MODULE aeropacity_mod IMPLICIT NONE INTEGER :: iddist ! flag for vertical dust ditribution type (when imposed) ! 0: Pollack90, 1: top set by "topdustref" ! 2: Viking scenario; =3 MGS scenario REAL :: topdustref ! Dust top altitude (km); only matters only if iddist=1) CONTAINS SUBROUTINE aeropacity(ngrid,nlayer,nq,zday,pplay,pplev,ls, & pq,pt,tauscaling,dust_rad_adjust,IRtoVIScoef,tau_pref_scenario, & tau_pref_gcm,tau,taucloudtes,aerosol,dsodust,reffrad, & QREFvis3d,QREFir3d,omegaREFir3d, & totstormfract,clearatm,dsords,dsotop, & nohmons, & clearsky,totcloudfrac) use ioipsl_getin_p_mod, only: getin_p use tracer_mod, only: noms, igcm_h2o_ice, igcm_dust_mass, & igcm_dust_submicron, rho_dust, rho_ice, & nqdust, igcm_stormdust_mass, & igcm_topdust_mass, igcm_co2_ice use geometry_mod, only: latitude ! grid point latitudes (rad) use comgeomfi_h, only: sinlat ! sines of grid point latitudes #ifdef DUSTSTORM use geometry_mod, only: longitude use tracer_mod, only: r3n_q, ref_r0, igcm_dust_number #endif use comcstfi_h, only: g, pi use dimradmars_mod, only: naerkind, name_iaer, & iaerdust,tauvis, & iaer_dust_conrath,iaer_dust_doubleq, & iaer_dust_submicron,iaer_h2o_ice, & iaer_stormdust_doubleq, & iaer_topdust_doubleq use dust_param_mod, only: odpref, freedust, & reff_driven_IRtoVIS_scenario use dust_scaling_mod, only: compute_dustscaling use density_co2_ice_mod, only: density_co2_ice use surfdat_h,only: alpha_hmons,contains_mons use read_dust_scenario_mod, only: read_dust_scenario IMPLICIT NONE c======================================================================= c subject: c -------- c Computing aerosol optical depth in each gridbox. c c author: F.Forget c ------ c update F. Montmessin (water ice scheme) c and S. Lebonnois (12/06/2003) compatibility dust/ice/chemistry c update J.-B. Madeleine 2008-2009: c - added 3D scattering by aerosols; c - dustopacity transferred from physiq.F to callradite.F, c and renamed into aeropacity.F; c update E. Millour, march 2012: c - reference pressure is now set to 610Pa (not 700Pa) c c======================================================================= include "callkeys.h" c----------------------------------------------------------------------- c c Declarations : c -------------- c c Input/Output c ------------ INTEGER,INTENT(IN) :: ngrid ! number of atmospheric columns INTEGER,INTENT(IN) :: nlayer ! number of atmospheric layers INTEGER,INTENT(IN) :: nq ! number of tracers REAL,INTENT(IN) :: ls ! Solar Longitude (rad) REAL,INTENT(IN) :: zday ! date (in martian sols) since Ls=0 REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! pressure (Pa) in the middle of ! each atmospheric layer REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! pressure (Pa) at the boundaries ! of the atmospheric layers REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! tracers REAL,INTENT(IN) :: pt(ngrid,nlayer) !temperature REAL,INTENT(OUT) :: tau_pref_scenario(ngrid) ! prescribed dust column ! visible opacity at odpref from scenario REAL,INTENT(OUT) :: tau_pref_gcm(ngrid) ! computed dust column ! visible opacity at odpref in the GCM REAL,INTENT(OUT) :: tau(ngrid,naerkind) ! column total visible ! optical depth of each aerosol REAL,INTENT(OUT) :: taucloudtes(ngrid)! Water ice cloud opacity at ! infrared reference wavelength using ! Qabs instead of Qext ! (for direct comparison with TES) REAL, INTENT(OUT) :: aerosol(ngrid,nlayer,naerkind) ! optical ! depth of each aerosol in each layer REAL, INTENT(OUT) :: dsodust(ngrid,nlayer) ! density scaled opacity ! of (background) dust REAL, INTENT(OUT) :: dsords(ngrid,nlayer) !dso of stormdust REAL, INTENT(OUT) :: dsotop(ngrid,nlayer) !dso of topdust REAL, INTENT(INOUT) :: reffrad(ngrid,nlayer,naerkind) ! effective radius ! of the aerosols in the grid boxes REAL, INTENT(IN) :: QREFvis3d(ngrid,nlayer,naerkind) ! 3D extinction ! coefficients (in the visible) of aerosols REAL, INTENT(IN) :: QREFir3d(ngrid,nlayer,naerkind) ! 3D extinction ! coefficients (in the infra-red) of aerosols REAL, INTENT(IN) :: omegaREFir3d(ngrid,nlayer,naerkind) ! at the ! reference wavelengths LOGICAL, INTENT(IN) :: clearatm ! true to compute RT without stormdust ! and false to compute RT in rocket dust storms REAL, INTENT(IN) :: totstormfract(ngrid) ! mesh fraction with a rocket ! dust storm LOGICAL, INTENT(IN) :: nohmons ! true to compute RT without topdust, ! false to compute RT in the topdust REAL,INTENT(OUT) :: tauscaling(ngrid) ! Scaling factor for qdust and Ndust REAL,INTENT(INOUT) :: dust_rad_adjust(ngrid) ! Radiative adjustment ! factor for dust REAL,INTENT(INOUT) :: IRtoVIScoef(ngrid) ! conversion coefficient to apply on ! scenario absorption IR (9.3um) CDOD ! = tau_pref_gcm_VIS / tau_pref_gcm_IR REAL,INTENT(IN) :: totcloudfrac(ngrid) ! total water ice cloud fraction LOGICAL,INTENT(IN) :: clearsky ! true to compute RT without water ice clouds ! false to compute RT with clouds (total or sub-grid clouds) c c Local variables : c ----------------- REAL CLFtot ! total cloud fraction real expfactor INTEGER l,ig,iq,i,j INTEGER iaer ! Aerosol index real topdust(ngrid) real zlsconst, zp real taueq,tauS,tauN c Mean Qext(vis)/Qext(ir) profile real msolsir(nlayer,naerkind) c Mean Qext(ir)/Qabs(ir) profile real mqextsqabs(nlayer,naerkind) c Variables used when multiple particle sizes are used c for dust or water ice particles in the radiative transfer c (see callradite.F for more information). REAL taucloudvis(ngrid)! Cloud opacity at visible ! reference wavelength REAL topdust0(ngrid) REAL aerosol_IRabs(ngrid,nlayer) REAL taudust_IRabs(ngrid) REAL taudust_VISext(ngrid) ! -- CO2 clouds real CLFtotco2 real taucloudco2vis(ngrid) real taucloudco2tes(ngrid) real totcloudco2frac(ngrid) ! a mettre en (in) [CM] double precision :: rho_ice_co2 #ifdef DUSTSTORM !! Local dust storms logical localstorm ! =true to create a local dust storm real taulocref,ztoploc,radloc,lonloc,latloc ! local dust storm parameters real reffstorm, yeah REAL ray(ngrid) ! distance from dust storm center REAL tauuser(ngrid) ! opacity perturbation due to dust storm REAL more_dust(ngrid,nlayer,2) ! Mass mixing ratio perturbation due to the dust storm REAL int_factor(ngrid) ! useful factor to compute mmr perturbation real l_top ! layer of the storm's top REAL zalt(ngrid, nlayer) ! useful factor to compute l_top #endif c local saved variables c --------------------- c Level under which the dust mixing ratio is held constant c when computing the dust opacity in each layer c (this applies when doubleq and active are true) INTEGER, PARAMETER :: cstdustlevel0 = 7 INTEGER, SAVE :: cstdustlevel LOGICAL,SAVE :: firstcall=.true. ! indexes of water ice and dust tracers: INTEGER,SAVE :: i_ice=0 ! water ice CHARACTER(LEN=20) :: txt ! to temporarly store text CHARACTER(LEN=1) :: txt2 ! to temporarly store text ! indexes of co2 ice : INTEGER,SAVE :: i_co2ice=0 ! co2 ice ! indexes of dust scatterers: INTEGER,SAVE :: naerdust ! number of dust scatterers !$OMP THREADPRIVATE(cstdustlevel,firstcall,i_ice, !$OMP& i_co2ice,naerdust) ! initializations tau(1:ngrid,1:naerkind)=0 ! identify tracers !! AS: firstcall OK absolute IF (firstcall) THEN ! identify scatterers that are dust naerdust=0 iaerdust(1:naerkind) = 0 nqdust(1:nq) = 0 DO iaer=1,naerkind txt=name_iaer(iaer) ! CW17: choice tauscaling for stormdust or not IF ((txt(1:4).eq."dust").OR.(txt(1:5).eq."storm") & .OR.(txt(1:3).eq."top")) THEN !MV19: topdust tracer naerdust=naerdust+1 iaerdust(naerdust)=iaer ENDIF ENDDO ! identify tracers which are dust i=0 DO iq=1,nq txt=noms(iq) IF (txt(1:4).eq."dust") THEN i=i+1 nqdust(i)=iq ENDIF ENDDO IF (water.AND.activice) THEN i_ice=igcm_h2o_ice write(*,*) "aeropacity: i_ice=",i_ice ENDIF IF (co2clouds.AND.activeco2ice) THEN i_co2ice=igcm_co2_ice write(*,*) "aeropacity: i_co2ice =",i_co2ice ENDIF c typical profile of solsir and (1-w)^(-1): c --- purely for diagnostics and printing msolsir(1:nlayer,1:naerkind)=0 mqextsqabs(1:nlayer,1:naerkind)=0 WRITE(*,*) "Typical profiles of Qext(vis)/Qext(IR)" WRITE(*,*) " and Qext(IR)/Qabs(IR):" DO iaer = 1, naerkind ! Loop on aerosol kind WRITE(*,*) "Aerosol # ",iaer DO l=1,nlayer DO ig=1,ngrid msolsir(l,iaer)=msolsir(l,iaer)+ & QREFvis3d(ig,l,iaer)/ & QREFir3d(ig,l,iaer) mqextsqabs(l,iaer)=mqextsqabs(l,iaer)+ & (1.E0-omegaREFir3d(ig,l,iaer))**(-1) ENDDO msolsir(l,iaer)=msolsir(l,iaer)/REAL(ngrid) mqextsqabs(l,iaer)=mqextsqabs(l,iaer)/REAL(ngrid) ENDDO WRITE(*,*) "solsir: ",msolsir(:,iaer) WRITE(*,*) "Qext/Qabs(IR): ",mqextsqabs(:,iaer) ENDDO ! load value of tauvis from callphys.def (if given there, ! otherwise default value read from starfi.nc file will be used) call getin_p("tauvis",tauvis) IF (freedust.or.rdstorm) THEN ! if rdstorm no need to held opacity constant at the first levels cstdustlevel = 1 ELSE cstdustlevel = cstdustlevel0 !Opacity in the first levels is held constant to !avoid unrealistic values due to constant lifting ENDIF #ifndef DUSTSTORM firstcall=.false. #endif END IF ! end of if firstcall ! 1. Get prescribed tau_pref_scenario, Dust column optical depth at "odpref" Pa !~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ IF(iaervar.eq.1) THEN do ig=1, ngrid tau_pref_scenario(ig)=max(tauvis,1.e-9) ! tauvis=cste (set in callphys.def ! or read in starfi end do ELSE IF (iaervar.eq.2) THEN ! << "Viking" Scenario>> tau_pref_scenario(1) = 0.7+.3*cos(ls+80.*pi/180.) ! like seen by VL1 do ig=2,ngrid tau_pref_scenario(ig) = tau_pref_scenario(1) end do ELSE IF (iaervar.eq.3) THEN ! << "MGS" scenario >> taueq= 0.2 +(0.5-0.2) *(cos(0.5*(ls-4.363)))**14 tauS= 0.1 +(0.5-0.1) *(cos(0.5*(ls-4.363)))**14 tauN = 0.1 do ig=1,ngrid if (latitude(ig).ge.0) then ! Northern hemisphere tau_pref_scenario(ig)= tauN + & (taueq-tauN)*0.5*(1+tanh((45-latitude(ig)*180./pi)*6/60)) else ! Southern hemisphere tau_pref_scenario(ig)= tauS + & (taueq-tauS)*0.5*(1+tanh((45+latitude(ig)*180./pi)*6/60)) endif enddo ! of do ig=1,ngrid ELSE IF (iaervar.eq.5) THEN ! << Escalier Scenario>> tau_pref_scenario(1) = 2.5 if ((ls.ge.30.*pi/180.).and.(ls.le.150.*pi/180.)) & tau_pref_scenario(1) = .2 do ig=2,ngrid tau_pref_scenario(ig) = tau_pref_scenario(1) end do !!!!!!!!!!!!!!!!!!!!!!!!!!! ! NB: here, IRtoVIScoef=2.6 ! ( useful to be here only if iddist=0 (Pollack90 vertical distribution) ) ELSE IF ((iaervar.ge.6).and.(iaervar.le.8)) THEN ! clim, cold or warm synthetic scenarios call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) ELSE IF ((iaervar.ge.24).and.(iaervar.le.35)) & THEN ! << MY... dust scenarios >> call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) ELSE IF ((iaervar.eq.4).or. & ((iaervar.ge.124).and.(iaervar.le.126))) THEN ! "old" TES assimation dust scenario (values at 700Pa in files!) call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) !!!!!!!!!!!!!!!!!!!!!!!!!!! ELSE call abort_physic("aeropacity","wrong value for iaervar",1) ENDIF ! ----------------------------------------------------------------- ! 2. Compute/set the opacity of each aerosol in each layer ! ----------------------------------------------------------------- DO iaer = 1, naerkind ! Loop on all aerosols c -------------------------------------------- aerkind: SELECT CASE (name_iaer(iaer)) c================================================================== CASE("dust_conrath") aerkind ! Typical dust profile c================================================================== c Altitude of the top of the dust layer c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ zlsconst=SIN(ls-2.76) if (iddist.eq.1) then do ig=1,ngrid topdust(ig)=topdustref ! constant dust layer top end do else if (iddist.eq.2) then ! "Viking" scenario do ig=1,ngrid ! altitude of the top of the aerosol layer (km) at Ls=2.76rad: ! in the Viking year scenario topdust0(ig)=60. -22.*sinlat(ig)**2 topdust(ig)=topdust0(ig)+18.*zlsconst end do else if(iddist.eq.3) then !"MGS" scenario do ig=1,ngrid topdust(ig)=60.+18.*zlsconst & -(32+18*zlsconst)*sin(latitude(ig))**4 & - 8*zlsconst*(sin(latitude(ig)))**5 end do endif c Optical depth in each layer : c ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if(iddist.ge.1) then expfactor=0. DO l=1,nlayer DO ig=1,ngrid c Typical mixing ratio profile if(pplay(ig,l).gt.odpref $ /(988.**(topdust(ig)/70.))) then zp=(odpref/pplay(ig,l))**(70./topdust(ig)) expfactor=max(exp(0.007*(1.-max(zp,1.))),1.e-3) else expfactor=1.e-3 endif c Vertical scaling function aerosol(ig,l,iaer)= (pplev(ig,l)-pplev(ig,l+1)) * & expfactor * & QREFvis3d(ig,l,iaer) / QREFvis3d(ig,1,iaer) ENDDO ENDDO else if(iddist.eq.0) then c old dust vertical distribution function (pollack90) DO l=1,nlayer DO ig=1,ngrid zp=odpref/pplay(ig,l) aerosol(ig,l,1)= tau_pref_scenario(ig)/odpref * s (pplev(ig,l)-pplev(ig,l+1)) s *max( exp(.03*(1.-max(zp,1.))) , 1.E-3 ) ENDDO ENDDO end if c================================================================== CASE("dust_doubleq") aerkind! Two-moment scheme for background dust c (transport of mass and number mixing ratio) c================================================================== ! Some initialisations for the IRtoVIScoef aerosol_IRabs(:,:)=0. taudust_IRabs(:)=0. taudust_VISext(:)=0. DO l=1,nlayer IF (l.LE.cstdustlevel) THEN c Opacity in the first levels is held constant to c avoid unrealistic values due to constant lifting: DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsodust(ig,l) = & ( 0.75 * QREFir3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_dust_mass) if (reff_driven_IRtoVIS_scenario) then if ((clearatm).and.(nohmons)) then ! the IRtoVIScoef is computed only during the first call to the RT ! OPTICAL DEPTH in IR absorption to compute the IRtoVIScoef aerosol_IRabs(ig,l) = & ( 0.75 * QREFir3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & ( 1. - omegaREFir3d(ig,cstdustlevel,iaer) ) * & pq(ig,cstdustlevel,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g endif endif ENDDO ELSE DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsodust(ig,l) = & ( 0.75 * QREFir3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_dust_mass) if (reff_driven_IRtoVIS_scenario) then if ((clearatm).and.(nohmons)) then ! the IRtoVIScoef is computed only during the first call to the RT ! OPTICAL DEPTH in IR absorption to compute the IRtoVIScoef aerosol_IRabs(ig,l) = & ( 0.75 * QREFir3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & ( 1. - omegaREFir3d(ig,l,iaer) ) * & pq(ig,l,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g endif endif ENDDO ENDIF if (reff_driven_IRtoVIS_scenario) then if ((clearatm).and.(nohmons)) then ! the IRtoVIScoef is computed only during the first call to the RT taudust_VISext(:) = taudust_VISext(:) + aerosol(:,l,iaer) taudust_IRabs(:) = taudust_IRabs(:) + aerosol_IRabs(:,l) endif endif ENDDO if (reff_driven_IRtoVIS_scenario) then if ((clearatm).and.(nohmons)) then ! the IRtoVIScoef is computed only during the first call to the RT IRtoVIScoef(:) = taudust_VISext(:) / taudust_IRabs(:) endif endif c================================================================== CASE("dust_submicron") aerkind ! Small dust population c================================================================== DO l=1,nlayer IF (l.LE.cstdustlevel) THEN c Opacity in the first levels is held constant to c avoid unrealistic values due to constant lifting: DO ig=1,ngrid aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_dust_submicron) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ENDDO ELSE DO ig=1,ngrid aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_dust_submicron) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ENDDO ENDIF ENDDO c================================================================== CASE("h2o_ice") aerkind ! Water ice crystals c================================================================== c 1. Initialization aerosol(1:ngrid,1:nlayer,iaer) = 0. taucloudvis(1:ngrid) = 0. taucloudtes(1:ngrid) = 0. c 2. Opacity calculation ! NO CLOUDS IF (clearsky) THEN aerosol(1:ngrid,1:nlayer,iaer) =1.e-9 ! CLOUDSs ELSE ! else (clearsky) DO ig=1, ngrid DO l=1,nlayer aerosol(ig,l,iaer) = max(1E-20, & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_ice * reffrad(ig,l,iaer) ) ) * & pq(ig,l,i_ice) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g & ) taucloudvis(ig) = taucloudvis(ig) + aerosol(ig,l,iaer) taucloudtes(ig) = taucloudtes(ig) + aerosol(ig,l,iaer)* & QREFir3d(ig,l,iaer) / QREFvis3d(ig,l,iaer) * & ( 1.E0 - omegaREFir3d(ig,l,iaer) ) ENDDO ENDDO ! SUB-GRID SCALE CLOUDS IF (CLFvarying) THEN DO ig=1, ngrid DO l=1,nlayer-1 CLFtot = max(totcloudfrac(ig),0.01) aerosol(ig,l,iaer)= & aerosol(ig,l,iaer)/CLFtot aerosol(ig,l,iaer) = & max(aerosol(ig,l,iaer),1.e-9) ENDDO ENDDO ENDIF ! end (CLFvarying) ENDIF ! end (clearsky) c================================================================== CASE("co2_ice") aerkind ! CO2 ice crystals c================================================================== c 1. Initialization aerosol(1:ngrid,1:nlayer,iaer) = 0. taucloudco2vis(1:ngrid) = 0. taucloudco2tes(1:ngrid) = 0. c 2. Opacity calculation ! NO CLOUDS IF (clearsky) THEN aerosol(1:ngrid,1:nlayer,iaer) = 1.e-9 ! CLOUDSs ELSE ! else (clearsky) DO ig = 1, ngrid DO l = 1, nlayer call density_co2_ice(dble(pt(ig,l)), rho_ice_co2) aerosol(ig,l,iaer) = max(1E-20, & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_ice_co2 * reffrad(ig,l,iaer) ) ) * & pq(ig,l,i_co2ice) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g & ) taucloudco2vis(ig) = taucloudco2vis(ig) & + aerosol(ig,l,iaer) taucloudco2tes(ig) = taucloudco2tes(ig) & + aerosol(ig,l,iaer) * & QREFir3d(ig,l,iaer) / QREFvis3d(ig,l,iaer) * & ( 1.E0 - omegaREFir3d(ig,l,iaer) ) ENDDO ENDDO ! SUB-GRID SCALE CLOUDS IF (CLFvaryingCO2) THEN DO ig=1, ngrid DO l= 1, nlayer-1 CLFtotco2 = max(totcloudco2frac(ig),0.01) aerosol(ig,l,iaer)= & aerosol(ig,l,iaer)/CLFtotco2 aerosol(ig,l,iaer) = & max(aerosol(ig,l,iaer),1.e-9) ENDDO ENDDO ENDIF ! end (CLFvaryingCO2) ENDIF ! end (clearsky) c================================================================== CASE("stormdust_doubleq") aerkind ! CW17 : Two-moment scheme for c stormdust (transport of mass and number mixing ratio) c================================================================== c aerosol is calculated twice : once within the dust storm (clearatm=false) c and once in the part of the mesh without dust storm (clearatm=true) aerosol(1:ngrid,1:nlayer,iaer) = 0. IF (clearatm) THEN ! considering part of the mesh without storm aerosol(1:ngrid,1:nlayer,iaer)=1.e-25 ELSE ! part of the mesh with concentred dust storm DO l=1,nlayer IF (l.LE.cstdustlevel) THEN c Opacity in the first levels is held constant to c avoid unrealistic values due to constant lifting: DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_stormdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsords(ig,l) = & ( 0.75 * QREFir3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_stormdust_mass) ENDDO ELSE DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_stormdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsords(ig,l) = & ( 0.75 * QREFir3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_stormdust_mass) ENDDO ENDIF ENDDO ENDIF c================================================================== CASE("topdust_doubleq") aerkind ! MV18 : Two-moment scheme for c topdust (transport of mass and number mixing ratio) c================================================================== c aerosol is calculated twice : once "above" the sub-grid mountain (nohmons=false) c and once in the part of the mesh without the sub-grid mountain (nohmons=true) aerosol(1:ngrid,1:nlayer,iaer) = 0. IF (nohmons) THEN ! considering part of the mesh without top dust flows aerosol(1:ngrid,1:nlayer,iaer)=1.e-25 ELSE ! part of the mesh with concentrated dust flows DO l=1,nlayer IF (l.LE.cstdustlevel) THEN c Opacity in the first levels is held constant to c avoid unrealistic values due to constant lifting: DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_topdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsotop(ig,l) = & ( 0.75 * QREFir3d(ig,cstdustlevel,iaer) / & ( rho_dust * reffrad(ig,cstdustlevel,iaer) ) ) * & pq(ig,cstdustlevel,igcm_topdust_mass) ENDDO ELSE DO ig=1,ngrid ! OPTICAL DEPTH used in the radiative transfer ! => visible wavelength aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_topdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ! DENSITY SCALED OPACITY : ! Diagnostic output to be compared with observations ! => infrared wavelength dsotop(ig,l) = & ( 0.75 * QREFir3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_topdust_mass) ENDDO ENDIF ENDDO ENDIF c================================================================== END SELECT aerkind c ----------------------------------- ENDDO ! iaer (loop on aerosol kind) ! 3. Specific treatments for the dust aerosols ! here IRtoVIScoef has been updated, we can call again read_dust_scenario if (reff_driven_IRtoVIS_scenario) then IF ((iaervar.ge.6).and.(iaervar.le.8)) THEN ! clim, cold or warm synthetic scenarios call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) ELSE IF ((iaervar.ge.24).and.(iaervar.le.35)) & THEN ! << MY... dust scenarios >> call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) ELSE IF ((iaervar.eq.4).or. & ((iaervar.ge.124).and.(iaervar.le.126))) THEN ! "old" TES assimation dust scenario (values at 700Pa in files!) call read_dust_scenario(ngrid,nlayer,zday,pplev, & IRtoVIScoef,tau_pref_scenario) ENDIF endif #ifdef DUSTSTORM c ----------------------------------------------------------------- ! Calculate reference opacity without perturbation c ----------------------------------------------------------------- IF (firstcall) THEN DO iaer=1,naerdust DO l=1,nlayer DO ig=1,ngrid tau_pref_gcm(ig) = tau_pref_gcm(ig) + & aerosol(ig,l,iaerdust(iaer)) ENDDO ENDDO ENDDO tau_pref_gcm(:) = tau_pref_gcm(:) * odpref / pplev(:,1) c-------------------------------------------------- c Get parameters of the opacity perturbation c-------------------------------------------------- iaer=1 ! just change dust write(*,*) "Add a local storm ?" localstorm=.true. ! default value call getin_p("localstorm",localstorm) write(*,*) " localstorm = ",localstorm IF (localstorm) THEN WRITE(*,*) "********************" WRITE(*,*) "ADDING A LOCAL STORM" WRITE(*,*) "********************" write(*,*) "ref opacity of local dust storm" taulocref = 4.25 ! default value call getin_p("taulocref",taulocref) write(*,*) " taulocref = ",taulocref write(*,*) "target altitude of local storm (km)" ztoploc = 10.0 ! default value call getin_p("ztoploc",ztoploc) write(*,*) " ztoploc = ",ztoploc write(*,*) "radius of dust storm (degree)" radloc = 0.5 ! default value call getin_p("radloc",radloc) write(*,*) " radloc = ",radloc write(*,*) "center longitude of storm (deg)" lonloc = 25.0 ! default value call getin_p("lonloc",lonloc) write(*,*) " lonloc = ",lonloc write(*,*) "center latitude of storm (deg)" latloc = -2.5 ! default value call getin_p("latloc",latloc) write(*,*) " latloc = ",latloc write(*,*) "reff storm (mic) 0. for background" reffstorm = 0.0 ! default value call getin_p("reffstorm",reffstorm) write(*,*) " reffstorm = ",reffstorm !! LOOP: modify opacity DO ig=1,ngrid !! distance to the center: ray(ig)=SQRT((latitude(ig)*180./pi-latloc)**2 + & (longitude(ig)*180./pi -lonloc)**2) !! transition factor for storm !! factor is hardcoded -- increase it to steepen yeah = (TANH(2.+(radloc-ray(ig))*10.)+1.)/2. !! new opacity field !! -- add an opacity set to taulocref !! -- the additional reference opacity will !! thus be taulocref*odpref/pplev tauuser(ig)=max( tau_pref_gcm(ig) * pplev(ig,1) /odpref , & taulocref * yeah ) !! compute l_top DO l=1,nlayer zalt(ig,l) = LOG( pplev(ig,1)/pplev(ig,l) ) & / g / 44.01 & * 8.31 * 210. IF ( (ztoploc .lt. zalt(ig,l) ) & .and. (ztoploc .gt. zalt(ig,l-1)) ) l_top=l-1 ENDDO !! change reffrad if ever needed IF (reffstorm .gt. 0.) THEN DO l=1,nlayer IF (l .lt. l_top+1) THEN reffrad(ig,l,iaer) = max( reffrad(ig,l,iaer), reffstorm & * 1.e-6 * yeah ) ENDIF ENDDO ENDIF ENDDO !! END LOOP !! compute perturbation in each layer (equation 8 in Spiga et al. JGR 2013) DO ig=1,ngrid int_factor(ig)=0. DO l=1,nlayer IF (l .lt. l_top+1) THEN int_factor(ig) = & int_factor(ig) + & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ENDIF ENDDO DO l=1, nlayer !! Mass mixing ratio perturbation due to local dust storm in each layer more_dust(ig,l,1)= & (tauuser(ig)-(tau_pref_gcm(ig) & * pplev(ig,1) /odpref)) / & int_factor(ig) more_dust(ig,l,2)= & (tauuser(ig)-(tau_pref_gcm(ig) * & pplev(ig,1) /odpref)) & / int_factor(ig) * & ((ref_r0/reffrad(ig,l,iaer))**3) & * r3n_q ENDDO ENDDO !! quantity of dust for each layer with the addition of the perturbation DO l=1, l_top pq(:,l,igcm_dust_mass)= pq(:,l,igcm_dust_mass) . + more_dust(:,l,1) pq(:,l,igcm_dust_number)= pq(:,l,igcm_dust_number) . + more_dust(:,l,2) ENDDO ENDIF !! IF (localstorm) tau_pref_gcm(:)=0. ENDIF !! IF (firstcall) #endif ! ! 3.1. Compute "tauscaling" and "dust_rad_adjust", the dust rescaling ! coefficients and adjust aerosol() dust opacities accordingly call compute_dustscaling(ngrid,nlayer,naerkind,naerdust,zday,pplev & ,tau_pref_scenario,IRtoVIScoef, & tauscaling,dust_rad_adjust,aerosol) ! 3.2. Recompute tau_pref_gcm, the reference dust opacity, based on dust tracer ! mixing ratios and their optical properties IF (freedust) THEN ! Initialisation : tau_pref_gcm(:)=0 DO iaer=1,naerdust DO l=1,nlayer DO ig=1,ngrid #ifdef DUSTSTORM !! recalculate opacity because storm perturbation has been added IF (firstcall) THEN aerosol(ig,l,iaer) = & ( 0.75 * QREFvis3d(ig,l,iaer) / & ( rho_dust * reffrad(ig,l,iaer) ) ) * & pq(ig,l,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ENDIF #endif c MV19: tau_pref_gcm must ALWAYS contain the opacity of all dust tracers ! GCM DUST OPTICAL DEPTH tau_pref_gcm is to be compared ! with the observation CDOD tau_pref_scenario ! => visible wavelength IF (name_iaer(iaerdust(iaer)).eq."dust_doubleq") THEN tau_pref_gcm(ig) = tau_pref_gcm(ig) + & ( 0.75 * QREFvis3d(ig,l,iaerdust(iaer)) / & ( rho_dust * reffrad(ig,l,iaerdust(iaer)) ) ) * & pq(ig,l,igcm_dust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ELSE IF (name_iaer(iaerdust(iaer)).eq."stormdust_doubleq") THEN tau_pref_gcm(ig) = tau_pref_gcm(ig) + & ( 0.75 * QREFvis3d(ig,l,iaerdust(iaer)) / & ( rho_dust * reffrad(ig,l,iaerdust(iaer)) ) ) * & pq(ig,l,igcm_stormdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ELSE IF (name_iaer(iaerdust(iaer)).eq."topdust_doubleq") THEN tau_pref_gcm(ig) = tau_pref_gcm(ig) + & ( 0.75 * QREFvis3d(ig,l,iaerdust(iaer)) / & ( rho_dust * reffrad(ig,l,iaerdust(iaer)) ) ) * & pq(ig,l,igcm_topdust_mass) * & ( pplev(ig,l) - pplev(ig,l+1) ) / g ENDIF ENDDO ENDDO ENDDO tau_pref_gcm(:) = tau_pref_gcm(:) * odpref / pplev(:,1) ELSE ! dust opacity strictly follows what is imposed by the dust scenario tau_pref_gcm(:)=tau_pref_scenario(:) ENDIF ! of IF (freedust) ! ----------------------------------------------------------------- ! 4. Total integrated visible optical depth of aerosols in each column ! ----------------------------------------------------------------- DO iaer=1,naerkind do l=1,nlayer do ig=1,ngrid tau(ig,iaer) = tau(ig,iaer) + aerosol(ig,l,iaer) end do end do ENDDO #ifdef DUSTSTORM IF (firstcall) THEN firstcall=.false. ENDIF #endif ! ! 5. Adapt aerosol() for the radiative transfer (i.e. account for ! cases when it refers to a fraction of the global mesh) ! c ----------------------------------------------------------------- c aerosol/X for stormdust to prepare calculation of radiative transfer c ----------------------------------------------------------------- IF (rdstorm) THEN DO l=1,nlayer DO ig=1,ngrid ! stormdust: opacity relative to the storm fraction (stormdust/x) aerosol(ig,l,iaer_stormdust_doubleq) = & aerosol(ig,l,iaer_stormdust_doubleq)/totstormfract(ig) ENDDO ENDDO ENDIF c ----------------------------------------------------------------- c aerosol/X for topdust to prepare calculation of radiative transfer c ----------------------------------------------------------------- IF (topflows) THEN DO ig=1,ngrid IF (contains_mons(ig)) THEN ! contains_mons=True ensures that alpha_hmons>0 DO l=1,nlayer ! topdust: opacity relative to the mons fraction (topdust/x) aerosol(ig,l,iaer_topdust_doubleq) = & aerosol(ig,l,iaer_topdust_doubleq)/alpha_hmons(ig) ENDDO ENDIF ENDDO ENDIF END SUBROUTINE aeropacity END MODULE aeropacity_mod