[1457] | 1 | /* aberration, Jean Meeus, "Astronomical Algorithms", Willman-Bell, 1995;
|
---|
| 2 | * based on secular unperturbed Kepler orbit
|
---|
| 3 | *
|
---|
[2551] | 4 | * the corrections should be applied to ra/dec and lam/beta at the
|
---|
[1457] | 5 | * epoch of date.
|
---|
| 6 | */
|
---|
| 7 |
|
---|
| 8 | #include <stdio.h>
|
---|
| 9 | #include <math.h>
|
---|
| 10 | #include <stdlib.h>
|
---|
| 11 |
|
---|
| 12 | #include "astro.h"
|
---|
| 13 |
|
---|
| 14 | #define ABERR_CONST (20.49552/3600./180.*PI) /* aberr const in rad */
|
---|
| 15 | #define AB_ECL_EOD 0
|
---|
| 16 | #define AB_EQ_EOD 1
|
---|
| 17 |
|
---|
[2551] | 18 | static void ab_aux (double mj, double *x, double *y, double lsn, int mode);
|
---|
[1457] | 19 |
|
---|
| 20 | /* apply aberration correction to ecliptical coordinates *lam and *bet
|
---|
[2551] | 21 | * (in radians) for a given time m and handily supplied longitude of sun,
|
---|
[1457] | 22 | * lsn (in radians)
|
---|
| 23 | */
|
---|
| 24 | void
|
---|
[2551] | 25 | ab_ecl (double mj, double lsn, double *lam, double *bet)
|
---|
[1457] | 26 | {
|
---|
[2551] | 27 | ab_aux(mj, lam, bet, lsn, AB_ECL_EOD);
|
---|
[1457] | 28 | }
|
---|
| 29 |
|
---|
| 30 | /* apply aberration correction to equatoreal coordinates *ra and *dec
|
---|
[2551] | 31 | * (in radians) for a given time m and handily supplied longitude of sun,
|
---|
[1457] | 32 | * lsn (in radians)
|
---|
| 33 | */
|
---|
| 34 | void
|
---|
[2551] | 35 | ab_eq (double mj, double lsn, double *ra, double *dec)
|
---|
[1457] | 36 | {
|
---|
[2551] | 37 | ab_aux(mj, ra, dec, lsn, AB_EQ_EOD);
|
---|
[1457] | 38 | }
|
---|
| 39 |
|
---|
| 40 | /* because the e-terms are secular, keep the real transformation for both
|
---|
| 41 | * coordinate systems in here with the secular variables cached.
|
---|
| 42 | * mode == AB_ECL_EOD: x = lam, y = bet (ecliptical)
|
---|
| 43 | * mode == AB_EQ_EOD: x = ra, y = dec (equatoreal)
|
---|
| 44 | */
|
---|
| 45 | static void
|
---|
[2551] | 46 | ab_aux (double mj, double *x, double *y, double lsn, int mode)
|
---|
[1457] | 47 | {
|
---|
[2551] | 48 | static double lastmj = -10000;
|
---|
[1457] | 49 | static double eexc; /* earth orbit excentricity */
|
---|
| 50 | static double leperi; /* ... and longitude of perihelion */
|
---|
| 51 | static char dirty = 1; /* flag for cached trig terms */
|
---|
| 52 |
|
---|
[2551] | 53 | if (mj != lastmj) {
|
---|
[1457] | 54 | double T; /* centuries since J2000 */
|
---|
| 55 |
|
---|
[2551] | 56 | T = (mj - J2000)/36525.;
|
---|
[1457] | 57 | eexc = 0.016708617 - (42.037e-6 + 0.1236e-6 * T) * T;
|
---|
| 58 | leperi = degrad(102.93735 + (0.71953 + 0.00046 * T) * T);
|
---|
[2551] | 59 | lastmj = mj;
|
---|
[1457] | 60 | dirty = 1;
|
---|
| 61 | }
|
---|
| 62 |
|
---|
| 63 | switch (mode) {
|
---|
| 64 | case AB_ECL_EOD: /* ecliptical coords */
|
---|
| 65 | {
|
---|
| 66 | double *lam = x, *bet = y;
|
---|
| 67 | double dlsun, dlperi;
|
---|
| 68 |
|
---|
| 69 | dlsun = lsn - *lam;
|
---|
| 70 | dlperi = leperi - *lam;
|
---|
| 71 |
|
---|
| 72 | /* valid only for *bet != +-PI/2 */
|
---|
| 73 | *lam -= ABERR_CONST/cos(*bet) * (cos(dlsun) -
|
---|
| 74 | eexc*cos(dlperi));
|
---|
| 75 | *bet -= ABERR_CONST*sin(*bet) * (sin(dlsun) -
|
---|
| 76 | eexc*sin(dlperi));
|
---|
| 77 | }
|
---|
| 78 | break;
|
---|
| 79 |
|
---|
| 80 | case AB_EQ_EOD: /* equatoreal coords */
|
---|
| 81 | {
|
---|
| 82 | double *ra = x, *dec = y;
|
---|
| 83 | double sr, cr, sd, cd, sls, cls;/* trig values coords */
|
---|
| 84 | static double cp, sp, ce, se; /* .. and perihel/eclipic */
|
---|
| 85 | double dra, ddec; /* changes in ra and dec */
|
---|
| 86 |
|
---|
| 87 | if (dirty) {
|
---|
| 88 | double eps;
|
---|
| 89 |
|
---|
| 90 | cp = cos(leperi);
|
---|
| 91 | sp = sin(leperi);
|
---|
[2551] | 92 | obliquity(mj, &eps);
|
---|
[1457] | 93 | se = sin(eps);
|
---|
| 94 | ce = cos(eps);
|
---|
| 95 | dirty = 0;
|
---|
| 96 | }
|
---|
| 97 |
|
---|
| 98 | sr = sin(*ra);
|
---|
| 99 | cr = cos(*ra);
|
---|
| 100 | sd = sin(*dec);
|
---|
| 101 | cd = cos(*dec);
|
---|
| 102 | sls = sin(lsn);
|
---|
| 103 | cls = cos(lsn);
|
---|
| 104 |
|
---|
| 105 | dra = ABERR_CONST/cd * ( -(cr * cls * ce + sr * sls) +
|
---|
| 106 | eexc * (cr * cp * ce + sr * sp));
|
---|
| 107 |
|
---|
| 108 | ddec = se/ce * cd - sr * sd; /* tmp use */
|
---|
| 109 | ddec = ABERR_CONST * ( -(cls * ce * ddec + cr * sd * sls) +
|
---|
| 110 | eexc * (cp * ce * ddec + cr * sd * sp) );
|
---|
| 111 |
|
---|
| 112 | *ra += dra;
|
---|
| 113 | range (ra, 2*PI);
|
---|
| 114 | *dec += ddec;
|
---|
| 115 | }
|
---|
| 116 | break;
|
---|
| 117 |
|
---|
| 118 | default:
|
---|
| 119 | printf ("ab_aux: bad mode: %d\n", mode);
|
---|
[2551] | 120 | abort();
|
---|
[1457] | 121 | break;
|
---|
| 122 |
|
---|
| 123 | } /* switch (mode) */
|
---|
| 124 | }
|
---|
| 125 |
|
---|
| 126 | /* For RCS Only -- Do Not Edit */
|
---|
[2818] | 127 | static char *rcsid[2] = {(char *)rcsid, "@(#) $RCSfile: aberration.c,v $ $Date: 2005-08-21 10:02:36 $ $Revision: 1.5 $ $Name: not supported by cvs2svn $"};
|
---|