1 /* zzgfspq.f -- translated by f2c (version 19980913).
2    You must link the resulting object file with the libraries:
3 	-lf2c -lm   (in that order)
4 */
5 
6 #include "f2c.h"
7 
8 /* Table of constant values */
9 
10 static doublereal c_b12 = 1e-12;
11 
12 /* $Procedure ZZGFSPQ ( GF, separation quantity ) */
zzgfspq_(doublereal * et,integer * targ1,integer * targ2,doublereal * r1,doublereal * r2,integer * obs,char * abcorr,char * ref,doublereal * value,ftnlen abcorr_len,ftnlen ref_len)13 /* Subroutine */ int zzgfspq_(doublereal *et, integer *targ1, integer *targ2,
14 	doublereal *r1, doublereal *r2, integer *obs, char *abcorr, char *ref,
15 	 doublereal *value, ftnlen abcorr_len, ftnlen ref_len)
16 {
17     /* System generated locals */
18     doublereal d__1;
19 
20     /* Local variables */
21     extern doublereal vsep_(doublereal *, doublereal *);
22     extern /* Subroutine */ int chkin_(char *, ftnlen);
23     doublereal theta;
24     extern /* Subroutine */ int errdp_(char *, doublereal *, ftnlen);
25     extern doublereal vnorm_(doublereal *);
26     doublereal range1, range2;
27     extern logical failed_(void);
28     doublereal lt;
29     extern doublereal dasine_(doublereal *, doublereal *), halfpi_(void);
30     extern /* Subroutine */ int sigerr_(char *, ftnlen), chkout_(char *,
31 	    ftnlen), setmsg_(char *, ftnlen), errint_(char *, integer *,
32 	    ftnlen), spkezp_(integer *, doublereal *, char *, char *, integer
33 	    *, doublereal *, doublereal *, ftnlen, ftnlen);
34     extern logical return_(void);
35     doublereal pv1[3], pv2[3], ang1, ang2;
36 
37 /* $ Abstract */
38 
39 /*     SPICE Private routine intended solely for the support of SPICE */
40 /*     routines.  Users should not call this routine directly due */
41 /*     to the volatile nature of this routine. */
42 
43 /*     Compute the angular separation between the limbs of two objects. */
44 
45 /* $ Disclaimer */
46 
47 /*     THIS SOFTWARE AND ANY RELATED MATERIALS WERE CREATED BY THE */
48 /*     CALIFORNIA INSTITUTE OF TECHNOLOGY (CALTECH) UNDER A U.S. */
49 /*     GOVERNMENT CONTRACT WITH THE NATIONAL AERONAUTICS AND SPACE */
50 /*     ADMINISTRATION (NASA). THE SOFTWARE IS TECHNOLOGY AND SOFTWARE */
51 /*     PUBLICLY AVAILABLE UNDER U.S. EXPORT LAWS AND IS PROVIDED "AS-IS" */
52 /*     TO THE RECIPIENT WITHOUT WARRANTY OF ANY KIND, INCLUDING ANY */
53 /*     WARRANTIES OF PERFORMANCE OR MERCHANTABILITY OR FITNESS FOR A */
54 /*     PARTICULAR USE OR PURPOSE (AS SET FORTH IN UNITED STATES UCC */
55 /*     SECTIONS 2312-2313) OR FOR ANY PURPOSE WHATSOEVER, FOR THE */
56 /*     SOFTWARE AND RELATED MATERIALS, HOWEVER USED. */
57 
58 /*     IN NO EVENT SHALL CALTECH, ITS JET PROPULSION LABORATORY, OR NASA */
59 /*     BE LIABLE FOR ANY DAMAGES AND/OR COSTS, INCLUDING, BUT NOT */
60 /*     LIMITED TO, INCIDENTAL OR CONSEQUENTIAL DAMAGES OF ANY KIND, */
61 /*     INCLUDING ECONOMIC DAMAGE OR INJURY TO PROPERTY AND LOST PROFITS, */
62 /*     REGARDLESS OF WHETHER CALTECH, JPL, OR NASA BE ADVISED, HAVE */
63 /*     REASON TO KNOW, OR, IN FACT, SHALL KNOW OF THE POSSIBILITY. */
64 
65 /*     RECIPIENT BEARS ALL RISK RELATING TO QUALITY AND PERFORMANCE OF */
66 /*     THE SOFTWARE AND ANY RELATED MATERIALS, AND AGREES TO INDEMNIFY */
67 /*     CALTECH AND NASA FOR ALL THIRD-PARTY CLAIMS RESULTING FROM THE */
68 /*     ACTIONS OF RECIPIENT IN THE USE OF THE SOFTWARE. */
69 
70 /* $ Required_Reading */
71 
72 /*     None. */
73 
74 /* $ Keywords */
75 
76 /*     GEOMETRY */
77 /*     ANGLE */
78 
79 /* $ Declarations */
80 /* $ Brief_I/O */
81 
82 /*     VARIABLE  I/O  DESCRIPTION */
83 /*     --------  ---  -------------------------------------------------- */
84 /*     ET         I   Ephemeris seconds past J2000 TDB */
85 /*     TARG1      I   NAIF ID for first target */
86 /*     TARG2      I   NAIF ID for second target */
87 /*     R1         I   Radius of a spherical model for TARG1 */
88 /*     R2         I   Radius of a spherical model for TARG2 */
89 /*     OBS        I   NAIF ID of observer */
90 /*     ABCORR     I   Aberration correction flag */
91 /*     REF        I   Reference frame of the angular separation */
92 /*     VALUE      O   Value of angular separation between objects */
93 
94 /* $ Detailed_Input */
95 
96 /*     ET       is the time in ephemeris seconds past J2000 TDB at */
97 /*              which the separation is to be measured. */
98 
99 /*     TARG1 */
100 /*     TARG2    the NAIF IDs of the two objects for which to */
101 /*              determine the angular separation. */
102 
103 /*     R1 */
104 /*     R2       are the radii of the two objects TARG1 and TARG2 */
105 /*              respectively. */
106 
107 /*     OBS      the NAIF ID identifying the body observing */
108 /*              TARG1 and TARG2. */
109 
110 /*     ABCORR   the string description of the aberration corrections */
111 /*              to apply to the state evaluations to account for */
112 /*              one-way light time and stellar aberration. */
113 
114 /*              This routine accepts the same aberration corrections */
115 /*              as does the SPICE routine SPKEZR. See the header of */
116 /*              SPKEZR for a detailed description of the aberration */
117 /*              correction options. For convenience, the options are */
118 /*              listed below: */
119 
120 /*                 'NONE'     Apply no correction. */
121 
122 /*                 'LT'       "Reception" case:  correct for */
123 /*                            one-way light time using a Newtonian */
124 /*                            formulation. */
125 
126 /*                 'LT+S'     "Reception" case:  correct for */
127 /*                            one-way light time and stellar */
128 /*                            aberration using a Newtonian */
129 /*                            formulation. */
130 
131 /*                 'CN'       "Reception" case:  converged */
132 /*                            Newtonian light time correction. */
133 
134 /*                 'CN+S'     "Reception" case:  converged */
135 /*                            Newtonian light time and stellar */
136 /*                            aberration corrections. */
137 
138 /*                 'XLT'      "Transmission" case:  correct for */
139 /*                            one-way light time using a Newtonian */
140 /*                            formulation. */
141 
142 /*                 'XLT+S'    "Transmission" case:  correct for */
143 /*                            one-way light time and stellar */
144 /*                            aberration using a Newtonian */
145 /*                            formulation. */
146 
147 /*                 'XCN'      "Transmission" case:  converged */
148 /*                            Newtonian light time correction. */
149 
150 /*                 'XCN+S'    "Transmission" case:  converged */
151 /*                            Newtonian light time and stellar */
152 /*                            aberration corrections. */
153 
154 /*                 The ABCORR string lacks sensitivity to case, leading */
155 /*                 and trailing blanks. */
156 
157 /*     REF         is the name of the reference frame relative to which */
158 /*                 the angular separation should be expressed. This may */
159 /*                 be any frame supported by the SPICE system, including */
160 /*                 built-in frames (documented in the Frames Required */
161 /*                 Reading) and frames defined by a loaded frame kernel. */
162 
163 /*                 When REF designates a non-inertial frame, the */
164 /*                 orientation of the frame is evaluated at an epoch */
165 /*                 dependent on the selected aberration correction. */
166 
167 /* $ Detailed_Output */
168 
169 /*     VALUE   is the light-time (and stellar aberration corrected */
170 /*             if this feature is enabled) separation of the two */
171 /*             objects TARG1 and TARG2 as observed from OBS. */
172 
173 /* $ Parameters */
174 
175 /*     None. */
176 
177 /* $ Exceptions */
178 
179 /*     1) SPICE(BADRADIUS) signals if either R1 or R2 have a negative */
180 /*        value. */
181 
182 /*     2) If the ephemeris data required to perform the needed state */
183 /*        look-ups are not loaded, routines called by this routine */
184 /*        will signal the error SPICE(SPKINSUFFDATA). */
185 
186 /* $ Files */
187 
188 /*     None. */
189 
190 /* $ Particulars */
191 
192 /*     This routine determines the apparent separation between the limbs */
193 /*     of two objects as observed from a third.  The value reported is */
194 /*     corrected for light time. Moreover, if at the time this routine */
195 /*     is called, stellar aberration corrections are enabled, this */
196 /*     correction will also be applied to the apparent positions of the */
197 /*     centers of the two objects. */
198 
199 /* $ Examples */
200 
201 /*     None. */
202 
203 /* $ Restrictions */
204 
205 /*     None. */
206 
207 /* $ Literature_References */
208 
209 /*     None. */
210 
211 /* $ Author_and_Institution */
212 
213 /*     W.L. Taber     (JPL) */
214 /*     L.S. Elson     (JPL) */
215 
216 /* $ Version */
217 
218 /* -    SPICELIB Version 1.0.1, 28-JUN-2012 (EDW) */
219 
220 /*        Minor edits to header, correcting spelling error and improving */
221 /*        syntax of Exceptions. */
222 
223 /*        Corrected a typo in SETMSG error message where TARG1 was quoted */
224 /*        twice instead of quoting TARG1 and TARG2. This edit does change */
225 /*        the error message output. */
226 
227 /* -    SPICELIB Version 1.0.0, 03-MAR-2009 (EDW) */
228 
229 /* -& */
230 /* $ Index_Entries */
231 
232 /*     compute the apparent relative angular separation */
233 
234 /* -& */
235 
236 /*     SPICELIB functions. */
237 
238 
239 /*     Local Variables. */
240 
241 
242 /*     ATOL is a tolerance value for computing arc sine. */
243 
244 
245 /*     Standard SPICE error handling. */
246 
247     if (return_()) {
248 	return 0;
249     }
250     chkin_("ZZGFSPQ", (ftnlen)7);
251 
252 /*     First check for bad inputs. */
253 
254     if (*r1 < 0. || *r2 < 0.) {
255 	setmsg_("A negative radius for a body was encountered. The radius fo"
256 		"r body # was given as #, the radius of body # was given as #"
257 		". ", (ftnlen)121);
258 	errint_("#", targ1, (ftnlen)1);
259 	errdp_("#", r1, (ftnlen)1);
260 	errint_("#", targ2, (ftnlen)1);
261 	errdp_("#", r2, (ftnlen)1);
262 	sigerr_("SPICE(BADRADIUS)", (ftnlen)16);
263 	chkout_("ZZGFSPQ", (ftnlen)7);
264 	return 0;
265     }
266 
267 /*     Get the state of the TARG1, TARG2 objects relative to OBS. */
268 
269     spkezp_(targ1, et, ref, abcorr, obs, pv1, &lt, ref_len, abcorr_len);
270     if (failed_()) {
271 	chkout_("ZZGFSPQ", (ftnlen)7);
272 	return 0;
273     }
274     spkezp_(targ2, et, ref, abcorr, obs, pv2, &lt, ref_len, abcorr_len);
275     if (failed_()) {
276 	chkout_("ZZGFSPQ", (ftnlen)7);
277 	return 0;
278     }
279 
280 /*     Compute the range to the objects of interest. */
281 
282     range1 = vnorm_(pv1);
283     range2 = vnorm_(pv2);
284 
285 /*     Compute the apparent angular radii as seen from OBS. */
286 
287     if (range1 > *r1) {
288 	d__1 = *r1 / range1;
289 	ang1 = dasine_(&d__1, &c_b12);
290 	if (failed_()) {
291 	    chkout_("ZZGFSPQ", (ftnlen)7);
292 	    return 0;
293 	}
294     } else {
295 	ang1 = halfpi_();
296     }
297     if (range2 > *r2) {
298 	d__1 = *r2 / range2;
299 	ang2 = dasine_(&d__1, &c_b12);
300 	if (failed_()) {
301 	    chkout_("ZZGFSPQ", (ftnlen)7);
302 	    return 0;
303 	}
304     } else {
305 	ang2 = halfpi_();
306     }
307 
308 /*     Finally compute the apparent separation. */
309 
310     theta = vsep_(pv1, pv2);
311     *value = theta - ang1 - ang2;
312     chkout_("ZZGFSPQ", (ftnlen)7);
313     return 0;
314 } /* zzgfspq_ */
315 
316