1 | #include "slalib.h"
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2 | #include "slamac.h"
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3 | double slaDpav ( double v1 [ 3 ], double v2 [ 3 ] )
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4 | /*
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5 | ** - - - - - - - -
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6 | ** s l a D 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 | ** (double precision)
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12 | **
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13 | ** Given:
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14 | ** v1 double[3] direction cosines of one point
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15 | ** v2 double[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 slaDbear 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 | ** Last revision: 12 December 1996
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32 | **
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33 | ** Copyright P.T.Wallace. All rights reserved.
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34 | */
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35 | {
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36 | double x0, y0, z0, w, x1, y1, z1, s, c;
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37 |
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38 |
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39 | /* Unit vector to point 1. */
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40 | x0 = v1 [ 0 ];
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41 | y0 = v1 [ 1 ];
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42 | z0 = v1 [ 2 ];
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43 | w = sqrt ( x0 * x0 + y0 * y0 + z0 * z0 );
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44 | if ( w != 0.0 ) { x0 /= w; y0 /= w; z0 /= w; }
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45 |
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46 | /* Vector to point 2. */
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47 | x1 = v2 [ 0 ];
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48 | y1 = v2 [ 1 ];
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49 | z1 = v2 [ 2 ];
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50 |
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51 | /* Position angle. */
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52 | s = y1 * x0 - x1 * y0;
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53 | c = z1 * ( x0 * x0 + y0 * y0 ) - z0 * ( x1 * x0 + y1 * y0 );
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54 | return ( s != 0.0 || c != 0.0 ) ? atan2 ( s, c ) : 0.0;
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55 | }
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