| line | stmt | bran | cond | sub | pod | time | code | 
| 1 |  |  |  |  |  |  | /* | 
| 2 |  |  |  |  |  |  | *+ | 
| 3 |  |  |  |  |  |  | *  Name: | 
| 4 |  |  |  |  |  |  | *     palPrebn | 
| 5 |  |  |  |  |  |  |  | 
| 6 |  |  |  |  |  |  | *  Purpose: | 
| 7 |  |  |  |  |  |  | *     Generate the matrix of precession between two objects (old) | 
| 8 |  |  |  |  |  |  |  | 
| 9 |  |  |  |  |  |  | *  Language: | 
| 10 |  |  |  |  |  |  | *     Starlink ANSI C | 
| 11 |  |  |  |  |  |  |  | 
| 12 |  |  |  |  |  |  | *  Type of Module: | 
| 13 |  |  |  |  |  |  | *     Library routine | 
| 14 |  |  |  |  |  |  |  | 
| 15 |  |  |  |  |  |  | *  Invocation: | 
| 16 |  |  |  |  |  |  | *     void palPrebn ( double bep0, double bep1, double rmatp[3][3] ); | 
| 17 |  |  |  |  |  |  |  | 
| 18 |  |  |  |  |  |  | *  Arguments: | 
| 19 |  |  |  |  |  |  | *     bep0 = double (Given) | 
| 20 |  |  |  |  |  |  | *        Beginning Besselian epoch. | 
| 21 |  |  |  |  |  |  | *     bep1 = double (Given) | 
| 22 |  |  |  |  |  |  | *        Ending Besselian epoch | 
| 23 |  |  |  |  |  |  | *     rmatp = double[3][3] (Returned) | 
| 24 |  |  |  |  |  |  | *        precession matrix in the sense V(BEP1) = RMATP * V(BEP0) | 
| 25 |  |  |  |  |  |  |  | 
| 26 |  |  |  |  |  |  | *  Description: | 
| 27 |  |  |  |  |  |  | *     Generate the matrix of precession between two epochs, | 
| 28 |  |  |  |  |  |  | *     using the old, pre-IAU1976, Bessel-Newcomb model, using | 
| 29 |  |  |  |  |  |  | *     Kinoshita's formulation | 
| 30 |  |  |  |  |  |  |  | 
| 31 |  |  |  |  |  |  | *  Authors: | 
| 32 |  |  |  |  |  |  | *     PTW: Pat Wallace (STFC) | 
| 33 |  |  |  |  |  |  | *     TIMJ: Tim Jenness (JAC, Hawaii) | 
| 34 |  |  |  |  |  |  | *     {enter_new_authors_here} | 
| 35 |  |  |  |  |  |  |  | 
| 36 |  |  |  |  |  |  | *  See Also: | 
| 37 |  |  |  |  |  |  | *     Kinoshita, H. (1975) 'Formulas for precession', SAO Special | 
| 38 |  |  |  |  |  |  | *     Report No. 364, Smithsonian Institution Astrophysical | 
| 39 |  |  |  |  |  |  | *     Observatory, Cambridge, Massachusetts. | 
| 40 |  |  |  |  |  |  |  | 
| 41 |  |  |  |  |  |  | *  History: | 
| 42 |  |  |  |  |  |  | *     2012-02-12(TIMJ): | 
| 43 |  |  |  |  |  |  | *        Initial version with documentation taken from Fortran SLA | 
| 44 |  |  |  |  |  |  | *        Adapted with permission from the Fortran SLALIB library. | 
| 45 |  |  |  |  |  |  | *     {enter_further_changes_here} | 
| 46 |  |  |  |  |  |  |  | 
| 47 |  |  |  |  |  |  | *  Copyright: | 
| 48 |  |  |  |  |  |  | *     Copyright (C) 1996 Rutherford Appleton Laboratory | 
| 49 |  |  |  |  |  |  | *     Copyright (C) 2012 Science and Technology Facilities Council. | 
| 50 |  |  |  |  |  |  | *     All Rights Reserved. | 
| 51 |  |  |  |  |  |  |  | 
| 52 |  |  |  |  |  |  | *  Licence: | 
| 53 |  |  |  |  |  |  | *     This program is free software: you can redistribute it and/or | 
| 54 |  |  |  |  |  |  | *     modify it under the terms of the GNU Lesser General Public | 
| 55 |  |  |  |  |  |  | *     License as published by the Free Software Foundation, either | 
| 56 |  |  |  |  |  |  | *     version 3 of the License, or (at your option) any later | 
| 57 |  |  |  |  |  |  | *     version. | 
| 58 |  |  |  |  |  |  | * | 
| 59 |  |  |  |  |  |  | *     This program is distributed in the hope that it will be useful, | 
| 60 |  |  |  |  |  |  | *     but WITHOUT ANY WARRANTY; without even the implied warranty of | 
| 61 |  |  |  |  |  |  | *     MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the | 
| 62 |  |  |  |  |  |  | *     GNU Lesser General Public License for more details. | 
| 63 |  |  |  |  |  |  | * | 
| 64 |  |  |  |  |  |  | *     You should have received a copy of the GNU Lesser General | 
| 65 |  |  |  |  |  |  | *     License along with this program.  If not, see | 
| 66 |  |  |  |  |  |  | *     . | 
| 67 |  |  |  |  |  |  |  | 
| 68 |  |  |  |  |  |  | *  Bugs: | 
| 69 |  |  |  |  |  |  | *     {note_any_bugs_here} | 
| 70 |  |  |  |  |  |  | *- | 
| 71 |  |  |  |  |  |  | */ | 
| 72 |  |  |  |  |  |  |  | 
| 73 |  |  |  |  |  |  | #include "pal.h" | 
| 74 |  |  |  |  |  |  | #include "palmac.h" | 
| 75 |  |  |  |  |  |  |  | 
| 76 | 3 |  |  |  |  |  | void palPrebn ( double bep0, double bep1, double rmatp[3][3] ) { | 
| 77 |  |  |  |  |  |  |  | 
| 78 |  |  |  |  |  |  | double t,bigt, zeta, theta, z, tas2r, w; | 
| 79 |  |  |  |  |  |  |  | 
| 80 |  |  |  |  |  |  | /* Interval between basic epoch B1850.0 and beginning epoch in TC */ | 
| 81 | 3 |  |  |  |  |  | bigt = (bep0-1850)/100.; | 
| 82 |  |  |  |  |  |  |  | 
| 83 |  |  |  |  |  |  | /*  Interval over which precession required, in tropical centuries */ | 
| 84 | 3 |  |  |  |  |  | t = (bep1-bep0)/100.; | 
| 85 |  |  |  |  |  |  |  | 
| 86 |  |  |  |  |  |  | /* Euler angles */ | 
| 87 | 3 |  |  |  |  |  | tas2r = t * PAL__DAS2R; | 
| 88 | 3 |  |  |  |  |  | w = 2303.5548 + ( 1.39720 + 0.000059 * bigt) * bigt; | 
| 89 |  |  |  |  |  |  |  | 
| 90 | 3 |  |  |  |  |  | zeta = ( w + ( 0.30242 - 0.000269 * bigt + 0.017996 * t ) * t ) * tas2r; | 
| 91 | 3 |  |  |  |  |  | z = ( w + ( 1.09478 + 0.000387 * bigt + 0.018324 * t ) * t ) * tas2r; | 
| 92 | 6 |  |  |  |  |  | theta = ( 2005.1125 + ( -0.85294 - 0.000365 * bigt ) * bigt + | 
| 93 | 3 |  |  |  |  |  | (-0.42647 - 0.000365 * bigt - 0.041802 * t ) * t ) * tas2r; | 
| 94 |  |  |  |  |  |  |  | 
| 95 |  |  |  |  |  |  | /*  Rotation matrix */ | 
| 96 | 3 |  |  |  |  |  | palDeuler("ZYZ", -zeta, theta, -z, rmatp); | 
| 97 |  |  |  |  |  |  |  | 
| 98 | 3 |  |  |  |  |  | } |