| 1 | #include "slalib.h" | 
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| 2 | #include "slamac.h" | 
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| 3 | void slaH2e ( float az, float el, float phi, float *ha, float *dec ) | 
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| 4 | /* | 
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| 5 | **  - - - - - - - | 
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| 6 | **   s l a H 2 e | 
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| 7 | **  - - - - - - - | 
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| 8 | ** | 
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| 9 | **  Horizon to equatorial coordinates:  Az,El to HA,Dec | 
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| 10 | ** | 
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| 11 | **  (single precision) | 
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| 12 | ** | 
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| 13 | **  Given: | 
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| 14 | **     az          float       azimuth | 
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| 15 | **     el          float       elevation | 
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| 16 | **     phi         float       observatory latitude | 
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| 17 | ** | 
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| 18 | **  Returned: | 
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| 19 | **     *ha         float       hour angle | 
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| 20 | **     *dec        float       declination | 
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| 21 | ** | 
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| 22 | **  Notes: | 
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| 23 | ** | 
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| 24 | **  1)  All the arguments are angles in radians. | 
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| 25 | ** | 
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| 26 | **  2)  The sign convention for azimuth is north zero, east +pi/2. | 
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| 27 | ** | 
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| 28 | **  3)  HA is returned in the range +/-pi.  Declination is returned | 
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| 29 | **      in the range +/-pi/2. | 
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| 30 | ** | 
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| 31 | **  4)  The latitude is (in principle) geodetic.  In critical | 
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| 32 | **      applications, corrections for polar motion should be applied. | 
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| 33 | ** | 
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| 34 | **  5)  In some applications it will be important to specify the | 
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| 35 | **      correct type of elevation in order to produce the required | 
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| 36 | **      type of HA,Dec.  In particular, it may be important to | 
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| 37 | **      distinguish between the elevation as affected by refraction, | 
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| 38 | **      which will yield the "observed" HA,Dec, and the elevation | 
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| 39 | **      in vacuo, which will yield the "topocentric" HA,Dec.  If the | 
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| 40 | **      effects of diurnal aberration can be neglected, the | 
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| 41 | **      topocentric HA,Dec may be used as an approximation to the | 
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| 42 | **      "apparent" HA,Dec. | 
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| 43 | ** | 
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| 44 | **  6)  No range checking of arguments is done. | 
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| 45 | ** | 
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| 46 | **  7)  In applications which involve many such calculations, rather | 
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| 47 | **      than calling the present routine it will be more efficient to | 
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| 48 | **      use inline code, having previously computed fixed terms such | 
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| 49 | **      as sine and cosine of latitude. | 
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| 50 | ** | 
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| 51 | **  Last revision:   21 February 1996 | 
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| 52 | ** | 
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| 53 | **  Copyright P.T.Wallace.  All rights reserved. | 
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| 54 | */ | 
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| 55 | { | 
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| 56 | float sa, ca, se, ce, sp, cp, x, y, z, r; | 
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| 57 |  | 
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| 58 | /* Useful trig functions */ | 
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| 59 | sa = (float) sin ( az ); | 
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| 60 | ca = (float) cos ( az ); | 
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| 61 | se = (float) sin ( el ); | 
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| 62 | ce = (float) cos ( el ); | 
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| 63 | sp = (float) sin ( phi ); | 
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| 64 | cp = (float) cos ( phi ); | 
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| 65 |  | 
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| 66 | /* HA,Dec as x,y,z */ | 
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| 67 | x = - ca * ce * sp + se * cp; | 
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| 68 | y = - sa * ce; | 
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| 69 | z = ca * ce * cp + se * sp; | 
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| 70 |  | 
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| 71 | /* To spherical */ | 
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| 72 | r = (float) sqrt ( x * x + y * y ); | 
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| 73 | *ha = ( r == 0.0f ) ? 0.0f : (float) atan2 ( y, x ) ; | 
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| 74 | *dec = (float) atan2 ( z, r ); | 
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| 75 | } | 
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