1 | MODULE trcdms_medusa |
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2 | !!====================================================================== |
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3 | !! *** MODULE trcdms_medusa *** |
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4 | !! TOP : MEDUSA |
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5 | !!====================================================================== |
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6 | !! History : |
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7 | !! - ! 2014-08 (J. Palmieri - A. Yool) added for UKESM1 project |
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8 | !! - ! 2017-05 (A. Yool) add extra Anderson scheme |
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9 | !! - ! 2018-10 (A. Yool) Add air-sea DMS flux |
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10 | !!---------------------------------------------------------------------- |
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11 | #if defined key_medusa && defined key_roam |
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12 | !!---------------------------------------------------------------------- |
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13 | !! MEDUSA DMS surface concentration |
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14 | !!---------------------------------------------------------------------- |
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15 | !! trc_dms_medusa : |
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16 | !!---------------------------------------------------------------------- |
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17 | USE oce_trc |
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18 | USE trc |
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19 | USE sms_medusa |
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20 | USE lbclnk |
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21 | USE prtctl_trc ! Print control for debugging |
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22 | USE in_out_manager ! I/O manager |
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23 | |
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24 | IMPLICIT NONE |
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25 | PRIVATE |
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26 | |
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27 | PUBLIC trc_dms_medusa ! called in trc_bio_medusa |
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28 | PUBLIC dms_flux_ocn ! called in air_sea |
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29 | |
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30 | !!* Substitution |
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31 | # include "domzgr_substitute.h90" |
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32 | !!---------------------------------------------------------------------- |
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33 | !! NEMO/TOP 2.0 , LOCEAN-IPSL (2007) |
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34 | !! $Id$ |
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35 | !! Software governed by the CeCILL licence (modipsl/doc/NEMO_CeCILL.txt) |
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36 | !!---------------------------------------------------------------------- |
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37 | |
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38 | |
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39 | CONTAINS |
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40 | |
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41 | !======================================================================= |
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42 | ! |
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43 | SUBROUTINE trc_dms_medusa( chn, chd, mld, xqsr, xdin, xlim, & !! inputs |
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44 | & dms_andr, dms_simo, dms_aran, dms_hall, dms_andm) !! outputs |
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45 | ! |
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46 | !======================================================================= |
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47 | !! |
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48 | !! Title : Calculates DMS ocean surface concentration |
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49 | !! Author : Julien Palmieri and Andrew Yool |
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50 | !! Date : 08/08/14 |
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51 | !! |
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52 | !! DMS module is called in trc_bio's huge jk,jj,ji loop |
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53 | !! --> DMS concentration is calculated in a specific cell |
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54 | !! (no need of ji,jj,jk) |
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55 | !! |
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56 | !! AXY (13/03/15): amend to include all four schemes tested |
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57 | !! during winter/spring 2015; these are: |
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58 | !! |
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59 | !! 1. Anderson et al. (2001); this uses fields |
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60 | !! of surface chl, irradiance and nutrients |
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61 | !! to empirically estimate DMS via a broken |
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62 | !! stick approach |
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63 | !! |
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64 | !! 2. Simo & Dachs (2002); this uses fields of |
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65 | !! surface chl and mixed layer depth |
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66 | !! |
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67 | !! 3. Aranami & Tsunogai (2004); this is an |
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68 | !! embellishment of Simo & Dachs |
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69 | !! |
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70 | !! 4. Halloran et al. (2010); this is an |
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71 | !! alternative embellishment of Sim & Dachs |
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72 | !! and is included because it is formally |
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73 | !! published (and different from the above) |
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74 | !! |
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75 | !! AXY (25/05/17): add extra "corrected" Anderson scheme |
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76 | !! |
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77 | !! 5. As Anderson et al. (2001) but modified to |
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78 | !! more accurately reflect nutrient limitation |
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79 | !! status of phytoplankton community |
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80 | !! |
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81 | !! AXY (08/07/15): amend to remove Julien's original calculation |
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82 | !! as this is now superfluous; the four schemes |
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83 | !! are calculated and one is chosen to be passed |
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84 | !! to the atmosphere in trc_bio_medusa |
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85 | !! |
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86 | !======================================================================= |
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87 | |
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88 | IMPLICIT NONE |
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89 | ! |
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90 | REAL(wp), INTENT( in ) :: chn !! non-diatom chlorophyll (mg/m3) |
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91 | REAL(wp), INTENT( in ) :: chd !! diatom chlorophyll (mg/m3) |
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92 | REAL(wp), INTENT( in ) :: mld !! mix layer depth (m) |
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93 | REAL(wp), INTENT( in ) :: xqsr !! surface irradiance (W/m2) |
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94 | REAL(wp), INTENT( in ) :: xdin !! surface DIN (mmol N/m3) |
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95 | REAL(wp), INTENT( in ) :: xlim !! surface DIN limitation (mmol N/m3) |
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96 | REAL(wp), INTENT( inout ) :: dms_andr !! DMS surface concentration (nmol/L) |
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97 | REAL(wp), INTENT( inout ) :: dms_simo !! DMS surface concentration (nmol/L) |
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98 | REAL(wp), INTENT( inout ) :: dms_aran !! DMS surface concentration (nmol/L) |
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99 | REAL(wp), INTENT( inout ) :: dms_hall !! DMS surface concentration (nmol/L) |
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100 | REAL(wp), INTENT( inout ) :: dms_andm !! DMS surface concentration (nmol/L) |
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101 | ! |
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102 | REAL(wp) :: CHL, cmr, sw_dms |
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103 | REAL(wp) :: Jterm, Qterm |
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104 | !! temporary variables |
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105 | REAL(wp) :: fq1,fq2,fq3 |
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106 | ! |
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107 | !======================================================================= |
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108 | ! |
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109 | ! AXY (13/03/15): per remarks above, the following calculations estimate |
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110 | ! DMS using all of the schemes examined for UKESM1 |
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111 | ! |
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112 | CHL = 0.0 |
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113 | CHL = chn+chd !! mg/m3 |
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114 | cmr = CHL / mld |
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115 | ! |
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116 | ! AXY (13/03/15): Anderson et al. (2001) |
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117 | !! JPALM --19-12-2017-- Tunable through the namelist |
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118 | !! within dmsmin - dmscut - dmsslp |
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119 | Jterm = xqsr + 1.0e-6 |
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120 | !! this next line makes a hard-coded assumption about the |
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121 | !! half-saturation constant of MEDUSA (which should be |
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122 | !! done properly; perhaps even scaled with the proportion |
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123 | !! of diatoms and non-diatoms) |
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124 | Qterm = xdin / (xdin + 0.5) |
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125 | fq1 = log10(CHL * Jterm * Qterm) |
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126 | if (fq1 > dmscut) then |
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127 | dms_andr = (dmsslp * (fq1 - dmscut)) + dmsmin |
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128 | else |
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129 | dms_andr = dmsmin |
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130 | endif |
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131 | ! |
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132 | ! AXY (13/03/15): Simo & Dachs (2002) |
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133 | fq1 = (-1.0 * log(mld)) + 5.7 |
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134 | fq2 = (55.8 * cmr) + 0.6 |
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135 | if (cmr < 0.02) then |
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136 | dms_simo = fq1 |
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137 | else |
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138 | dms_simo = fq2 |
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139 | endif |
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140 | ! |
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141 | ! AXY (13/03/15): Aranami & Tsunogai (2004) |
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142 | fq1 = 60.0 / mld |
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143 | fq2 = (55.8 * cmr) + 0.6 |
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144 | if (cmr < 0.02) then |
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145 | dms_aran = fq1 |
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146 | else |
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147 | dms_aran = fq2 |
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148 | endif |
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149 | ! |
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150 | ! AXY (13/03/15): Halloran et al. (2010) |
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151 | fq1 = (-1.0 * log(mld)) + 5.7 |
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152 | fq2 = (55.8 * cmr) + 0.6 |
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153 | fq3 = (90.0 / mld) |
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154 | if (cmr < 0.02) then |
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155 | dms_hall = fq1 |
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156 | else |
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157 | dms_hall = fq2 |
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158 | endif |
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159 | if (mld > 182.5) then |
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160 | dms_hall = fq3 |
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161 | endif |
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162 | ! |
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163 | ! AXY (25/05/17): modified Anderson et al. (2001) |
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164 | Jterm = xqsr + 1.0e-6 |
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165 | !! this version fixes the hard-coded assumption above |
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166 | Qterm = xlim |
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167 | fq1 = log10(CHL * Jterm * Qterm) |
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168 | if (fq1 > 1.72) then |
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169 | dms_andm = (8.24 * (fq1 - 1.72)) + 2.29 |
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170 | else |
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171 | dms_andm = 2.29 |
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172 | endif |
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173 | |
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174 | END SUBROUTINE trc_dms_medusa |
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175 | |
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176 | |
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177 | !======================================================================= |
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178 | !======================================================================= |
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179 | !======================================================================= |
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180 | |
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181 | |
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182 | !======================================================================= |
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183 | ! |
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184 | SUBROUTINE dms_flux_ocn( wind_10m, tstar, dms_conc, i_dms_flux, & !! inputs |
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185 | & f_dms ) !! outputs |
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186 | ! |
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187 | !======================================================================= |
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188 | !! |
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189 | !! Title : Calculates DMS air-sea exchange |
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190 | !! Author : Andrew Yool, based on UKMO original code |
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191 | !! Date : 11/10/18 |
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192 | !! |
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193 | !! Air-sea DMS flux is normally calculated by the UM atmosphere, |
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194 | !! as part of its aerosols; however, the OMIP simulation for CMIP6 |
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195 | !! is ocean-only and does not include the UM; consequently, this |
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196 | !! code has been added to permit ocean-only UKESM1 to produce an |
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197 | !! air-sea DMS flux in addition to surface DMS which, hitherto, |
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198 | !! was all it would produce; code is largely copy-pasted from the |
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199 | !! UKMO original (UM code block is dms_flux_4A.F90); the code |
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200 | !! here is hard-wired to use single input values (i.e. not a 2D |
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201 | !! area) and make use of the Liss & Merlivat (1986) function |
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202 | !! |
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203 | !! This DMS function is called from air_sea.F90 |
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204 | |
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205 | !--------------------------------------------------------------------- |
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206 | ! Purpose: To calculate the flux of DMS (as kg m-2 s-1 of sulphur) |
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207 | ! from the ocean surface as a function of its concentration |
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208 | ! in seawater and of windspeed. The sea-air exchange can |
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209 | ! be determined according to one of three commonly-used |
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210 | ! parametrization schemes, those of Liss & Merlivat (1986), |
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211 | ! Wanninkhof (1992) or Nightingale et al. (2000). The routine |
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212 | ! is called by Aero_Ctl. |
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213 | ! |
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214 | ! Method: The Schmidt number |
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215 | ! for DMS is calculated as in Saltzman et al. (1993), and |
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216 | ! used with the windspeed to determine the mass transfer (or |
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217 | ! "piston") velocity according to the desired parametrization. |
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218 | ! This is then used to determine the sea-air mass flux of DMS |
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219 | ! as a function of sea-water DMS concentration. High surface |
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220 | ! temperatures (caused by the land portion of a gridbox when |
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221 | ! coastal tiling is not active) cause negative Sc values which |
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222 | ! would give a floating-point error in the k_DMS calculation, |
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223 | ! so the Tstar values are capped. This shouldn't be a problem |
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224 | ! when coastal tiling is on as then the Tstar values passed in |
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225 | ! are those for sea only. |
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226 | ! |
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227 | ! Code Owner: Please refer to the UM file CodeOwners.txt |
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228 | ! This file belongs in section: Aerosols |
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229 | ! |
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230 | ! Code Description: |
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231 | ! Language: Fortran 90 |
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232 | ! This code is written to UMDP3 v8 programming standards |
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233 | ! |
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234 | !--------------------------------------------------------------------- |
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235 | |
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236 | IMPLICIT NONE |
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237 | ! |
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238 | REAL(wp), INTENT( in ) :: wind_10m !! 10m wind (m/s) |
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239 | REAL(wp), INTENT( in ) :: tstar !! SST (degrees C) |
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240 | REAL(wp), INTENT( in ) :: dms_conc !! surface DMS (nmol / l) |
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241 | INTEGER, INTENT(in) :: i_dms_flux !! gas transfer choice |
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242 | ! |
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243 | REAL(wp), INTENT( inout ) :: f_dms !! DMS flux (kg S m-2 s-1) |
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244 | |
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245 | ! Local variables: |
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246 | REAL :: sc ! Schmidt number |
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247 | REAL :: k_dms ! Piston velocity of DMS (cm h-1) |
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248 | REAL :: t_c ! Surface temperature in degrees Celsius |
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249 | ! Piston velocities for gases with Schmidt numbers of 600 & 660 resp. (cm h-1) |
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250 | REAL :: k_600 |
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251 | REAL :: k_660 |
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252 | REAL :: n ! Schmidt number exponent |
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253 | REAL, PARAMETER :: t_max = 47.0 !! Max T to avoid breaking the Sc fit (C) |
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254 | |
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255 | ! Calculate the Schmidt number (Sc): |
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256 | t_c = MIN(tstar, t_max) |
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257 | sc = 2674.0 - (147.12*t_c) + (3.726*t_c**2) & |
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258 | - (0.038*t_c**3) |
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259 | |
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260 | ! Determine the mass transfer (or "piston") velocity (k_DMS) over sea |
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261 | ! according to the specified parametrization scheme: |
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262 | |
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263 | if (i_dms_flux .eq. 1) then |
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264 | ! ---------------------------------------------------------------------- |
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265 | ! Liss & Merlivat (1986) |
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266 | IF (wind_10m .le. 3.6) THEN |
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267 | k_600 = 0.17 * wind_10m |
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268 | n = -2.0/3.0 |
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269 | ELSEIF ( wind_10m .gt. 3.6 .AND. wind_10m .le. 13.0 ) THEN |
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270 | k_600 = (2.85 * wind_10m) - 9.65 |
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271 | n = -0.5 |
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272 | ELSE |
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273 | k_600 = (5.90 * wind_10m) - 49.3 |
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274 | n = -0.5 |
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275 | END IF |
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276 | k_dms = k_600 * (sc / 600.0)**n |
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277 | elseif (i_dms_flux .eq. 2) then |
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278 | ! ---------------------------------------------------------------------- |
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279 | ! Wanninkhof (1992) |
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280 | k_660 = 0.31 * wind_10m**2 |
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281 | n = -0.5 |
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282 | k_dms = k_660 * (sc / 660.0)**n |
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283 | elseif (i_dms_flux .eq. 3) then |
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284 | ! ---------------------------------------------------------------------- |
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285 | ! Nightingale et al. (2000) |
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286 | k_600 = (0.222 * wind_10m**2) + (0.333 * wind_10m) |
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287 | n = -0.5 |
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288 | k_dms = k_600 * (sc / 600.0)**n |
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289 | else |
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290 | ! ---------------------------------------------------------------------- |
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291 | ! You shouldn't be here |
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292 | k_dms = 0.0 |
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293 | endif |
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294 | |
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295 | ! Finally, calculate the sea-air flux of DMS as a function of k_DMS |
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296 | ! and dissolved DMS concentration. The former requires a conversion |
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297 | ! from cm hour-1 to ms-1, and the latter from nanomoles per litre to |
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298 | ! kg[S] m-3, to return the flux in kg[S] m-2 sec-1. |
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299 | |
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300 | f_dms = (k_dms / 3.6e5) * (dms_conc * 32.0e-9) |
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301 | |
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302 | END SUBROUTINE dms_flux_ocn |
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303 | |
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304 | |
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305 | !======================================================================= |
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306 | !======================================================================= |
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307 | !======================================================================= |
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308 | |
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309 | #else |
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310 | !!====================================================================== |
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311 | !! Dummy module : No MEDUSA bio-model |
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312 | !!====================================================================== |
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313 | |
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314 | CONTAINS |
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315 | |
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316 | !======================================================================= |
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317 | ! |
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318 | SUBROUTINE trc_dms_medusa( kt ) !! EMPTY Routine |
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319 | ! |
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320 | ! |
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321 | INTEGER, INTENT( in ) :: kt |
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322 | ! |
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323 | |
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324 | WRITE(*,*) 'trc_dms_medusa: You should not have seen this print! error?' |
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325 | |
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326 | END SUBROUTINE trc_dms_medusa |
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327 | #endif |
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328 | |
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329 | !!====================================================================== |
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330 | END MODULE trcdms_medusa |
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331 | |
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332 | |
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333 | |
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