flightgear/Scenery/sun.c

/**************************************************************************
 * sun.c
 *
 * Written 1997 by Durk Talsma, started October, 1997.  For the flight gear
 * project.
 *
 * 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.
 *
 * $Id$
 * (Log is kept at end of this file)
 **************************************************************************/

#include <GL/glut.h>
#include "../XGL/xgl.h"

#include "../Time/fg_time.h"
#include "../Main/views.h"
#include "orbits.h"
#include "sun.h"

GLint sun_obj;

static struct CelestialCoord sunPos;

float xSun, ySun, zSun;

struct SunPos fgCalcSunPos(struct OrbElements params)
{
    double
    	EccAnom, lonSun,
        xv, yv, v, r;
    struct SunPos
    	solarPosition;

    /* calculate the eccentric anomaly */
    EccAnom = fgCalcEccAnom(params.M, params.e);

    /* calculate the Suns distance (r) and its true anomaly (v) */
	 xv = cos(EccAnom) - params.e;
    yv = sqrt(1.0 - params.e*params.e) * sin(EccAnom);
    v = atan2(yv, xv);
    r = sqrt(xv*xv + yv*yv);

    /* calculate the the Sun's true longitude (lonsun) */
    lonSun = v + params.w;

	/* convert true longitude and distance to ecliptic rectangular geocentric
      coordinates (xs, ys) */
    solarPosition.xs = r * cos(lonSun);
    solarPosition.ys = r * sin(lonSun);
    return solarPosition;
}


struct CelestialCoord fgCalculateSun(struct OrbElements params, struct fgTIME t)
{
	struct CelestialCoord
		result;
    struct SunPos
    	SolarPosition;
    double
    	xe, ye, ze, ecl, actTime;

    /* calculate the angle between ecliptic and equatorial coordinate system */
    actTime = fgCalcActTime(t);
    ecl = fgDegToRad(23.4393 - 3.563E-7 * actTime);			// Angle now in Rads

    /* calculate the sun's ecliptic position */
    SolarPosition = fgCalcSunPos(params);

	/* convert ecliptic coordinates to equatorial rectangular geocentric coordinates */
    xe = SolarPosition.xs;
    ye = SolarPosition.ys * cos(ecl);
    ze = SolarPosition.ys * sin(ecl);

    /* and finally... Calulate Right Ascention and Declination */
    result.RightAscension = atan2( ye, xe);
    result.Declination = atan2(ze, sqrt(xe*xe + ye*ye));
    return result;
}


/* Initialize the Sun */
void fgSunInit() {
    static int dl_exists = 0;

    fgSolarSystemUpdate(&(pltOrbElements[0]), cur_time_params);
    sunPos = fgCalculateSun(pltOrbElements[0], cur_time_params);
#ifdef DEBUG
    printf("Sun found at %f (ra), %f (dec)\n", sunPos.RightAscension, 
	   sunPos.Declination);
#endif

    if ( !dl_exists ) {
	dl_exists = 1;

	/* printf("First time through, creating sun display list\n"); */

	sun_obj = xglGenLists(1);
	xglNewList(sun_obj, GL_COMPILE );

	xSun = 60000.0 * cos(sunPos.RightAscension) * cos(sunPos.Declination);
	ySun = 60000.0 * sin(sunPos.RightAscension) * cos(sunPos.Declination);
	zSun = 60000.0 * sin(sunPos.Declination);

	glutSolidSphere(1.0, 10, 10);

	xglEndList();
    }
}


/* Draw the Sun */
void fgSunRender() {
    struct fgVIEW *v;
    struct fgTIME *t;
    GLfloat color[4] = { 0.85, 0.65, 0.05, 1.0 };
    /* double x_2, x_4, x_8, x_10; */
    /* GLfloat ambient; */
    /* GLfloat amb[3], diff[3]; */


    t = &cur_time_params;
    v = &current_view;

    /* x_2 = t->sun_angle * t->sun_angle;
    x_4 = x_2 * x_2;
    x_8 = x_4 * x_4;
    x_10 = x_8 * x_2; */

    /* ambient = (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] = 0.50 + ((ambient * 6.66) - 1.6);
    amb[1] = 0.00 + ((ambient * 6.66) - 1.6);
    amb[2] = 0.00 + ((ambient * 6.66) - 1.6);
    amb[3] = 0.00;
#ifdef DEBUG
    printf("Color of the sun: %f, %f, %f\n"
	   "Ambient value   : %f\n"
	   "Sun Angle       : %f\n" , amb[0], amb[1], amb[2], ambient, t->sun_angle);
#endif
    diff[0] = 0.0;
    diff[1] = 0.0;
    diff[2] = 0.0;
    diff[3] = 0.0; */

    /* set lighting parameters */
    /* xglLightfv(GL_LIGHT0, GL_AMBIENT, color );
    xglLightfv(GL_LIGHT0, GL_DIFFUSE, color );
    xglMaterialfv(GL_FRONT, GL_AMBIENT, amb);
    xglMaterialfv(GL_FRONT, GL_DIFFUSE, diff); */

    xglDisable( GL_LIGHTING );

    xglPushMatrix();
    xglTranslatef(xSun, ySun, zSun);
    xglScalef(1400, 1400, 1400);

    xglColor3f(0.85, 0.65, 0.05);

    /* xglColor3fv( color ); */
    /* xglutSolidSphere(1.0, 25, 25); */
    xglCallList(sun_obj);

    xglPopMatrix();

    xglEnable( GL_LIGHTING );
}


/* $Log$
/* Revision 1.7  1997/12/17 23:12:16  curt
/* Fixed so moon and sun display lists aren't recreate periodically.
/*
 * Revision 1.6  1997/12/15 23:55:04  curt
 * Add xgl wrappers for debugging.
 * Generate terrain normals on the fly.
 *
 * Revision 1.5  1997/12/12 21:41:31  curt
 * More light/material property tweaking ... still a ways off.
 *
 * Revision 1.4  1997/12/10 22:37:53  curt
 * Prepended "fg" on the name of all global structures that didn't have it yet.
 * i.e. "struct WEATHER {}" became "struct fgWEATHER {}"
 *
 * Revision 1.3  1997/12/09 05:11:56  curt
 * Working on tweaking lighting.
 *
 * Revision 1.2  1997/11/25 19:25:39  curt
 * Changes to integrate Durk's moon/sun code updates + clean up.
 *
 * Revision 1.1  1997/10/25 03:16:11  curt
 * Initial revision of code contributed by Durk Talsma.
 *
 */