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This program demonstrates converting equatorial vectors to ecliptic vectors using a rotation matrix.
78 lines
2.0 KiB
C
78 lines
2.0 KiB
C
/*
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ecliptic_vector.c - by Don Cross - 2022-05-20
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Example C program for Astronomy Engine:
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https://github.com/cosinekitty/astronomy
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An example of converting equatorial coordinates to ecliptic coordinates.
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*/
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#include <stdio.h>
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#include "astro_demo_common.h"
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int PrintUsage(void)
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{
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fprintf(stderr,
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"\n"
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"USAGE: ecliptic_vector [yyyy-mm-ddThh:mm:ssZ]\n"
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"\n"
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"Displays cartesian ecliptic vectors for the Sun, Moon, and planets\n"
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"at the time specified on the command line (if present), or at the\n"
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"current time (if absent).\n"
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"\n"
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);
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return 1;
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}
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int main(int argc, const char *argv[])
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{
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static const astro_body_t body[] = {
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BODY_SUN, BODY_MERCURY, BODY_VENUS, BODY_EARTH, BODY_MOON, BODY_MARS,
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BODY_JUPITER, BODY_SATURN, BODY_URANUS, BODY_NEPTUNE, BODY_PLUTO
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};
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int i;
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astro_time_t time;
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int num_bodies = sizeof(body) / sizeof(body[0]);
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astro_rotation_t rot;
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if (argc == 1)
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{
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/* Use the computer's current time. */
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time = Astronomy_CurrentTime();
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}
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else if (argc == 2)
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{
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/* Read the time from the command line. */
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if (0 != ParseTime(argv[1], &time))
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return 1;
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}
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else
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{
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return PrintUsage();
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}
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printf("UTC date = ");
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PrintTime(time);
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printf("\n");
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/* Get a rotation matrix that converts equatorial J2000 (EQJ) vectors to ecliptic vectors (ECL). */
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rot = Astronomy_Rotation_EQJ_ECL();
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printf("BODY X Y Z\n");
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for (i=0; i < num_bodies; ++i)
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{
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astro_vector_t eqj = Astronomy_HelioVector(body[i], time);
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astro_vector_t ecl = Astronomy_RotateVector(rot, eqj);
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const char *name = Astronomy_BodyName(body[i]);
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if (ecl.status != ASTRO_SUCCESS)
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{
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fprintf(stderr, "ERROR %d calculating vector for %s.\n", (int)ecl.status, name);
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return 1;
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}
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printf("%-8s %11.6lf %11.6lf %11.6lf\n", name, ecl.x, ecl.y, ecl.z);
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}
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return 0;
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}
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