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Last change
on this file since 1118 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 | double slaPav ( float v1 [ 3 ], float v2 [ 3 ] )
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| 4 | /*
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| 5 | ** - - - - - - -
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| 6 | ** s l a P a v
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| 7 | ** - - - - - - -
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| 8 | **
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| 9 | ** Position angle of one celestial direction with respect to another.
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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 | ** v1 float[3] direction cosines of one point
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| 15 | ** v2 float[3] direction cosines of the other point
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| 16 | **
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| 17 | ** (The coordinate frames correspond to RA,Dec, Long,Lat etc.)
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| 18 | **
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| 19 | ** The result is the bearing (position angle), in radians, of point
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| 20 | ** v2 with respect to point v1. It is in the range +/- pi. The
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| 21 | ** sense is such that if v2 is a small distance east of v1, the
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| 22 | ** bearing is about +pi/2. Zero is returned if the two points
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| 23 | ** are coincident.
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| 24 | **
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| 25 | ** The vectors v1 and v2 need not be unit vectors.
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| 26 | **
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| 27 | ** The routine slaBear performs an equivalent function except
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| 28 | ** that the points are specified in the form of spherical
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| 29 | ** coordinates.
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| 30 | **
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| 31 | ** Called: slaDpav
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| 32 | **
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| 33 | ** Last revision: 9 December 1996
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| 34 | **
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| 35 | ** Copyright P.T.Wallace. All rights reserved.
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| 36 | */
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| 37 | {
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| 38 | int i;
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| 39 | double d1 [ 3 ], d2 [ 3 ];
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| 40 |
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| 41 |
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| 42 | /* Call the double precision version. */
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| 43 | for ( i = 0; i < 3; i++ ) {
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| 44 | d1 [ i ] = (double) v1 [ i ];
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| 45 | d2 [ i ] = (double) v2 [ i ];
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| 46 | }
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| 47 | return (float) slaDpav ( d1, d2 );
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| 48 | }
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