476 lines
16 KiB
C++
476 lines
16 KiB
C++
// coremag.cxx -- compute local magnetic variation given position,
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// altitude, and date
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//
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// This is an implementation of the NIMA (formerly DMA) WMM2000
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//
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// http://www.nima.mil/GandG/ngdc-wmm2000.html
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//
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// Copyright (C) 2000 Edward A Williams <Ed_Williams@compuserve.com>
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//
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// Adapted from Excel 3.0 version 3/27/94 EAW
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// Recoded in C++ by Starry Chan
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// WMM95 added and rearranged in ANSI-C EAW 7/9/95
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// Put shell around program and made Borland & GCC compatible EAW 11/22/95
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// IGRF95 added 2/96 EAW
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// WMM2000 IGR2000 added 2/00 EAW
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// Released under GPL 3/26/00 EAW
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// Adaptions and modifications for the SimGear project 3/27/2000 CLO
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//
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// Removed all pow() calls and made static roots[][] arrays to
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// save many sqrt() calls on subsequent invocations
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// left old code as SGMagVarOrig() for testing purposes
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// 3/28/2000 Norman Vine -- nhv@yahoo.com
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//
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// Put in some bullet-proofing to handle magnetic and geographic poles.
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// 3/28/2000 EAW
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//
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// Updated coefficient arrays to use the current wmm2005 model,
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// (valid between 2005.0 and 2010.0)
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// Also removed unused variables and corrected earth radii constants
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// to the values for WGS84 and WMM2005.
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// Reference:
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// McLean, S., S. Macmillan, S. Maus, V. Lesur, A.
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// Thomson, and D. Dater, December 2004, The
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// US/UK World Magnetic Model for 2005-2010,
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// NOAA Technical Report NESDIS/NGDC-1.
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//
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// 25/10/2006 Wim Van Hoydonck -- wim.van.hoydonck@gmail.com
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//
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//
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// Updated coefficient arrays to use the current WMM2015 model,
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// (valid between 2015.0 and 2020.0)
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// Also removed unused variables and corrected earth radii constants
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// to the values for WGS84 and WMM2015.
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// Reference:
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// A. Chulliat , S. Macmillan, P. Alken, C. Beggan, M.
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// Nair, B. Hamilton, A. Woods, V. Ridley,
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// S Maus, and A Thomson, December 2014, The
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// US/UK World Magnetic Model for 2015-2020,
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// NOAA Technical Report WMM2015_Report.pdf
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//
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// 18/06/2015 Jean-Paul Anceaux -- j.p.r.anceaux@gmail.com
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// The routine uses a spherical harmonic expansion of the magnetic
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// potential up to twelfth order, together with its time variation, as
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// described in Chapter 4 of "Geomagnetism, Vol 1, Ed. J.A.Jacobs,
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// Academic Press (London 1987)". The program first converts geodetic
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// coordinates (lat/long on elliptic earth and altitude) to spherical
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// geocentric (spherical lat/long and radius) coordinates. Using this,
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// the spherical (B_r, B_theta, B_phi) magnetic field components are
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// computed from the model. These are finally referred to surface (X, Y,
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// Z) coordinates.
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//
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// Fields are accurate to better than 200nT, variation and dip to
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// better than 0.5 degrees, with the exception of the declination near
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// the magnetic poles (where it is ill-defined) where the error may reach
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// 4 degrees or more.
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//
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// Variation is undefined at both the geographic and
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// magnetic poles, even though the field itself is well-behaved. To
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// avoid the routine blowing up, latitude entries corresponding to
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// the geographic poles are slightly offset. At the magnetic poles,
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// the routine returns zero variation.
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//
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// This library is free software; you can redistribute it and/or
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// modify it under the terms of the GNU Library General Public
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// License as published by the Free Software Foundation; either
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// version 2 of the License, or (at your option) any later version.
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//
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// This library is distributed in the hope that it will be useful,
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// but WITHOUT ANY WARRANTY; without even the implied warranty of
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// MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
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// Library General Public License for more details.
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//
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// You should have received a copy of the GNU General Public License
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// along with this program; if not, write to the Free Software
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// Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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//
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// $Id$
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#include <stdio.h>
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#include <stdlib.h>
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#include <cmath>
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#include <simgear/constants.h>
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#include <simgear/sg_inlines.h>
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#include "coremag.hxx"
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static const double a = 6378.137; /* semi-major axis (equatorial radius) of WGS84 ellipsoid */
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static const double b = 6356.7523142; /* semi-minor axis referenced to the WGS84 ellipsoid */
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static const double r_0 = 6371.2; /* standard Earth magnetic reference radius */
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static double gnm_wmm2015[13][13] =
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{
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{0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-29438.5, -1501.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-2445.3, 3012.5, 1676.6, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{1351.1, -2352.3, 1225.6, 581.9, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{907.2, 813.7, 120.3, -335.0, 70.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-232.6, 360.1, 192.4, -141.0, -157.4, 4.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{69.5, 67.4, 72.8, -129.8, -29.0, 13.2, -70.9, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{81.6, -76.1, -6.8, 51.9, 15.0, 9.3, -2.8, 6.7, 0.0, 0.0, 0.0, 0.0, 0.0},
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{24.0, 8.6, -16.9, -3.2, -20.6, 13.3, 11.7, -16.0, -2.0, 0.0, 0.0, 0.0, 0.0},
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{5.4, 8.8, 3.1, -3.1, 0.6, -13.3, -0.1, 8.7, -9.1, -10.5, 0.0, 0.0, 0.0},
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{-1.9, -6.5, 0.2, 0.6, -0.6, 1.7, -0.7, 2.1, 2.3, -1.8, -3.6, 0.0, 0.0},
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{3.1, -1.5, -2.3, 2.1, -0.9, 0.6, -0.7, 0.2, 1.7, -0.2, 0.4, 3.5, 0.0},
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{-2.0, -0.3, 0.4, 1.3, -0.9, 0.9, 0.1, 0.5, -0.4, -0.4, 0.2, -0.9, 0.0},
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};
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static double hnm_wmm2015[13][13]=
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{
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{0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 4796.2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -2845.6, -642.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -115.3, 245.0, -538.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 283.4, -188.6, 180.9, -329.5, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 47.4, 196.9, -119.4, 16.1, 100.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -20.7, 33.2, 58.8, -66.5, 7.3, 62.5, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -54.1, -19.4, 5.6, 24.4, 3.3, -27.5, -2.3, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 10.2, -18.1, 13.2, -14.6, 16.2, 5.7, -9.1, 2.2, 0.0, 0.0, 0.0, 0.0},
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{0.0, -21.6, 10.8, 11.7, -6.8, -6.9, 7.8, 1.0, -3.9, 8.5, 0.0, 0.0, 0.0},
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{0.0, 3.3, -0.3, 4.6, 4.4, -7.9, -0.6, -4.1, -2.8, -1.1, -8.7, 0.0, 0.0},
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{0.0, -0.1, 2.1, -0.7, -1.1, 0.7, -0.2, -2.1, -1.5, -2.5, -2.0, -2.3, 0.0},
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{0.0, -1.0, 0.5, 1.8, -2.2, 0.3, 0.7, -0.1, 0.3, 0.2, -0.9, -0.2, 0.7},
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};
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static double gtnm_wmm2015[13][13]=
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{
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{0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{10.7, 17.9, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-8.6, -3.3, 2.4, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{3.1, -6.2, -0.4, -10.4, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-0.4, 0.8, -9.2, 4.0, -4.2, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-0.2, 0.1, -1.4, 0.0, 1.3, 3.8, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{-0.5, -0.2, -0.6, 2.4, -1.1, 0.3, 1.5, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.2, -0.2, -0.4, 1.3, 0.2, -0.4, -0.9, 0.3, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 0.1, -0.5, 0.5, -0.2, 0.4, 0.2, -0.4, 0.3, 0.0, 0.0, 0.0, 0.0},
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{0.0, -0.1, -0.1, 0.4, -0.5, -0.2, 0.1, 0.0, -0.2, -0.1, 0.0, 0.0, 0.0},
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{0.0, 0.0, -0.1, 0.3, -0.1, -0.1, -0.1, 0.0, -0.2, -0.1, -0.2, 0.0, 0.0},
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{0.0, 0.0, -0.1, 0.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, -0.1, -0.1, 0.0},
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{0.1, 0.0, 0.0, 0.1, -0.1, 0.0, 0.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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};
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static double htnm_wmm2015[13][13]=
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{
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{0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -26.8, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -27.1, -13.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 8.4, -0.4, 2.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -0.6, 5.3, 3.0, -5.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 0.4, 1.6, -1.1, 3.3, 0.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 0.0, -2.2, -0.7, 0.1, 1.0, 1.3, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, 0.7, 0.5, -0.2, -0.1, -0.7, 0.1, 0.1, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -0.3, 0.3, 0.3, 0.6, -0.1, -0.2, 0.3, 0.0, 0.0, 0.0, 0.0, 0.0},
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{0.0, -0.2, -0.1, -0.2, 0.1, 0.1, 0.0, -0.2, 0.4, 0.3, 0.0, 0.0, 0.0},
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{0.0, 0.1, -0.1, 0.0, 0.0, -0.2, 0.1, -0.1, -0.2, 0.1, -0.1, 0.0, 0.0},
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{0.0, 0.0, 0.1, 0.0, 0.1, 0.0, 0.0, 0.1, 0.0, -0.1, 0.0, -0.1, 0.0},
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{0.0, 0.0, 0.0, -0.1, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
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};
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static const int nmax = 12;
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static double P[13][13];
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static double DP[13][13];
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static double gnm[13][13];
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static double hnm[13][13];
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static double sm[13];
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static double cm[13];
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static double root[13];
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static double roots[13][13][2];
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/* Convert date to Julian day 1950-2049 */
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unsigned long int yymmdd_to_julian_days( int yy, int mm, int dd )
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{
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unsigned long jd;
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yy = (yy < 50) ? (2000 + yy) : (1900 + yy);
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jd = dd - 32075L + 1461L * (yy + 4800L + (mm - 14) / 12 ) / 4;
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jd = jd + 367L * (mm - 2 - (mm - 14) / 12*12) / 12;
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jd = jd - 3 * ((yy + 4900L + (mm - 14) / 12) / 100) / 4;
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/* printf("julian date = %d\n", jd ); */
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return jd;
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}
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/*
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* return variation (in radians) given geodetic latitude (radians),
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* longitude(radians), height (km) and (Julian) date
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* N and E lat and long are positive, S and W negative
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*/
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double calc_magvar( double lat, double lon, double h, long dat, double* field )
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{
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/* output field B_r,B_th,B_phi,B_x,B_y,B_z */
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int n,m;
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/* reference date for current model is 1 januari 2015 */
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long date0_wmm2015 = yymmdd_to_julian_days(15,1,1);
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double yearfrac,sr,r,theta,c,s,psi,fn,fn_0,B_r,B_theta,B_phi,X,Y,Z;
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double sinpsi, cospsi, inv_s;
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static int been_here = 0;
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double sinlat = sin(lat);
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double coslat = cos(lat);
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/* convert to geocentric coords: */
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// sr = sqrt(pow(a*coslat,2.0)+pow(b*sinlat,2.0));
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sr = sqrt(a*a*coslat*coslat + b*b*sinlat*sinlat);
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/* sr is effective radius */
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theta = atan2(coslat * (h*sr + a*a),
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sinlat * (h*sr + b*b));
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/* theta is geocentric co-latitude */
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r = h*h + 2.0*h * sr +
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(a*a*a*a - ( a*a*a*a - b*b*b*b ) * sinlat*sinlat ) /
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(a*a - (a*a - b*b) * sinlat*sinlat );
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r = sqrt(r);
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/* r is geocentric radial distance */
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c = cos(theta);
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s = sin(theta);
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/* protect against zero divide at geographic poles */
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inv_s = 1.0 / (s + (s == 0.)*1.0e-8);
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/* zero out arrays */
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for ( n = 0; n <= nmax; n++ ) {
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for ( m = 0; m <= n; m++ ) {
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P[n][m] = 0;
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DP[n][m] = 0;
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}
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}
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/* diagonal elements */
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P[0][0] = 1;
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P[1][1] = s;
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DP[0][0] = 0;
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DP[1][1] = c;
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P[1][0] = c ;
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DP[1][0] = -s;
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// these values will not change for subsequent function calls
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if( !been_here ) {
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for ( n = 2; n <= nmax; n++ ) {
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root[n] = sqrt((2.0*n-1) / (2.0*n));
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}
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for ( m = 0; m <= nmax; m++ ) {
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double mm = m*m;
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for ( n = SG_MAX2(m + 1, 2); n <= nmax; n++ ) {
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roots[m][n][0] = sqrt((n-1)*(n-1) - mm);
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roots[m][n][1] = 1.0 / sqrt( n*n - mm);
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}
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}
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been_here = 1;
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}
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for ( n=2; n <= nmax; n++ ) {
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// double root = sqrt((2.0*n-1) / (2.0*n));
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P[n][n] = P[n-1][n-1] * s * root[n];
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DP[n][n] = (DP[n-1][n-1] * s + P[n-1][n-1] * c) *
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root[n];
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}
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/* lower triangle */
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for ( m = 0; m <= nmax; m++ ) {
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// double mm = m*m;
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for ( n = SG_MAX2(m + 1, 2); n <= nmax; n++ ) {
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// double root1 = sqrt((n-1)*(n-1) - mm);
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// double root2 = 1.0 / sqrt( n*n - mm);
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P[n][m] = (P[n-1][m] * c * (2.0*n-1) -
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P[n-2][m] * roots[m][n][0]) *
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roots[m][n][1];
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DP[n][m] = ((DP[n-1][m] * c - P[n-1][m] * s) *
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(2.0*n-1) - DP[n-2][m] * roots[m][n][0]) *
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roots[m][n][1];
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}
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}
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/* compute Gauss coefficients gnm and hnm of degree n and order m for the desired time
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achieved by adjusting the coefficients at time t0 for linear secular variation */
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/* WMM2015 */
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yearfrac = (dat - date0_wmm2015) / 365.25;
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for ( n = 1; n <= nmax; n++ ) {
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for ( m = 0; m <= nmax; m++ ) {
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gnm[n][m] = gnm_wmm2015[n][m] + yearfrac * gtnm_wmm2015[n][m];
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hnm[n][m] = hnm_wmm2015[n][m] + yearfrac * htnm_wmm2015[n][m];
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}
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}
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/* compute sm (sin(m lon) and cm (cos(m lon)) */
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for ( m = 0; m <= nmax; m++ ) {
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sm[m] = sin(m * lon);
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cm[m] = cos(m * lon);
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}
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/* compute B fields */
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B_r = 0.0;
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B_theta = 0.0;
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B_phi = 0.0;
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fn_0 = r_0/r;
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fn = fn_0 * fn_0;
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for ( n = 1; n <= nmax; n++ ) {
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double c1_n=0;
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double c2_n=0;
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|
double c3_n=0;
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|
for ( m = 0; m <= n; m++ ) {
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|
double tmp = (gnm[n][m] * cm[m] + hnm[n][m] * sm[m]);
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|
c1_n=c1_n + tmp * P[n][m];
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|
c2_n=c2_n + tmp * DP[n][m];
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|
c3_n=c3_n + m * (gnm[n][m] * sm[m] - hnm[n][m] * cm[m]) * P[n][m];
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|
}
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|
// fn=pow(r_0/r,n+2.0);
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|
fn *= fn_0;
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|
B_r = B_r + (n + 1) * c1_n * fn;
|
|
B_theta = B_theta - c2_n * fn;
|
|
B_phi = B_phi + c3_n * fn * inv_s;
|
|
}
|
|
|
|
/* Find geodetic field components: */
|
|
psi = theta - ((M_PI / 2.0) - lat);
|
|
sinpsi = sin(psi);
|
|
cospsi = cos(psi);
|
|
X = -B_theta * cospsi - B_r * sinpsi;
|
|
Y = B_phi;
|
|
Z = B_theta * sinpsi - B_r * cospsi;
|
|
|
|
field[0]=B_r;
|
|
field[1]=B_theta;
|
|
field[2]=B_phi;
|
|
field[3]=X;
|
|
field[4]=Y;
|
|
field[5]=Z; /* output fields */
|
|
|
|
/* find variation in radians */
|
|
/* return zero variation at magnetic pole X=Y=0. */
|
|
/* E is positive */
|
|
return (X != 0. || Y != 0.) ? atan2(Y, X) : (double) 0.;
|
|
}
|
|
|
|
|
|
#ifdef TEST_NHV_HACKS
|
|
double SGMagVarOrig( double lat, double lon, double h, long dat, double* field )
|
|
{
|
|
/* output field B_r,B_th,B_phi,B_x,B_y,B_z */
|
|
int n,m;
|
|
/* reference dates */
|
|
long date0_wmm2015 = yymmdd_to_julian_days(5,1,1);
|
|
|
|
double yearfrac,sr,r,theta,c,s,psi,fn,B_r,B_theta,B_phi,X,Y,Z;
|
|
|
|
/* convert to geocentric coords: */
|
|
sr = sqrt(pow(a*cos(lat),2.0)+pow(b*sin(lat),2.0));
|
|
/* sr is effective radius */
|
|
theta = atan2(cos(lat) * (h * sr + a * a),
|
|
sin(lat) * (h * sr + b * b));
|
|
/* theta is geocentric co-latitude */
|
|
|
|
r = h * h + 2.0*h * sr +
|
|
(pow(a,4.0) - (pow(a,4.0) - pow(b,4.0)) * pow(sin(lat),2.0)) /
|
|
(a * a - (a * a - b * b) * pow(sin(lat),2.0));
|
|
|
|
r = sqrt(r);
|
|
|
|
/* r is geocentric radial distance */
|
|
c = cos(theta);
|
|
s = sin(theta);
|
|
|
|
/* zero out arrays */
|
|
for ( n = 0; n <= nmax; n++ ) {
|
|
for ( m = 0; m <= n; m++ ) {
|
|
P[n][m] = 0;
|
|
DP[n][m] = 0;
|
|
}
|
|
}
|
|
|
|
/* diagonal elements */
|
|
P[0][0] = 1;
|
|
P[1][1] = s;
|
|
DP[0][0] = 0;
|
|
DP[1][1] = c;
|
|
P[1][0] = c ;
|
|
DP[1][0] = -s;
|
|
|
|
for ( n = 2; n <= nmax; n++ ) {
|
|
P[n][n] = P[n-1][n-1] * s * sqrt((2.0*n-1) / (2.0*n));
|
|
DP[n][n] = (DP[n-1][n-1] * s + P[n-1][n-1] * c) *
|
|
sqrt((2.0*n-1) / (2.0*n));
|
|
}
|
|
|
|
/* lower triangle */
|
|
for ( m = 0; m <= nmax; m++ ) {
|
|
for ( n = SG_MAX2(m + 1, 2); n <= nmax; n++ ) {
|
|
P[n][m] = (P[n-1][m] * c * (2.0*n-1) - P[n-2][m] *
|
|
sqrt(1.0*(n-1)*(n-1) - m * m)) /
|
|
sqrt(1.0* n * n - m * m);
|
|
DP[n][m] = ((DP[n-1][m] * c - P[n-1][m] * s) *
|
|
(2.0*n-1) - DP[n-2][m] *
|
|
sqrt(1.0*(n-1) * (n-1) - m * m)) /
|
|
sqrt(1.0* n * n - m * m);
|
|
}
|
|
}
|
|
|
|
/* compute gnm, hnm at dat */
|
|
/* WMM2015 */
|
|
yearfrac = (dat - date0_wmm2015) / 365.25;
|
|
for ( n = 1; n <= nmax; n++ ) {
|
|
for ( m = 0; m <= nmax; m++ ) {
|
|
gnm[n][m] = gnm_wmm2015[n][m] + yearfrac * gtnm_wmm2015[n][m];
|
|
hnm[n][m] = hnm_wmm2015[n][m] + yearfrac * htnm_wmm2015[n][m];
|
|
}
|
|
}
|
|
|
|
/* compute sm (sin(m lon) and cm (cos(m lon)) */
|
|
for ( m = 0; m <= nmax; m++ ) {
|
|
sm[m] = sin(m * lon);
|
|
cm[m] = cos(m * lon);
|
|
}
|
|
|
|
/* compute B fields */
|
|
B_r = 0.0;
|
|
B_theta = 0.0;
|
|
B_phi = 0.0;
|
|
|
|
for ( n = 1; n <= nmax; n++ ) {
|
|
double c1_n=0;
|
|
double c2_n=0;
|
|
double c3_n=0;
|
|
for ( m = 0; m <= n; m++ ) {
|
|
c1_n=c1_n + (gnm[n][m] * cm[m] + hnm[n][m] * sm[m]) * P[n][m];
|
|
c2_n=c2_n + (gnm[n][m] * cm[m] + hnm[n][m] * sm[m]) * DP[n][m];
|
|
c3_n=c3_n + m * (gnm[n][m] * sm[m] - hnm[n][m] * cm[m]) * P[n][m];
|
|
}
|
|
fn=pow(r_0/r,n+2.0);
|
|
B_r = B_r + (n + 1) * c1_n * fn;
|
|
B_theta = B_theta - c2_n * fn;
|
|
B_phi = B_phi + c3_n * fn / s;
|
|
}
|
|
|
|
/* Find geodetic field components: */
|
|
psi = theta - (pi / 2.0 - lat);
|
|
X = -B_theta * cos(psi) - B_r * sin(psi);
|
|
Y = B_phi;
|
|
Z = B_theta * sin(psi) - B_r * cos(psi);
|
|
|
|
field[0]=B_r;
|
|
field[1]=B_theta;
|
|
field[2]=B_phi;
|
|
field[3]=X;
|
|
field[4]=Y;
|
|
field[5]=Z; /* output fields */
|
|
|
|
/* find variation, leave in radians! */
|
|
return atan2(Y, X); /* E is positive */
|
|
}
|
|
#endif // TEST_NHV_HACKS
|