1 | subroutine calc_rayleigh |
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2 | |
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3 | !================================================================== |
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4 | ! |
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5 | ! Purpose |
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6 | ! ------- |
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7 | ! Average the Rayleigh scattering in each band, weighting the |
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8 | ! average by the blackbody function at temperature tstellar. |
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9 | ! Works for an arbitrary mix of gases (currently CO2, N2 and |
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10 | ! H2 are possible). |
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11 | ! |
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12 | ! Authors |
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13 | ! ------- |
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14 | ! Robin Wordsworth (2010) |
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15 | ! |
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16 | ! Called by |
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17 | ! --------- |
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18 | ! setspv.F |
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19 | ! |
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20 | ! Calls |
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21 | ! ----- |
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22 | ! none |
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23 | ! |
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24 | !================================================================== |
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25 | |
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26 | use radinc_h, only: L_NSPECTV |
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27 | use radcommon_h, only: WAVEV, BWNV, DWNV, tstellar, tauray, scalep |
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28 | use gases_h |
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29 | |
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30 | implicit none |
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31 | |
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32 | #include "comcstfi.h" |
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33 | #include "callkeys.h" |
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34 | |
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35 | real*8 wl |
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36 | integer N,Nfine,ifine,igas |
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37 | parameter(Nfine=500.0) |
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38 | real*8 :: P0 = 9.423D+6 ! Rayleigh scattering reference pressure in pascals. |
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39 | |
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40 | logical typeknown |
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41 | real*8 tauvar,tausum,tauwei,bwidth,bstart |
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42 | double precision df |
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43 | |
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44 | real*8 tauconsti(ngasmx) |
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45 | real*8 tauvari(ngasmx) |
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46 | |
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47 | ! tau0/p0=tau/p (Hansen 1974) |
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48 | ! Then calculate tau0 = (8*pi^3*p_1atm)/(3*N0^2) * 4*delta^2/(g*mugaz*lambda^4) |
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49 | ! where delta=n-1 and N0 is an amagat |
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50 | |
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51 | typeknown=.false. |
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52 | do igas=1,ngasmx |
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53 | if(igas.eq.vgas)then |
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54 | print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// & |
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55 | 'as it is variable.' |
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56 | elseif(gfrac(igas).lt.5.e-2)then |
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57 | print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// & |
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58 | 'as its mixing ratio is less than 0.05.' |
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59 | ! ignore variable gas in Rayleigh calculation |
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60 | ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation |
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61 | tauconsti(igas) = 0.0 |
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62 | else |
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63 | if(gnom(igas).eq.'CO2')then |
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64 | tauconsti(igas) = (8.7/g)*1.527*scalep/P0 |
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65 | elseif(gnom(igas).eq.'N2_')then |
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66 | tauconsti(igas) = (9.81/g)*8.569E-3*scalep/(P0/93.0) |
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67 | elseif(gnom(igas).eq.'H2O')then |
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68 | tauconsti(igas) = (10.0/g)*9.22E-3*scalep/101325.0 |
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69 | elseif(gnom(igas).eq.'H2_')then |
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70 | tauconsti(igas) = (10.0/g)*0.0241*scalep/101325.0 |
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71 | !tauconsti(igas) = (10.0/g)*0.0487*scalep/(101325.0) |
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72 | ! uses n=1.000132 from Optics, Fourth Edition. |
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73 | ! was out by a factor 2! |
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74 | elseif(gnom(igas).eq.'He_')then |
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75 | print*,'Helium not ready yet!' |
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76 | else |
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77 | print*,'Error in calc_rayleigh: Gas species not recognised!' |
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78 | call abort |
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79 | endif |
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80 | |
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81 | if(gfrac(igas).eq.1.0)then |
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82 | print*,'Rayleigh scattering is for a pure ',gnom(igas),' atmosphere.' |
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83 | typeknown=.true. |
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84 | endif |
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85 | |
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86 | endif |
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87 | enddo |
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88 | |
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89 | if(.not.typeknown)then |
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90 | print*,'Rayleigh scattering is for a mixed gas atmosphere.' |
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91 | typeknown=.true. |
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92 | endif |
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93 | |
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94 | |
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95 | do N=1,L_NSPECTV |
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96 | |
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97 | tausum = 0.0 |
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98 | tauwei = 0.0 |
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99 | bstart = 10000.0/BWNV(N+1) |
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100 | bwidth = (10000.0/BWNV(N)) - (10000.0/BWNV(N+1)) |
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101 | do ifine=1,Nfine |
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102 | wl=bstart+dble(ifine)*bwidth/Nfine |
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103 | |
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104 | tauvar=0.0 |
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105 | do igas=1,ngasmx |
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106 | if((igas.eq.vgas).or.(gfrac(igas).lt.5.e-2))then |
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107 | ! ignore variable gas in Rayleigh calculation |
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108 | ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation |
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109 | tauvari(igas) = 0.0 |
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110 | else |
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111 | if(gnom(igas).eq.'CO2')then |
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112 | tauvari(igas) = (1.0+0.013/wl**2)/wl**4 |
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113 | elseif(gnom(igas).eq.'N2_')then |
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114 | tauvari(igas) = (1.0+0.0113/wl**2+0.00013/wl**4)/wl**4 |
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115 | elseif(gnom(igas).eq.'H2O')then |
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116 | tauvari(igas) = 1.0/wl**4 ! to be improved... |
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117 | elseif(gnom(igas).eq.'H2_')then |
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118 | tauvari(igas) = 1.0/wl**4 |
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119 | else |
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120 | print*,'Error in calc_rayleigh: Gas species not recognised!' |
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121 | call abort |
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122 | endif |
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123 | endif |
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124 | |
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125 | tauvar=tauvar+tauconsti(igas)*tauvari(igas)*gfrac(igas) |
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126 | |
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127 | enddo |
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128 | |
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129 | call blackl(dble(wl*1e-6),dble(tstellar),df) |
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130 | df=df*bwidth/Nfine |
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131 | tauwei=tauwei+df |
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132 | tausum=tausum+tauvar*df |
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133 | |
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134 | enddo |
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135 | TAURAY(N)=tausum/tauwei |
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136 | ! we multiply by scalep here (100) because plev, which is used in optcv, |
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137 | ! is in units of mBar, so we need to convert. |
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138 | |
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139 | end do |
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140 | |
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141 | print*,'At 1 atm and lambda = ',WAVEV(L_NSPECTV-6),' um' |
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142 | print*,'tau_R = ',TAURAY(L_NSPECTV-6)*1013.25 |
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143 | print*,'sig_R = ',TAURAY(L_NSPECTV-6)*g*mugaz*1.67e-27*100, & |
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144 | 'cm^2 molecule^-1' |
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145 | |
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146 | end subroutine calc_rayleigh |
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