRARIES maintainer-clean-libLIBRARIES uninstall-libLIBRARIES \
install-libLIBRARIES mostlyclean-compile distclean-compile \
clean-compile maintainer-clean-compile uninstall-includeHEADERS \
install-includeHEADERS tags mostlyclean-tags distclean-tags clean-tags \
maintainer-clean-tags distdir mostlyclean-depend distclean-depend \
clean-depend maintainer-clean-depend info dvi installcheck install-exec \
install-data install uninstall all installdirs mostlyclean-generic \
distclean-generic clean-generic maintainer-clean-generic clean \
mostlyclean distclean maintainer-clean
INCLUDES += \
-I$(top_builddir) \
-I$(top_builddir)/bucket \
-I$(top_builddir)/math \
$(ZLIB_INCL)
# Tell versions [3.59,3.63) of GNU make to not export all variables.
# Otherwise a system limit (for SysV at least) may be exceeded.
.NOEXPORT:
+101
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@@ -0,0 +1,101 @@
//
// fgpath.cxx -- routines to abstract out path separator differences
// between MacOS and the rest of the world
//
// Written by Curtis L. Olson, started April 1999.
//
// Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include "fgpath.hxx"
// If Unix, replace all ":" with "/". If MacOS, replace all "/" with
// ":" it should go without saying that neither of these characters
// should be used in file or directory names. In windoze, allow the
// second character to be a ":" for things like c:\foo\bar
static string fix_path( const string path ) {
string result = path;
for ( int i = 0; i < (int)path.size(); ++i ) {
#if defined( WIN32 )
// for windoze, don't replace the ":" for the second character
if ( i == 1 ) {
continue;
}
#endif
if ( result[i] == FG_BAD_PATH_SEP ) {
result[i] = FG_PATH_SEP;
}
}
return result;
}
// default constructor
FGPath::FGPath() {
path = "";
}
// create a path based on "path"
FGPath::FGPath( const string p ) {
set( p );
}
// destructor
FGPath::~FGPath() {
}
// set path
void FGPath::set( const string p ) {
path = fix_path( p );
}
// append another piece to the existing path
void FGPath::append( const string p ) {
string part = fix_path( p );
if ( path.size() == 0 ) {
path = part;
} else {
if ( part[0] != FG_PATH_SEP ) {
path += FG_PATH_SEP;
}
path += part;
}
}
// concatenate a string to the end of the path without inserting a
// path separator
void FGPath::concat( const string p ) {
string part = fix_path( p );
if ( path.size() == 0 ) {
path = part;
} else {
path += part;
}
}
+85
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@@ -0,0 +1,85 @@
//
// fgpath.hxx -- routines to abstract out path separator differences
// between MacOS and the rest of the world
//
// Written by Curtis L. Olson, started April 1999.
//
// Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _FGPATH_HXX
#define _FGPATH_HXX
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <simgear/compiler.h>
#include STL_STRING
FG_USING_STD(string);
#ifdef MACOS
# define FG_PATH_SEP ':'
# define FG_BAD_PATH_SEP '/'
#else
# define FG_PATH_SEP '/'
# define FG_BAD_PATH_SEP ':'
#endif
class FGPath {
private:
string path;
public:
// default constructor
FGPath();
// create a path based on "path"
FGPath( const string p );
// destructor
~FGPath();
// set path
void set( const string p );
// append another piece to the existing path
void append( const string p );
// concatenate a string to the end of the path without inserting a
// path separator
void concat( const string p );
// get the path string
inline string str() const { return path; }
inline const char *c_str() { return path.c_str(); }
};
#endif // _FGPATH_HXX
+158
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@@ -0,0 +1,158 @@
// zlib input file stream wrapper.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include <ctype.h> // isspace()
#include "fgstream.hxx"
fg_gzifstream::fg_gzifstream()
: istream(&gzbuf)
{
}
//-----------------------------------------------------------------------------
//
// Open a possibly gzipped file for reading.
//
fg_gzifstream::fg_gzifstream( const string& name, ios_openmode io_mode )
: istream(&gzbuf)
{
this->open( name, io_mode );
}
//-----------------------------------------------------------------------------
//
// Attach a stream to an already opened file descriptor.
//
fg_gzifstream::fg_gzifstream( int fd, ios_openmode io_mode )
: istream(&gzbuf)
{
gzbuf.attach( fd, io_mode );
}
//-----------------------------------------------------------------------------
//
// Open a possibly gzipped file for reading.
// If the initial open fails and the filename has a ".gz" extension then
// remove the extension and try again.
// If the initial open fails and the filename doesn't have a ".gz" extension
// then append ".gz" and try again.
//
void
fg_gzifstream::open( const string& name, ios_openmode io_mode )
{
gzbuf.open( name.c_str(), io_mode );
if ( ! gzbuf.is_open() )
{
string s = name;
if ( s.substr( s.length() - 3, 3 ) == ".gz" )
{
// remove ".gz" suffix
s.replace( s.length() - 3, 3, "" );
// s.erase( s.length() - 3, 3 );
}
else
{
// Append ".gz" suffix
s += ".gz";
}
// Try again.
gzbuf.open( s.c_str(), io_mode );
}
}
void
fg_gzifstream::attach( int fd, ios_openmode io_mode )
{
gzbuf.attach( fd, io_mode );
}
//
// Manipulators
//
istream&
skipeol( istream& in )
{
char c = '\0';
// skip to end of line.
#ifdef __MWERKS__
while ( in.get(c) && c != '\0' ) {
#else
while ( in.get(c) ) {
#endif
if ( (c == '\n') || (c == '\r') ) {
break;
}
}
return in;
}
istream&
skipws( istream& in ) {
char c;
#ifdef __MWERKS__
while ( in.get(c) && c != '\0' ) {
#else
while ( in.get(c) ) {
#endif
#ifdef __MWERKS__
if ( ! isspace( c ) && c != '\n' ) {
#else
if ( ! isspace( c ) ) {
#endif
// put pack the non-space character
in.putback(c);
break;
}
}
return in;
}
istream&
skipcomment( istream& in )
{
while ( in )
{
// skip whitespace
#ifdef __MWERKS__
in >> ::skipws;
#else
in >> skipws;
#endif
char c;
if ( in.get( c ) && c != '#' )
{
// not a comment
in.putback(c);
break;
}
in >> skipeol;
}
return in;
}
+102
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@@ -0,0 +1,102 @@
// zlib input file stream wrapper.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _FGSTREAM_HXX
#define _FGSTREAM_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include <simgear/compiler.h>
#if defined( FG_HAVE_STD_INCLUDES )
# include <istream>
#elif defined ( FG_HAVE_NATIVE_SGI_COMPILERS )
# include <CC/stream.h>
#elif defined ( __BORLANDC__ )
# include <iostream>
#else
# include <istream.h>
#endif
#include STL_STRING
#include <simgear/zfstream.hxx>
FG_USING_STD(string);
#ifndef FG_HAVE_NATIVE_SGI_COMPILERS
FG_USING_STD(istream);
#endif
//-----------------------------------------------------------------------------
//
// Envelope class for gzifstream.
//
class fg_gzifstream : private gzifstream_base, public istream
{
public:
//
fg_gzifstream();
// Attempt to open a file with and without ".gz" extension.
fg_gzifstream( const string& name,
ios_openmode io_mode = ios_in | ios_binary );
//
fg_gzifstream( int fd, ios_openmode io_mode = ios_in|ios_binary );
// Attempt to open a file with and without ".gz" extension.
void open( const string& name,
ios_openmode io_mode = ios_in|ios_binary );
void attach( int fd, ios_openmode io_mode = ios_in|ios_binary );
void close() { gzbuf.close(); }
bool is_open() { return gzbuf.is_open(); }
private:
// Not defined!
fg_gzifstream( const fg_gzifstream& );
void operator= ( const fg_gzifstream& );
};
// istream manipulator that skips to end of line.
istream& skipeol( istream& in );
// istream manipulator that skips over white space.
istream& skipws( istream& in );
// istream manipulator that skips comments and white space.
// A comment starts with '#'.
istream& skipcomment( istream& in );
#endif /* _FGSTREAM_HXX */
+121
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@@ -0,0 +1,121 @@
/***************************************************************************
* stopwatch.hxx Timer class, for use in benchmarking
*
* Based on blitz/Timer.h
*
* $Id$
*
* Copyright (C) 1997,1998 Todd Veldhuizen <tveldhui@seurat.uwaterloo.ca>
*
* This program is free software; you can redistribute it and/or
* modify it under the terms of the GNU General Public License
* as published by the Free Software Foundation; either version 2
* of the License, or (at your option) any later version.
*
* This program is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* Suggestions: blitz-suggest@cybervision.com
* Bugs: blitz-bugs@cybervision.com
*
* For more information, please see the Blitz++ Home Page:
* http://seurat.uwaterloo.ca/blitz/
*
*/
// This class is not portable to non System V platforms.
// It will need to be rewritten for Windows, NT, Mac.
// NEEDS_WORK
#ifndef _STOPWATCH_HXX
#define _STOPWATCH_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#if defined(__linux__) && ! defined(HAVE_GETRUSAGE)
# define HAVE_GETRUSAGE
#endif
#if defined( WIN32 ) && defined( HAVE_GETRUSAGE )
# undef HAVE_GETRUSAGE
#endif // WIN32
#if defined( HAVE_GETRUSAGE )
# if defined( __FreeBSD__ )
# include <sys/types.h>
# endif
# include <sys/time.h>
# include <sys/resource.h>
# include <unistd.h>
#elif defined( WIN32 )
# include <windows.h>
#else
# include <time.h>
#endif
class StopWatch {
public:
StopWatch()
{
// state_ = uninitialized;
}
void start()
{
// state_ = running;
t1_ = systemTime();
}
void stop()
{
t2_ = systemTime();
// BZPRECONDITION(state_ == running);
// state_ = stopped;
}
double elapsedSeconds()
{
// BZPRECONDITION(state_ == stopped);
return t2_ - t1_;
}
private:
StopWatch(StopWatch&) { }
void operator=(StopWatch&) { }
double systemTime()
{
#if defined( HAVE_GETRUSAGE )
getrusage(RUSAGE_SELF, &resourceUsage_);
double seconds = resourceUsage_.ru_utime.tv_sec
+ resourceUsage_.ru_stime.tv_sec;
double micros = resourceUsage_.ru_utime.tv_usec
+ resourceUsage_.ru_stime.tv_usec;
return seconds + micros/1.0e6;
#elif defined( WIN32 )
return double(GetTickCount()) * double(1e-3);
#else
return clock() / (double) CLOCKS_PER_SEC;
#endif
}
// enum { uninitialized, running, stopped } state_;
#if defined( HAVE_GETRUSAGE )
struct rusage resourceUsage_;
#endif
double t1_, t2_;
};
#endif // _STOPWATCH_HXX
+71
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@@ -0,0 +1,71 @@
// String utilities.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include "strutils.hxx"
const string whitespace = " \n\r\t";
//
string
trimleft( const string& s, const string& trimmings )
{
string result;
string::size_type pos = s.find_first_not_of( trimmings );
if ( pos != string::npos )
{
result.assign( s.substr( pos ) );
}
return result;
}
//
string
trimright( const string& s, const string& trimmings )
{
string result;
string::size_type pos = s.find_last_not_of( trimmings );
if ( pos == string::npos )
{
// Not found, return the original string.
result = s;
}
else
{
result.assign( s.substr( 0, pos+1 ) );
}
return result;
}
//
string
trim( const string& s, const string& trimmings )
{
return trimright( trimleft( s, trimmings ), trimmings );
}
+65
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@@ -0,0 +1,65 @@
// String utilities.
//
// Written by Bernie Bright, 1998
//
// Copyright (C) 1998 Bernie Bright - bbright@c031.aone.net.au
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef STRUTILS_H
#define STRUTILS_H
#include <simgear/compiler.h>
#include STL_STRING
#ifdef FG_HAVE_STD_INCLUDES
# include <cstdlib>
#else
# include <stdlib.h>
#endif
FG_USING_STD(string);
// Default characters to remove.
extern const string whitespace;
// Returns a string with trailing characters removed.
string trimleft( const string& s, const string& trimmings = whitespace );
// Returns a string with leading characters removed.
string trimright( const string& s, const string& trimmings = whitespace );
// Returns a string with leading and trailing characters removed.
string trim( const string& s, const string& trimmings = whitespace );
//-----------------------------------------------------------------------------
inline double
atof( const string& str )
{
return ::atof( str.c_str() );
}
inline int
atoi( const string& str )
{
return ::atoi( str.c_str() );
}
#endif // STRUTILS_H
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// texcoord.hxx -- routine(s) to handle texture coordinate generation
//
// Written by Curtis Olson, started March 1999.
//
// Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#include "texcoord.hxx"
#define FG_STANDARD_TEXTURE_DIMENSION 1000.0 // meters
#define MAX_TEX_COORD 8.0
#define HALF_MAX_TEX_COORD ( MAX_TEX_COORD / 2.0 )
// return the basic unshifted/unmoded texture coordinate for a lat/lon
inline Point3D basic_tex_coord( const Point3D& p,
double degree_width, double degree_height,
double scale )
{
return Point3D( p.x() * ( degree_width * scale /
FG_STANDARD_TEXTURE_DIMENSION ),
p.y() * ( degree_width * scale /
FG_STANDARD_TEXTURE_DIMENSION ),
0.0 );
}
// traverse the specified fan/strip/list of vertices and attempt to
// calculate "none stretching" texture coordinates
point_list calc_tex_coords( const FGBucket& b, const point_list& geod_nodes,
const int_list& fan, double scale )
{
// cout << "calculating texture coordinates for a specific fan of size = "
// << fan.size() << endl;
// calculate perimeter based on center of this degree (not center
// of bucket)
double clat = (int)b.get_center_lat();
if ( clat > 0 ) {
clat = (int)clat + 0.5;
} else {
clat = (int)clat - 0.5;
}
double clat_rad = clat * DEG_TO_RAD;
double cos_lat = cos( clat_rad );
double local_radius = cos_lat * EQUATORIAL_RADIUS_M;
double local_perimeter = 2.0 * local_radius * FG_PI;
double degree_width = local_perimeter / 360.0;
// cout << "clat = " << clat << endl;
// cout << "clat (radians) = " << clat_rad << endl;
// cout << "cos(lat) = " << cos_lat << endl;
// cout << "local_radius = " << local_radius << endl;
// cout << "local_perimeter = " << local_perimeter << endl;
// cout << "degree_width = " << degree_width << endl;
double perimeter = 2.0 * EQUATORIAL_RADIUS_M * FG_PI;
double degree_height = perimeter / 360.0;
// cout << "degree_height = " << degree_height << endl;
// find min/max of fan
Point3D tmin, tmax, p, t;
bool first = true;
for ( int i = 0; i < (int)fan.size(); ++i ) {
p = geod_nodes[ fan[i] ];
// cout << "point p = " << p << endl;
t = basic_tex_coord( p, degree_width, degree_height, scale );
// cout << "basic_tex_coord = " << t << endl;
if ( first ) {
tmin = tmax = t;
first = false;
} else {
if ( t.x() < tmin.x() ) {
tmin.setx( t.x() );
}
if ( t.y() < tmin.y() ) {
tmin.sety( t.y() );
}
if ( t.x() > tmax.x() ) {
tmax.setx( t.x() );
}
if ( t.y() > tmax.y() ) {
tmax.sety( t.y() );
}
}
}
double dx = fabs( tmax.x() - tmin.x() );
double dy = fabs( tmax.y() - tmin.y() );
// cout << "dx = " << dx << " dy = " << dy << endl;
bool do_shift = false;
Point3D mod_shift;
if ( (dx > HALF_MAX_TEX_COORD) || (dy > HALF_MAX_TEX_COORD) ) {
// structure is too big, we'll just have to shift it so that
// tmin = (0,0). This messes up subsequent texture scaling,
// but is the best we can do.
// cout << "SHIFTING" << endl;
do_shift = true;
tmin.setx( (double)( (int)tmin.x() + 1 ) );
tmin.sety( (double)( (int)tmin.y() + 1 ) );
// cout << "found tmin = " << tmin << endl;
} else {
// structure is small enough ... we can mod it so we can
// properly scale the texture coordinates later.
// cout << "MODDING" << endl;
double x1 = fmod(tmin.x(), MAX_TEX_COORD);
while ( x1 < 0 ) { x1 += MAX_TEX_COORD; }
double y1 = fmod(tmin.y(), MAX_TEX_COORD);
while ( y1 < 0 ) { y1 += MAX_TEX_COORD; }
double x2 = fmod(tmax.x(), MAX_TEX_COORD);
while ( x2 < 0 ) { x2 += MAX_TEX_COORD; }
double y2 = fmod(tmax.y(), MAX_TEX_COORD);
while ( y2 < 0 ) { y2 += MAX_TEX_COORD; }
// At this point we know that the object is < 16 wide in
// texture coordinate space. If the modulo of the tmin is >
// the mod of the tmax at this point, then we know that the
// starting tex coordinate for the tmin > 16 so we can shift
// everything down by 16 and get it within the 0-32 range.
if ( x1 > x2 ) {
mod_shift.setx( HALF_MAX_TEX_COORD );
} else {
mod_shift.setx( 0.0 );
}
if ( y1 > y2 ) {
mod_shift.sety( HALF_MAX_TEX_COORD );
} else {
mod_shift.sety( 0.0 );
}
// cout << "mod_shift = " << mod_shift << endl;
}
// generate tex_list
Point3D adjusted_t;
point_list tex;
tex.clear();
for ( int i = 0; i < (int)fan.size(); ++i ) {
p = geod_nodes[ fan[i] ];
t = basic_tex_coord( p, degree_width, degree_height, scale );
// cout << "second t = " << t << endl;
if ( do_shift ) {
adjusted_t = t - tmin;
} else {
adjusted_t.setx( fmod(t.x() + mod_shift.x(), MAX_TEX_COORD) );
while ( adjusted_t.x() < 0 ) {
adjusted_t.setx( adjusted_t.x() + MAX_TEX_COORD );
}
adjusted_t.sety( fmod(t.y() + mod_shift.y(), MAX_TEX_COORD) );
while ( adjusted_t.y() < 0 ) {
adjusted_t.sety( adjusted_t.y() + MAX_TEX_COORD );
}
// cout << "adjusted_t " << adjusted_t << endl;
}
if ( adjusted_t.x() < FG_EPSILON ) {
adjusted_t.setx( 0.0 );
}
if ( adjusted_t.y() < FG_EPSILON ) {
adjusted_t.sety( 0.0 );
}
adjusted_t.setz( 0.0 );
// cout << "adjusted_t = " << adjusted_t << endl;
tex.push_back( adjusted_t );
}
return tex;
}
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// texcoord.hxx -- routine(s) to handle texture coordinate generation
//
// Written by Curtis Olson, started March 1999.
//
// Copyright (C) 1999 Curtis L. Olson - curt@flightgear.org
//
// This program is free software; you can redistribute it and/or
// modify it under the terms of the GNU General Public License as
// published by the Free Software Foundation; either version 2 of the
// License, or (at your option) any later version.
//
// This program is distributed in the hope that it will be useful, but
// WITHOUT ANY WARRANTY; without even the implied warranty of
// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
// General Public License for more details.
//
// You should have received a copy of the GNU General Public License
// along with this program; if not, write to the Free Software
// Foundation, Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
//
// $Id$
#ifndef _TEXCOORD_HXX
#define _TEXCOORD_HXX
#ifndef __cplusplus
# error This library requires C++
#endif
#include <simgear/newbucket.hxx>
#include <simgear/fg_types.hxx>
// traverse the specified fan/strip/list of vertices and attempt to
// calculate "none stretching" texture coordinates
point_list calc_tex_coords( const FGBucket& b, const point_list& geod_nodes,
const int_list& fan, double scale = 1.0 );
#endif // _TEXCOORD_HXX

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