#include #include #include "astro.h" static void ecleq_aux (int sw, double mj, double x, double y, double *p, double *q); #define EQtoECL 1 #define ECLtoEQ (-1) /* given the modified Julian date, mj, and an equitorial ra and dec, each in * radians, find the corresponding geocentric ecliptic latitude, *lt, and * longititude, *lg, also each in radians. * correction for the effect on the angle of the obliquity due to nutation is * not included. */ void eq_ecl (double mj, double ra, double dec, double *lt, double *lg) { ecleq_aux (EQtoECL, mj, ra, dec, lg, lt); } /* given the modified Julian date, mj, and a geocentric ecliptic latitude, * *lt, and longititude, *lg, each in radians, find the corresponding * equitorial ra and dec, also each in radians. * correction for the effect on the angle of the obliquity due to nutation is * not included. */ void ecl_eq (double mj, double lt, double lg, double *ra, double *dec) { ecleq_aux (ECLtoEQ, mj, lg, lt, ra, dec); } static void ecleq_aux ( int sw, /* +1 for eq to ecliptic, -1 for vv. */ double mj, double x, double y, /* sw==1: x==ra, y==dec. sw==-1: x==lg, y==lt. */ double *p, double *q) /* sw==1: p==lg, q==lt. sw==-1: p==ra, q==dec. */ { static double lastmj = -10000; /* last mj calculated */ static double seps, ceps; /* sin and cos of mean obliquity */ double sx, cx, sy, cy, ty, sq; if (mj != lastmj) { double eps; obliquity (mj, &eps); /* mean obliquity for date */ seps = sin(eps); ceps = cos(eps); lastmj = mj; } sy = sin(y); cy = cos(y); /* always non-negative */ if (fabs(cy)<1e-20) cy = 1e-20; /* insure > 0 */ ty = sy/cy; cx = cos(x); sx = sin(x); sq = (sy*ceps)-(cy*seps*sx*sw); if (sq < -1) sq = -1; if (sq > 1) sq = 1; *q = asin(sq); *p = atan(((sx*ceps)+(ty*seps*sw))/cx); if (cx<0) *p += PI; /* account for atan quad ambiguity */ range (p, 2*PI); } /* For RCS Only -- Do Not Edit */ static char *rcsid[2] = {(char *)rcsid, "@(#) $RCSfile: eq_ecl.c,v $ $Date: 2009-07-16 10:34:37 $ $Revision: 1.8 $ $Name: not supported by cvs2svn $"};