1 | /*
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2 | *+
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3 | * Name:
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4 | * palAirmas
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5 |
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6 | * Purpose:
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7 | * Air mass at given zenith distance
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8 |
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9 | * Language:
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10 | * Starlink ANSI C
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11 |
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12 | * Type of Module:
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13 | * Library routine
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14 |
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15 | * Invocation:
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16 | * double palAirmas( double zd );
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17 |
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18 | * Arguments:
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19 | * zd = double (Given)
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20 | * Observed zenith distance (radians)
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21 |
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22 | * Description:
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23 | * Calculates the airmass at the observed zenith distance.
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24 |
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25 | * Authors:
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26 | * PTW: Patrick Wallace (STFC)
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27 | * TIMJ: Tim Jenness (JAC, Hawaii)
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28 | * {enter_new_authors_here}
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29 |
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30 | * Notes:
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31 | * - The "observed" zenith distance referred to above means "as
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32 | * affected by refraction".
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33 | * - Uses Hardie's (1962) polynomial fit to Bemporad's data for
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34 | * the relative air mass, X, in units of thickness at the zenith
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35 | * as tabulated by Schoenberg (1929). This is adequate for all
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36 | * normal needs as it is accurate to better than 0.1% up to X =
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37 | * 6.8 and better than 1% up to X = 10. Bemporad's tabulated
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38 | * values are unlikely to be trustworthy to such accuracy
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39 | * because of variations in density, pressure and other
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40 | * conditions in the atmosphere from those assumed in his work.
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41 | * - The sign of the ZD is ignored.
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42 | * - At zenith distances greater than about ZD = 87 degrees the
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43 | * air mass is held constant to avoid arithmetic overflows.
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44 |
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45 | * See Also:
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46 | * - Hardie, R.H., 1962, in "Astronomical Techniques"
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47 | * ed. W.A. Hiltner, University of Chicago Press, p180.
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48 | * - Schoenberg, E., 1929, Hdb. d. Ap.,
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49 | * Berlin, Julius Springer, 2, 268.
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50 |
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51 | * History:
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52 | * 2012-03-02 (TIMJ):
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53 | * Initial version from the SLA/F version including documentation.
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54 | * Adapted with permission from the Fortran SLALIB library.
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55 | * {enter_further_changes_here}
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56 |
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57 | * Copyright:
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58 | * Copyright (C) 1999 Rutherford Appleton Laboratory.
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59 | * Copyright (C) 2012 Science and Technology Facilities Council.
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60 | * All Rights Reserved.
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61 |
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62 | * Licence:
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63 | * This program is free software; you can redistribute it and/or
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64 | * modify it under the terms of the GNU General Public License as
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65 | * published by the Free Software Foundation; either version 3 of
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66 | * the License, or (at your option) any later version.
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67 | *
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68 | * This program is distributed in the hope that it will be
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69 | * useful, but WITHOUT ANY WARRANTY; without even the implied
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70 | * warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
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71 | * PURPOSE. See the GNU General Public License for more details.
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72 | *
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73 | * You should have received a copy of the GNU General Public License
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74 | * along with this program; if not, write to the Free Software
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75 | * Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston,
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76 | * MA 02110-1301, USA.
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77 |
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78 | * Bugs:
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79 | * {note_any_bugs_here}
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80 | *-
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81 | */
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82 |
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83 | #include "pal.h"
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84 | #include "palmac.h"
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85 |
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86 | double palAirmas ( double zd ) {
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87 | double seczm1;
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88 | double airmass;
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89 |
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90 | /* Have maximum zenith distance of 87 deg */
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91 | const double MAXZD = 87.0 * PAL__DD2R;
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92 |
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93 | zd = fabs(zd);
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94 | zd = ( zd > MAXZD ? MAXZD : zd );
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95 |
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96 | seczm1 = (1.0 / cos(zd)) - 1.0;
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97 | airmass = 1.0 + seczm1*(0.9981833 - seczm1*(0.002875 + 0.0008083*seczm1));
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98 | return airmass;
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99 | }
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