| 1 | /* jupiter moon info */
|
|---|
| 2 |
|
|---|
| 3 | #include <stdio.h>
|
|---|
| 4 | #include <stdlib.h>
|
|---|
| 5 | #include <string.h>
|
|---|
| 6 | #include <math.h>
|
|---|
| 7 |
|
|---|
| 8 | #include "astro.h"
|
|---|
| 9 | #include "bdl.h"
|
|---|
| 10 |
|
|---|
| 11 | static int use_bdl (double jd, char *dir, MoonData md[J_NMOONS]);
|
|---|
| 12 | static void meeus_jupiter (double d, double *cmlI, double *cmlII,
|
|---|
| 13 | MoonData md[J_NMOONS]);
|
|---|
| 14 | static void moonradec (double jupsize, MoonData md[J_NMOONS]);
|
|---|
| 15 | static void moonSVis (Obj *eop, Obj *jop, MoonData md[J_NMOONS]);
|
|---|
| 16 | static void moonEVis (MoonData md[J_NMOONS]);
|
|---|
| 17 |
|
|---|
| 18 | /* moon table and a few other goodies and when it was last computed */
|
|---|
| 19 | static double mdmjd = -123456;
|
|---|
| 20 | static MoonData jmd[J_NMOONS] = {
|
|---|
| 21 | {"Jupiter", NULL},
|
|---|
| 22 | {"Io", "I"},
|
|---|
| 23 | {"Europa", "II"},
|
|---|
| 24 | {"Ganymede", "III"},
|
|---|
| 25 | {"Callisto", "IV"}
|
|---|
| 26 | };
|
|---|
| 27 | static double sizemjd; /* size at last mjd */
|
|---|
| 28 | static double cmlImjd; /* central meridian long sys I, at last mjd */
|
|---|
| 29 | static double cmlIImjd; /* " II " */
|
|---|
| 30 |
|
|---|
| 31 | /* file containing BDL coefficients */
|
|---|
| 32 | static char jbdlfn[] = "jupiter.9910";
|
|---|
| 33 |
|
|---|
| 34 | /* get jupiter info in md[0], moon info in md[1..J_NMOONS-1].
|
|---|
| 35 | * if !dir always use meeus model.
|
|---|
| 36 | * if !jop caller just wants md[] for names
|
|---|
| 37 | * N.B. we assume eop and jop are updated.
|
|---|
| 38 | */
|
|---|
| 39 | void
|
|---|
| 40 | jupiter_data (
|
|---|
| 41 | double Mjd, /* mjd */
|
|---|
| 42 | char dir[], /* dir in which to look for helper files */
|
|---|
| 43 | Obj *eop, /* earth == Sun */
|
|---|
| 44 | Obj *jop, /* jupiter */
|
|---|
| 45 | double *sizep, /* jup angular diam, rads */
|
|---|
| 46 | double *cmlI, double *cmlII, /* central meridian longitude, rads */
|
|---|
| 47 | MoonData md[J_NMOONS]) /* return info */
|
|---|
| 48 | {
|
|---|
| 49 | double JD;
|
|---|
| 50 |
|
|---|
| 51 | /* always copy back at least for name */
|
|---|
| 52 | memcpy (md, jmd, sizeof(jmd));
|
|---|
| 53 |
|
|---|
| 54 | /* nothing else if repeat call or just want names */
|
|---|
| 55 | if (Mjd == mdmjd || !jop) {
|
|---|
| 56 | if (jop) {
|
|---|
| 57 | *sizep = sizemjd;
|
|---|
| 58 | *cmlI = cmlImjd;
|
|---|
| 59 | *cmlII = cmlIImjd;
|
|---|
| 60 | }
|
|---|
| 61 | return;
|
|---|
| 62 | }
|
|---|
| 63 | JD = Mjd + MJD0;
|
|---|
| 64 |
|
|---|
| 65 | /* planet in [0] */
|
|---|
| 66 | md[0].ra = jop->s_ra;
|
|---|
| 67 | md[0].dec = jop->s_dec;
|
|---|
| 68 | md[0].mag = get_mag(jop);
|
|---|
| 69 | md[0].x = 0;
|
|---|
| 70 | md[0].y = 0;
|
|---|
| 71 | md[0].z = 0;
|
|---|
| 72 | md[0].evis = 1;
|
|---|
| 73 | md[0].svis = 1;
|
|---|
| 74 |
|
|---|
| 75 | /* size is straight from jop */
|
|---|
| 76 | *sizep = degrad(jop->s_size/3600.0);
|
|---|
| 77 |
|
|---|
| 78 | /* mags from JPL ephemeris */
|
|---|
| 79 | md[1].mag = 5.7;
|
|---|
| 80 | md[2].mag = 5.8;
|
|---|
| 81 | md[3].mag = 5.3;
|
|---|
| 82 | md[4].mag = 6.7;
|
|---|
| 83 |
|
|---|
| 84 | /* get moon data from BDL if possible, else Meeus' model.
|
|---|
| 85 | * always use Meeus for cml
|
|---|
| 86 | */
|
|---|
| 87 | if (dir && use_bdl (JD, dir, md) == 0)
|
|---|
| 88 | meeus_jupiter (Mjd, cmlI, cmlII, NULL);
|
|---|
| 89 | else
|
|---|
| 90 | meeus_jupiter (Mjd, cmlI, cmlII, md);
|
|---|
| 91 |
|
|---|
| 92 | /* set visibilities */
|
|---|
| 93 | moonSVis (eop, jop, md);
|
|---|
| 94 | moonEVis (md);
|
|---|
| 95 |
|
|---|
| 96 | /* fill in moon ra and dec */
|
|---|
| 97 | moonradec (*sizep, md);
|
|---|
| 98 |
|
|---|
| 99 | /* save */
|
|---|
| 100 | mdmjd = Mjd;
|
|---|
| 101 | sizemjd = *sizep;
|
|---|
| 102 | cmlImjd = *cmlI;
|
|---|
| 103 | cmlIImjd = *cmlII;
|
|---|
| 104 | memcpy (jmd, md, sizeof(jmd));
|
|---|
| 105 | }
|
|---|
| 106 |
|
|---|
| 107 | /* hunt for BDL file in dir[] and use if possible
|
|---|
| 108 | * return 0 if ok, else -1
|
|---|
| 109 | */
|
|---|
| 110 | static int
|
|---|
| 111 | use_bdl (
|
|---|
| 112 | double JD, /* julian date */
|
|---|
| 113 | char dir[], /* directory */
|
|---|
| 114 | MoonData md[J_NMOONS]) /* fill md[1..NM-1].x/y/z for each moon */
|
|---|
| 115 | {
|
|---|
| 116 | #define JUPRAU .0004769108 /* jupiter radius, AU */
|
|---|
| 117 | double x[J_NMOONS], y[J_NMOONS], z[J_NMOONS];
|
|---|
| 118 | char buf[1024];
|
|---|
| 119 | FILE *fp;
|
|---|
| 120 | int i;
|
|---|
| 121 |
|
|---|
| 122 | /* only valid 1999 through 2010 */
|
|---|
| 123 | if (JD < 2451179.50000 || JD >= 2455562.5)
|
|---|
| 124 | return (-1);
|
|---|
| 125 |
|
|---|
| 126 | /* open */
|
|---|
| 127 | (void) sprintf (buf, "%s/%s", dir, jbdlfn);
|
|---|
| 128 | fp = fopen (buf, "r");
|
|---|
| 129 | if (!fp)
|
|---|
| 130 | return (-1);
|
|---|
| 131 |
|
|---|
| 132 | /* use it */
|
|---|
| 133 | if ((i = read_bdl (fp, JD, x, y, z, buf)) < 0) {
|
|---|
| 134 | fprintf (stderr, "%s: %s\n", jbdlfn, buf);
|
|---|
| 135 | fclose (fp);
|
|---|
| 136 | return (-1);
|
|---|
| 137 | }
|
|---|
| 138 | if (i != J_NMOONS-1) {
|
|---|
| 139 | fprintf (stderr, "%s: BDL says %d moons, code expects %d", jbdlfn,
|
|---|
| 140 | i, J_NMOONS-1);
|
|---|
| 141 | fclose (fp);
|
|---|
| 142 | return (-1);
|
|---|
| 143 | }
|
|---|
| 144 |
|
|---|
| 145 | /* copy into md[1..NM-1] with our scale and sign conventions */
|
|---|
| 146 | for (i = 1; i < J_NMOONS; i++) {
|
|---|
| 147 | md[i].x = x[i-1]/JUPRAU; /* we want jup radii +E */
|
|---|
| 148 | md[i].y = -y[i-1]/JUPRAU; /* we want jup radii +S */
|
|---|
| 149 | md[i].z = -z[i-1]/JUPRAU; /* we want jup radii +front */
|
|---|
| 150 | }
|
|---|
| 151 |
|
|---|
| 152 | /* ok */
|
|---|
| 153 | fclose (fp);
|
|---|
| 154 | return (0);
|
|---|
| 155 | }
|
|---|
| 156 |
|
|---|
| 157 | /* compute location of GRS and Galilean moons.
|
|---|
| 158 | * if md == NULL, just to cml.
|
|---|
| 159 | * from "Astronomical Formulae for Calculators", 2nd ed, by Jean Meeus,
|
|---|
| 160 | * Willmann-Bell, Richmond, Va., U.S.A. (c) 1982, chapters 35 and 36.
|
|---|
| 161 | */
|
|---|
| 162 | static void
|
|---|
| 163 | meeus_jupiter(
|
|---|
| 164 | double d,
|
|---|
| 165 | double *cmlI, double *cmlII, /* central meridian longitude, rads */
|
|---|
| 166 | MoonData md[J_NMOONS]) /* fill in md[1..NM-1].x/y/z for each moon.
|
|---|
| 167 | * N.B. md[0].ra/dec must already be set
|
|---|
| 168 | */
|
|---|
| 169 | {
|
|---|
| 170 | #define POLE_RA degrad(268.05) /* RA of Jupiter's north pole */
|
|---|
| 171 | #define POLE_DEC degrad(64.50) /* Dec of Jupiter's north pole */
|
|---|
| 172 | #define dsin(x) sin(degrad(x))
|
|---|
| 173 | #define dcos(x) cos(degrad(x))
|
|---|
| 174 | double A, B, Del, J, K, M, N, R, V;
|
|---|
| 175 | double cor_u1, cor_u2, cor_u3, cor_u4;
|
|---|
| 176 | double solc, tmp, G, H, psi, r, r1, r2, r3, r4;
|
|---|
| 177 | double u1, u2, u3, u4;
|
|---|
| 178 | double lam, Ds;
|
|---|
| 179 | double z1, z2, z3, z4;
|
|---|
| 180 | double De, dsinDe;
|
|---|
| 181 | double theta, phi;
|
|---|
| 182 | double tvc, pvc;
|
|---|
| 183 | double salpha, calpha;
|
|---|
| 184 | int i;
|
|---|
| 185 |
|
|---|
| 186 | V = 134.63 + 0.00111587 * d;
|
|---|
| 187 |
|
|---|
| 188 | M = (358.47583 + 0.98560003*d);
|
|---|
| 189 | N = (225.32833 + 0.0830853*d) + 0.33 * dsin (V);
|
|---|
| 190 |
|
|---|
| 191 | J = 221.647 + 0.9025179*d - 0.33 * dsin(V);
|
|---|
| 192 |
|
|---|
| 193 | A = 1.916*dsin(M) + 0.02*dsin(2*M);
|
|---|
| 194 | B = 5.552*dsin(N) + 0.167*dsin(2*N);
|
|---|
| 195 | K = (J+A-B);
|
|---|
| 196 | R = 1.00014 - 0.01672 * dcos(M) - 0.00014 * dcos(2*M);
|
|---|
| 197 | r = 5.20867 - 0.25192 * dcos(N) - 0.00610 * dcos(2*N);
|
|---|
| 198 | Del = sqrt (R*R + r*r - 2*R*r*dcos(K));
|
|---|
| 199 | psi = raddeg (asin (R/Del*dsin(K)));
|
|---|
| 200 |
|
|---|
| 201 | *cmlI = degrad(268.28 + 877.8169088*(d - Del/173) + psi - B);
|
|---|
| 202 | range (cmlI, 2*PI);
|
|---|
| 203 | *cmlII = degrad(290.28 + 870.1869088*(d - Del/173) + psi - B);
|
|---|
| 204 | range (cmlII, 2*PI);
|
|---|
| 205 |
|
|---|
| 206 | /* that's it if don't want moon info too */
|
|---|
| 207 | if (!md)
|
|---|
| 208 | return;
|
|---|
| 209 |
|
|---|
| 210 | solc = (d - Del/173.); /* speed of light correction */
|
|---|
| 211 | tmp = psi - B;
|
|---|
| 212 |
|
|---|
| 213 | u1 = 84.5506 + 203.4058630 * solc + tmp;
|
|---|
| 214 | u2 = 41.5015 + 101.2916323 * solc + tmp;
|
|---|
| 215 | u3 = 109.9770 + 50.2345169 * solc + tmp;
|
|---|
| 216 | u4 = 176.3586 + 21.4879802 * solc + tmp;
|
|---|
| 217 |
|
|---|
| 218 | G = 187.3 + 50.310674 * solc;
|
|---|
| 219 | H = 311.1 + 21.569229 * solc;
|
|---|
| 220 |
|
|---|
| 221 | cor_u1 = 0.472 * dsin (2*(u1-u2));
|
|---|
| 222 | cor_u2 = 1.073 * dsin (2*(u2-u3));
|
|---|
| 223 | cor_u3 = 0.174 * dsin (G);
|
|---|
| 224 | cor_u4 = 0.845 * dsin (H);
|
|---|
| 225 |
|
|---|
| 226 | r1 = 5.9061 - 0.0244 * dcos (2*(u1-u2));
|
|---|
| 227 | r2 = 9.3972 - 0.0889 * dcos (2*(u2-u3));
|
|---|
| 228 | r3 = 14.9894 - 0.0227 * dcos (G);
|
|---|
| 229 | r4 = 26.3649 - 0.1944 * dcos (H);
|
|---|
| 230 |
|
|---|
| 231 | md[1].x = -r1 * dsin (u1+cor_u1);
|
|---|
| 232 | md[2].x = -r2 * dsin (u2+cor_u2);
|
|---|
| 233 | md[3].x = -r3 * dsin (u3+cor_u3);
|
|---|
| 234 | md[4].x = -r4 * dsin (u4+cor_u4);
|
|---|
| 235 |
|
|---|
| 236 | lam = 238.05 + 0.083091*d + 0.33*dsin(V) + B;
|
|---|
| 237 | Ds = 3.07*dsin(lam + 44.5);
|
|---|
| 238 | De = Ds - 2.15*dsin(psi)*dcos(lam+24.)
|
|---|
| 239 | - 1.31*(r-Del)/Del*dsin(lam-99.4);
|
|---|
| 240 | dsinDe = dsin(De);
|
|---|
| 241 |
|
|---|
| 242 | z1 = r1 * dcos(u1+cor_u1);
|
|---|
| 243 | z2 = r2 * dcos(u2+cor_u2);
|
|---|
| 244 | z3 = r3 * dcos(u3+cor_u3);
|
|---|
| 245 | z4 = r4 * dcos(u4+cor_u4);
|
|---|
| 246 |
|
|---|
| 247 | md[1].y = z1*dsinDe;
|
|---|
| 248 | md[2].y = z2*dsinDe;
|
|---|
| 249 | md[3].y = z3*dsinDe;
|
|---|
| 250 | md[4].y = z4*dsinDe;
|
|---|
| 251 |
|
|---|
| 252 | /* compute sky transformation angle as triple vector product */
|
|---|
| 253 | tvc = PI/2.0 - md[0].dec;
|
|---|
| 254 | pvc = md[0].ra;
|
|---|
| 255 | theta = PI/2.0 - POLE_DEC;
|
|---|
| 256 | phi = POLE_RA;
|
|---|
| 257 | salpha = -sin(tvc)*sin(theta)*(cos(pvc)*sin(phi) - sin(pvc)*cos(phi));
|
|---|
| 258 | calpha = sqrt (1.0 - salpha*salpha);
|
|---|
| 259 |
|
|---|
| 260 | for (i = 0; i < J_NMOONS; i++) {
|
|---|
| 261 | double tx = md[i].x*calpha + md[i].y*salpha;
|
|---|
| 262 | double ty = -md[i].x*salpha + md[i].y*calpha;
|
|---|
| 263 | md[i].x = tx;
|
|---|
| 264 | md[i].y = ty;
|
|---|
| 265 | }
|
|---|
| 266 |
|
|---|
| 267 | md[1].z = z1;
|
|---|
| 268 | md[2].z = z2;
|
|---|
| 269 | md[3].z = z3;
|
|---|
| 270 | md[4].z = z4;
|
|---|
| 271 | }
|
|---|
| 272 |
|
|---|
| 273 |
|
|---|
| 274 | /* given jupiter loc in md[0].ra/dec and size, and location of each moon in
|
|---|
| 275 | * md[1..NM-1].x/y in jup radii, find ra/dec of each moon in md[1..NM-1].ra/dec.
|
|---|
| 276 | */
|
|---|
| 277 | static void
|
|---|
| 278 | moonradec (
|
|---|
| 279 | double jupsize, /* jup diameter, rads */
|
|---|
| 280 | MoonData md[J_NMOONS]) /* fill in RA and Dec */
|
|---|
| 281 | {
|
|---|
| 282 | double juprad = jupsize/2;
|
|---|
| 283 | double jupra = md[0].ra;
|
|---|
| 284 | double jupdec = md[0].dec;
|
|---|
| 285 | int i;
|
|---|
| 286 |
|
|---|
| 287 | for (i = 1; i < J_NMOONS; i++) {
|
|---|
| 288 | double dra = juprad * md[i].x;
|
|---|
| 289 | double ddec = juprad * md[i].y;
|
|---|
| 290 | md[i].ra = jupra + dra;
|
|---|
| 291 | md[i].dec = jupdec - ddec;
|
|---|
| 292 | }
|
|---|
| 293 | }
|
|---|
| 294 |
|
|---|
| 295 | /* set svis according to whether moon is in sun light */
|
|---|
| 296 | static void
|
|---|
| 297 | moonSVis(
|
|---|
| 298 | Obj *eop, /* earth == SUN */
|
|---|
| 299 | Obj *jop, /* jupiter */
|
|---|
| 300 | MoonData md[J_NMOONS])
|
|---|
| 301 | {
|
|---|
| 302 | double esd = eop->s_edist;
|
|---|
| 303 | double eod = jop->s_edist;
|
|---|
| 304 | double sod = jop->s_sdist;
|
|---|
| 305 | double soa = degrad(jop->s_elong);
|
|---|
| 306 | double esa = asin(esd*sin(soa)/sod);
|
|---|
| 307 | double h = sod*jop->s_hlat;
|
|---|
| 308 | double nod = h*(1./eod - 1./sod);
|
|---|
| 309 | double sca = cos(esa), ssa = sin(esa);
|
|---|
| 310 | int i;
|
|---|
| 311 |
|
|---|
| 312 | for (i = 1; i < J_NMOONS; i++) {
|
|---|
| 313 | MoonData *mdp = &md[i];
|
|---|
| 314 | double xp = sca*mdp->x + ssa*mdp->z;
|
|---|
| 315 | double yp = mdp->y;
|
|---|
| 316 | double zp = -ssa*mdp->x + sca*mdp->z;
|
|---|
| 317 | double ca = cos(nod), sa = sin(nod);
|
|---|
| 318 | double xpp = xp;
|
|---|
| 319 | double ypp = ca*yp - sa*zp;
|
|---|
| 320 | double zpp = sa*yp + ca*zp;
|
|---|
| 321 | int outside = xpp*xpp + ypp*ypp > 1.0;
|
|---|
| 322 | int infront = zpp > 0.0;
|
|---|
| 323 | mdp->svis = outside || infront;
|
|---|
| 324 | }
|
|---|
| 325 | }
|
|---|
| 326 |
|
|---|
| 327 | /* set evis according to whether moon is geometrically visible from earth */
|
|---|
| 328 | static void
|
|---|
| 329 | moonEVis (MoonData md[J_NMOONS])
|
|---|
| 330 | {
|
|---|
| 331 | int i;
|
|---|
| 332 |
|
|---|
| 333 | for (i = 1; i < J_NMOONS; i++) {
|
|---|
| 334 | MoonData *mdp = &md[i];
|
|---|
| 335 | int outside = mdp->x*mdp->x + mdp->y*mdp->y > 1.0;
|
|---|
| 336 | int infront = mdp->z > 0.0;
|
|---|
| 337 | mdp->evis = outside || infront;
|
|---|
| 338 | }
|
|---|
| 339 | }
|
|---|
| 340 |
|
|---|
| 341 | /* For RCS Only -- Do Not Edit */
|
|---|
| 342 | static char *rcsid[2] = {(char *)rcsid, "@(#) $RCSfile: jupmoon.c,v $ $Date: 2004-06-15 16:54:12 $ $Revision: 1.1 $ $Name: not supported by cvs2svn $"};
|
|---|
![(please configure the [header_logo] section in trac.ini)](/PI/chrome/site/your_project_logo.png){kind=logo}
