| 1 | SUBROUTINE callradite(icount,ngrid,nlayer,nq,zday,ls,pq,albedo, |
|---|
| 2 | $ emis,mu0,pplev,pplay,pt,tsurf,fract,dist_sol,igout, |
|---|
| 3 | $ dtlw,dtsw,fluxsurf_lw,fluxsurf_sw,fluxtop_lw,fluxtop_sw, |
|---|
| 4 | & tauref,tau,aerosol,ccn,rdust,rice,nuice) |
|---|
| 5 | |
|---|
| 6 | IMPLICIT NONE |
|---|
| 7 | c======================================================================= |
|---|
| 8 | c subject: |
|---|
| 9 | c -------- |
|---|
| 10 | c Subroutine designed to call the main canonic |
|---|
| 11 | c radiative transfer subroutine "lwmain" et "swmain" |
|---|
| 12 | c to compute radiative heating and cooling rate and |
|---|
| 13 | c radiative fluxes to the surface. |
|---|
| 14 | c |
|---|
| 15 | c These calculations are only valid on the part of the atmosphere |
|---|
| 16 | c where Local Thermal Equilibrium (NLTE) is verified. In practice |
|---|
| 17 | c The calculations are only performed for the first "nlaylte" |
|---|
| 18 | c parameters (nlaylte is calculated by subroutine "nlthermeq" |
|---|
| 19 | c and stored in common "yomlw.h"). |
|---|
| 20 | c |
|---|
| 21 | c The purpose of this subroutine is to: |
|---|
| 22 | c 1) Make some initial calculation at first call |
|---|
| 23 | c 2) Split the calculation in several sub-grid |
|---|
| 24 | c ("sub-domain") to save memory and |
|---|
| 25 | c be able run on a workstation at high resolution |
|---|
| 26 | c The sub-grid size is defined in dimradmars.h |
|---|
| 27 | c 3) Compute the 3D scattering parameters depending on the |
|---|
| 28 | c size distribution of the different tracers (added by JBM) |
|---|
| 29 | c 4) call "lwmain" and "swmain" |
|---|
| 30 | c |
|---|
| 31 | c |
|---|
| 32 | c authors: |
|---|
| 33 | c ------ |
|---|
| 34 | c Francois Forget / Christophe Hourdin / J.-B. Madeleine (2009) |
|---|
| 35 | c |
|---|
| 36 | c |
|---|
| 37 | c 3D scattering scheme user's guide (J.-B. Madeleine) |
|---|
| 38 | c --------------------------------- |
|---|
| 39 | c |
|---|
| 40 | c This routine has been modified to take into account 3D, time |
|---|
| 41 | c dependent scattering properties of the aerosols. |
|---|
| 42 | c---- The look-up tables that contain the scattering parameters |
|---|
| 43 | c of a given tracer, for different sizes, are read by SUAER.F90. |
|---|
| 44 | c The names of the corresponding ASCII files have to be set in |
|---|
| 45 | c this subroutine (file_id variable), and files must be in the |
|---|
| 46 | c directory specified in datafile.h. Please make sure that the |
|---|
| 47 | c ASCII files are correctly written, and that the range |
|---|
| 48 | c of particle sizes is consistent with what you would expect. |
|---|
| 49 | c---- SUAER.F90 is in charge of reading the ASCII files and averaging |
|---|
| 50 | c the scattering parameters in each GCM channel, using the three last |
|---|
| 51 | c equations of Forget et al. 1998 (GRL 25, No.7, p.1105-1108). |
|---|
| 52 | c---- These look-up tables, loaded during the firstcall, are then |
|---|
| 53 | c constantly used by the subroutine "aeroptproperties.F" to compute, |
|---|
| 54 | c online, the 3D scattering parameters, based on the size distribution |
|---|
| 55 | c (reffrad and nueffrad) of the different tracers, in each grid box. |
|---|
| 56 | c These 3D size distributions are loaded by the "updatereffrad.F" |
|---|
| 57 | c subroutine. A log-normal distribution is then assumed in |
|---|
| 58 | c "aeroptproperties.F", along with a Gauss-Legendre integration. |
|---|
| 59 | c---- The optical depth at the visible reference wavelength (set in |
|---|
| 60 | c SUAER.F90, after the file_id variable) is then computed by |
|---|
| 61 | c the subroutine "aeropacity.F", by using the size and spatial |
|---|
| 62 | c distribution of the corresponding tracer. This connection has to |
|---|
| 63 | c be implemented in "aeropacity.F" when adding a new tracer. To do so, |
|---|
| 64 | c one can use equation 2 of Forget et al. 1998 (Icarus 131, p.302-316). |
|---|
| 65 | c---- The resulting variables "aerosol", "QVISsQREF3d", "omegaVIS3d" and |
|---|
| 66 | c "gVIS3d" (same in the infrared) are finally used by lwmain.F and |
|---|
| 67 | c swmain.F to solve the radiative transfer equation. |
|---|
| 68 | c |
|---|
| 69 | c changes: |
|---|
| 70 | c ------- |
|---|
| 71 | c |
|---|
| 72 | c > SRL 7/2000 |
|---|
| 73 | c |
|---|
| 74 | c This version has been modified to only calculate radiative tendencies |
|---|
| 75 | c over layers 1..NFLEV (set in dimradmars.h). Returns zero for higher |
|---|
| 76 | c layers, if any. |
|---|
| 77 | c In other routines, nlayermx -> nflev. |
|---|
| 78 | c Routines affected: lwflux, lwi, lwmain, lwxb, lwxd, lwxn. |
|---|
| 79 | c |
|---|
| 80 | c > J.-B. Madeleine 10W12 |
|---|
| 81 | c This version uses the variable's splitting, which can be usefull |
|---|
| 82 | c when performing very high resolution simulation like LES. |
|---|
| 83 | c |
|---|
| 84 | c ---------- |
|---|
| 85 | c Here, solar band#1 is spectral interval between "long1vis" and "long2vis" |
|---|
| 86 | c set in dimradmars.h |
|---|
| 87 | c Here, solar band#2 is spectral interval between "long2vis" and "long3vis" |
|---|
| 88 | c set in dimradmars.h |
|---|
| 89 | c |
|---|
| 90 | c input: |
|---|
| 91 | c ----- |
|---|
| 92 | c icount counter of call to subroutine physic by gcm |
|---|
| 93 | c ngrid number of gridpoint of horizontal grid |
|---|
| 94 | c nlayer Number of layer |
|---|
| 95 | c nq Number of tracer |
|---|
| 96 | c ls Solar longitude (Ls) , radian |
|---|
| 97 | c zday Date (time since Ls=0, in martian days) |
|---|
| 98 | c pq(ngrid,nlayer,nq) Advected fields |
|---|
| 99 | c |
|---|
| 100 | c albedo (ngrid,2) hemispheric surface albedo |
|---|
| 101 | c albedo (i,1) : mean albedo for solar band#1 |
|---|
| 102 | c (see below) |
|---|
| 103 | c albedo (i,2) : mean albedo for solar band#2 |
|---|
| 104 | c (see below) |
|---|
| 105 | c emis Thermal IR surface emissivity (no unit) |
|---|
| 106 | c mu0(ngridmx) cos of solar zenith angle |
|---|
| 107 | c (=1 when sun at zenith) |
|---|
| 108 | c pplay(ngrid,nlayer) pressure (Pa) in the middle of each layer |
|---|
| 109 | c pplev(ngrid,nlayer+1) pressure (Pa) at boundaries of each layer |
|---|
| 110 | c pt(ngrid,nlayer) atmospheric temperature in each layer (K) |
|---|
| 111 | c tsurf(ngrid) surface temperature (K) |
|---|
| 112 | c fract(ngridmx) day fraction of the time interval |
|---|
| 113 | c =1 during the full day ; =0 during the night |
|---|
| 114 | c declin latitude of subsolar point |
|---|
| 115 | c dist_sol sun-Mars distance (AU) |
|---|
| 116 | c igout coordinate of analysed point for debugging |
|---|
| 117 | c reffrad(ngrid,nlayer,naerkind) Aerosol effective radius |
|---|
| 118 | c nueffrad(ngrid,nlayer,naerkind) Aerosol effective variance |
|---|
| 119 | |
|---|
| 120 | c |
|---|
| 121 | c output: |
|---|
| 122 | c ------- |
|---|
| 123 | c dtlw (ngrid,nlayer) longwave (IR) heating rate (K/s) |
|---|
| 124 | c dtsw(ngrid,nlayer) shortwave (Solar) heating rate (K/s) |
|---|
| 125 | c fluxsurf_lw(ngrid) surface downward flux tota LW (thermal IR) (W.m-2) |
|---|
| 126 | c fluxsurf_sw(ngrid,1) surface downward flux SW for solar band#1 (W.m-2) |
|---|
| 127 | c fluxsurf_sw(ngrid,2) surface downward flux SW for solar band#2 (W.m-2) |
|---|
| 128 | c |
|---|
| 129 | c fluxtop_lw(ngrid) outgoing upward flux tota LW (thermal IR) (W.m-2) |
|---|
| 130 | c fluxtop_sw(ngrid,1) outgoing upward flux SW for solar band#1 (W.m-2) |
|---|
| 131 | c fluxtop_sw(ngrid,2) outgoing upward flux SW for solar band#2 (W.m-2) |
|---|
| 132 | |
|---|
| 133 | c tauref Prescribed mean column optical depth at 700 Pa |
|---|
| 134 | c tau Column total visible dust optical depth at each point |
|---|
| 135 | c aerosol(ngrid,nlayer,naerkind) aerosol extinction optical depth |
|---|
| 136 | c at reference wavelength "longrefvis" set |
|---|
| 137 | c in dimradmars.h , in each layer, for one of |
|---|
| 138 | c the "naerkind" kind of aerosol optical |
|---|
| 139 | c properties. |
|---|
| 140 | |
|---|
| 141 | c======================================================================= |
|---|
| 142 | c |
|---|
| 143 | c Declarations : |
|---|
| 144 | c ------------- |
|---|
| 145 | c |
|---|
| 146 | #include "dimensions.h" |
|---|
| 147 | #include "dimphys.h" |
|---|
| 148 | #include "dimradmars.h" |
|---|
| 149 | #include "comcstfi.h" |
|---|
| 150 | #include "callkeys.h" |
|---|
| 151 | #include "yomlw.h" |
|---|
| 152 | #include "aerkind.h" |
|---|
| 153 | |
|---|
| 154 | c----------------------------------------------------------------------- |
|---|
| 155 | c Input/Output |
|---|
| 156 | c ------------ |
|---|
| 157 | INTEGER icount |
|---|
| 158 | INTEGER ngrid,nlayer,nq |
|---|
| 159 | INTEGER igout |
|---|
| 160 | |
|---|
| 161 | REAL pq(ngrid,nlayer,nq) |
|---|
| 162 | REAL ccn(ngridmx,nlayermx) ! Cloud condensation nuclei |
|---|
| 163 | ! (particules kg-1) |
|---|
| 164 | REAL albedo(ngrid,2),emis(ngrid) |
|---|
| 165 | REAL ls,zday |
|---|
| 166 | |
|---|
| 167 | REAL pplev(ngrid,nlayer+1),pplay(ngrid,nlayer) |
|---|
| 168 | REAL pt(ngrid,nlayer) |
|---|
| 169 | REAL tsurf(ngrid) |
|---|
| 170 | REAL dist_sol,mu0(ngrid),fract(ngrid) |
|---|
| 171 | REAL dtlw(ngridmx,nlayermx),dtsw(ngridmx,nlayermx) |
|---|
| 172 | REAL fluxsurf_lw(ngridmx), fluxtop_lw(ngridmx) |
|---|
| 173 | REAL fluxsurf_sw(ngridmx,2), fluxtop_sw(ngridmx,2) |
|---|
| 174 | |
|---|
| 175 | REAL tauref(ngrid), tau(ngrid,naerkind) |
|---|
| 176 | REAL aerosol(ngrid,nlayer,naerkind) |
|---|
| 177 | REAL rdust(ngridmx,nlayermx) ! Dust geometric mean radius (m) |
|---|
| 178 | REAL rice(ngridmx,nlayermx) ! Ice geometric mean radius (m) |
|---|
| 179 | REAL nuice(ngridmx,nlayermx) ! Estimated effective variance |
|---|
| 180 | c |
|---|
| 181 | c Local variables : |
|---|
| 182 | c ----------------- |
|---|
| 183 | |
|---|
| 184 | INTEGER j,l,ig,n,ich |
|---|
| 185 | INTEGER aer_count,iaer |
|---|
| 186 | INTEGER jd,ig0,nd |
|---|
| 187 | |
|---|
| 188 | real cste_mars ! solar constant on Mars (Wm-2) |
|---|
| 189 | REAL ptlev(ngridmx,nlayermx+1) |
|---|
| 190 | |
|---|
| 191 | INTEGER ndomain |
|---|
| 192 | parameter (ndomain = (ngridmx-1) / ndomainsz + 1) |
|---|
| 193 | |
|---|
| 194 | c Thermal IR net radiative budget (W m-2) |
|---|
| 195 | |
|---|
| 196 | real znetrad(ndomainsz,nflev) |
|---|
| 197 | |
|---|
| 198 | real zfluxd_sw(ndomainsz,nflev+1,2) |
|---|
| 199 | real zfluxu_sw(ndomainsz,nflev+1,2) |
|---|
| 200 | |
|---|
| 201 | REAL zplev(ndomainsz,nflev+1) |
|---|
| 202 | REAL zztlev(ndomainsz,nflev+1) |
|---|
| 203 | REAL zplay(ndomainsz,nflev) |
|---|
| 204 | REAL zt(ndomainsz,nflev) |
|---|
| 205 | REAL zaerosol(ndomainsz,nflev,naerkind) |
|---|
| 206 | REAL zalbedo(ndomainsz,2) |
|---|
| 207 | REAL zdp(ndomainsz,nflev) |
|---|
| 208 | REAL zdt0(ndomainsz) |
|---|
| 209 | |
|---|
| 210 | REAL zzdtlw(ndomainsz,nflev) |
|---|
| 211 | REAL zzdtsw(ndomainsz,nflev) |
|---|
| 212 | REAL zzflux(ndomainsz,6) |
|---|
| 213 | real zrmuz |
|---|
| 214 | |
|---|
| 215 | REAL :: zQVISsQREF3d(ndomainsz,nflev,nsun,naerkind) |
|---|
| 216 | REAL :: zomegaVIS3d(ndomainsz,nflev,nsun,naerkind) |
|---|
| 217 | REAL :: zgVIS3d(ndomainsz,nflev,nsun,naerkind) |
|---|
| 218 | |
|---|
| 219 | REAL :: zQIRsQREF3d(ndomainsz,nflev,nir,naerkind) |
|---|
| 220 | REAL :: zomegaIR3d(ndomainsz,nflev,nir,naerkind) |
|---|
| 221 | REAL :: zgIR3d(ndomainsz,nflev,nir,naerkind) |
|---|
| 222 | |
|---|
| 223 | c Aerosol size distribution |
|---|
| 224 | REAL :: reffrad(ngrid,nlayer,naerkind) |
|---|
| 225 | REAL :: nueffrad(ngrid,nlayer,naerkind) |
|---|
| 226 | c Aerosol optical properties |
|---|
| 227 | REAL :: QVISsQREF3d(ngridmx,nlayermx,nsun,naerkind) |
|---|
| 228 | REAL :: omegaVIS3d(ngridmx,nlayermx,nsun,naerkind) |
|---|
| 229 | REAL :: gVIS3d(ngridmx,nlayermx,nsun,naerkind) |
|---|
| 230 | |
|---|
| 231 | REAL :: QIRsQREF3d(ngridmx,nlayermx,nir,naerkind) |
|---|
| 232 | REAL :: omegaIR3d(ngridmx,nlayermx,nir,naerkind) |
|---|
| 233 | REAL :: gIR3d(ngridmx,nlayermx,nir,naerkind) |
|---|
| 234 | |
|---|
| 235 | REAL :: QREFvis3d(ngridmx,nlayermx,naerkind) |
|---|
| 236 | REAL :: QREFir3d(ngridmx,nlayermx,naerkind) |
|---|
| 237 | |
|---|
| 238 | REAL :: omegaREFvis3d(ngridmx,nlayermx,naerkind) |
|---|
| 239 | REAL :: omegaREFir3d(ngridmx,nlayermx,naerkind) |
|---|
| 240 | |
|---|
| 241 | c local saved variables |
|---|
| 242 | c --------------------- |
|---|
| 243 | |
|---|
| 244 | real pview(ngridmx) |
|---|
| 245 | save pview |
|---|
| 246 | |
|---|
| 247 | real zco2 ! volume fraction of CO2 in Mars atmosphere |
|---|
| 248 | DATA zco2/0.95/ |
|---|
| 249 | SAVE zco2 |
|---|
| 250 | |
|---|
| 251 | LOGICAL firstcall |
|---|
| 252 | DATA firstcall/.true./ |
|---|
| 253 | SAVE firstcall |
|---|
| 254 | |
|---|
| 255 | c---------------------------------------------------------------------- |
|---|
| 256 | |
|---|
| 257 | c Initialisation |
|---|
| 258 | c -------------- |
|---|
| 259 | |
|---|
| 260 | IF (firstcall) THEN |
|---|
| 261 | |
|---|
| 262 | c Please name the different scatterers here ---------------- |
|---|
| 263 | c PLEASE MAKE SURE that you set up the right number of |
|---|
| 264 | c scatterers in dimradmars.h (naerkind); |
|---|
| 265 | name_iaer(1) = "dust_conrath" !! default choice is good old Conrath profile |
|---|
| 266 | name_iaer(2) = "dummy" !! default choice is no radiatively-active clouds |
|---|
| 267 | IF (doubleq.AND.active) name_iaer(1) = "dust_doubleq" !! two-moment scheme |
|---|
| 268 | IF (water.AND.activice) name_iaer(2) = "h2o_ice" !! radiatively-active clouds |
|---|
| 269 | IF (submicron.AND.active) name_iaer(2) = "dust_submicron" !! JBM experimental stuff |
|---|
| 270 | c ---------------------------------------------------------- |
|---|
| 271 | |
|---|
| 272 | c Assign a number to the different scatterers |
|---|
| 273 | c ------------------------------------------- |
|---|
| 274 | |
|---|
| 275 | iaer_dust_conrath=0 |
|---|
| 276 | iaer_dust_doubleq=0 |
|---|
| 277 | iaer_dust_submicron=0 |
|---|
| 278 | iaer_h2o_ice=0 |
|---|
| 279 | |
|---|
| 280 | aer_count=0 |
|---|
| 281 | if (.NOT.active) then |
|---|
| 282 | do iaer=1,naerkind |
|---|
| 283 | if (name_iaer(iaer).eq."dust_conrath") then |
|---|
| 284 | iaer_dust_conrath = iaer |
|---|
| 285 | aer_count = aer_count + 1 |
|---|
| 286 | endif |
|---|
| 287 | enddo |
|---|
| 288 | endif |
|---|
| 289 | if (doubleq.AND.active) then |
|---|
| 290 | do iaer=1,naerkind |
|---|
| 291 | if (name_iaer(iaer).eq."dust_doubleq") then |
|---|
| 292 | iaer_dust_doubleq = iaer |
|---|
| 293 | aer_count = aer_count + 1 |
|---|
| 294 | endif |
|---|
| 295 | enddo |
|---|
| 296 | endif |
|---|
| 297 | if (submicron.AND.active) then |
|---|
| 298 | do iaer=1,naerkind |
|---|
| 299 | if (name_iaer(iaer).eq."dust_submicron") then |
|---|
| 300 | iaer_dust_submicron = iaer |
|---|
| 301 | aer_count = aer_count + 1 |
|---|
| 302 | endif |
|---|
| 303 | enddo |
|---|
| 304 | endif |
|---|
| 305 | if (water.AND.activice) then |
|---|
| 306 | do iaer=1,naerkind |
|---|
| 307 | if (name_iaer(iaer).eq."h2o_ice") then |
|---|
| 308 | iaer_h2o_ice = iaer |
|---|
| 309 | aer_count = aer_count + 1 |
|---|
| 310 | endif |
|---|
| 311 | enddo |
|---|
| 312 | endif |
|---|
| 313 | |
|---|
| 314 | c Check that we identified all tracers: |
|---|
| 315 | if (aer_count.ne.naerkind) then |
|---|
| 316 | write(*,*) "callradite: found only ",aer_count," scatterers" |
|---|
| 317 | write(*,*) " expected ",naerkind |
|---|
| 318 | write(*,*) "please make sure that the number of" |
|---|
| 319 | write(*,*) "scatterers in dimradmars.h, the names" |
|---|
| 320 | write(*,*) "in callradite.F, and the flags in" |
|---|
| 321 | write(*,*) "callphys.def are all consistent!" |
|---|
| 322 | do iaer=1,naerkind |
|---|
| 323 | write(*,*)' ',iaer,' ',trim(name_iaer(iaer)) |
|---|
| 324 | enddo |
|---|
| 325 | stop |
|---|
| 326 | else |
|---|
| 327 | write(*,*) "callradite: found all scatterers, namely:" |
|---|
| 328 | do iaer=1,naerkind |
|---|
| 329 | write(*,*)' ',iaer,' ',trim(name_iaer(iaer)) |
|---|
| 330 | enddo |
|---|
| 331 | endif |
|---|
| 332 | c ------------------------------------------- |
|---|
| 333 | |
|---|
| 334 | DO ig=1,ngrid |
|---|
| 335 | pview(ig)=1.66 ! cosecant of viewing angle |
|---|
| 336 | ENDDO |
|---|
| 337 | gcp = g/cpp |
|---|
| 338 | |
|---|
| 339 | c Logical tests for radiatively active water-ice clouds: |
|---|
| 340 | IF ( (activice.AND.(.NOT.water)).OR. |
|---|
| 341 | & (activice.AND.(naerkind.LT.2)) ) THEN |
|---|
| 342 | WRITE(*,*) 'If activice is TRUE, water has to be set' |
|---|
| 343 | WRITE(*,*) 'to TRUE, and "naerkind" must be at least' |
|---|
| 344 | WRITE(*,*) 'equal to 2 in dimradmars.h.' |
|---|
| 345 | CALL ABORT |
|---|
| 346 | ELSE IF ( (.NOT.activice).AND.(naerkind.GT.1) ) THEN |
|---|
| 347 | WRITE(*,*) 'naerkind is greater than unity, but' |
|---|
| 348 | WRITE(*,*) 'activice has not been set to .true.' |
|---|
| 349 | WRITE(*,*) 'in callphys.def; this is not logical!' |
|---|
| 350 | CALL ABORT |
|---|
| 351 | ENDIF |
|---|
| 352 | |
|---|
| 353 | c Loading the optical properties in external look-up tables: |
|---|
| 354 | CALL SUAER |
|---|
| 355 | CALL SULW |
|---|
| 356 | |
|---|
| 357 | write(*,*) 'Splitting radiative calculations: ', |
|---|
| 358 | $ ' ngridmx,ngrid,ndomainsz,ndomain', |
|---|
| 359 | $ ngridmx,ngrid,ndomainsz,ndomain |
|---|
| 360 | if (ngridmx .EQ. 1) then |
|---|
| 361 | if (ndomainsz .NE. 1) then |
|---|
| 362 | print* |
|---|
| 363 | print*,'ATTENTION !!!' |
|---|
| 364 | print*,'pour tourner en 1D, ' |
|---|
| 365 | print*,'fixer ndomainsz=1 dans phymars/dimradmars.h' |
|---|
| 366 | print* |
|---|
| 367 | call exit(1) |
|---|
| 368 | endif |
|---|
| 369 | endif |
|---|
| 370 | firstcall=.false. |
|---|
| 371 | END IF |
|---|
| 372 | |
|---|
| 373 | c Computing aerosol optical properties and opacity |
|---|
| 374 | c ------------------------------------------------ |
|---|
| 375 | |
|---|
| 376 | c Updating aerosol size distributions: |
|---|
| 377 | CALL updatereffrad(ngrid,nlayer, |
|---|
| 378 | & rdust,rice,nuice, |
|---|
| 379 | & reffrad,nueffrad, |
|---|
| 380 | & pq) |
|---|
| 381 | |
|---|
| 382 | c Computing 3D scattering parameters: |
|---|
| 383 | CALL aeroptproperties(ngrid,nlayer,reffrad,nueffrad, |
|---|
| 384 | & QVISsQREF3d,omegaVIS3d,gVIS3d, |
|---|
| 385 | & QIRsQREF3d,omegaIR3d,gIR3d, |
|---|
| 386 | & QREFvis3d,QREFir3d, |
|---|
| 387 | & omegaREFvis3d,omegaREFir3d) |
|---|
| 388 | |
|---|
| 389 | c Computing aerosol optical depth in each layer: |
|---|
| 390 | CALL aeropacity(ngrid,nlayer,nq,zday,pplay,pplev,ls, |
|---|
| 391 | & pq,ccn,tauref,tau,aerosol,reffrad,nueffrad, |
|---|
| 392 | & QREFvis3d,QREFir3d,omegaREFvis3d,omegaREFir3d) |
|---|
| 393 | |
|---|
| 394 | c Starting loop on sub-domain |
|---|
| 395 | c ---------------------------- |
|---|
| 396 | |
|---|
| 397 | DO jd=1,ndomain |
|---|
| 398 | ig0=(jd-1)*ndomainsz |
|---|
| 399 | if (jd.eq.ndomain) then |
|---|
| 400 | nd=ngridmx-ig0 |
|---|
| 401 | else |
|---|
| 402 | nd=ndomainsz |
|---|
| 403 | endif |
|---|
| 404 | |
|---|
| 405 | c Spliting input variable in sub-domain input variables |
|---|
| 406 | c --------------------------------------------------- |
|---|
| 407 | |
|---|
| 408 | do l=1,nlaylte |
|---|
| 409 | do ig = 1,nd |
|---|
| 410 | do iaer = 1, naerkind |
|---|
| 411 | do ich = 1, nsun |
|---|
| 412 | zQVISsQREF3d(ig,l,ich,iaer) = |
|---|
| 413 | & QVISsQREF3d(ig0+ig,l,ich,iaer) |
|---|
| 414 | zomegaVIS3d(ig,l,ich,iaer) = |
|---|
| 415 | & omegaVIS3d(ig0+ig,l,ich,iaer) |
|---|
| 416 | zgVIS3d(ig,l,ich,iaer) = |
|---|
| 417 | & gVIS3d(ig0+ig,l,ich,iaer) |
|---|
| 418 | enddo |
|---|
| 419 | do ich = 1, nir |
|---|
| 420 | zQIRsQREF3d(ig,l,ich,iaer) = |
|---|
| 421 | & QIRsQREF3d(ig0+ig,l,ich,iaer) |
|---|
| 422 | zomegaIR3d(ig,l,ich,iaer) = |
|---|
| 423 | & omegaIR3d(ig0+ig,l,ich,iaer) |
|---|
| 424 | zgIR3d(ig,l,ich,iaer) = |
|---|
| 425 | & gIR3d(ig0+ig,l,ich,iaer) |
|---|
| 426 | enddo |
|---|
| 427 | enddo |
|---|
| 428 | enddo |
|---|
| 429 | enddo |
|---|
| 430 | |
|---|
| 431 | do l=1,nlaylte+1 |
|---|
| 432 | do ig = 1,nd |
|---|
| 433 | zplev(ig,l) = pplev(ig0+ig,l) |
|---|
| 434 | enddo |
|---|
| 435 | enddo |
|---|
| 436 | |
|---|
| 437 | do l=1,nlaylte |
|---|
| 438 | do ig = 1,nd |
|---|
| 439 | zplay(ig,l) = pplay(ig0+ig,l) |
|---|
| 440 | zt(ig,l) = pt(ig0+ig,l) |
|---|
| 441 | c Thickness of each layer (Pa) : |
|---|
| 442 | zdp(ig,l)= pplev(ig0+ig,l) - pplev(ig0+ig,l+1) |
|---|
| 443 | enddo |
|---|
| 444 | enddo |
|---|
| 445 | |
|---|
| 446 | do n=1,naerkind |
|---|
| 447 | do l=1,nlaylte |
|---|
| 448 | do ig=1,nd |
|---|
| 449 | zaerosol(ig,l,n) = aerosol(ig0+ig,l,n) |
|---|
| 450 | enddo |
|---|
| 451 | enddo |
|---|
| 452 | enddo |
|---|
| 453 | |
|---|
| 454 | do j=1,2 |
|---|
| 455 | do ig = 1,nd |
|---|
| 456 | zalbedo(ig,j) = albedo(ig0+ig,j) |
|---|
| 457 | enddo |
|---|
| 458 | enddo |
|---|
| 459 | |
|---|
| 460 | c Intermediate levels: (computing tlev) |
|---|
| 461 | c --------------------------------------- |
|---|
| 462 | c Extrapolation for the air temperature above the surface |
|---|
| 463 | DO ig=1,nd |
|---|
| 464 | zztlev(ig,1)=zt(ig,1)+ |
|---|
| 465 | s (zplev(ig,1)-zplay(ig,1))* |
|---|
| 466 | s (zt(ig,1)-zt(ig,2))/(zplay(ig,1)-zplay(ig,2)) |
|---|
| 467 | |
|---|
| 468 | zdt0(ig) = tsurf(ig0+ig) - zztlev(ig,1) |
|---|
| 469 | ENDDO |
|---|
| 470 | |
|---|
| 471 | DO l=2,nlaylte |
|---|
| 472 | DO ig=1, nd |
|---|
| 473 | zztlev(ig,l)=0.5*(zt(ig,l-1)+zt(ig,l)) |
|---|
| 474 | ENDDO |
|---|
| 475 | ENDDO |
|---|
| 476 | |
|---|
| 477 | DO ig=1, nd |
|---|
| 478 | zztlev(ig,nlaylte+1)=zt(ig,nlaylte) |
|---|
| 479 | ENDDO |
|---|
| 480 | |
|---|
| 481 | |
|---|
| 482 | c Longwave ("lw") radiative transfer (= thermal infrared) |
|---|
| 483 | c ------------------------------------------------------- |
|---|
| 484 | call lwmain (ig0,icount,nd,nflev |
|---|
| 485 | . ,zdp,zdt0,emis(ig0+1),zplev,zztlev,zt |
|---|
| 486 | . ,zaerosol,zzdtlw |
|---|
| 487 | . ,fluxsurf_lw(ig0+1),fluxtop_lw(ig0+1) |
|---|
| 488 | . ,znetrad |
|---|
| 489 | & ,zQIRsQREF3d,zomegaIR3d,zgIR3d) |
|---|
| 490 | |
|---|
| 491 | c Shortwave ("sw") radiative transfer (= solar radiation) |
|---|
| 492 | c ------------------------------------------------------- |
|---|
| 493 | c Mars solar constant (W m-2) |
|---|
| 494 | c 1370 W.m-2 is the solar constant at 1 AU. |
|---|
| 495 | cste_mars=1370./(dist_sol*dist_sol) |
|---|
| 496 | |
|---|
| 497 | call swmain ( nd, nflev, |
|---|
| 498 | S cste_mars, zalbedo, |
|---|
| 499 | S mu0(ig0+1), zdp, zplev, zaerosol, fract(ig0+1), |
|---|
| 500 | S zzdtsw, zfluxd_sw, zfluxu_sw, |
|---|
| 501 | & zQVISsQREF3d,zomegaVIS3d,zgVIS3d) |
|---|
| 502 | |
|---|
| 503 | c ------------------------------------------------------------ |
|---|
| 504 | c Un-spliting output variable from sub-domain input variables |
|---|
| 505 | c ------------------------------------------------------------ |
|---|
| 506 | |
|---|
| 507 | do l=1,nlaylte |
|---|
| 508 | do ig = 1,nd |
|---|
| 509 | dtlw(ig0+ig,l) = zzdtlw(ig,l) |
|---|
| 510 | dtsw(ig0+ig,l) = zzdtsw(ig,l) |
|---|
| 511 | enddo |
|---|
| 512 | enddo |
|---|
| 513 | |
|---|
| 514 | do l=1,nlaylte+1 |
|---|
| 515 | do ig = 1,nd |
|---|
| 516 | ptlev(ig0+ig,l) = zztlev(ig,l) |
|---|
| 517 | enddo |
|---|
| 518 | enddo |
|---|
| 519 | |
|---|
| 520 | do ig = 1,nd |
|---|
| 521 | fluxsurf_sw(ig0+ig,1) = zfluxd_sw(ig,1,1) |
|---|
| 522 | fluxsurf_sw(ig0+ig,2) = zfluxd_sw(ig,1,2) |
|---|
| 523 | fluxtop_sw(ig0+ig,1) = zfluxu_sw(ig,nlaylte+1,1) |
|---|
| 524 | fluxtop_sw(ig0+ig,2) = zfluxu_sw(ig,nlaylte+1,2) |
|---|
| 525 | enddo |
|---|
| 526 | |
|---|
| 527 | ENDDO ! (boucle jd=1, ndomain) |
|---|
| 528 | |
|---|
| 529 | c Zero tendencies for any remaining layers between nlaylte and nlayer |
|---|
| 530 | if (nlayer.gt.nlaylte) then |
|---|
| 531 | do l = nlaylte+1, nlayer |
|---|
| 532 | do ig = 1, ngrid |
|---|
| 533 | dtlw(ig, l) = 0. |
|---|
| 534 | dtsw(ig, l) = 0. |
|---|
| 535 | enddo |
|---|
| 536 | enddo |
|---|
| 537 | endif |
|---|
| 538 | |
|---|
| 539 | c Output for debugging if lwrite=T |
|---|
| 540 | c -------------------------------- |
|---|
| 541 | c Write all nlayer layers, even though only nlaylte layers may have |
|---|
| 542 | c non-zero tendencies. |
|---|
| 543 | |
|---|
| 544 | IF(lwrite) THEN |
|---|
| 545 | PRINT*,'Diagnotique for the radiation' |
|---|
| 546 | PRINT*,'albedo, emissiv, mu0,fract,fluxsurf_lw,fluxsurf_sw' |
|---|
| 547 | PRINT*,albedo(igout,1),emis(igout),mu0(igout), |
|---|
| 548 | s fract(igout), fluxsurf_lw(igout), |
|---|
| 549 | $ fluxsurf_sw(igout,1)+fluxsurf_sw(igout,2) |
|---|
| 550 | PRINT*,'Tlay Tlev Play Plev dT/dt SW dT/dt LW (K/s)' |
|---|
| 551 | PRINT*,'daysec',daysec |
|---|
| 552 | DO l=1,nlayer |
|---|
| 553 | PRINT*,pt(igout,l),ptlev(igout,l), |
|---|
| 554 | s pplay(igout,l),pplev(igout,l), |
|---|
| 555 | s dtsw(igout,l),dtlw(igout,l) |
|---|
| 556 | ENDDO |
|---|
| 557 | ENDIF |
|---|
| 558 | |
|---|
| 559 | |
|---|
| 560 | return |
|---|
| 561 | end |
|---|
