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/* |
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*+ |
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* Name: |
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* palDh2e |
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* Purpose: |
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* Horizon to equatorial coordinates: Az,El to HA,Dec |
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* Language: |
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* Starlink ANSI C |
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12
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* Type of Module: |
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* Library routine |
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15
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* Invocation: |
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* palDh2e( double az, double el, double phi, double * ha, double * dec ); |
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18
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* Arguments: |
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* az = double (Given) |
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* Azimuth (radians) |
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* el = double (Given) |
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* Elevation (radians) |
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* phi = double (Given) |
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* Observatory latitude (radians) |
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* ha = double * (Returned) |
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* Hour angle (radians) |
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* dec = double * (Returned) |
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* Declination (radians) |
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* Description: |
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* Convert horizon to equatorial coordinates. |
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33
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* Authors: |
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34
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* PTW: Pat Wallace (STFC) |
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35
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* TIMJ: Tim Jenness (JAC, Hawaii) |
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* {enter_new_authors_here} |
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* Notes: |
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* - All the arguments are angles in radians. |
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* - The sign convention for azimuth is north zero, east +pi/2. |
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* - HA is returned in the range +/-pi. Declination is returned |
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* in the range +/-pi/2. |
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* - The latitude is (in principle) geodetic. In critical |
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* applications, corrections for polar motion should be applied. |
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* - In some applications it will be important to specify the |
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* correct type of elevation in order to produce the required |
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* type of HA,Dec. In particular, it may be important to |
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* distinguish between the elevation as affected by refraction, |
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* which will yield the "observed" HA,Dec, and the elevation |
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* in vacuo, which will yield the "topocentric" HA,Dec. If the |
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* effects of diurnal aberration can be neglected, the |
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* topocentric HA,Dec may be used as an approximation to the |
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* "apparent" HA,Dec. |
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* - No range checking of arguments is done. |
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* - In applications which involve many such calculations, rather |
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* than calling the present routine it will be more efficient to |
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57
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* use inline code, having previously computed fixed terms such |
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58
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* as sine and cosine of latitude. |
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60
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* History: |
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* 2012-02-08 (TIMJ): |
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* Initial version with documentation taken from Fortran SLA |
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* Adapted with permission from the Fortran SLALIB library. |
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* {enter_further_changes_here} |
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66
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* Copyright: |
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* Copyright (C) 1996 Rutherford Appleton Laboratory |
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* Copyright (C) 2012 Science and Technology Facilities Council. |
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* All Rights Reserved. |
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71
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* Licence: |
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72
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* This program is free software: you can redistribute it and/or |
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73
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* modify it under the terms of the GNU Lesser General Public |
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74
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* License as published by the Free Software Foundation, either |
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75
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* version 3 of the License, or (at your option) any later |
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76
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* version. |
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77
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* |
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* This program is distributed in the hope that it will be useful, |
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79
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* but WITHOUT ANY WARRANTY; without even the implied warranty of |
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80
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* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the |
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81
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* GNU Lesser General Public License for more details. |
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* |
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83
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* You should have received a copy of the GNU Lesser General |
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84
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* License along with this program. If not, see |
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85
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* . |
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86
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87
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* Bugs: |
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88
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* {note_any_bugs_here} |
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89
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*- |
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*/ |
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91
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92
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#include "pal.h" |
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93
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#include |
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94
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95
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void |
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96
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0
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palDh2e ( double az, double el, double phi, double *ha, double *dec) { |
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97
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98
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double sa; |
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99
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double ca; |
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100
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double se; |
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101
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double ce; |
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102
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double sp; |
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103
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double cp; |
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104
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105
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double x; |
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106
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double y; |
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107
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double z; |
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108
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double r; |
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109
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110
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/* Useful trig functions */ |
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111
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0
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sa = sin(az); |
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112
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0
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ca = cos(az); |
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113
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0
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se = sin(el); |
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114
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0
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ce = cos(el); |
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115
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0
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sp = sin(phi); |
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116
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0
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cp = cos(phi); |
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117
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118
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/* HA,Dec as x,y,z */ |
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119
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0
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x = -ca * ce * sp + se * cp; |
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120
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0
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y = -sa * ce; |
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121
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0
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z = ca * ce * cp + se * sp; |
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122
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123
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/* To HA,Dec */ |
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124
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0
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r = sqrt(x * x + y * y); |
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125
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0
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0
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if (r == 0.) { |
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126
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0
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*ha = 0.; |
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127
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} else { |
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128
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0
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*ha = atan2(y, x); |
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129
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} |
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130
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0
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*dec = atan2(z, r); |
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131
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132
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0
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return; |
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133
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} |