1 | module radinc_h |
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2 | |
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3 | implicit none |
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4 | |
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5 | #include "dimensions.h" |
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6 | #include "bands.h" |
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7 | |
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8 | !======================================================================C |
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9 | ! |
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10 | ! RADINC.H RADiation INCludes |
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11 | ! |
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12 | ! Includes for the radiation code; RADIATION LAYERS, LEVELS, |
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13 | ! number of spectral intervals. . . |
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14 | ! |
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15 | !======================================================================C |
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16 | |
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17 | ! RADIATION parameters |
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18 | |
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19 | ! In radiation code, layer 1 corresponds to the stratosphere. Level |
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20 | ! 1 is the top of the stratosphere. The dummy layer is at the same |
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21 | ! temperature as the (vertically isothermal) stratosphere, and |
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22 | ! any time it is explicitly needed, the appropriate quantities will |
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23 | ! be dealt with (aka "top". . .) |
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24 | |
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25 | ! L_NLEVRAD corresponds to the surface - i.e., the GCM Level that |
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26 | ! is at the surface. PLEV(L_NLEVRAD) = P(J,I)+PTROP, |
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27 | ! PLEV(2) = PTROP, PLEV(1) = ptop |
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28 | |
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29 | ! L_NLAYRAD is the number of radiation code layers |
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30 | ! L_NLEVRAD is the number of radiation code levels. Level N is the |
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31 | ! top of layer N. |
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32 | ! |
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33 | ! L_NSPECTI is the number of IR spectral intervals |
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34 | ! L_NSPECTV is the number of Visual(or Solar) spectral intervals |
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35 | ! L_NGAUSS is the number of Gauss points for K-coefficients |
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36 | ! GAUSS POINT 17 (aka the last one) is the special case |
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37 | ! |
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38 | ! L_NPREF is the number of reference pressures that the |
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39 | ! k-coefficients are calculated on |
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40 | ! L_PINT is the number of Lagrange interpolated reference |
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41 | ! pressures for the gas k-coefficients - now for a |
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42 | ! smaller p-grid than before |
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43 | ! L_NTREF is the number of reference temperatures for the |
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44 | ! k-coefficients |
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45 | ! L_TAUMAX is the largest optical depth - larger ones are set |
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46 | ! to this value |
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47 | ! |
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48 | ! L_REFVAR The number of different mixing ratio values for |
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49 | ! the k-coefficients. Variable component of the mixture |
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50 | ! can in princple be anything: currently it's H2O. |
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51 | ! |
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52 | ! NAERKIND The number of radiatively active aerosol types |
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53 | ! |
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54 | ! NSIZEMAX The maximum number of aerosol particle sizes |
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55 | ! |
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56 | !----------------------------------------------------------------------C |
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57 | |
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58 | integer, parameter :: L_NLAYRAD = llm |
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59 | integer, parameter :: L_LEVELS = 2*(llm-1)+3 |
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60 | integer, parameter :: L_NLEVRAD = llm+1 |
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61 | |
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62 | ! Below are various parameter combinations that will work for the |
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63 | ! radiative datasets indicated. For the moment, you must change these |
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64 | ! values manually before compiling, each time you want to change the |
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65 | ! dataset. |
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66 | |
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67 | integer, parameter :: L_NGAUSS = 17 |
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68 | |
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69 | integer, parameter :: L_NPREF = 9 |
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70 | integer, parameter :: L_NTREF = 7 |
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71 | integer, parameter :: L_REFVAR = 7 ! earth / earlymars |
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72 | ! ! CO2_H2Ovar / N2OCO2rich_H2Ovar / N2OCO2poor_H2Ovar |
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73 | ! integer, parameter :: L_REFVAR = 4 ! N2_CH4 |
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74 | |
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75 | ! integer, parameter :: L_NPREF = 8 |
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76 | ! integer, parameter :: L_NTREF = 11 |
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77 | ! integer, parameter :: L_REFVAR = 8 ! N2_H2Ovar |
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78 | |
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79 | ! integer, parameter :: L_NPREF = 8 |
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80 | ! integer, parameter :: L_NTREF = 5 |
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81 | ! integer, parameter :: L_REFVAR = 1 ! therm_test2 |
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82 | |
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83 | ! integer, parameter :: L_NPREF = 12 |
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84 | ! integer, parameter :: L_NTREF = 20 |
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85 | ! integer, parameter :: L_REFVAR = 1 ! null (for H2 etc.) |
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86 | |
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87 | ! integer, parameter :: L_NPREF = 10 |
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88 | ! integer, parameter :: L_NTREF = 5 |
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89 | ! integer, parameter :: L_REFVAR = 7 ! N2_CO2var |
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90 | |
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91 | ! integer, parameter :: L_NPREF = 8 |
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92 | ! integer, parameter :: L_NTREF = 6 |
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93 | ! integer, parameter :: L_REFVAR = 1 ! pureCO2 |
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94 | |
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95 | ! integer, parameter :: L_NPREF = 7 |
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96 | ! integer, parameter :: L_NTREF = 5 |
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97 | ! integer, parameter :: L_REFVAR = 1 ! degraded_pure |
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98 | |
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99 | ! integer, parameter :: L_NPREF = 9 |
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100 | ! integer, parameter :: L_NTREF = 14 |
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101 | ! integer, parameter :: L_REFVAR = 1 ! megaCO2 |
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102 | |
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103 | integer, parameter :: L_NSPECTI = NBinfrared |
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104 | integer, parameter :: L_NSPECTV = NBvisible |
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105 | |
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106 | integer, parameter :: L_PINT = (L_NPREF-1)*5+1 |
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107 | integer, parameter :: NAERKIND = 2 |
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108 | real, parameter :: L_TAUMAX = 35 |
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109 | !integer, parameter :: L_TAUMAX = 35 |
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110 | !integer, parameter :: L_TAUMAX = 40 |
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111 | |
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112 | ! For Planck function integration: |
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113 | ! equivalent temperatures are 1/10 of these values |
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114 | integer, parameter :: NTstar = 500 |
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115 | integer, parameter :: NTstop = 9000 ! new default for all non hot Jupiter runs |
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116 | !integer, parameter :: NTstop = 6000 ! for GJ581d / earlymars runs |
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117 | |
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118 | ! Maximum number of grain size classes |
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119 | ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
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120 | ! This parameter has to be set to the maximum number of particle |
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121 | ! sizes contained in the optical parameter database; For example, |
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122 | ! if only one grain size is used to describe dust, and 30 are used |
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123 | ! to describe water-ice crystals in the visible and 15 in the IR, |
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124 | ! nsizemax has to be set to 30. |
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125 | ! If only one grain size is considered for all the aerosols, set |
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126 | ! this parameter to 1 and convolution will be turned off during |
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127 | ! the radiative calculations. |
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128 | |
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129 | integer, parameter :: nsizemax = 60 |
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130 | ! integer, parameter :: nsizemax = 1 |
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131 | |
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132 | character (len=20) :: corrkdir |
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133 | save corrkdir |
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134 | |
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135 | character (len=30) :: banddir |
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136 | save banddir |
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137 | |
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138 | end module radinc_h |
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