1 | #include <stdio.h>
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2 | #include <math.h>
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3 |
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4 | #include "astro.h"
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5 |
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6 | static void ecleq_aux (int sw, double mj, double x, double y,
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7 | double *p, double *q);
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8 |
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9 | #define EQtoECL 1
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10 | #define ECLtoEQ (-1)
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11 |
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12 |
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13 | /* given the modified Julian date, mj, and an equitorial ra and dec, each in
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14 | * radians, find the corresponding geocentric ecliptic latitude, *lt, and
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15 | * longititude, *lg, also each in radians.
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16 | * correction for the effect on the angle of the obliquity due to nutation is
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17 | * not included.
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18 | */
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19 | void
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20 | eq_ecl (double mj, double ra, double dec, double *lt, double *lg)
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21 | {
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22 | ecleq_aux (EQtoECL, mj, ra, dec, lg, lt);
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23 | }
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24 |
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25 | /* given the modified Julian date, mj, and a geocentric ecliptic latitude,
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26 | * *lt, and longititude, *lg, each in radians, find the corresponding
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27 | * equitorial ra and dec, also each in radians.
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28 | * correction for the effect on the angle of the obliquity due to nutation is
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29 | * not included.
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30 | */
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31 | void
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32 | ecl_eq (double mj, double lt, double lg, double *ra, double *dec)
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33 | {
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34 | ecleq_aux (ECLtoEQ, mj, lg, lt, ra, dec);
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35 | }
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36 |
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37 | static void
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38 | ecleq_aux (
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39 | int sw, /* +1 for eq to ecliptic, -1 for vv. */
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40 | double mj,
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41 | double x, double y, /* sw==1: x==ra, y==dec. sw==-1: x==lg, y==lt. */
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42 | double *p, double *q) /* sw==1: p==lg, q==lt. sw==-1: p==ra, q==dec. */
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43 | {
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44 | static double lastmj = -10000; /* last mj calculated */
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45 | static double seps, ceps; /* sin and cos of mean obliquity */
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46 | double sx, cx, sy, cy, ty, sq;
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47 |
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48 | if (mj != lastmj) {
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49 | double eps;
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50 | obliquity (mj, &eps); /* mean obliquity for date */
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51 | seps = sin(eps);
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52 | ceps = cos(eps);
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53 | lastmj = mj;
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54 | }
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55 |
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56 | sy = sin(y);
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57 | cy = cos(y); /* always non-negative */
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58 | if (fabs(cy)<1e-20) cy = 1e-20; /* insure > 0 */
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59 | ty = sy/cy;
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60 | cx = cos(x);
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61 | sx = sin(x);
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62 | sq = (sy*ceps)-(cy*seps*sx*sw);
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63 | if (sq < -1) sq = -1;
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64 | if (sq > 1) sq = 1;
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65 | *q = asin(sq);
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66 | *p = atan(((sx*ceps)+(ty*seps*sw))/cx);
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67 | if (cx<0) *p += PI; /* account for atan quad ambiguity */
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68 | range (p, 2*PI);
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69 | }
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70 |
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71 | /* For RCS Only -- Do Not Edit */
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72 | static char *rcsid[2] = {(char *)rcsid, "@(#) $RCSfile: eq_ecl.c,v $ $Date: 2006-11-22 13:53:29 $ $Revision: 1.6 $ $Name: not supported by cvs2svn $"};
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