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 on this file since 8395 was             731, checked in by tbretz, 25 years ago | 
        
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| 1 | #include "slalib.h" | 
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| 2 | #include "slamac.h" | 
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| 3 | float slaRverot ( float phi, float ra, float da, float st ) | 
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| 4 | /* | 
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| 5 | **  - - - - - - - - - - | 
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| 6 | **   s l a R v e r o t | 
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| 7 | **  - - - - - - - - - - | 
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| 8 | ** | 
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| 9 | **  Velocity component in a given direction due to Earth rotation. | 
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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 | **     phi     float    latitude of observing station (geodetic) | 
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| 15 | **     ra,da   float    apparent RA,Dec | 
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| 16 | **     st      float    local apparent sidereal time | 
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| 17 | ** | 
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| 18 | **     phi, ra, dec and st are all in radians. | 
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| 19 | ** | 
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| 20 | **  Result: | 
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| 21 | **     Component of Earth rotation in direction ra,da (km/s) | 
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| 22 | ** | 
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| 23 | **  Sign convention: | 
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| 24 | **     The result is +ve when the observer is receding from the | 
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| 25 | **     given point on the sky. | 
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| 26 | ** | 
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| 27 | **  Accuracy: | 
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| 28 | **     The simple algorithm used assumes a spherical Earth, of | 
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| 29 | **     a radius chosen to give results accurate to about 0.0005 km/s | 
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| 30 | **     for observing stations at typical latitudes and heights.  For | 
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| 31 | **     applications requiring greater precision, use the routine | 
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| 32 | **     slaPvobs. | 
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| 33 | ** | 
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| 34 | **  Last revision:   9 April 1998 | 
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| 35 | ** | 
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| 36 | **  Copyright P.T.Wallace.  All rights reserved. | 
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| 37 | */ | 
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| 38 |  | 
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| 39 | #define ESPEED 0.4655   /* Nominal mean sidereal speed of Earth equator | 
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| 40 | in km/s (the actual value is about 0.4651) */ | 
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| 41 |  | 
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| 42 | { | 
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| 43 | return (float) ( ESPEED * cos ( (double) phi ) * | 
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| 44 | sin ( (double) ( st - ra ) ) * | 
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| 45 | cos ( (double) da ) ); | 
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| 46 | } | 
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