Initial revision
This commit is contained in:
@@ -0,0 +1,19 @@
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noinst_LIBRARIES = libAstro.a
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libAstro_a_SOURCES = \
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celestialBody.cxx celestialBody.hxx \
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jupiter.cxx jupiter.hxx \
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mars.cxx mars.hxx \
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mercury.cxx mercury.hxx \
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moon.cxx moon.hxx \
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neptune.cxx neptune.hxx \
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pluto.hxx \
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saturn.cxx saturn.hxx \
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sky.cxx sky.hxx \
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solarsystem.cxx solarsystem.hxx \
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star.cxx star.hxx \
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stars.cxx stars.hxx \
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uranus.cxx uranus.hxx \
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venus.cxx venus.hxx
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INCLUDES += -I$(top_builddir) -I$(top_builddir)/Lib -I$(top_builddir)/Simulator
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@@ -0,0 +1,176 @@
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/**************************************************************************
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* celestialBody.cxx
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* 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.
|
||||
*
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||||
* $Id$
|
||||
**************************************************************************/
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#include "celestialBody.hxx"
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#include "star.hxx"
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#include <Debug/logstream.hxx>
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#ifdef FG_MATH_EXCEPTION_CLASH
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# define exception c_exception
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#endif
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#include <math.h>
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/**************************************************************************
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* void CelestialBody::updatePosition(fgTIME *t, Star *ourSun)
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*
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* Basically, this member function provides a general interface for
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* calculating the right ascension and declinaion. This function is
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* used for calculating the planetary positions. For the planets, an
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* overloaded member function is provided to additionally calculate the
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* planet's magnitude.
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* The sun and moon have their own overloaded updatePosition member, as their
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* position is calculated an a slightly different manner.
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*
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* arguments:
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* fgTIME t: provides the current time.
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* Star *ourSun: the sun's position is needed to convert heliocentric
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* coordinates into geocentric coordinates.
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*
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* return value: none
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*
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*************************************************************************/
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void CelestialBody::updatePosition(FGTime *t, Star *ourSun)
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{
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double eccAnom, v, ecl, actTime,
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xv, yv, xh, yh, zh, xg, yg, zg, xe, ye, ze;
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updateOrbElements(t);
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actTime = fgCalcActTime(t);
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// calcualate the angle bewteen ecliptic and equatorial coordinate system
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ecl = DEG_TO_RAD * (23.4393 - 3.563E-7 *actTime);
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eccAnom = fgCalcEccAnom(M, e); //calculate the eccentric anomaly
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xv = a * (cos(eccAnom) - e);
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yv = a * (sqrt (1.0 - e*e) * sin(eccAnom));
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v = atan2(yv, xv); // the planet's true anomaly
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r = sqrt (xv*xv + yv*yv); // the planet's distance
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// calculate the planet's position in 3D space
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xh = r * (cos(N) * cos(v+w) - sin(N) * sin(v+w) * cos(i));
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yh = r * (sin(N) * cos(v+w) + cos(N) * sin(v+w) * cos(i));
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zh = r * (sin(v+w) * sin(i));
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// calculate the ecliptic longitude and latitude
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xg = xh + ourSun->getxs();
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yg = yh + ourSun->getys();
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zg = zh;
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lonEcl = atan2(yh, xh);
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latEcl = atan2(zh, sqrt(xh*xh+yh*yh));
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xe = xg;
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ye = yg * cos(ecl) - zg * sin(ecl);
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ze = yg * sin(ecl) + zg * cos(ecl);
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rightAscension = atan2(ye, xe);
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declination = atan2(ze, sqrt(xe*xe + ye*ye));
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FG_LOG(FG_GENERAL, FG_INFO, "Planet found at : "
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<< rightAscension << " (ra), " << declination << " (dec)" );
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//calculate some variables specific to calculating the magnitude
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//of the planet
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R = sqrt (xg*xg + yg*yg + zg*zg);
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s = ourSun->getDistance();
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// It is possible from these calculations for the argument to acos
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// to exceed the valid range for acos(). So we do a little extra
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// checking.
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double tmp = (r*r + R*R - s*s) / (2*r*R);
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if ( tmp > 1.0) {
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tmp = 1.0;
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} else if ( tmp < -1.0) {
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tmp = -1.0;
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}
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FV = RAD_TO_DEG * acos( tmp );
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};
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/****************************************************************************
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* double CelestialBody::fgCalcEccAnom(double M, double e)
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* this private member calculates the eccentric anomaly of a celestial body,
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* given its mean anomaly and eccentricity.
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*
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* -Mean anomaly: the approximate angle between the perihelion and the current
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* position. this angle increases uniformly with time.
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*
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* True anomaly: the actual angle between perihelion and current position.
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*
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* Eccentric anomaly: this is an auxilary angle, used in calculating the true
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* anomaly from the mean anomaly.
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*
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* -eccentricity. Indicates the amount in which the orbit deviates from a
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* circle (0 = circle, 0-1, is ellipse, 1 = parabola, > 1 = hyperbola).
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*
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* This function is also known as solveKeplersEquation()
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*
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* arguments:
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* M: the mean anomaly
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* e: the eccentricity
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*
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* return value:
|
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* the eccentric anomaly
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*
|
||||
****************************************************************************/
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double CelestialBody::fgCalcEccAnom(double M, double e)
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{
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double
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eccAnom, E0, E1, diff;
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|
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eccAnom = M + e * sin(M) * (1.0 + e * cos (M));
|
||||
// iterate to achieve a greater precision for larger eccentricities
|
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if (e > 0.05)
|
||||
{
|
||||
E0 = eccAnom;
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do
|
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{
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E1 = E0 - (E0 - e * sin(E0) - M) / (1 - e *cos(E0));
|
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diff = fabs(E0 - E1);
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E0 = E1;
|
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}
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while (diff > (DEG_TO_RAD * 0.001));
|
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return E0;
|
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}
|
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return eccAnom;
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}
|
||||
|
||||
|
||||
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|
||||
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||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
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@@ -0,0 +1,195 @@
|
||||
/**************************************************************************
|
||||
* 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_
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#define _CELESTIALBODY_H_
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#ifndef __cplusplus
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# error This library requires C++
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#endif
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|
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|
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#include <Time/fg_time.hxx>
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#include <Include/fg_constants.h>
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class Star;
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class CelestialBody
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{
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protected: // make the data protected, in order to give the inherited
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// classes direct access to the data
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double NFirst; /* longitude of the ascending node first part */
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double NSec; /* longitude of the ascending node second part */
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double iFirst; /* inclination to the ecliptic first part */
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double iSec; /* inclination to the ecliptic second part */
|
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double wFirst; /* first part of argument of perihelion */
|
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double wSec; /* second part of argument of perihelion */
|
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double aFirst; /* semimayor axis first part*/
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double aSec; /* semimayor axis second part */
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double eFirst; /* eccentricity first part */
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double eSec; /* eccentricity second part */
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double MFirst; /* Mean anomaly first part */
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double MSec; /* Mean anomaly second part */
|
||||
|
||||
double N, i, w, a, e, M; /* the resulting orbital elements, obtained from the former */
|
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|
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double rightAscension, declination;
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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,
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||||
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.
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* 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_
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
@@ -0,0 +1,65 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
}
|
||||
|
||||
|
||||
|
||||
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,59 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
}
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,61 @@
|
||||
/**************************************************************************
|
||||
* 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);
|
||||
}
|
||||
|
||||
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,401 @@
|
||||
/**************************************************************************
|
||||
* 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 <FDM/flight.hxx>
|
||||
|
||||
#include <string.h>
|
||||
#include "moon.hxx"
|
||||
|
||||
#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>
|
||||
|
||||
|
||||
/*************************************************************************
|
||||
* 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;
|
||||
|
||||
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 = (int)((double)0xff * (t * t));
|
||||
*(p+1) = (int)((double) 0xff * (t*t));
|
||||
*(p+2) = (int)((double) 0xff * (t*t));
|
||||
*(p+3) = 0x11;
|
||||
}
|
||||
else
|
||||
{
|
||||
*p = 0x00;
|
||||
*(p+1) = 0x00;
|
||||
*(p+2) = 0x00;
|
||||
*(p+3) = 0x11;
|
||||
}
|
||||
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 = ¤t_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 = 750;
|
||||
|
||||
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);
|
||||
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 );
|
||||
// xglEnable( 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
|
||||
{
|
||||
}
|
||||
}
|
||||
@@ -0,0 +1,56 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,59 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
}
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,36 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,69 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
}
|
||||
|
||||
@@ -0,0 +1,45 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
@@ -0,0 +1,367 @@
|
||||
// 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 float inner_color[12][4];
|
||||
static float middle_color[12][4];
|
||||
static float 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] = l->sky_color[j] - diff * 0.3;
|
||||
middle_color[i][j] = l->sky_color[j] - diff * 0.9 + middle_amt[j];
|
||||
outer_color[i][j] = l->fog_color[j] + outer_amt[j];
|
||||
|
||||
if ( inner_color[i][j] > 1.00 ) { inner_color[i][j] = 1.00; }
|
||||
if ( inner_color[i][j] < 0.10 ) { inner_color[i][j] = 0.10; }
|
||||
if ( middle_color[i][j] > 1.00 ) { middle_color[i][j] = 1.00; }
|
||||
if ( middle_color[i][j] < 0.10 ) { middle_color[i][j] = 0.10; }
|
||||
if ( outer_color[i][j] > 1.00 ) { outer_color[i][j] = 1.00; }
|
||||
if ( outer_color[i][j] < 0.10 ) { outer_color[i][j] = 0.10; }
|
||||
}
|
||||
inner_color[i][3] = middle_color[i][3] = outer_color[i][3] =
|
||||
l->sky_color[3];
|
||||
|
||||
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] = l->sky_color[j] - diff * 0.3;
|
||||
middle_color[i][j] = l->sky_color[j] - diff * 0.9 + middle_amt[j];
|
||||
outer_color[i][j] = l->fog_color[j] + outer_amt[j];
|
||||
|
||||
if ( inner_color[i][j] > 1.00 ) { inner_color[i][j] = 1.00; }
|
||||
if ( inner_color[i][j] < 0.10 ) { inner_color[i][j] = 0.10; }
|
||||
if ( middle_color[i][j] > 1.00 ) { middle_color[i][j] = 1.00; }
|
||||
if ( middle_color[i][j] < 0.10 ) { middle_color[i][j] = 0.10; }
|
||||
if ( outer_color[i][j] > 1.00 ) { outer_color[i][j] = 1.00; }
|
||||
if ( outer_color[i][j] < 0.15 ) { outer_color[i][j] = 0.15; }
|
||||
}
|
||||
inner_color[i][3] = middle_color[i][3] = outer_color[i][3] =
|
||||
l->sky_color[3];
|
||||
|
||||
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;
|
||||
float inner_color[4];
|
||||
float middle_color[4];
|
||||
float 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] = l->sky_color[i] - diff * 0.3;
|
||||
middle_color[i] = l->sky_color[i] - diff * 0.9;
|
||||
outer_color[i] = l->adj_fog_color[i];
|
||||
}
|
||||
inner_color[3] = middle_color[3] = outer_color[3] = l->adj_fog_color[3];
|
||||
|
||||
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 );
|
||||
xglColor4fv(l->sky_color);
|
||||
xglVertex3f(0.0, 0.0, CENTER_ELEV);
|
||||
for ( i = 11; i >= 0; i-- ) {
|
||||
xglColor4fv( inner_color );
|
||||
xglVertex3fv( inner_vertex[i] );
|
||||
}
|
||||
xglColor4fv( inner_color );
|
||||
xglVertex3fv( inner_vertex[11] );
|
||||
xglEnd();
|
||||
|
||||
// Draw the middle ring
|
||||
xglBegin( GL_TRIANGLE_STRIP );
|
||||
for ( i = 0; i < 12; i++ ) {
|
||||
xglColor4fv( 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] );
|
||||
xglColor4fv( 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] );
|
||||
}
|
||||
xglColor4fv( middle_color );
|
||||
// xglColor4f(1.0, 0.0, 0.0, 1.0);
|
||||
xglVertex3fv( middle_vertex[0] );
|
||||
xglColor4fv( 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++ ) {
|
||||
xglColor4fv( outer_color );
|
||||
xglVertex3fv( outer_vertex[i] );
|
||||
xglColor4fv( middle_color );
|
||||
xglVertex3fv( middle_vertex[i] );
|
||||
}
|
||||
xglColor4fv( outer_color );
|
||||
xglVertex3fv( outer_vertex[0] );
|
||||
xglColor4fv( middle_color );
|
||||
xglVertex3fv( middle_vertex[0] );
|
||||
xglEnd();
|
||||
|
||||
// Draw the bottom skirt
|
||||
xglBegin( GL_TRIANGLE_STRIP );
|
||||
xglColor4fv( 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();
|
||||
}
|
||||
|
||||
|
||||
@@ -0,0 +1,45 @@
|
||||
// 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
|
||||
|
||||
|
||||
// (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
|
||||
|
||||
|
||||
@@ -0,0 +1,215 @@
|
||||
/**************************************************************************
|
||||
* 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();
|
||||
}
|
||||
@@ -0,0 +1,91 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,271 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
|
||||
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 = (int)((double)0xff * (t * t));
|
||||
*(p+1) = (int)((double) 0xff * (t*t));
|
||||
*(p+2) = (int)((double) 0xff * (t*t));
|
||||
*(p+3) = (int)((double) 0xff * (t*t));
|
||||
}
|
||||
else
|
||||
{
|
||||
*p = 0x00;
|
||||
*(p+1) = 0x00;
|
||||
*(p+2) = 0x00;
|
||||
*(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 = 750;
|
||||
|
||||
// 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);
|
||||
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
|
||||
}
|
||||
}
|
||||
@@ -0,0 +1,98 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
|
||||
@@ -0,0 +1,267 @@
|
||||
// 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");
|
||||
}
|
||||
}
|
||||
|
||||
|
||||
@@ -0,0 +1,47 @@
|
||||
// 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
|
||||
|
||||
|
||||
@@ -0,0 +1,60 @@
|
||||
/**************************************************************************
|
||||
* 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;
|
||||
}
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
@@ -0,0 +1,60 @@
|
||||
/**************************************************************************
|
||||
* 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);
|
||||
}
|
||||
@@ -0,0 +1,38 @@
|
||||
/**************************************************************************
|
||||
* 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_
|
||||
Reference in New Issue
Block a user