1 | #include "slalib.h"
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2 | #include "slamac.h"
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3 | float slaRvlg ( float r2000, float d2000 )
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4 | /*
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5 | ** - - - - - - - -
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6 | ** s l a R v l g
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7 | ** - - - - - - - -
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8 | **
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9 | ** Velocity component in a given direction due to the combination
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10 | ** of the rotation of the Galaxy and the motion of the Galaxy
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11 | ** relative to the mean motion of the local group.
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12 | **
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13 | ** (single precision)
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14 | **
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15 | ** Given:
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16 | ** r2000,d2000 float J2000.0 mean RA,Dec (radians)
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17 | **
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18 | ** Result:
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19 | ** Component of solar motion in direction r2000,d2000 (km/s)
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20 | **
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21 | ** Sign convention:
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22 | ** The result is +ve when the Sun is receding from the
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23 | ** given point on the sky.
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24 | **
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25 | ** Reference:
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26 | ** IAU trans 1976, 168, p201.
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27 | **
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28 | ** Called:
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29 | ** slaCs2c, slaVdv
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30 | **
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31 | ** Last revision: 15 July 1993
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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 | /*
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37 | ** Solar velocity due to galactic rotation and translation
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38 | **
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39 | ** speed = 300 km/s
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40 | **
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41 | ** apex = l2,b2 90deg, 0deg
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42 | ** = RA,dec 21 12 01.1 +48 19 47 J2000.0
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43 | **
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44 | ** This is expressed in the form of a J2000.0 x,y,z vector:
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45 | **
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46 | ** va(1) = x = -speed*cos(ra)*cos(dec)
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47 | ** va(2) = y = -speed*sin(ra)*cos(dec)
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48 | ** va(3) = z = -speed*sin(dec)
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49 | */
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50 | static float va[3] = { -148.23284f, 133.44888f, -224.09467f };
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51 | float vb[3];
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52 |
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53 | /* Convert given J2000 RA,dec to x,y,z */
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54 | slaCs2c ( r2000, d2000, vb );
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55 |
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56 | /* Compute dot product with solar motion vector */
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57 | return slaVdv ( va, vb);
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58 | }
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