| 1 | #include "sofa.h"
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| 2 |
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| 3 | void iauApio(double sp, double theta,
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| 4 | double elong, double phi, double hm, double xp, double yp,
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| 5 | double refa, double refb,
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| 6 | iauASTROM *astrom)
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| 7 | /*
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| 8 | ** - - - - - - - -
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| 9 | ** i a u A p i o
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| 10 | ** - - - - - - - -
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| 11 | **
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| 12 | ** For a terrestrial observer, prepare star-independent astrometry
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| 13 | ** parameters for transformations between CIRS and observed
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| 14 | ** coordinates. The caller supplies the Earth orientation information
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| 15 | ** and the refraction constants as well as the site coordinates.
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| 16 | **
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| 17 | ** This function is part of the International Astronomical Union's
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| 18 | ** SOFA (Standards of Fundamental Astronomy) software collection.
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| 19 | **
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| 20 | ** Status: support function.
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| 21 | **
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| 22 | ** Given:
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| 23 | ** sp double the TIO locator s' (radians, Note 1)
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| 24 | ** theta double Earth rotation angle (radians)
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| 25 | ** elong double longitude (radians, east +ve, Note 2)
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| 26 | ** phi double geodetic latitude (radians, Note 2)
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| 27 | ** hm double height above ellipsoid (m, geodetic Note 2)
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| 28 | ** xp,yp double polar motion coordinates (radians, Note 3)
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| 29 | ** refa double refraction constant A (radians, Note 4)
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| 30 | ** refb double refraction constant B (radians, Note 4)
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| 31 | **
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| 32 | ** Returned:
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| 33 | ** astrom iauASTROM* star-independent astrometry parameters:
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| 34 | ** pmt double unchanged
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| 35 | ** eb double[3] unchanged
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| 36 | ** eh double[3] unchanged
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| 37 | ** em double unchanged
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| 38 | ** v double[3] unchanged
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| 39 | ** bm1 double unchanged
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| 40 | ** bpn double[3][3] unchanged
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| 41 | ** along double longitude + s' (radians)
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| 42 | ** xpl double polar motion xp wrt local meridian (radians)
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| 43 | ** ypl double polar motion yp wrt local meridian (radians)
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| 44 | ** sphi double sine of geodetic latitude
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| 45 | ** cphi double cosine of geodetic latitude
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| 46 | ** diurab double magnitude of diurnal aberration vector
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| 47 | ** eral double "local" Earth rotation angle (radians)
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| 48 | ** refa double refraction constant A (radians)
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| 49 | ** refb double refraction constant B (radians)
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| 50 | **
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| 51 | ** Notes:
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| 52 | **
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| 53 | ** 1) sp, the TIO locator s', is a tiny quantity needed only by the
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| 54 | ** most precise applications. It can either be set to zero or
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| 55 | ** predicted using the SOFA function iauSp00.
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| 56 | **
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| 57 | ** 2) The geographical coordinates are with respect to the WGS84
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| 58 | ** reference ellipsoid. TAKE CARE WITH THE LONGITUDE SIGN: the
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| 59 | ** longitude required by the present function is east-positive
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| 60 | ** (i.e. right-handed), in accordance with geographical convention.
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| 61 | **
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| 62 | ** 3) The polar motion xp,yp can be obtained from IERS bulletins. The
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| 63 | ** values are the coordinates (in radians) of the Celestial
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| 64 | ** Intermediate Pole with respect to the International Terrestrial
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| 65 | ** Reference System (see IERS Conventions 2003), measured along the
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| 66 | ** meridians 0 and 90 deg west respectively. For many applications,
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| 67 | ** xp and yp can be set to zero.
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| 68 | **
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| 69 | ** Internally, the polar motion is stored in a form rotated onto the
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| 70 | ** local meridian.
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| 71 | **
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| 72 | ** 4) The refraction constants refa and refb are for use in a
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| 73 | ** dZ = A*tan(Z)+B*tan^3(Z) model, where Z is the observed
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| 74 | ** (i.e. refracted) zenith distance and dZ is the amount of
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| 75 | ** refraction.
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| 76 | **
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| 77 | ** 5) It is advisable to take great care with units, as even unlikely
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| 78 | ** values of the input parameters are accepted and processed in
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| 79 | ** accordance with the models used.
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| 80 | **
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| 81 | ** 6) In cases where the caller does not wish to provide the Earth
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| 82 | ** rotation information and refraction constants, the function
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| 83 | ** iauApio13 can be used instead of the present function. This
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| 84 | ** starts from UTC and weather readings etc. and computes suitable
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| 85 | ** values using other SOFA functions.
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| 86 | **
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| 87 | ** 7) This is one of several functions that inserts into the astrom
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| 88 | ** structure star-independent parameters needed for the chain of
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| 89 | ** astrometric transformations ICRS <-> GCRS <-> CIRS <-> observed.
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| 90 | **
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| 91 | ** The various functions support different classes of observer and
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| 92 | ** portions of the transformation chain:
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| 93 | **
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| 94 | ** functions observer transformation
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| 95 | **
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| 96 | ** iauApcg iauApcg13 geocentric ICRS <-> GCRS
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| 97 | ** iauApci iauApci13 terrestrial ICRS <-> CIRS
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| 98 | ** iauApco iauApco13 terrestrial ICRS <-> observed
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| 99 | ** iauApcs iauApcs13 space ICRS <-> GCRS
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| 100 | ** iauAper iauAper13 terrestrial update Earth rotation
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| 101 | ** iauApio iauApio13 terrestrial CIRS <-> observed
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| 102 | **
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| 103 | ** Those with names ending in "13" use contemporary SOFA models to
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| 104 | ** compute the various ephemerides. The others accept ephemerides
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| 105 | ** supplied by the caller.
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| 106 | **
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| 107 | ** The transformation from ICRS to GCRS covers space motion,
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| 108 | ** parallax, light deflection, and aberration. From GCRS to CIRS
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| 109 | ** comprises frame bias and precession-nutation. From CIRS to
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| 110 | ** observed takes account of Earth rotation, polar motion, diurnal
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| 111 | ** aberration and parallax (unless subsumed into the ICRS <-> GCRS
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| 112 | ** transformation), and atmospheric refraction.
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| 113 | **
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| 114 | ** 8) The context structure astrom produced by this function is used by
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| 115 | ** iauAtioq and iauAtoiq.
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| 116 | **
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| 117 | ** Called:
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| 118 | ** iauPvtob position/velocity of terrestrial station
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| 119 | ** iauAper astrometry parameters: update ERA
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| 120 | **
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| 121 | ** This revision: 2013 October 9
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| 122 | **
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| 123 | ** SOFA release 2015-02-09
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| 124 | **
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| 125 | ** Copyright (C) 2015 IAU SOFA Board. See notes at end.
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| 126 | */
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| 127 | {
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| 128 | double sl, cl, pv[2][3];
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| 129 |
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| 130 | /* Longitude with adjustment for TIO locator s'. */
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| 131 | astrom->along = elong + sp;
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| 132 |
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| 133 | /* Polar motion, rotated onto the local meridian. */
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| 134 | sl = sin(astrom->along);
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| 135 | cl = cos(astrom->along);
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| 136 | astrom->xpl = xp*cl - yp*sl;
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| 137 | astrom->ypl = xp*sl + yp*cl;
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| 138 |
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| 139 | /* Functions of latitude. */
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| 140 | astrom->sphi = sin(phi);
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| 141 | astrom->cphi = cos(phi);
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| 142 |
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| 143 | /* Observer's geocentric position and velocity (m, m/s, CIRS). */
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| 144 | iauPvtob(elong, phi, hm, xp, yp, sp, theta, pv);
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| 145 |
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| 146 | /* Magnitude of diurnal aberration vector. */
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| 147 | astrom->diurab = sqrt(pv[1][0]*pv[1][0]+pv[1][1]*pv[1][1]) / CMPS;
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| 148 |
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| 149 | /* Refraction constants. */
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| 150 | astrom->refa = refa;
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| 151 | astrom->refb = refb;
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| 152 |
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| 153 | /* Local Earth rotation angle. */
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| 154 | iauAper(theta, astrom);
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| 155 |
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| 156 | /* Finished. */
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| 157 |
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| 158 | /*----------------------------------------------------------------------
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| 159 | **
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| 160 | ** Copyright (C) 2015
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| 161 | ** Standards Of Fundamental Astronomy Board
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| 162 | ** of the International Astronomical Union.
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| 163 | **
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| 164 | ** =====================
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| 165 | ** SOFA Software License
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| 166 | ** =====================
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| 167 | **
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| 168 | ** NOTICE TO USER:
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| 169 | **
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| 170 | ** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
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| 171 | ** CONDITIONS WHICH APPLY TO ITS USE.
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| 172 | **
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| 173 | ** 1. The Software is owned by the IAU SOFA Board ("SOFA").
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| 174 | **
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| 175 | ** 2. Permission is granted to anyone to use the SOFA software for any
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| 176 | ** purpose, including commercial applications, free of charge and
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| 177 | ** without payment of royalties, subject to the conditions and
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| 178 | ** restrictions listed below.
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| 179 | **
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| 180 | ** 3. You (the user) may copy and distribute SOFA source code to others,
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| 181 | ** and use and adapt its code and algorithms in your own software,
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| 182 | ** on a world-wide, royalty-free basis. That portion of your
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| 183 | ** distribution that does not consist of intact and unchanged copies
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| 184 | ** of SOFA source code files is a "derived work" that must comply
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| 185 | ** with the following requirements:
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| 186 | **
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| 187 | ** a) Your work shall be marked or carry a statement that it
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| 188 | ** (i) uses routines and computations derived by you from
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| 189 | ** software provided by SOFA under license to you; and
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| 190 | ** (ii) does not itself constitute software provided by and/or
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| 191 | ** endorsed by SOFA.
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| 192 | **
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| 193 | ** b) The source code of your derived work must contain descriptions
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| 194 | ** of how the derived work is based upon, contains and/or differs
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| 195 | ** from the original SOFA software.
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| 196 | **
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| 197 | ** c) The names of all routines in your derived work shall not
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| 198 | ** include the prefix "iau" or "sofa" or trivial modifications
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| 199 | ** thereof such as changes of case.
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| 200 | **
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| 201 | ** d) The origin of the SOFA components of your derived work must
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| 202 | ** not be misrepresented; you must not claim that you wrote the
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| 203 | ** original software, nor file a patent application for SOFA
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| 204 | ** software or algorithms embedded in the SOFA software.
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| 205 | **
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| 206 | ** e) These requirements must be reproduced intact in any source
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| 207 | ** distribution and shall apply to anyone to whom you have
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| 208 | ** granted a further right to modify the source code of your
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| 209 | ** derived work.
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| 210 | **
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| 211 | ** Note that, as originally distributed, the SOFA software is
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| 212 | ** intended to be a definitive implementation of the IAU standards,
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| 213 | ** and consequently third-party modifications are discouraged. All
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| 214 | ** variations, no matter how minor, must be explicitly marked as
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| 215 | ** such, as explained above.
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| 216 | **
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| 217 | ** 4. You shall not cause the SOFA software to be brought into
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| 218 | ** disrepute, either by misuse, or use for inappropriate tasks, or
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| 219 | ** by inappropriate modification.
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| 220 | **
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| 221 | ** 5. The SOFA software is provided "as is" and SOFA makes no warranty
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| 222 | ** as to its use or performance. SOFA does not and cannot warrant
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| 223 | ** the performance or results which the user may obtain by using the
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| 224 | ** SOFA software. SOFA makes no warranties, express or implied, as
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| 225 | ** to non-infringement of third party rights, merchantability, or
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| 226 | ** fitness for any particular purpose. In no event will SOFA be
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| 227 | ** liable to the user for any consequential, incidental, or special
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| 228 | ** damages, including any lost profits or lost savings, even if a
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| 229 | ** SOFA representative has been advised of such damages, or for any
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| 230 | ** claim by any third party.
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| 231 | **
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| 232 | ** 6. The provision of any version of the SOFA software under the terms
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| 233 | ** and conditions specified herein does not imply that future
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| 234 | ** versions will also be made available under the same terms and
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| 235 | ** conditions.
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| 236 | *
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| 237 | ** In any published work or commercial product which uses the SOFA
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| 238 | ** software directly, acknowledgement (see www.iausofa.org) is
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| 239 | ** appreciated.
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| 240 | **
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| 241 | ** Correspondence concerning SOFA software should be addressed as
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| 242 | ** follows:
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| 243 | **
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| 244 | ** By email: sofa@ukho.gov.uk
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| 245 | ** By post: IAU SOFA Center
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| 246 | ** HM Nautical Almanac Office
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| 247 | ** UK Hydrographic Office
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| 248 | ** Admiralty Way, Taunton
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| 249 | ** Somerset, TA1 2DN
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| 250 | ** United Kingdom
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| 251 | **
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| 252 | **--------------------------------------------------------------------*/
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| 253 |
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| 254 | }
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