1 | SUBROUTINE swrayleigh(kdlon,knu,ppsol,prmu,prayl) |
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2 | USE comcstfi_h |
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3 | IMPLICIT NONE |
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4 | c======================================================================= |
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5 | c subject: |
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6 | c -------- |
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7 | c Computing total rayleigh scat atmospheric optical depth |
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8 | c |
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9 | c author: F.Forget |
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10 | c ------ |
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11 | c |
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12 | c input: |
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13 | c ----- |
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14 | c kdlon Number of gridpoint of horizontal grid |
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15 | c knu : Solar band # (1 or 2) |
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16 | c ppsol surface pressure (Pa) |
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17 | c prmu cos of solar zenith angle (=1 when sun at zenith) |
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18 | c (CORRECTED for high zenith angle (atmosphere), unlike mu0) |
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19 | c |
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20 | c output: |
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21 | c ------- |
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22 | c prayl column optical depth in each model column |
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23 | c |
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24 | c======================================================================= |
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25 | |
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26 | c----------------------------------------------------------------------- |
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27 | c |
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28 | c Declarations : |
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29 | c -------------- |
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30 | c |
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31 | c Input/Output |
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32 | c ------------ |
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33 | INTEGER kdlon, knu |
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34 | |
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35 | real ppsol(kdlon),prmu(kdlon),prayl(kdlon) |
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36 | c |
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37 | c Local variables : |
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38 | c ----------------- |
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39 | integer JL, K |
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40 | c |
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41 | c local saved variables |
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42 | c --------------------- |
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43 | c rayleigh scattering coefficients (from Morcrete et al.EARTH model !) |
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44 | real cray(2,6) |
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45 | |
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46 | DATA (CRAY(1,K),K=1,6) / |
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47 | S .428937E-01, .890743E+00,-.288555E+01, |
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48 | S .522744E+01,-.469173E+01, .161645E+01/ |
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49 | |
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50 | DATA (CRAY(2,K),K=1,6) / |
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51 | S .697200E-02, .173297E-01,-.850903E-01, |
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52 | S .248261E+00,-.302031E+00, .129662E+00/ |
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53 | save cray |
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54 | |
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55 | !$OMP THREADPRIVATE(cray) |
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56 | |
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57 | c---------------------------------------------------------------------- |
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58 | |
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59 | DO JL = 1 , KDLON |
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60 | |
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61 | c Total Rayleigh Optical thickness on Earth at 101325 Pa level |
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62 | c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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63 | c WARNING : the CRAY coefficients are only valid for |
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64 | c Spectral interval used in Earth model !!! |
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65 | c (i.e. 0.25-0.68 micron and 0.68-4.00 micron |
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66 | c ---> should be modified for Mars model !!! |
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67 | |
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68 | PRAYL(JL) = CRAY(KNU,1) + PRMU(JL) * (CRAY(KNU,2) + PRMU(JL) |
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69 | S * (CRAY(KNU,3) + PRMU(JL) * (CRAY(KNU,4) + PRMU(JL) |
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70 | S * (CRAY(KNU,5) + PRMU(JL) * CRAY(KNU,6) )))) |
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71 | |
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72 | c Total local Rayleigh Optical thickness on Mars |
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73 | c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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74 | c - PRAYL above is the total Rayleigh Optical thickness |
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75 | c at 101325Pa for Earth atmosphere |
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76 | c -> Total Rayleigh Optical thickness on Mars |
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77 | c = PRAYL*(Psurf/101325)*9.81/g *2.5 |
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78 | c (Extinction coeff of CO2 = 2.5 * N2) |
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79 | |
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80 | c (Comment the following line to get back bugged version before 01/2000) |
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81 | c PRAYL(JL) = PRAYL(JL) * PPSOL(JL) * 2.42e-4/g |
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82 | |
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83 | END DO |
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84 | |
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85 | |
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86 | return |
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87 | end |
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88 | |
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