subroutine physiq(ngrid,nlayer,nq, & nametrac, & firstcall,lastcall, & pday,ptime,ptimestep, & pplev,pplay,pphi, & pu,pv,pt,pq, & flxw, & pdu,pdv,pdt,pdq,pdpsrf,tracerdyn) use radinc_h, only : L_NSPECTI,L_NSPECTV,naerkind use watercommon_h, only : RLVTT, Psat_water,epsi use gases_h, only: gnom, gfrac use radcommon_h, only: sigma, glat, grav use radii_mod, only: h2o_reffrad, co2_reffrad use aerosol_mod, only: iaero_co2, iaero_h2o use surfdat_h, only: phisfi, albedodat, zmea, zstd, zsig, zgam, zthe, & dryness, watercaptag use comdiurn_h, only: coslat, sinlat, coslon, sinlon use comsaison_h, only: mu0, fract, dist_star, declin, right_ascen use comsoil_h, only: nsoilmx, layer, mlayer, inertiedat USE comgeomfi_h, only: long, lati, area, totarea, totarea_planet USE tracer_h, only: noms, mmol, radius, rho_q, qext, & alpha_lift, alpha_devil, qextrhor, & igcm_h2o_ice, igcm_h2o_vap, igcm_dustbin, & igcm_co2_ice use control_mod, only: ecritphy, iphysiq, nday use phyredem, only: physdem0, physdem1 use slab_ice_h use ocean_slab_mod, only :ocean_slab_init, ocean_slab_ice, & ocean_slab_get_vars,ocean_slab_final use surf_heat_transp_mod,only :init_masquv use planetwide_mod, only: planetwide_minval,planetwide_maxval,planetwide_sumval use mod_phys_lmdz_para, only : is_master use planete_mod, only: apoastr, periastr, year_day, peri_day, & obliquit, nres, z0 use comcstfi_mod, only: pi, g, rcp, r, rad, mugaz, cpp, daysec use callkeys_mod implicit none !================================================================== ! ! Purpose ! ------- ! Central subroutine for all the physics parameterisations in the ! universal model. Originally adapted from the Mars LMDZ model. ! ! The model can be run without or with tracer transport ! depending on the value of "tracer" in file "callphys.def". ! ! ! It includes: ! ! I. Initialization : ! I.1 Firstcall initializations. ! I.2 Initialization for every call to physiq. ! ! II. Compute radiative transfer tendencies (longwave and shortwave) : ! II.a Option 1 : Call correlated-k radiative transfer scheme. ! II.b Option 2 : Call Newtonian cooling scheme. ! II.c Option 3 : Atmosphere has no radiative effect. ! ! III. Vertical diffusion (turbulent mixing) : ! ! IV. Dry Convective adjustment : ! ! V. Condensation and sublimation of gases (currently just CO2). ! ! VI. Tracers ! VI.1. Water and water ice. ! VI.2. Aerosols and particles. ! VI.3. Updates (pressure variations, surface budget). ! VI.4. Slab Ocean. ! VI.5. Surface Tracer Update. ! ! VII. Surface and sub-surface soil temperature. ! ! VIII. Perform diagnostics and write output files. ! ! ! arguments ! --------- ! ! INPUT ! ----- ! ! ngrid Size of the horizontal grid. ! nlayer Number of vertical layers. ! nq Number of advected fields. ! nametrac Name of corresponding advected fields. ! ! firstcall True at the first call. ! lastcall True at the last call. ! ! pday Number of days counted from the North. Spring equinoxe. ! ptime Universal time (00 WHEN DOWNWARDS !!) integer l,ig,ierr,iq ! FOR DIAGNOSTIC : real,dimension(:),allocatable,save :: fluxsurf_lw ! Incident Long Wave (IR) surface flux (W.m-2). real,dimension(:),allocatable,save :: fluxsurf_sw ! incident Short Wave (stellar) surface flux (W.m-2). real,dimension(:),allocatable,save :: fluxtop_lw ! Outgoing LW (IR) flux to space (W.m-2). real,dimension(:),allocatable,save :: fluxabs_sw ! Absorbed SW (stellar) flux (W.m-2). real,dimension(:),allocatable,save :: fluxtop_dn ! Incoming SW (stellar) radiation at the top of the atmosphere (W.m-2). real,dimension(:),allocatable,save :: fluxdyn ! Horizontal heat transport by dynamics (W.m-2). real,dimension(:,:),allocatable,save :: OLR_nu ! Outgoing LW radiation in each band (Normalized to the band width (W/m2/cm-1)). real,dimension(:,:),allocatable,save :: OSR_nu ! Outgoing SW radiation in each band (Normalized to the band width (W/m2/cm-1)). real,dimension(:,:),allocatable,save :: zdtlw ! LW heating tendencies (K/s). real,dimension(:,:),allocatable,save :: zdtsw ! SW heating tendencies (K/s). real,dimension(:),allocatable,save :: sensibFlux ! Turbulent flux given by the atmosphere to the surface (W.m-2). !$OMP THREADPRIVATE(fluxsurf_lw,fluxsurf_sw,fluxtop_lw,fluxabs_sw,fluxtop_dn,fluxdyn,OLR_nu,OSR_nu,& !$OMP zdtlw,zdtsw,sensibFlux) real zls ! Solar longitude (radians). real zlss ! Sub solar point longitude (radians). real zday ! Date (time since Ls=0, calculated in sols). real zzlay(ngrid,nlayer) ! Altitude at the middle of the atmospheric layers. real zzlev(ngrid,nlayer+1) ! Altitude at the atmospheric layer boundaries. ! TENDENCIES due to various processes : ! For Surface Temperature : (K/s) real zdtsurf(ngrid) ! Cumulated tendencies. real zdtsurfmr(ngrid) ! Mass_redistribution routine. real zdtsurfc(ngrid) ! Condense_co2 routine. real zdtsdif(ngrid) ! Turbdiff/vdifc routines. real zdtsurf_hyd(ngrid) ! Hydrol routine. ! For Atmospheric Temperatures : (K/s) real dtlscale(ngrid,nlayer) ! Largescale routine. real zdtc(ngrid,nlayer) ! Condense_co2 routine. real zdtdif(ngrid,nlayer) ! Turbdiff/vdifc routines. real zdtmr(ngrid,nlayer) ! Mass_redistribution routine. real zdtrain(ngrid,nlayer) ! Rain routine. real dtmoist(ngrid,nlayer) ! Moistadj routine. real dt_ekman(ngrid,noceanmx), dt_hdiff(ngrid,noceanmx) ! Slab_ocean routine. real zdtsw1(ngrid,nlayer), zdtlw1(ngrid,nlayer) ! Callcorrk routine. ! For Surface Tracers : (kg/m2/s) real dqsurf(ngrid,nq) ! Cumulated tendencies. real zdqslscale(ngrid,nq) ! Largescale routine. real zdqsdif(ngrid,nq) ! Turbdiff/vdifc routines. real zdqssed(ngrid,nq) ! Callsedim routine. real zdqsurfmr(ngrid,nq) ! Mass_redistribution routine. real zdqsrain(ngrid), zdqssnow(ngrid) ! Rain routine. real dqs_hyd(ngrid,nq) ! Hydrol routine. ! For Tracers : (kg/kg_of_air/s) real zdqc(ngrid,nlayer,nq) ! Condense_co2 routine. real zdqadj(ngrid,nlayer,nq) ! Convadj routine. real zdqdif(ngrid,nlayer,nq) ! Turbdiff/vdifc routines. real zdqevap(ngrid,nlayer) ! Turbdiff routine. real zdqsed(ngrid,nlayer,nq) ! Callsedim routine. real zdqmr(ngrid,nlayer,nq) ! Mass_redistribution routine. real zdqrain(ngrid,nlayer,nq) ! Rain routine. real dqmoist(ngrid,nlayer,nq) ! Moistadj routine. real dqvaplscale(ngrid,nlayer) ! Largescale routine. real dqcldlscale(ngrid,nlayer) ! Largescale routine. ! For Winds : (m/s/s) real zdvc(ngrid,nlayer),zduc(ngrid,nlayer) ! Condense_co2 routine. real zdvadj(ngrid,nlayer),zduadj(ngrid,nlayer) ! Convadj routine. real zdumr(ngrid,nlayer),zdvmr(ngrid,nlayer) ! Mass_redistribution routine. real zdvdif(ngrid,nlayer),zdudif(ngrid,nlayer) ! Turbdiff/vdifc routines. real zdhdif(ngrid,nlayer) ! Turbdiff/vdifc routines. real zdhadj(ngrid,nlayer) ! Convadj routine. ! For Pressure and Mass : real zdmassmr(ngrid,nlayer) ! Atmospheric Mass tendency for mass_redistribution (kg_of_air/m2/s). real zdmassmr_col(ngrid) ! Atmospheric Column Mass tendency for mass_redistribution (kg_of_air/m2/s). real zdpsrfmr(ngrid) ! Pressure tendency for mass_redistribution routine (Pa/s). ! Local variables for LOCAL CALCULATIONS: ! --------------------------------------- real zflubid(ngrid) real zplanck(ngrid),zpopsk(ngrid,nlayer) real ztim1,ztim2,ztim3, z1,z2 real ztime_fin real zdh(ngrid,nlayer) real gmplanet real taux(ngrid),tauy(ngrid) ! local variables for DIAGNOSTICS : (diagfi & stat) ! ------------------------------------------------- real ps(ngrid) ! Surface Pressure. real zt(ngrid,nlayer) ! Atmospheric Temperature. real zu(ngrid,nlayer),zv(ngrid,nlayer) ! Zonal and Meridional Winds. real zq(ngrid,nlayer,nq) ! Atmospheric Tracers. real zdtadj(ngrid,nlayer) ! Convadj Diagnostic. real zdtdyn(ngrid,nlayer) ! Dynamical Heating (K/s). real,allocatable,dimension(:,:),save :: ztprevious ! Previous loop Atmospheric Temperature (K) ! Useful for Dynamical Heating calculation. !$OMP THREADPRIVATE(ztprevious) real reff(ngrid,nlayer) ! Effective dust radius (used if doubleq=T). real vmr(ngrid,nlayer) ! volume mixing ratio real time_phys real,allocatable,dimension(:),save :: tau_col ! Total Aerosol Optical Depth. !$OMP THREADPRIVATE(tau_col) real ISR,ASR,OLR,GND,DYN,GSR,Ts1,Ts2,Ts3,TsS ! for Diagnostic. real qcol(ngrid,nq) ! Tracer Column Mass (kg/m2). ! included by RW for H2O Manabe scheme real rneb_man(ngrid,nlayer) ! H2O cloud fraction (moistadj). real rneb_lsc(ngrid,nlayer) ! H2O cloud fraction (large scale). ! to test energy conservation (RW+JL) real mass(ngrid,nlayer),massarea(ngrid,nlayer) real dEtot, dEtots, AtmToSurf_TurbFlux real,save :: dEtotSW, dEtotsSW, dEtotLW, dEtotsLW !$OMP THREADPRIVATE(dEtotSW, dEtotsSW, dEtotLW, dEtotsLW) real dEzRadsw(ngrid,nlayer),dEzRadlw(ngrid,nlayer),dEzdiff(ngrid,nlayer) real dEdiffs(ngrid),dEdiff(ngrid) real madjdE(ngrid), lscaledE(ngrid),madjdEz(ngrid,nlayer), lscaledEz(ngrid,nlayer) !JL12 conservation test for mean flow kinetic energy has been disabled temporarily real dtmoist_max,dtmoist_min real dItot, dItot_tmp, dVtot, dVtot_tmp real,allocatable,save :: hice(:) ! Oceanic Ice height. by BC !$OMP THREADPRIVATE(hice) real h2otot ! Total Amount of water. For diagnostic. real icesrf,liqsrf,icecol,vapcol ! Total Amounts of water (ice,liq,vap). For diagnostic. real dWtot, dWtot_tmp, dWtots, dWtots_tmp logical,save :: watertest !$OMP THREADPRIVATE(watertest) real qsat(ngrid,nlayer) ! Water Vapor Volume Mixing Ratio at saturation (kg/kg_of_air). real RH(ngrid,nlayer) ! Relative humidity. real H2Omaxcol(ngrid) ! Maximum possible H2O column amount (at 100% saturation) (kg/m2). real psat_tmp logical clearsky ! For double radiative transfer call. By BC real fluxsurf_lw1(ngrid), fluxsurf_sw1(ngrid), fluxtop_lw1(ngrid), fluxabs_sw1(ngrid) ! For SW/LW flux diagnostics. real tau_col1(ngrid) ! For aerosol optical depth diagnostic. real OLR_nu1(ngrid,L_NSPECTI), OSR_nu1(ngrid,L_NSPECTV) ! For Outgoing Radiation diagnostics. real tf, ntf real,allocatable,dimension(:,:),save :: cloudfrac ! Fraction of clouds (%). real,allocatable,dimension(:),save :: totcloudfrac ! Column fraction of clouds (%). !$OMP THREADPRIVATE(cloudfrac,totcloudfrac) real nconsMAX, vdifcncons(ngrid), cadjncons(ngrid) ! Vdfic water conservation test. By RW real,allocatable,dimension(:,:),save :: qsurf_hist !$OMP THREADPRIVATE(qsurf_hist) real muvar(ngrid,nlayer+1) ! For Runaway Greenhouse 1D study. By RW real,allocatable,dimension(:,:,:),save :: reffrad ! Aerosol effective radius (m). By RW real,allocatable,dimension(:,:,:),save :: nueffrad ! Aerosol effective radius variance. By RW !$OMP THREADPRIVATE(reffrad,nueffrad) real reffcol(ngrid,naerkind) ! Sourceevol for 'accelerated ice evolution'. By RW real,allocatable,dimension(:),save :: ice_initial real delta_ice,ice_tot real,allocatable,dimension(:),save :: ice_min integer num_run logical,save :: ice_update !$OMP THREADPRIVATE(ice_initial,ice_min,ice_update) ! For slab ocean. By BC real, dimension(:),allocatable,save :: pctsrf_sic real, dimension(:,:),allocatable,save :: tslab real, dimension(:),allocatable,save :: tsea_ice real, dimension(:),allocatable,save :: sea_ice real, dimension(:),allocatable,save :: zmasq integer, dimension(:),allocatable,save ::knindex !$OMP THREADPRIVATE(pctsrf_sic,tslab,tsea_ice,sea_ice,zmasq,knindex) real :: tsurf2(ngrid) real :: flux_o(ngrid),flux_g(ngrid),fluxgrdocean(ngrid) real :: flux_sens_lat(ngrid) real :: qsurfint(ngrid,nq) !================================================================================================== ! ----------------- ! I. INITIALISATION ! ----------------- ! -------------------------------- ! I.1 First Call Initialisation. ! -------------------------------- if (firstcall) then ! Allocate saved arrays. ALLOCATE(tsurf(ngrid)) ALLOCATE(tsoil(ngrid,nsoilmx)) ALLOCATE(albedo(ngrid)) ALLOCATE(albedo0(ngrid)) ALLOCATE(rnat(ngrid)) ALLOCATE(emis(ngrid)) ALLOCATE(dtrad(ngrid,nlayer)) ALLOCATE(fluxrad_sky(ngrid)) ALLOCATE(fluxrad(ngrid)) ALLOCATE(capcal(ngrid)) ALLOCATE(fluxgrd(ngrid)) ALLOCATE(qsurf(ngrid,nq)) ALLOCATE(q2(ngrid,nlayer+1)) ALLOCATE(ztprevious(ngrid,nlayer)) ALLOCATE(cloudfrac(ngrid,nlayer)) ALLOCATE(totcloudfrac(ngrid)) ALLOCATE(hice(ngrid)) ALLOCATE(qsurf_hist(ngrid,nq)) ALLOCATE(reffrad(ngrid,nlayer,naerkind)) ALLOCATE(nueffrad(ngrid,nlayer,naerkind)) ALLOCATE(ice_initial(ngrid)) ALLOCATE(ice_min(ngrid)) ALLOCATE(fluxsurf_lw(ngrid)) ALLOCATE(fluxsurf_sw(ngrid)) ALLOCATE(fluxtop_lw(ngrid)) ALLOCATE(fluxabs_sw(ngrid)) ALLOCATE(fluxtop_dn(ngrid)) ALLOCATE(fluxdyn(ngrid)) ALLOCATE(OLR_nu(ngrid,L_NSPECTI)) ALLOCATE(OSR_nu(ngrid,L_NSPECTV)) ALLOCATE(sensibFlux(ngrid)) ALLOCATE(zdtlw(ngrid,nlayer)) ALLOCATE(zdtsw(ngrid,nlayer)) ALLOCATE(tau_col(ngrid)) ALLOCATE(pctsrf_sic(ngrid)) ALLOCATE(tslab(ngrid,noceanmx)) ALLOCATE(tsea_ice(ngrid)) ALLOCATE(sea_ice(ngrid)) ALLOCATE(zmasq(ngrid)) ALLOCATE(knindex(ngrid)) ! This is defined in comsaison_h ALLOCATE(mu0(ngrid)) ALLOCATE(fract(ngrid)) ! This is defined in radcommon_h ALLOCATE(glat(ngrid)) ! Variables set to 0 ! ~~~~~~~~~~~~~~~~~~ dtrad(:,:) = 0.0 fluxrad(:) = 0.0 tau_col(:) = 0.0 zdtsw(:,:) = 0.0 zdtlw(:,:) = 0.0 ! Initialize aerosol indexes. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~ call iniaerosol() ! Initialize tracer names, indexes and properties. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ tracerdyn=tracer IF (.NOT.ALLOCATED(noms)) ALLOCATE(noms(nq)) ! (because noms is an argument of physdem1 whether or not tracer is on) if (tracer) then call initracer(ngrid,nq,nametrac) endif ! Read 'startfi.nc' file. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ call phyetat0(ngrid,nlayer,"startfi.nc",0,0,nsoilmx,nq, & day_ini,time_phys,tsurf,tsoil,emis,q2,qsurf, & cloudfrac,totcloudfrac,hice, & rnat,pctsrf_sic,tslab, tsea_ice,sea_ice) if (pday.ne.day_ini) then write(*,*) "ERROR in physiq.F90:" write(*,*) "bad synchronization between physics and dynamics" write(*,*) "dynamics day: ",pday write(*,*) "physics day: ",day_ini stop endif write (*,*) 'In physiq day_ini =', day_ini ! Initialize albedo and orbital calculation. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ call surfini(ngrid,nq,qsurf,albedo0) call iniorbit(apoastr,periastr,year_day,peri_day,obliquit) albedo(:)=albedo0(:) if(tlocked)then print*,'Planet is tidally locked at resonance n=',nres print*,'Make sure you have the right rotation rate!!!' endif ! Initialize oceanic variables. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if (ok_slab_ocean)then call ocean_slab_init(ngrid,ptimestep, tslab, & sea_ice, pctsrf_sic) knindex(:) = 0 do ig=1,ngrid zmasq(ig)=1 knindex(ig) = ig if (nint(rnat(ig)).eq.0) then zmasq(ig)=0 endif enddo CALL init_masquv(ngrid,zmasq) endif ! end of 'ok_slab_ocean'. ! Initialize soil. ! ~~~~~~~~~~~~~~~~ if (callsoil) then call soil(ngrid,nsoilmx,firstcall,lastcall,inertiedat, & ptimestep,tsurf,tsoil,capcal,fluxgrd) if (ok_slab_ocean) then do ig=1,ngrid if (nint(rnat(ig)).eq.2) then capcal(ig)=capcalocean if (pctsrf_sic(ig).gt.0.5) then capcal(ig)=capcalseaice if (qsurf(ig,igcm_h2o_ice).gt.0.) then capcal(ig)=capcalsno endif endif endif enddo endif ! end of 'ok_slab_ocean'. else ! else of 'callsoil'. print*,'WARNING! Thermal conduction in the soil turned off' capcal(:)=1.e6 fluxgrd(:)=intheat print*,'Flux from ground = ',intheat,' W m^-2' endif ! end of 'callsoil'. icount=1 ! Decide whether to update ice at end of run. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ ice_update=.false. if(sourceevol)then !$OMP MASTER open(128,file='num_run',form='formatted', & status="old",iostat=ierr) if (ierr.ne.0) then write(*,*) "physiq: Error! No num_run file!" write(*,*) " (which is needed for sourceevol option)" stop endif read(128,*) num_run close(128) !$OMP END MASTER !$OMP BARRIER if(num_run.ne.0.and.mod(num_run,2).eq.0)then print*,'Updating ice at end of this year!' ice_update=.true. ice_min(:)=1.e4 endif endif ! end of 'sourceevol'. ! Here is defined the type of the surface : Continent or Ocean. ! BC2014 : This is now already done in newstart. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if (.not.ok_slab_ocean) then rnat(:)=1. do ig=1,ngrid if(inertiedat(ig,1).gt.1.E4)then rnat(ig)=0 endif enddo print*,'WARNING! Surface type currently decided by surface inertia' print*,'This should be improved e.g. in newstart.F' endif ! end of 'ok_slab_ocean'. ! Initialize surface history variable. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ qsurf_hist(:,:)=qsurf(:,:) ! Initialize variable for dynamical heating diagnostic. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ ztprevious(:,:)=pt(:,:) ! Set temperature just above condensation temperature (for Early Mars) ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if(nearco2cond) then write(*,*)' WARNING! Starting at Tcond+1K' do l=1, nlayer do ig=1,ngrid pdt(ig,l)= ((-3167.8)/(log(.01*pplay(ig,l))-23.23)+4 & -pt(ig,l)) / ptimestep enddo enddo endif if(meanOLR)then call system('rm -f rad_bal.out') ! to record global radiative balance. call system('rm -f tem_bal.out') ! to record global mean/max/min temperatures. call system('rm -f h2o_bal.out') ! to record global hydrological balance. endif watertest=.false. if(water)then ! Initialize variables for water cycle if(enertest)then watertest = .true. endif if(ice_update)then ice_initial(:)=qsurf(:,igcm_h2o_ice) endif endif call su_watercycle ! even if we don't have a water cycle, we might ! need epsi for the wvp definitions in callcorrk.F if (ngrid.ne.1) then ! Note : no need to create a restart file in 1d. call physdem0("restartfi.nc",long,lati,nsoilmx,ngrid,nlayer,nq, & ptimestep,pday+nday,time_phys,area, & albedodat,inertiedat,zmea,zstd,zsig,zgam,zthe) endif endif ! end of 'firstcall' ! ------------------------------------------------------ ! I.2 Initializations done at every physical timestep: ! ------------------------------------------------------ ! Initialize various variables ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if ( .not.nearco2cond ) then pdt(1:ngrid,1:nlayer) = 0.0 endif zdtsurf(1:ngrid) = 0.0 pdq(1:ngrid,1:nlayer,1:nq) = 0.0 dqsurf(1:ngrid,1:nq)= 0.0 pdu(1:ngrid,1:nlayer) = 0.0 pdv(1:ngrid,1:nlayer) = 0.0 pdpsrf(1:ngrid) = 0.0 zflubid(1:ngrid) = 0.0 flux_sens_lat(1:ngrid) = 0.0 taux(1:ngrid) = 0.0 tauy(1:ngrid) = 0.0 zday=pday+ptime ! Compute time, in sols (and fraction thereof). ! Compute Stellar Longitude (Ls), and orbital parameters. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if (season) then call stellarlong(zday,zls) else call stellarlong(float(day_ini),zls) end if call orbite(zls,dist_star,declin,right_ascen) if (tlocked) then zlss=Mod(-(2.*pi*(zday/year_day)*nres - right_ascen),2.*pi) elseif (diurnal) then zlss=-2.*pi*(zday-.5) else if(diurnal .eqv. .false.) then zlss=9999. endif ! Compute variations of g with latitude (oblate case). ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if (oblate .eqv. .false.) then glat(:) = g else if (flatten .eq. 0.0 .or. J2 .eq. 0.0 .or. Rmean .eq. 0.0 .or. MassPlanet .eq. 0.0) then print*,'I need values for flatten, J2, Rmean and MassPlanet to compute glat (else set oblate=.false.)' call abort else gmplanet = MassPlanet*grav*1e24 do ig=1,ngrid glat(ig)= gmplanet/(Rmean**2) * (1.D0 + 0.75 *J2 - 2.0*flatten/3. + (2.*flatten - 15./4.* J2) * cos(2. * (pi/2. - lati(ig)))) end do endif ! Compute geopotential between layers. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ zzlay(1:ngrid,1:nlayer)=pphi(1:ngrid,1:nlayer) do l=1,nlayer zzlay(1:ngrid,l)= zzlay(1:ngrid,l)/glat(1:ngrid) enddo zzlev(1:ngrid,1)=0. zzlev(1:ngrid,nlayer+1)=1.e7 ! Dummy top of last layer above 10000 km... do l=2,nlayer do ig=1,ngrid z1=(pplay(ig,l-1)+pplev(ig,l))/(pplay(ig,l-1)-pplev(ig,l)) z2=(pplev(ig,l)+pplay(ig,l))/(pplev(ig,l)-pplay(ig,l)) zzlev(ig,l)=(z1*zzlay(ig,l-1)+z2*zzlay(ig,l))/(z1+z2) enddo enddo ! Compute potential temperature ! Note : Potential temperature calculation may not be the same in physiq and dynamic... ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ do l=1,nlayer do ig=1,ngrid zpopsk(ig,l)=(pplay(ig,l)/pplev(ig,1))**rcp zh(ig,l)=pt(ig,l)/zpopsk(ig,l) mass(ig,l) = (pplev(ig,l) - pplev(ig,l+1))/glat(ig) massarea(ig,l)=mass(ig,l)*area(ig) enddo enddo ! Compute vertical velocity (m/s) from vertical mass flux ! w = F / (rho*area) and rho = P/(r*T) ! But first linearly interpolate mass flux to mid-layers do l=1,nlayer-1 pw(1:ngrid,l)=0.5*(flxw(1:ngrid,l)+flxw(1:ngrid,l+1)) enddo pw(1:ngrid,nlayer)=0.5*flxw(1:ngrid,nlayer) ! since flxw(nlayer+1)=0 do l=1,nlayer pw(1:ngrid,l)=(pw(1:ngrid,l)*r*pt(1:ngrid,l)) / & (pplay(1:ngrid,l)*area(1:ngrid)) enddo !--------------------------------- ! II. Compute radiative tendencies !--------------------------------- if (callrad) then if( mod(icount-1,iradia).eq.0.or.lastcall) then ! Compute local stellar zenith angles ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if (tlocked) then ! JL14 corrects tidally resonant (and inclined) cases. nres=omega_rot/omega_orb ztim1=SIN(declin) ztim2=COS(declin)*COS(zlss) ztim3=COS(declin)*SIN(zlss) call stelang(ngrid,sinlon,coslon,sinlat,coslat, & ztim1,ztim2,ztim3,mu0,fract, flatten) elseif (diurnal) then ztim1=SIN(declin) ztim2=COS(declin)*COS(2.*pi*(zday-.5)) ztim3=-COS(declin)*SIN(2.*pi*(zday-.5)) call stelang(ngrid,sinlon,coslon,sinlat,coslat, & ztim1,ztim2,ztim3,mu0,fract, flatten) else if(diurnal .eqv. .false.) then call mucorr(ngrid,declin,lati,mu0,fract,10000.,rad,flatten) ! WARNING: this function appears not to work in 1D endif ! Eclipse incoming sunlight (e.g. Saturn ring shadowing). if(rings_shadow) then call call_rings(ngrid, ptime, pday, diurnal) endif if (corrk) then ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ ! II.a Call correlated-k radiative transfer scheme ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if(kastprof)then print*,'kastprof should not = true here' call abort endif if(water) then muvar(1:ngrid,1:nlayer)=mugaz/(1.e0+(1.e0/epsi-1.e0)*pq(1:ngrid,1:nlayer,igcm_h2o_vap)) muvar(1:ngrid,nlayer+1)=mugaz/(1.e0+(1.e0/epsi-1.e0)*pq(1:ngrid,nlayer,igcm_h2o_vap)) ! take into account water effect on mean molecular weight else muvar(1:ngrid,1:nlayer+1)=mugaz endif if(ok_slab_ocean) then tsurf2(:)=tsurf(:) do ig=1,ngrid if (nint(rnat(ig))==0) then tsurf(ig)=((1.-pctsrf_sic(ig))*tslab(ig,1)**4+pctsrf_sic(ig)*tsea_ice(ig)**4)**0.25 endif enddo endif !(ok_slab_ocean) ! standard callcorrk clearsky=.false. call callcorrk(ngrid,nlayer,pq,nq,qsurf, & albedo,emis,mu0,pplev,pplay,pt, & tsurf,fract,dist_star,aerosol,muvar, & zdtlw,zdtsw,fluxsurf_lw,fluxsurf_sw,fluxtop_lw, & fluxabs_sw,fluxtop_dn,OLR_nu,OSR_nu, & tau_col,cloudfrac,totcloudfrac, & clearsky,firstcall,lastcall) ! Option to call scheme once more for clear regions if(CLFvarying)then ! ---> PROBLEMS WITH ALLOCATED ARRAYS : temporary solution in callcorrk: do not deallocate if CLFvarying ... clearsky=.true. call callcorrk(ngrid,nlayer,pq,nq,qsurf, & albedo,emis,mu0,pplev,pplay,pt, & tsurf,fract,dist_star,aerosol,muvar, & zdtlw1,zdtsw1,fluxsurf_lw1,fluxsurf_sw1,fluxtop_lw1, & fluxabs_sw1,fluxtop_dn,OLR_nu1,OSR_nu1, & tau_col1,cloudfrac,totcloudfrac, & clearsky,firstcall,lastcall) clearsky = .false. ! just in case. ! Sum the fluxes and heating rates from cloudy/clear cases do ig=1,ngrid tf=totcloudfrac(ig) ntf=1.-tf fluxsurf_lw(ig) = ntf*fluxsurf_lw1(ig) + tf*fluxsurf_lw(ig) fluxsurf_sw(ig) = ntf*fluxsurf_sw1(ig) + tf*fluxsurf_sw(ig) fluxtop_lw(ig) = ntf*fluxtop_lw1(ig) + tf*fluxtop_lw(ig) fluxabs_sw(ig) = ntf*fluxabs_sw1(ig) + tf*fluxabs_sw(ig) tau_col(ig) = ntf*tau_col1(ig) + tf*tau_col(ig) zdtlw(ig,1:nlayer) = ntf*zdtlw1(ig,1:nlayer) + tf*zdtlw(ig,1:nlayer) zdtsw(ig,1:nlayer) = ntf*zdtsw1(ig,1:nlayer) + tf*zdtsw(ig,1:nlayer) OSR_nu(ig,1:L_NSPECTV) = ntf*OSR_nu1(ig,1:L_NSPECTV) + tf*OSR_nu(ig,1:L_NSPECTV) OLR_nu(ig,1:L_NSPECTI) = ntf*OLR_nu1(ig,1:L_NSPECTI) + tf*OLR_nu(ig,1:L_NSPECTI) enddo endif ! end of CLFvarying. if(ok_slab_ocean) then tsurf(:)=tsurf2(:) endif ! Radiative flux from the sky absorbed by the surface (W.m-2) GSR=0.0 fluxrad_sky(1:ngrid)=emis(1:ngrid)*fluxsurf_lw(1:ngrid)+fluxsurf_sw(1:ngrid)*(1.-albedo(1:ngrid)) !if(noradsurf)then ! no lower surface; SW flux just disappears ! GSR = SUM(fluxsurf_sw(1:ngrid)*area(1:ngrid))/totarea ! fluxrad_sky(1:ngrid)=emis(1:ngrid)*fluxsurf_lw(1:ngrid) ! print*,'SW lost in deep atmosphere = ',GSR,' W m^-2' !endif ! Net atmospheric radiative heating rate (K.s-1) dtrad(1:ngrid,1:nlayer)=zdtsw(1:ngrid,1:nlayer)+zdtlw(1:ngrid,1:nlayer) elseif(newtonian)then ! II.b Call Newtonian cooling scheme ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ call newtrelax(ngrid,nlayer,mu0,sinlat,zpopsk,pt,pplay,pplev,dtrad,firstcall) zdtsurf(1:ngrid) = +(pt(1:ngrid,1)-tsurf(1:ngrid))/ptimestep ! e.g. surface becomes proxy for 1st atmospheric layer ? else ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ ! II.c Atmosphere has no radiative effect ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ fluxtop_dn(1:ngrid) = fract(1:ngrid)*mu0(1:ngrid)*Fat1AU/dist_star**2 if(ngrid.eq.1)then ! / by 4 globally in 1D case... fluxtop_dn(1) = fract(1)*Fat1AU/dist_star**2/2.0 endif fluxsurf_sw(1:ngrid) = fluxtop_dn(1:ngrid) fluxrad_sky(1:ngrid) = fluxtop_dn(1:ngrid)*(1.-albedo(1:ngrid)) fluxtop_lw(1:ngrid) = emis(1:ngrid)*sigma*tsurf(1:ngrid)**4 dtrad(1:ngrid,1:nlayer)=0.0 ! no atmospheric radiative heating endif ! end of corrk endif ! of if(mod(icount-1,iradia).eq.0) ! Transformation of the radiative tendencies ! ------------------------------------------ zplanck(1:ngrid)=tsurf(1:ngrid)*tsurf(1:ngrid) zplanck(1:ngrid)=emis(1:ngrid)*sigma*zplanck(1:ngrid)*zplanck(1:ngrid) fluxrad(1:ngrid)=fluxrad_sky(1:ngrid)-zplanck(1:ngrid) pdt(1:ngrid,1:nlayer)=pdt(1:ngrid,1:nlayer)+dtrad(1:ngrid,1:nlayer) ! Test of energy conservation !---------------------------- if(enertest)then call planetwide_sumval(cpp*massarea(:,:)*zdtsw(:,:)/totarea_planet,dEtotSW) call planetwide_sumval(cpp*massarea(:,:)*zdtlw(:,:)/totarea_planet,dEtotLW) call planetwide_sumval(fluxsurf_sw(:)*(1.-albedo(:))*area(:)/totarea_planet,dEtotsSW) !JL13 carefull, albedo can have changed since the last time we called corrk call planetwide_sumval((fluxsurf_lw(:)*emis(:)-zplanck(:))*area(:)/totarea_planet,dEtotsLW) dEzRadsw(:,:)=cpp*mass(:,:)*zdtsw(:,:) dEzRadlw(:,:)=cpp*mass(:,:)*zdtlw(:,:) if (is_master) then print*,'---------------------------------------------------------------' print*,'In corrk SW atmospheric heating =',dEtotSW,' W m-2' print*,'In corrk LW atmospheric heating =',dEtotLW,' W m-2' print*,'atmospheric net rad heating (SW+LW) =',dEtotLW+dEtotSW,' W m-2' print*,'In corrk SW surface heating =',dEtotsSW,' W m-2' print*,'In corrk LW surface heating =',dEtotsLW,' W m-2' print*,'surface net rad heating (SW+LW) =',dEtotsLW+dEtotsSW,' W m-2' endif endif ! end of 'enertest' endif ! of if (callrad) ! -------------------------------------------- ! III. Vertical diffusion (turbulent mixing) : ! -------------------------------------------- if (calldifv) then zflubid(1:ngrid)=fluxrad(1:ngrid)+fluxgrd(1:ngrid) ! JL12 the following if test is temporarily there to allow us to compare the old vdifc with turbdiff. if (UseTurbDiff) then call turbdiff(ngrid,nlayer,nq,rnat, & ptimestep,capcal,lwrite, & pplay,pplev,zzlay,zzlev,z0, & pu,pv,pt,zpopsk,pq,tsurf,emis,qsurf, & pdt,pdq,zflubid, & zdudif,zdvdif,zdtdif,zdtsdif, & sensibFlux,q2,zdqdif,zdqevap,zdqsdif, & taux,tauy,lastcall) else zdh(1:ngrid,1:nlayer)=pdt(1:ngrid,1:nlayer)/zpopsk(1:ngrid,1:nlayer) call vdifc(ngrid,nlayer,nq,rnat,zpopsk, & ptimestep,capcal,lwrite, & pplay,pplev,zzlay,zzlev,z0, & pu,pv,zh,pq,tsurf,emis,qsurf, & zdh,pdq,zflubid, & zdudif,zdvdif,zdhdif,zdtsdif, & sensibFlux,q2,zdqdif,zdqsdif, & taux,tauy,lastcall) zdtdif(1:ngrid,1:nlayer)=zdhdif(1:ngrid,1:nlayer)*zpopsk(1:ngrid,1:nlayer) ! for diagnostic only zdqevap(1:ngrid,1:nlayer)=0. end if !end of 'UseTurbDiff' pdv(1:ngrid,1:nlayer)=pdv(1:ngrid,1:nlayer)+zdvdif(1:ngrid,1:nlayer) pdu(1:ngrid,1:nlayer)=pdu(1:ngrid,1:nlayer)+zdudif(1:ngrid,1:nlayer) pdt(1:ngrid,1:nlayer)=pdt(1:ngrid,1:nlayer)+zdtdif(1:ngrid,1:nlayer) zdtsurf(1:ngrid)=zdtsurf(1:ngrid)+zdtsdif(1:ngrid) if(ok_slab_ocean)then flux_sens_lat(1:ngrid)=(zdtsdif(1:ngrid)*capcal(1:ngrid)-fluxrad(1:ngrid)) endif if (tracer) then pdq(1:ngrid,1:nlayer,1:nq)=pdq(1:ngrid,1:nlayer,1:nq)+ zdqdif(1:ngrid,1:nlayer,1:nq) dqsurf(1:ngrid,1:nq)=dqsurf(1:ngrid,1:nq) + zdqsdif(1:ngrid,1:nq) end if ! of if (tracer) ! test energy conservation !------------------------- if(enertest)then dEzdiff(:,:)=cpp*mass(:,:)*zdtdif(:,:) do ig = 1, ngrid dEdiff(ig)=SUM(dEzdiff (ig,:))+ sensibFlux(ig)! subtract flux to the ground dEzdiff(ig,1)= dEzdiff(ig,1)+ sensibFlux(ig)! subtract flux to the ground enddo call planetwide_sumval(dEdiff(:)*area(:)/totarea_planet,dEtot) dEdiffs(:)=capcal(:)*zdtsdif(:)-zflubid(:)-sensibFlux(:) call planetwide_sumval(dEdiffs(:)*area(:)/totarea_planet,dEtots) call planetwide_sumval(sensibFlux(:)*area(:)/totarea_planet,AtmToSurf_TurbFlux) if (is_master) then if (UseTurbDiff) then print*,'In TurbDiff sensible flux (atm=>surf) =',AtmToSurf_TurbFlux,' W m-2' print*,'In TurbDiff non-cons atm nrj change =',dEtot,' W m-2' print*,'In TurbDiff (correc rad+latent heat) surf nrj change =',dEtots,' W m-2' else print*,'In vdifc sensible flux (atm=>surf) =',AtmToSurf_TurbFlux,' W m-2' print*,'In vdifc non-cons atm nrj change =',dEtot,' W m-2' print*,'In vdifc (correc rad+latent heat) surf nrj change =',dEtots,' W m-2' end if endif ! end of 'is_master' ! JL12 : note that the black body radiative flux emitted by the surface has been updated by the implicit scheme but not given back elsewhere. endif ! end of 'enertest' ! Test water conservation. if(watertest.and.water)then call planetwide_sumval(massarea(:,:)*zdqdif(:,:,igcm_h2o_vap)*ptimestep/totarea_planet,dWtot_tmp) call planetwide_sumval(zdqsdif(:,igcm_h2o_vap)*area(:)*ptimestep/totarea_planet,dWtots_tmp) do ig = 1, ngrid vdifcncons(ig)=SUM(mass(ig,:)*zdqdif(ig,:,igcm_h2o_vap)) enddo call planetwide_sumval(massarea(:,:)*zdqdif(:,:,igcm_h2o_ice)*ptimestep/totarea_planet,dWtot) call planetwide_sumval(zdqsdif(:,igcm_h2o_ice)*area(:)*ptimestep/totarea_planet,dWtots) dWtot = dWtot + dWtot_tmp dWtots = dWtots + dWtots_tmp do ig = 1, ngrid vdifcncons(ig)=vdifcncons(ig) + SUM(mass(ig,:)*zdqdif(ig,:,igcm_h2o_ice)) enddo call planetwide_maxval(vdifcncons(:),nconsMAX) if (is_master) then print*,'---------------------------------------------------------------' print*,'In difv atmospheric water change =',dWtot,' kg m-2' print*,'In difv surface water change =',dWtots,' kg m-2' print*,'In difv non-cons factor =',dWtot+dWtots,' kg m-2' print*,'In difv MAX non-cons factor =',nconsMAX,' kg m-2 s-1' endif endif ! end of 'watertest' !------------------------- else ! calldifv if(.not.newtonian)then zdtsurf(1:ngrid) = zdtsurf(1:ngrid) + (fluxrad(1:ngrid) + fluxgrd(1:ngrid))/capcal(1:ngrid) endif endif ! end of 'calldifv' !---------------------------------- ! IV. Dry convective adjustment : !---------------------------------- if(calladj) then zdh(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer)/zpopsk(1:ngrid,1:nlayer) zduadj(1:ngrid,1:nlayer)=0.0 zdvadj(1:ngrid,1:nlayer)=0.0 zdhadj(1:ngrid,1:nlayer)=0.0 call convadj(ngrid,nlayer,nq,ptimestep, & pplay,pplev,zpopsk, & pu,pv,zh,pq, & pdu,pdv,zdh,pdq, & zduadj,zdvadj,zdhadj, & zdqadj) pdu(1:ngrid,1:nlayer) = pdu(1:ngrid,1:nlayer) + zduadj(1:ngrid,1:nlayer) pdv(1:ngrid,1:nlayer) = pdv(1:ngrid,1:nlayer) + zdvadj(1:ngrid,1:nlayer) pdt(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer) + zdhadj(1:ngrid,1:nlayer)*zpopsk(1:ngrid,1:nlayer) zdtadj(1:ngrid,1:nlayer) = zdhadj(1:ngrid,1:nlayer)*zpopsk(1:ngrid,1:nlayer) ! for diagnostic only if(tracer) then pdq(1:ngrid,1:nlayer,1:nq) = pdq(1:ngrid,1:nlayer,1:nq) + zdqadj(1:ngrid,1:nlayer,1:nq) end if ! Test energy conservation if(enertest)then call planetwide_sumval(cpp*massarea(:,:)*zdtadj(:,:)/totarea_planet,dEtot) if (is_master) print*,'In convadj atmospheric energy change =',dEtot,' W m-2' endif ! Test water conservation if(watertest)then call planetwide_sumval(massarea(:,:)*zdqadj(:,:,igcm_h2o_vap)*ptimestep/totarea_planet,dWtot_tmp) do ig = 1, ngrid cadjncons(ig)=SUM(mass(ig,:)*zdqadj(ig,:,igcm_h2o_vap)) enddo call planetwide_sumval(massarea(:,:)*zdqadj(:,:,igcm_h2o_ice)*ptimestep/totarea_planet,dWtot) dWtot = dWtot + dWtot_tmp do ig = 1, ngrid cadjncons(ig)=cadjncons(ig) + SUM(mass(ig,:)*zdqadj(ig,:,igcm_h2o_ice)) enddo call planetwide_maxval(cadjncons(:),nconsMAX) if (is_master) then print*,'In convadj atmospheric water change =',dWtot,' kg m-2' print*,'In convadj MAX non-cons factor =',nconsMAX,' kg m-2 s-1' endif endif ! end of 'watertest' endif ! end of 'calladj' !----------------------------------------------- ! V. Carbon dioxide condensation-sublimation : !----------------------------------------------- if (co2cond) then if (.not.tracer) then print*,'We need a CO2 ice tracer to condense CO2' call abort endif call condense_co2(ngrid,nlayer,nq,ptimestep, & capcal,pplay,pplev,tsurf,pt, & pphi,pdt,pdu,pdv,zdtsurf,pu,pv,pq,pdq, & qsurf(1,igcm_co2_ice),albedo,emis, & zdtc,zdtsurfc,pdpsrf,zduc,zdvc, & zdqc) pdt(1:ngrid,1:nlayer)=pdt(1:ngrid,1:nlayer)+zdtc(1:ngrid,1:nlayer) pdv(1:ngrid,1:nlayer)=pdv(1:ngrid,1:nlayer)+zdvc(1:ngrid,1:nlayer) pdu(1:ngrid,1:nlayer)=pdu(1:ngrid,1:nlayer)+zduc(1:ngrid,1:nlayer) zdtsurf(1:ngrid) = zdtsurf(1:ngrid) + zdtsurfc(1:ngrid) pdq(1:ngrid,1:nlayer,1:nq)=pdq(1:ngrid,1:nlayer,1:nq)+ zdqc(1:ngrid,1:nlayer,1:nq) ! test energy conservation if(enertest)then call planetwide_sumval(cpp*massarea(:,:)*zdtc(:,:)/totarea_planet,dEtot) call planetwide_sumval(capcal(:)*zdtsurfc(:)*area(:)/totarea_planet,dEtots) if (is_master) then print*,'In co2cloud atmospheric energy change =',dEtot,' W m-2' print*,'In co2cloud surface energy change =',dEtots,' W m-2' endif endif endif ! end of 'co2cond' !--------------------------------------------- ! VI. Specific parameterizations for tracers !--------------------------------------------- if (tracer) then ! --------------------- ! VI.1. Water and ice ! --------------------- if (water) then ! Water ice condensation in the atmosphere if(watercond.and.(RLVTT.gt.1.e-8))then dqmoist(1:ngrid,1:nlayer,1:nq)=0. dtmoist(1:ngrid,1:nlayer)=0. ! Moist Convective Adjustment. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~ call moistadj(ngrid,nlayer,nq,pt,pq,pdq,pplev,pplay,dtmoist,dqmoist,ptimestep,rneb_man) pdq(1:ngrid,1:nlayer,igcm_h2o_vap) = pdq(1:ngrid,1:nlayer,igcm_h2o_vap) & + dqmoist(1:ngrid,1:nlayer,igcm_h2o_vap) pdq(1:ngrid,1:nlayer,igcm_h2o_ice) = pdq(1:ngrid,1:nlayer,igcm_h2o_ice) & + dqmoist(1:ngrid,1:nlayer,igcm_h2o_ice) pdt(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer)+dtmoist(1:ngrid,1:nlayer) ! Test energy conservation. if(enertest)then call planetwide_sumval(cpp*massarea(:,:)*dtmoist(:,:)/totarea_planet,dEtot) call planetwide_maxval(dtmoist(:,:),dtmoist_max) call planetwide_minval(dtmoist(:,:),dtmoist_min) madjdEz(:,:)=cpp*mass(:,:)*dtmoist(:,:) do ig=1,ngrid madjdE(ig) = cpp*SUM(mass(:,:)*dtmoist(:,:)) enddo if (is_master) then print*,'In moistadj atmospheric energy change =',dEtot,' W m-2' print*,'In moistadj MAX atmospheric energy change =',dtmoist_max*ptimestep,'K/step' print*,'In moistadj MIN atmospheric energy change =',dtmoist_min*ptimestep,'K/step' endif call planetwide_sumval(massarea(:,:)*dqmoist(:,:,igcm_h2o_vap)*ptimestep/totarea_planet+ & massarea(:,:)*dqmoist(:,:,igcm_h2o_ice)*ptimestep/totarea_planet,dWtot) if (is_master) print*,'In moistadj atmospheric water change =',dWtot,' kg m-2' endif ! end of 'enertest' ! Large scale condensation/evaporation. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ call largescale(ngrid,nlayer,nq,ptimestep,pplev,pplay,pt,pq,pdt,pdq,dtlscale,dqvaplscale,dqcldlscale,rneb_lsc) pdt(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer)+dtlscale(1:ngrid,1:nlayer) pdq(1:ngrid,1:nlayer,igcm_h2o_vap) = pdq(1:ngrid,1:nlayer,igcm_h2o_vap)+dqvaplscale(1:ngrid,1:nlayer) pdq(1:ngrid,1:nlayer,igcm_h2o_ice) = pdq(1:ngrid,1:nlayer,igcm_h2o_ice)+dqcldlscale(1:ngrid,1:nlayer) ! Test energy conservation. if(enertest)then lscaledEz(:,:) = cpp*mass(:,:)*dtlscale(:,:) do ig=1,ngrid lscaledE(ig) = cpp*SUM(mass(:,:)*dtlscale(:,:)) enddo call planetwide_sumval(cpp*massarea(:,:)*dtlscale(:,:)/totarea_planet,dEtot) if (is_master) print*,'In largescale atmospheric energy change =',dEtot,' W m-2' ! Test water conservation. call planetwide_sumval(massarea(:,:)*dqvaplscale(:,:)*ptimestep/totarea_planet+ & SUM(massarea(:,:)*dqcldlscale(:,:))*ptimestep/totarea_planet,dWtot) if (is_master) print*,'In largescale atmospheric water change =',dWtot,' kg m-2' endif ! end of 'enertest' ! Compute cloud fraction. do l = 1, nlayer do ig=1,ngrid cloudfrac(ig,l)=MAX(rneb_lsc(ig,l),rneb_man(ig,l)) enddo enddo endif ! end of 'watercond' ! Water ice / liquid precipitation. ! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ if(waterrain)then zdqrain(1:ngrid,1:nlayer,1:nq) = 0.0 zdqsrain(1:ngrid) = 0.0 zdqssnow(1:ngrid) = 0.0 call rain(ngrid,nlayer,nq,ptimestep,pplev,pplay,pt,pdt,pq,pdq, & zdtrain,zdqrain,zdqsrain,zdqssnow,cloudfrac) pdq(1:ngrid,1:nlayer,igcm_h2o_vap) = pdq(1:ngrid,1:nlayer,igcm_h2o_vap) & + zdqrain(1:ngrid,1:nlayer,igcm_h2o_vap) pdq(1:ngrid,1:nlayer,igcm_h2o_ice) = pdq(1:ngrid,1:nlayer,igcm_h2o_ice) & + zdqrain(1:ngrid,1:nlayer,igcm_h2o_ice) pdt(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer)+zdtrain(1:ngrid,1:nlayer) dqsurf(1:ngrid,igcm_h2o_vap) = dqsurf(1:ngrid,igcm_h2o_vap)+zdqsrain(1:ngrid) dqsurf(1:ngrid,igcm_h2o_ice) = dqsurf(1:ngrid,igcm_h2o_ice)+zdqssnow(1:ngrid) ! Test energy conservation. if(enertest)then call planetwide_sumval(cpp*massarea(:,:)*zdtrain(:,:)/totarea_planet,dEtot) if (is_master) print*,'In rain atmospheric T energy change =',dEtot,' W m-2' call planetwide_sumval(massarea(:,:)*zdqrain(:,:,igcm_h2o_ice)/totarea_planet*RLVTT/cpp,dItot_tmp) call planetwide_sumval(area(:)*zdqssnow(:)/totarea_planet*RLVTT/cpp,dItot) dItot = dItot + dItot_tmp call planetwide_sumval(massarea(:,:)*zdqrain(:,:,igcm_h2o_vap)*ptimestep/totarea_planet,dVtot_tmp) call planetwide_sumval(area(:)*zdqsrain(:)/totarea_planet*RLVTT/cpp,dVtot) dVtot = dVtot + dVtot_tmp dEtot = dItot + dVtot if (is_master) then print*,'In rain dItot =',dItot,' W m-2' print*,'In rain dVtot =',dVtot,' W m-2' print*,'In rain atmospheric L energy change =',dEtot,' W m-2' endif ! Test water conservation call planetwide_sumval(massarea(:,:)*zdqrain(:,:,igcm_h2o_vap)*ptimestep/totarea_planet+ & massarea(:,:)*zdqrain(:,:,igcm_h2o_ice)*ptimestep/totarea_planet,dWtot) call planetwide_sumval((zdqsrain(:)+zdqssnow(:))*area(:)*ptimestep/totarea_planet,dWtots) if (is_master) then print*,'In rain atmospheric water change =',dWtot,' kg m-2' print*,'In rain surface water change =',dWtots,' kg m-2' print*,'In rain non-cons factor =',dWtot+dWtots,' kg m-2' endif endif ! end of 'enertest' end if ! enf of 'waterrain' end if ! end of 'water' ! ------------------------- ! VI.2. Aerosol particles ! ------------------------- ! Sedimentation. if (sedimentation) then zdqsed(1:ngrid,1:nlayer,1:nq) = 0.0 zdqssed(1:ngrid,1:nq) = 0.0 if(watertest)then iq=igcm_h2o_ice call planetwide_sumval(massarea(:,:)*pq(:,:,iq)*ptimestep/totarea_planet,dWtot) call planetwide_sumval(massarea(:,:)*pdq(:,:,iq)*ptimestep/totarea_planet,dWtots) if (is_master) then print*,'Before sedim pq =',dWtot,' kg m-2' print*,'Before sedim pdq =',dWtots,' kg m-2' endif endif call callsedim(ngrid,nlayer,ptimestep, & pplev,zzlev,pt,pdt,pq,pdq, & zdqsed,zdqssed,nq) if(watertest)then iq=igcm_h2o_ice call planetwide_sumval(massarea(:,:)*pq(:,:,iq)*ptimestep/totarea_planet,dWtot) call planetwide_sumval(massarea(:,:)*pdq(:,:,iq)*ptimestep/totarea_planet,dWtots) if (is_master) then print*,'After sedim pq =',dWtot,' kg m-2' print*,'After sedim pdq =',dWtots,' kg m-2' endif endif ! Whether it falls as rain or snow depends only on the surface temperature pdq(1:ngrid,1:nlayer,1:nq) = pdq(1:ngrid,1:nlayer,1:nq) + zdqsed(1:ngrid,1:nlayer,1:nq) dqsurf(1:ngrid,1:nq) = dqsurf(1:ngrid,1:nq) + zdqssed(1:ngrid,1:nq) ! Test water conservation if(watertest)then call planetwide_sumval(massarea(:,:)*(zdqsed(:,:,igcm_h2o_vap)+zdqsed(:,:,igcm_h2o_ice))*ptimestep/totarea_planet,dWtot) call planetwide_sumval((zdqssed(:,igcm_h2o_vap)+zdqssed(:,igcm_h2o_ice))*area(:)*ptimestep/totarea_planet,dWtots) if (is_master) then print*,'In sedim atmospheric ice change =',dWtot,' kg m-2' print*,'In sedim surface ice change =',dWtots,' kg m-2' print*,'In sedim non-cons factor =',dWtot+dWtots,' kg m-2' endif endif end if ! end of 'sedimentation' ! --------------- ! VI.3. Updates ! --------------- ! Updating Atmospheric Mass and Tracers budgets. if(mass_redistrib) then zdmassmr(1:ngrid,1:nlayer) = mass(1:ngrid,1:nlayer) * & ( zdqevap(1:ngrid,1:nlayer) & + zdqrain(1:ngrid,1:nlayer,igcm_h2o_vap) & + dqmoist(1:ngrid,1:nlayer,igcm_h2o_vap) & + dqvaplscale(1:ngrid,1:nlayer) ) do ig = 1, ngrid zdmassmr_col(ig)=SUM(zdmassmr(ig,1:nlayer)) enddo call writediagfi(ngrid,"mass_evap","mass gain"," ",3,zdmassmr) call writediagfi(ngrid,"mass_evap_col","mass gain col"," ",2,zdmassmr_col) call writediagfi(ngrid,"mass","mass","kg/m2",3,mass) call mass_redistribution(ngrid,nlayer,nq,ptimestep, & rnat,capcal,pplay,pplev,pt,tsurf,pq,qsurf, & pu,pv,pdt,zdtsurf,pdq,pdu,pdv,zdmassmr, & zdtmr,zdtsurfmr,zdpsrfmr,zdumr,zdvmr,zdqmr,zdqsurfmr) pdq(1:ngrid,1:nlayer,1:nq) = pdq(1:ngrid,1:nlayer,1:nq) + zdqmr(1:ngrid,1:nlayer,1:nq) dqsurf(1:ngrid,1:nq) = dqsurf(1:ngrid,1:nq) + zdqsurfmr(1:ngrid,1:nq) pdt(1:ngrid,1:nlayer) = pdt(1:ngrid,1:nlayer) + zdtmr(1:ngrid,1:nlayer) pdu(1:ngrid,1:nlayer) = pdu(1:ngrid,1:nlayer) + zdumr(1:ngrid,1:nlayer) pdv(1:ngrid,1:nlayer) = pdv(1:ngrid,1:nlayer) + zdvmr(1:ngrid,1:nlayer) pdpsrf(1:ngrid) = pdpsrf(1:ngrid) + zdpsrfmr(1:ngrid) zdtsurf(1:ngrid) = zdtsurf(1:ngrid) + zdtsurfmr(1:ngrid) endif ! ------------------ ! VI.4. Slab Ocean ! ------------------ if (ok_slab_ocean)then do ig=1,ngrid qsurfint(:,igcm_h2o_ice)=qsurf(:,igcm_h2o_ice) enddo call ocean_slab_ice(ptimestep, & ngrid, knindex, tsea_ice, fluxrad, & zdqssnow, qsurf(:,igcm_h2o_ice), & - zdqsdif(:,igcm_h2o_vap), & flux_sens_lat,tsea_ice, pctsrf_sic, & taux,tauy,icount) call ocean_slab_get_vars(ngrid,tslab, & sea_ice, flux_o, & flux_g, dt_hdiff, & dt_ekman) do ig=1,ngrid if (nint(rnat(ig)).eq.1)then tslab(ig,1) = 0. tslab(ig,2) = 0. tsea_ice(ig) = 0. sea_ice(ig) = 0. pctsrf_sic(ig) = 0. qsurf(ig,igcm_h2o_ice) = qsurfint(ig,igcm_h2o_ice) endif enddo endif ! end of 'ok_slab_ocean' ! ----------------------------- ! VI.5. Surface Tracer Update ! ----------------------------- if(hydrology)then call hydrol(ngrid,nq,ptimestep,rnat,tsurf,qsurf,dqsurf,dqs_hyd, & capcal,albedo0,albedo,mu0,zdtsurf,zdtsurf_hyd,hice,pctsrf_sic, & sea_ice) zdtsurf(1:ngrid) = zdtsurf(1:ngrid) + zdtsurf_hyd(1:ngrid) qsurf(1:ngrid,1:nq) = qsurf(1:ngrid,1:nq) + ptimestep*dqs_hyd(1:ngrid,1:nq) ! Test energy conservation if(enertest)then call planetwide_sumval(area(:)*capcal(:)*zdtsurf_hyd(:)/totarea_planet,dEtots) if (is_master) print*,'In hydrol surface energy change =',dEtots,' W m-2' endif ! test water conservation if(watertest)then call planetwide_sumval(dqs_hyd(:,igcm_h2o_ice)*area(:)*ptimestep/totarea_planet,dWtots) if (is_master) print*,'In hydrol surface ice change =',dWtots,' kg m-2' call planetwide_sumval(dqs_hyd(:,igcm_h2o_vap)*area(:)*ptimestep/totarea_planet,dWtots) if (is_master) then print*,'In hydrol surface water change =',dWtots,' kg m-2' print*,'---------------------------------------------------------------' endif endif else ! of if (hydrology) qsurf(1:ngrid,1:nq)=qsurf(1:ngrid,1:nq)+ptimestep*dqsurf(1:ngrid,1:nq) end if ! of if (hydrology) ! Add qsurf to qsurf_hist, which is what we save in diagfi.nc. At the same time, we set the water ! content of ocean gridpoints back to zero, in order to avoid rounding errors in vdifc, rain. qsurf_hist(:,:) = qsurf(:,:) if(ice_update)then ice_min(1:ngrid)=min(ice_min(1:ngrid),qsurf(1:ngrid,igcm_h2o_ice)) endif endif! end of if 'tracer' !------------------------------------------------ ! VII. Surface and sub-surface soil temperature !------------------------------------------------ ! Increment surface temperature if(ok_slab_ocean)then do ig=1,ngrid if (nint(rnat(ig)).eq.0)then zdtsurf(ig)= (tslab(ig,1) & + pctsrf_sic(ig)*(tsea_ice(ig)-tslab(ig,1))-tsurf(ig))/ptimestep endif tsurf(ig)=tsurf(ig)+ptimestep*zdtsurf(ig) enddo else tsurf(1:ngrid)=tsurf(1:ngrid)+ptimestep*zdtsurf(1:ngrid) endif ! end of 'ok_slab_ocean' ! Compute soil temperatures and subsurface heat flux. if (callsoil) then call soil(ngrid,nsoilmx,.false.,lastcall,inertiedat, & ptimestep,tsurf,tsoil,capcal,fluxgrd) endif if (ok_slab_ocean) then do ig=1,ngrid fluxgrdocean(ig)=fluxgrd(ig) if (nint(rnat(ig)).eq.0) then capcal(ig)=capcalocean fluxgrd(ig)=0. fluxgrdocean(ig)=pctsrf_sic(ig)*flux_g(ig)+(1-pctsrf_sic(ig))*(dt_hdiff(ig,1)+dt_ekman(ig,1)) do iq=1,nsoilmx tsoil(ig,iq)=tsurf(ig) enddo if (pctsrf_sic(ig).gt.0.5) then capcal(ig)=capcalseaice if (qsurf(ig,igcm_h2o_ice).gt.0.) then capcal(ig)=capcalsno endif endif endif enddo endif !end of 'ok_slab_ocean' ! Test energy conservation if(enertest)then call planetwide_sumval(area(:)*capcal(:)*zdtsurf(:)/totarea_planet,dEtots) if (is_master) print*,'Surface energy change =',dEtots,' W m-2' endif !--------------------------------------------------- ! VIII. Perform diagnostics and write output files !--------------------------------------------------- ! Note : For output only: the actual model integration is performed in the dynamics. ! Temperature, zonal and meridional winds. zt(1:ngrid,1:nlayer) = pt(1:ngrid,1:nlayer) + pdt(1:ngrid,1:nlayer)*ptimestep zu(1:ngrid,1:nlayer) = pu(1:ngrid,1:nlayer) + pdu(1:ngrid,1:nlayer)*ptimestep zv(1:ngrid,1:nlayer) = pv(1:ngrid,1:nlayer) + pdv(1:ngrid,1:nlayer)*ptimestep ! Diagnostic. zdtdyn(1:ngrid,1:nlayer) = pt(1:ngrid,1:nlayer)-ztprevious(1:ngrid,1:nlayer) ztprevious(1:ngrid,1:nlayer) = zt(1:ngrid,1:nlayer) if(firstcall)then zdtdyn(1:ngrid,1:nlayer)=0.0 endif ! Dynamical heating diagnostic. do ig=1,ngrid fluxdyn(ig)= SUM(zdtdyn(ig,:) *mass(ig,:))*cpp/ptimestep enddo ! Tracers. zq(1:ngrid,1:nlayer,1:nq) = pq(1:ngrid,1:nlayer,1:nq) + pdq(1:ngrid,1:nlayer,1:nq)*ptimestep ! Surface pressure. ps(1:ngrid) = pplev(1:ngrid,1) + pdpsrf(1:ngrid)*ptimestep ! Surface and soil temperature information call planetwide_sumval(area(:)*tsurf(:)/totarea_planet,Ts1) call planetwide_minval(tsurf(:),Ts2) call planetwide_maxval(tsurf(:),Ts3) if(callsoil)then TsS = SUM(area(:)*tsoil(:,nsoilmx))/totarea ! mean temperature at bottom soil layer print*,' ave[Tsurf] min[Tsurf] max[Tsurf] ave[Tdeep]' print*,Ts1,Ts2,Ts3,TsS else if (is_master) then print*,' ave[Tsurf] min[Tsurf] max[Tsurf]' print*,Ts1,Ts2,Ts3 endif end if ! Check the energy balance of the simulation during the run if(corrk)then call planetwide_sumval(area(:)*fluxtop_dn(:)/totarea_planet,ISR) call planetwide_sumval(area(:)*fluxabs_sw(:)/totarea_planet,ASR) call planetwide_sumval(area(:)*fluxtop_lw(:)/totarea_planet,OLR) call planetwide_sumval(area(:)*fluxgrd(:)/totarea_planet,GND) call planetwide_sumval(area(:)*fluxdyn(:)/totarea_planet,DYN) do ig=1,ngrid if(fluxtop_dn(ig).lt.0.0)then print*,'fluxtop_dn has gone crazy' print*,'fluxtop_dn=',fluxtop_dn(ig) print*,'tau_col=',tau_col(ig) print*,'aerosol=',aerosol(ig,:,:) print*,'temp= ',pt(ig,:) print*,'pplay= ',pplay(ig,:) call abort endif end do if(ngrid.eq.1)then DYN=0.0 endif if (is_master) then print*,' ISR ASR OLR GND DYN [W m^-2]' print*, ISR,ASR,OLR,GND,DYN endif if(enertest .and. is_master)then print*,'SW flux/heating difference SW++ - ASR = ',dEtotSW+dEtotsSW-ASR,' W m-2' print*,'LW flux/heating difference LW++ - OLR = ',dEtotLW+dEtotsLW+OLR,' W m-2' print*,'LW energy balance LW++ + ASR = ',dEtotLW+dEtotsLW+ASR,' W m-2' endif if(meanOLR .and. is_master)then if((ngrid.gt.1) .or. (mod(icount-1,ecritphy).eq.0))then ! to record global radiative balance open(92,file="rad_bal.out",form='formatted',position='append') write(92,*) zday,ISR,ASR,OLR close(92) open(93,file="tem_bal.out",form='formatted',position='append') if(callsoil)then write(93,*) zday,Ts1,Ts2,Ts3,TsS else write(93,*) zday,Ts1,Ts2,Ts3 endif close(93) endif endif endif ! end of 'corrk' ! Diagnostic to test radiative-convective timescales in code. if(testradtimes)then open(38,file="tau_phys.out",form='formatted',position='append') ig=1 do l=1,nlayer write(38,*) -1./pdt(ig,l),pt(ig,l),pplay(ig,l) enddo close(38) print*,'As testradtimes enabled,' print*,'exiting physics on first call' call abort endif ! Compute column amounts (kg m-2) if tracers are enabled. if(tracer)then qcol(1:ngrid,1:nq)=0.0 do iq=1,nq do ig=1,ngrid qcol(ig,iq) = SUM( zq(ig,1:nlayer,iq) * mass(ig,1:nlayer)) enddo enddo ! Generalised for arbitrary aerosols now. By LK reffcol(1:ngrid,1:naerkind)=0.0 if(co2cond.and.(iaero_co2.ne.0))then call co2_reffrad(ngrid,nlayer,nq,zq,reffrad(1,1,iaero_co2)) do ig=1,ngrid reffcol(ig,iaero_co2) = SUM(zq(ig,1:nlayer,igcm_co2_ice)*reffrad(ig,1:nlayer,iaero_co2)*mass(ig,1:nlayer)) enddo endif if(water.and.(iaero_h2o.ne.0))then call h2o_reffrad(ngrid,nlayer,zq(1,1,igcm_h2o_ice),zt, & reffrad(1,1,iaero_h2o),nueffrad(1,1,iaero_h2o)) do ig=1,ngrid reffcol(ig,iaero_h2o) = SUM(zq(ig,1:nlayer,igcm_h2o_ice)*reffrad(ig,1:nlayer,iaero_h2o)*mass(ig,1:nlayer)) enddo endif endif ! end of 'tracer' ! Test for water conservation. if(water)then call planetwide_sumval(area(:)*qsurf_hist(:,igcm_h2o_ice)/totarea_planet,icesrf) call planetwide_sumval(area(:)*qsurf_hist(:,igcm_h2o_vap)/totarea_planet,liqsrf) call planetwide_sumval(area(:)*qcol(:,igcm_h2o_ice)/totarea_planet,icecol) call planetwide_sumval(area(:)*qcol(:,igcm_h2o_vap)/totarea_planet,vapcol) h2otot = icesrf + liqsrf + icecol + vapcol if (is_master) then print*,' Total water amount [kg m^-2]: ',h2otot print*,' Surface ice Surface liq. Atmos. con. Atmos. vap. [kg m^-2] ' print*, icesrf,liqsrf,icecol,vapcol endif if(meanOLR .and. is_master)then if((ngrid.gt.1) .or. (mod(icount-1,ecritphy).eq.0))then ! to record global water balance open(98,file="h2o_bal.out",form='formatted',position='append') write(98,*) zday,icesrf,liqsrf,icecol,vapcol close(98) endif endif endif ! Calculate RH (Relative Humidity) for diagnostic. if(water)then do l = 1, nlayer do ig=1,ngrid call Psat_water(zt(ig,l),pplay(ig,l),psat_tmp,qsat(ig,l)) RH(ig,l) = zq(ig,l,igcm_h2o_vap) / qsat(ig,l) enddo enddo ! Compute maximum possible H2O column amount (100% saturation). do ig=1,ngrid H2Omaxcol(ig) = SUM( qsat(ig,:) * mass(ig,:)) enddo endif ! end of 'water' print*,'--> Ls =',zls*180./pi !---------------------------------------------------------------------- ! Writing NetCDF file "RESTARTFI" at the end of the run !---------------------------------------------------------------------- ! Note: 'restartfi' is stored just before dynamics are stored ! in 'restart'. Between now and the writting of 'restart', ! there will have been the itau=itau+1 instruction and ! a reset of 'time' (lastacll = .true. when itau+1= itaufin) ! thus we store for time=time+dtvr if(lastcall) then ztime_fin = ptime + ptimestep/(float(iphysiq)*daysec) ! Update surface ice distribution to iterate to steady state if requested if(ice_update)then do ig=1,ngrid delta_ice = (qsurf(ig,igcm_h2o_ice)-ice_initial(ig)) ! add multiple years of evolution qsurf_hist(ig,igcm_h2o_ice) = qsurf_hist(ig,igcm_h2o_ice) + delta_ice*icetstep ! if ice has gone -ve, set to zero if(qsurf_hist(ig,igcm_h2o_ice).lt.0.0)then qsurf_hist(ig,igcm_h2o_ice) = 0.0 endif ! if ice is seasonal, set to zero (NEW) if(ice_min(ig).lt.0.01)then qsurf_hist(ig,igcm_h2o_ice) = 0.0 endif enddo ! enforce ice conservation ice_tot= SUM(qsurf_hist(:,igcm_h2o_ice)*area(:) ) qsurf_hist(:,igcm_h2o_ice) = qsurf_hist(:,igcm_h2o_ice)*(icesrf/ice_tot) endif if (ngrid.ne.1) then write(*,*)'PHYSIQ: for physdem ztime_fin =',ztime_fin call physdem1("restartfi.nc",nsoilmx,ngrid,nlayer,nq, & ptimestep,ztime_fin, & tsurf,tsoil,emis,q2,qsurf_hist, & cloudfrac,totcloudfrac,hice, & rnat,pctsrf_sic,tslab,tsea_ice,sea_ice) endif if(ok_slab_ocean) then call ocean_slab_final!(tslab, seaice) end if endif ! end of 'lastcall' !----------------------------------- ! Saving statistics : !----------------------------------- ! Note :("stats" stores and accumulates 8 key variables in file "stats.nc" ! which can later be used to make the statistic files of the run: ! "stats") only possible in 3D runs !!! if (callstats) then call wstats(ngrid,"ps","Surface pressure","Pa",2,ps) call wstats(ngrid,"tsurf","Surface temperature","K",2,tsurf) call wstats(ngrid,"fluxsurf_lw", & "Thermal IR radiative flux to surface","W.m-2",2, & fluxsurf_lw) call wstats(ngrid,"fluxtop_lw", & "Thermal IR radiative flux to space","W.m-2",2, & fluxtop_lw) ! call wstats(ngrid,"fluxsurf_sw", & ! "Solar radiative flux to surface","W.m-2",2, & ! fluxsurf_sw_tot) ! call wstats(ngrid,"fluxtop_sw", & ! "Solar radiative flux to space","W.m-2",2, & ! fluxtop_sw_tot) call wstats(ngrid,"ISR","incoming stellar rad.","W m-2",2,fluxtop_dn) call wstats(ngrid,"ASR","absorbed stellar rad.","W m-2",2,fluxabs_sw) call wstats(ngrid,"OLR","outgoing longwave rad.","W m-2",2,fluxtop_lw) call wstats(ngrid,"ALB","Surface albedo"," ",2,albedo) call wstats(ngrid,"p","Pressure","Pa",3,pplay) call wstats(ngrid,"temp","Atmospheric temperature","K",3,zt) call wstats(ngrid,"u","Zonal (East-West) wind","m.s-1",3,zu) call wstats(ngrid,"v","Meridional (North-South) wind","m.s-1",3,zv) call wstats(ngrid,"w","Vertical (down-up) wind","m.s-1",3,pw) call wstats(ngrid,"q2","Boundary layer eddy kinetic energy","m2.s-2",3,q2) if (tracer) then do iq=1,nq call wstats(ngrid,noms(iq),noms(iq),'kg/kg',3,zq(1,1,iq)) call wstats(ngrid,trim(noms(iq))//'_surf',trim(noms(iq))//'_surf', & 'kg m^-2',2,qsurf(1,iq) ) call wstats(ngrid,trim(noms(iq))//'_col',trim(noms(iq))//'_col', & 'kg m^-2',2,qcol(1,iq) ) ! call wstats(ngrid,trim(noms(iq))//'_reff', & ! trim(noms(iq))//'_reff', & ! 'm',3,reffrad(1,1,iq)) end do if (water) then vmr=zq(1:ngrid,1:nlayer,igcm_h2o_vap)*mugaz/mmol(igcm_h2o_vap) call wstats(ngrid,"vmr_h2ovapor", & "H2O vapour volume mixing ratio","mol/mol", & 3,vmr) endif endif ! end of 'tracer' if(watercond.and.CLFvarying)then call wstats(ngrid,"rneb_man","H2O cloud fraction (conv)"," ",3,rneb_man) call wstats(ngrid,"rneb_lsc","H2O cloud fraction (large scale)"," ",3,rneb_lsc) call wstats(ngrid,"CLF","H2O cloud fraction"," ",3,cloudfrac) call wstats(ngrid,"CLFt","H2O column cloud fraction"," ",2,totcloudfrac) call wstats(ngrid,"RH","relative humidity"," ",3,RH) endif if (ok_slab_ocean) then call wstats(ngrid,"dt_hdiff1","dt_hdiff1","K/s",2,dt_hdiff(:,1)) call wstats(ngrid,"dt_hdiff2","dt_hdiff2","K/s",2,dt_hdiff(:,2)) call wstats(ngrid,"dt_ekman1","dt_ekman1","K/s",2,dt_ekman(:,1)) call wstats(ngrid,"dt_ekman2","dt_ekman2","K/s",2,dt_ekman(:,2)) call wstats(ngrid,"tslab1","tslab1","K",2,tslab(:,1)) call wstats(ngrid,"tslab2","tslab2","K",2,tslab(:,2)) call wstats(ngrid,"pctsrf_sic","pct ice/sea","",2,pctsrf_sic) call wstats(ngrid,"tsea_ice","tsea_ice","K",2,tsea_ice) call wstats(ngrid,"sea_ice","sea ice","kg/m2",2,sea_ice) call wstats(ngrid,"rnat","nature of the surface","",2,rnat) endif if(lastcall) then write (*,*) "Writing stats..." call mkstats(ierr) endif endif ! end of 'callstats' !----------------------------------------------------------------------------------------------------- ! OUTPUT in netcdf file "DIAGFI.NC", containing any variable for diagnostic ! ! Note 1 : output with period "ecritphy", set in "run.def" ! ! Note 2 : writediagfi can also be called from any other subroutine for any variable, ! but its preferable to keep all the calls in one place ... !----------------------------------------------------------------------------------------------------- call writediagfi(ngrid,"Ls","solar longitude","deg",0,zls*180./pi) call writediagfi(ngrid,"Lss","sub solar longitude","deg",0,zlss*180./pi) call writediagfi(ngrid,"RA","right ascension","deg",0,right_ascen*180./pi) call writediagfi(ngrid,"Declin","solar declination","deg",0,declin*180./pi) call writediagfi(ngrid,"tsurf","Surface temperature","K",2,tsurf) call writediagfi(ngrid,"ps","Surface pressure","Pa",2,ps) call writediagfi(ngrid,"temp","temperature","K",3,zt) call writediagfi(ngrid,"teta","potential temperature","K",3,zh) call writediagfi(ngrid,"u","Zonal wind","m.s-1",3,zu) call writediagfi(ngrid,"v","Meridional wind","m.s-1",3,zv) call writediagfi(ngrid,"w","Vertical wind","m.s-1",3,pw) call writediagfi(ngrid,"p","Pressure","Pa",3,pplay) ! Subsurface temperatures ! call writediagsoil(ngrid,"tsurf","Surface temperature","K",2,tsurf) ! call writediagsoil(ngrid,"temp","temperature","K",3,tsoil) ! Oceanic layers if(ok_slab_ocean) then call writediagfi(ngrid,"pctsrf_sic","pct ice/sea","",2,pctsrf_sic) call writediagfi(ngrid,"tsea_ice","tsea_ice","K",2,tsea_ice) call writediagfi(ngrid,"sea_ice","sea ice","kg/m2",2,sea_ice) call writediagfi(ngrid,"tslab1","tslab1","K",2,tslab(:,1)) call writediagfi(ngrid,"tslab2","tslab2","K",2,tslab(:,2)) call writediagfi(ngrid,"dt_hdiff1","dt_hdiff1","K/s",2,dt_hdiff(:,1)) call writediagfi(ngrid,"dt_hdiff2","dt_hdiff2","K/s",2,dt_hdiff(:,2)) call writediagfi(ngrid,"dt_ekman1","dt_ekman1","K/s",2,dt_ekman(:,1)) call writediagfi(ngrid,"dt_ekman2","dt_ekman2","K/s",2,dt_ekman(:,2)) call writediagfi(ngrid,"rnat","nature of the surface","",2,rnat) call writediagfi(ngrid,"sensibFlux","sensible heat flux","w.m^-2",2,sensibFlux) call writediagfi(ngrid,"latentFlux","latent heat flux","w.m^-2",2,zdqsdif(:,igcm_h2o_vap)*RLVTT) endif ! Total energy balance diagnostics if(callrad.and.(.not.newtonian))then call writediagfi(ngrid,"ALB","Surface albedo"," ",2,albedo) call writediagfi(ngrid,"ISR","incoming stellar rad.","W m-2",2,fluxtop_dn) call writediagfi(ngrid,"ASR","absorbed stellar rad.","W m-2",2,fluxabs_sw) call writediagfi(ngrid,"OLR","outgoing longwave rad.","W m-2",2,fluxtop_lw) call writediagfi(ngrid,"shad","rings"," ", 2, fract) ! call writediagfi(ngrid,"ASRcs","absorbed stellar rad (cs).","W m-2",2,fluxabs_sw1) ! call writediagfi(ngrid,"OLRcs","outgoing longwave rad (cs).","W m-2",2,fluxtop_lw1) ! call writediagfi(ngrid,"fluxsurfsw","sw surface flux.","W m-2",2,fluxsurf_sw) ! call writediagfi(ngrid,"fluxsurflw","lw back radiation.","W m-2",2,fluxsurf_lw) ! call writediagfi(ngrid,"fluxsurfswcs","sw surface flux (cs).","W m-2",2,fluxsurf_sw1) ! call writediagfi(ngrid,"fluxsurflwcs","lw back radiation (cs).","W m-2",2,fluxsurf_lw1) if(ok_slab_ocean) then call writediagfi(ngrid,"GND","heat flux from ground","W m-2",2,fluxgrdocean) else call writediagfi(ngrid,"GND","heat flux from ground","W m-2",2,fluxgrd) endif call writediagfi(ngrid,"DYN","dynamical heat input","W m-2",2,fluxdyn) endif ! end of 'callrad' if(enertest) then if (calldifv) then call writediagfi(ngrid,"q2","turbulent kinetic energy","J.kg^-1",3,q2) call writediagfi(ngrid,"sensibFlux","sensible heat flux","w.m^-2",2,sensibFlux) ! call writediagfi(ngrid,"dEzdiff","turbulent diffusion heating (-sensible flux)","w.m^-2",3,dEzdiff) ! call writediagfi(ngrid,"dEdiff","integrated turbulent diffusion heating (-sensible flux)","w.m^-2",2,dEdiff) ! call writediagfi(ngrid,"dEdiffs","In TurbDiff (correc rad+latent heat) surf nrj change","w.m^-2",2,dEdiffs) endif if (corrk) then call writediagfi(ngrid,"dEzradsw","radiative heating","w.m^-2",3,dEzradsw) call writediagfi(ngrid,"dEzradlw","radiative heating","w.m^-2",3,dEzradlw) endif if(watercond) then call writediagfi(ngrid,"lscaledE","heat from largescale","W m-2",2,lscaledE) call writediagfi(ngrid,"madjdE","heat from moistadj","W m-2",2,madjdE) call writediagfi(ngrid,"qsatatm","atm qsat"," ",3,qsat) ! call writediagfi(ngrid,"lscaledEz","heat from largescale","W m-2",3,lscaledEz) ! call writediagfi(ngrid,"madjdEz","heat from moistadj","W m-2",3,madjdEz) ! call writediagfi(ngrid,"h2o_max_col","maximum H2O column amount","kg.m^-2",2,H2Omaxcol) endif endif ! end of 'enertest' ! Temporary inclusions for heating diagnostics. !call writediagfi(ngrid,"zdtsw","SW heating","T s-1",3,zdtsw) !call writediagfi(ngrid,"zdtlw","LW heating","T s-1",3,zdtlw) !call writediagfi(ngrid,"dtrad","radiative heating","K s-1",3,dtrad) ! call writediagfi(ngrid,"zdtdyn","Dyn. heating","T s-1",3,zdtdyn) ! For Debugging. !call writediagfi(ngrid,'rnat','Terrain type',' ',2,real(rnat)) !call writediagfi(ngrid,'pphi','Geopotential',' ',3,pphi) ! Output aerosols. if (igcm_co2_ice.ne.0.and.iaero_co2.ne.0) & call writediagfi(ngrid,'CO2ice_reff','CO2ice_reff','m',3,reffrad(1,1,iaero_co2)) if (igcm_h2o_ice.ne.0.and.iaero_h2o.ne.0) & call writediagfi(ngrid,'H2Oice_reff','H2Oice_reff','m',3,reffrad(:,:,iaero_h2o)) if (igcm_co2_ice.ne.0.and.iaero_co2.ne.0) & call writediagfi(ngrid,'CO2ice_reffcol','CO2ice_reffcol','um kg m^-2',2,reffcol(1,iaero_co2)) if (igcm_h2o_ice.ne.0.and.iaero_h2o.ne.0) & call writediagfi(ngrid,'H2Oice_reffcol','H2Oice_reffcol','um kg m^-2',2,reffcol(1,iaero_h2o)) ! Output tracers. if (tracer) then do iq=1,nq call writediagfi(ngrid,noms(iq),noms(iq),'kg/kg',3,zq(1,1,iq)) call writediagfi(ngrid,trim(noms(iq))//'_surf',trim(noms(iq))//'_surf', & 'kg m^-2',2,qsurf_hist(1,iq) ) call writediagfi(ngrid,trim(noms(iq))//'_col',trim(noms(iq))//'_col', & 'kg m^-2',2,qcol(1,iq) ) ! call writediagfi(ngrid,trim(noms(iq))//'_surf',trim(noms(iq))//'_surf', & ! 'kg m^-2',2,qsurf(1,iq) ) if(watercond.or.CLFvarying)then call writediagfi(ngrid,"rneb_man","H2O cloud fraction (conv)"," ",3,rneb_man) call writediagfi(ngrid,"rneb_lsc","H2O cloud fraction (large scale)"," ",3,rneb_lsc) call writediagfi(ngrid,"CLF","H2O cloud fraction"," ",3,cloudfrac) call writediagfi(ngrid,"CLFt","H2O column cloud fraction"," ",2,totcloudfrac) call writediagfi(ngrid,"RH","relative humidity"," ",3,RH) endif if(waterrain)then call writediagfi(ngrid,"rain","rainfall","kg m-2 s-1",2,zdqsrain) call writediagfi(ngrid,"snow","snowfall","kg m-2 s-1",2,zdqssnow) endif if((hydrology).and.(.not.ok_slab_ocean))then call writediagfi(ngrid,"hice","oceanic ice height","m",2,hice) endif if(ice_update)then call writediagfi(ngrid,"ice_min","min annual ice","m",2,ice_min) call writediagfi(ngrid,"ice_ini","initial annual ice","m",2,ice_initial) endif do ig=1,ngrid if(tau_col(ig).gt.1.e3)then print*,'WARNING: tau_col=',tau_col(ig) print*,'at ig=',ig,'in PHYSIQ' endif end do call writediagfi(ngrid,"tau_col","Total aerosol optical depth","[]",2,tau_col) enddo ! end of 'nq' loop endif ! end of 'tracer' ! Output spectrum. if(specOLR.and.corrk)then call writediagspecIR(ngrid,"OLR3D","OLR(lon,lat,band)","W/m^2/cm^-1",3,OLR_nu) call writediagspecVI(ngrid,"OSR3D","OSR(lon,lat,band)","W/m^2/cm^-1",3,OSR_nu) endif icount=icount+1 end subroutine physiq