| 1 | subroutine callcorrk(ngrid,nlayer,pq,nq,qsurf, & |
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| 2 | albedo,albedo_equivalent,emis,mu0,pplev,pplay,pt, & |
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| 3 | tsurf,fract,dist_star,aerosol,muvar, & |
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| 4 | dtlw,dtsw,fluxsurf_lw, & |
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| 5 | fluxsurf_sw,fluxsurfabs_sw,fluxtop_lw, & |
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| 6 | fluxabs_sw,fluxtop_dn, & |
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| 7 | OLR_nu,OSR_nu, & |
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| 8 | tau_col,cloudfrac,totcloudfrac, & |
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| 9 | clearsky,firstcall,lastcall) |
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| 10 | |
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| 11 | use radinc_h |
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| 12 | use radcommon_h |
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| 13 | use watercommon_h |
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| 14 | use datafile_mod, only: datadir |
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| 15 | ! use ioipsl_getincom |
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| 16 | use ioipsl_getincom_p |
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| 17 | use gases_h |
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| 18 | use radii_mod, only : su_aer_radii,co2_reffrad,h2o_reffrad,dust_reffrad,h2so4_reffrad,back2lay_reffrad |
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| 19 | use aerosol_mod, only : iaero_co2,iaero_h2o,iaero_dust,iaero_h2so4, iaero_back2lay |
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| 20 | USE tracer_h |
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| 21 | use comcstfi_mod, only: pi, mugaz, cpp |
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| 22 | use callkeys_mod, only: varactive,diurnal,tracer,water,nosurf,varfixed,satval, & |
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| 23 | kastprof,strictboundcorrk,specOLR,CLFvarying |
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| 24 | |
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| 25 | implicit none |
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| 26 | |
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| 27 | !================================================================== |
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| 28 | ! |
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| 29 | ! Purpose |
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| 30 | ! ------- |
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| 31 | ! Solve the radiative transfer using the correlated-k method for |
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| 32 | ! the gaseous absorption and the Toon et al. (1989) method for |
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| 33 | ! scatttering due to aerosols. |
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| 34 | ! |
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| 35 | ! Authors |
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| 36 | ! ------- |
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| 37 | ! Emmanuel 01/2001, Forget 09/2001 |
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| 38 | ! Robin Wordsworth (2009) |
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| 39 | ! |
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| 40 | !================================================================== |
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| 41 | |
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| 42 | !----------------------------------------------------------------------- |
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| 43 | ! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid |
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| 44 | ! Layer #1 is the layer near the ground. |
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| 45 | ! Layer #nlayer is the layer at the top. |
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| 46 | |
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| 47 | INTEGER,INTENT(IN) :: ngrid ! number of atmospheric columns |
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| 48 | INTEGER,INTENT(IN) :: nlayer ! number of atmospheric layers |
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| 49 | REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! tracers (.../kg_of_air) |
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| 50 | integer,intent(in) :: nq ! number of tracers |
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| 51 | REAL,INTENT(IN) :: qsurf(ngrid,nq) ! tracer on surface (kg.m-2) |
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| 52 | REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral SW albedo.MT2015. |
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| 53 | REAL,INTENT(IN) :: emis(ngrid) ! LW emissivity |
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| 54 | real,intent(in) :: mu0(ngrid) ! cosine of sun incident angle |
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| 55 | REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! inter-layer pressure (Pa) |
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| 56 | REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! mid-layer pressure (Pa) |
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| 57 | REAL,INTENT(IN) :: pt(ngrid,nlayer) ! air temperature (K) |
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| 58 | REAL,INTENT(IN) :: tsurf(ngrid) ! surface temperature (K) |
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| 59 | REAL,INTENT(IN) :: fract(ngrid) ! fraction of day |
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| 60 | REAL,INTENT(IN) :: dist_star ! distance star-planet (AU) |
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| 61 | REAL,INTENT(OUT) :: aerosol(ngrid,nlayer,naerkind) ! aerosol tau (kg/kg) |
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| 62 | real,intent(in) :: muvar(ngrid,nlayer+1) |
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| 63 | REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! heating rate (K/s) due to LW |
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| 64 | REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! heating rate (K/s) due to SW |
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| 65 | REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! incident LW flux to surf (W/m2) |
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| 66 | REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! incident SW flux to surf (W/m2) |
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| 67 | REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! absorbed SW flux by the surface (W/m2). By MT2015. |
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| 68 | REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! outgoing LW flux to space (W/m2) |
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| 69 | REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by planet (W/m2) |
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| 70 | REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! incident top of atmosphere SW flux (W/m2) |
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| 71 | REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI)! Outgoing LW radition in each band (Normalized to the band width (W/m2/cm-1) |
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| 72 | REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV)! Outgoing SW radition in each band (Normalized to the band width (W/m2/cm-1) |
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| 73 | REAL,INTENT(OUT) :: tau_col(ngrid) ! diagnostic from aeropacity |
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| 74 | REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015 |
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| 75 | ! for H2O cloud fraction in aeropacity |
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| 76 | real,intent(in) :: cloudfrac(ngrid,nlayer) |
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| 77 | real,intent(out) :: totcloudfrac(ngrid) |
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| 78 | logical,intent(in) :: clearsky |
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| 79 | logical,intent(in) :: firstcall ! signals first call to physics |
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| 80 | logical,intent(in) :: lastcall ! signals last call to physics |
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| 81 | |
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| 82 | ! Globally varying aerosol optical properties on GCM grid |
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| 83 | ! Not needed everywhere so not in radcommon_h |
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| 84 | REAL :: QVISsQREF3d(ngrid,nlayer,L_NSPECTV,naerkind) |
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| 85 | REAL :: omegaVIS3d(ngrid,nlayer,L_NSPECTV,naerkind) |
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| 86 | REAL :: gVIS3d(ngrid,nlayer,L_NSPECTV,naerkind) |
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| 87 | |
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| 88 | REAL :: QIRsQREF3d(ngrid,nlayer,L_NSPECTI,naerkind) |
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| 89 | REAL :: omegaIR3d(ngrid,nlayer,L_NSPECTI,naerkind) |
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| 90 | REAL :: gIR3d(ngrid,nlayer,L_NSPECTI,naerkind) |
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| 91 | |
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| 92 | ! REAL :: omegaREFvis3d(ngrid,nlayer,naerkind) |
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| 93 | ! REAL :: omegaREFir3d(ngrid,nlayer,naerkind) ! not sure of the point of these... |
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| 94 | |
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| 95 | REAL,ALLOCATABLE,SAVE :: reffrad(:,:,:) ! aerosol effective radius (m) |
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| 96 | REAL,ALLOCATABLE,SAVE :: nueffrad(:,:,:) ! aerosol effective variance |
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| 97 | !$OMP THREADPRIVATE(reffrad,nueffrad) |
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| 98 | |
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| 99 | !----------------------------------------------------------------------- |
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| 100 | ! Declaration of the variables required by correlated-k subroutines |
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| 101 | ! Numbered from top to bottom unlike in the GCM! |
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| 102 | |
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| 103 | REAL*8 tmid(L_LEVELS),pmid(L_LEVELS) |
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| 104 | REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS) |
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| 105 | |
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| 106 | ! Optical values for the optci/cv subroutines |
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| 107 | REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV) |
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| 108 | REAL*8 dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 109 | REAL*8 dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 110 | REAL*8 cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 111 | REAL*8 cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 112 | REAL*8 wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 113 | REAL*8 wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 114 | REAL*8 tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS) |
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| 115 | REAL*8 taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS) |
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| 116 | REAL*8 taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS) |
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| 117 | |
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| 118 | REAL*8 tauaero(L_LEVELS+1,naerkind) |
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| 119 | REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn |
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| 120 | real*8 nfluxoutv_nu(L_NSPECTV) ! outgoing band-resolved VI flux at TOA (W/m2) |
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| 121 | real*8 nfluxtopi_nu(L_NSPECTI) ! net band-resolved IR flux at TOA (W/m2) |
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| 122 | real*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! for 1D diagnostic |
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| 123 | REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD) |
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| 124 | REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD) |
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| 125 | REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD) |
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| 126 | REAL*8 albi,acosz |
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| 127 | REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo. |
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| 128 | |
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| 129 | INTEGER ig,l,k,nw,iaer,irad |
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| 130 | INTEGER icount |
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| 131 | |
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| 132 | real szangle |
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| 133 | logical global1d |
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| 134 | save szangle,global1d |
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| 135 | !$OMP THREADPRIVATE(szangle,global1d) |
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| 136 | real*8 taugsurf(L_NSPECTV,L_NGAUSS-1) |
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| 137 | real*8 taugsurfi(L_NSPECTI,L_NGAUSS-1) |
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| 138 | |
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| 139 | real*8 qvar(L_LEVELS) ! mixing ratio of variable component (mol/mol) |
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| 140 | |
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| 141 | ! Local aerosol optical properties for each column on RADIATIVE grid |
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| 142 | real*8,save :: QXVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 143 | real*8,save :: QSVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 144 | real*8,save :: GVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 145 | real*8,save :: QXIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 146 | real*8,save :: QSIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 147 | real*8,save :: GIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 148 | |
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| 149 | !REAL :: QREFvis3d(ngrid,nlayer,naerkind) |
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| 150 | !REAL :: QREFir3d(ngrid,nlayer,naerkind) |
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| 151 | !save QREFvis3d, QREFir3d |
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| 152 | real, dimension(:,:,:), save, allocatable :: QREFvis3d |
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| 153 | real, dimension(:,:,:), save, allocatable :: QREFir3d |
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| 154 | !$OMP THREADPRIVATE(QXVAER,QSVAER,GVAER,QXIAER,QSIAER,GIAER,QREFvis3d,QREFir3d) |
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| 155 | |
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| 156 | |
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| 157 | ! Misc. |
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| 158 | logical nantest |
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| 159 | real*8 tempv(L_NSPECTV) |
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| 160 | real*8 tempi(L_NSPECTI) |
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| 161 | real*8 temp,temp1,temp2,pweight |
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| 162 | character(len=10) :: tmp1 |
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| 163 | character(len=10) :: tmp2 |
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| 164 | |
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| 165 | ! for fixed water vapour profiles |
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| 166 | integer i_var |
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| 167 | real RH |
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| 168 | real*8 pq_temp(nlayer) |
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| 169 | real ptemp, Ttemp, qsat |
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| 170 | |
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| 171 | ! real(KIND=r8) :: pq_temp(nlayer) ! better F90 way.. DOESNT PORT TO F77!!! |
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| 172 | |
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| 173 | !real ptime, pday |
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| 174 | logical OLRz |
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| 175 | real*8 NFLUXGNDV_nu(L_NSPECTV) |
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| 176 | |
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| 177 | |
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| 178 | ! for weird cloud test |
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| 179 | real pqtest(ngrid,nlayer,nq) |
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| 180 | |
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| 181 | real maxrad, minrad |
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| 182 | |
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| 183 | real,external :: CBRT |
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| 184 | |
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| 185 | ! included by RW for runaway greenhouse 1D study |
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| 186 | real vtmp(nlayer) |
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| 187 | REAL*8 muvarrad(L_LEVELS) |
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| 188 | |
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| 189 | ! included by MT for albedo calculations. |
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| 190 | REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation. |
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| 191 | |
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| 192 | !=============================================================== |
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| 193 | ! Initialization on first call |
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| 194 | |
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| 195 | qxvaer(:,:,:)=0.0 |
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| 196 | qsvaer(:,:,:)=0.0 |
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| 197 | gvaer(:,:,:) =0.0 |
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| 198 | |
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| 199 | qxiaer(:,:,:)=0.0 |
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| 200 | qsiaer(:,:,:)=0.0 |
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| 201 | giaer(:,:,:) =0.0 |
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| 202 | |
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| 203 | if(firstcall) then |
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| 204 | |
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| 205 | !!! ALLOCATED instances are necessary because of CLFvarying |
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| 206 | !!! strategy to call callcorrk twice in physiq... |
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| 207 | IF(.not.ALLOCATED(QREFvis3d)) ALLOCATE(QREFvis3d(ngrid,nlayer,naerkind)) |
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| 208 | IF(.not.ALLOCATED(QREFir3d)) ALLOCATE(QREFir3d(ngrid,nlayer,naerkind)) |
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| 209 | ! Effective radius and variance of the aerosols |
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| 210 | IF(.not.ALLOCATED(reffrad)) allocate(reffrad(ngrid,nlayer,naerkind)) |
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| 211 | IF(.not.ALLOCATED(nueffrad)) allocate(nueffrad(ngrid,nlayer,naerkind)) |
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| 212 | |
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| 213 | call system('rm -f surf_vals_long.out') |
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| 214 | |
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| 215 | if(naerkind.gt.4)then |
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| 216 | print*,'Code not general enough to deal with naerkind > 4 yet.' |
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| 217 | call abort |
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| 218 | endif |
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| 219 | call su_aer_radii(ngrid,nlayer,reffrad,nueffrad) |
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| 220 | |
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| 221 | !-------------------------------------------------- |
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| 222 | ! set up correlated k |
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| 223 | print*, "callcorrk: Correlated-k data base folder:",trim(datadir) |
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| 224 | call getin_p("corrkdir",corrkdir) |
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| 225 | print*, "corrkdir = ",corrkdir |
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| 226 | write( tmp1, '(i3)' ) L_NSPECTI |
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| 227 | write( tmp2, '(i3)' ) L_NSPECTV |
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| 228 | banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2)) |
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| 229 | banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir)) |
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| 230 | |
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| 231 | call setspi ! basic infrared properties |
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| 232 | call setspv ! basic visible properties |
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| 233 | call sugas_corrk ! set up gaseous absorption properties |
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| 234 | call suaer_corrk ! set up aerosol optical properties |
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| 235 | |
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| 236 | |
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| 237 | if((igcm_h2o_vap.eq.0) .and. varactive)then |
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| 238 | print*,'varactive in callcorrk but no h2o_vap tracer.' |
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| 239 | stop |
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| 240 | endif |
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| 241 | |
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| 242 | OLR_nu(:,:) = 0. |
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| 243 | OSR_nu(:,:) = 0. |
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| 244 | |
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| 245 | if (ngrid.eq.1) then |
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| 246 | PRINT*, 'Simulate global averaged conditions ?' |
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| 247 | global1d = .false. ! default value |
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| 248 | call getin_p("global1d",global1d) |
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| 249 | write(*,*) "global1d = ",global1d |
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| 250 | ! Test of incompatibility: |
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| 251 | ! if global1d is true, there should not be any diurnal cycle |
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| 252 | if (global1d.and.diurnal) then |
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| 253 | print*,'if global1d is true, diurnal must be set to false' |
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| 254 | stop |
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| 255 | endif |
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| 256 | |
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| 257 | if (global1d) then |
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| 258 | PRINT *,'Solar Zenith angle (deg.) ?' |
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| 259 | PRINT *,'(assumed for averaged solar flux S/4)' |
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| 260 | szangle=60.0 ! default value |
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| 261 | call getin_p("szangle",szangle) |
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| 262 | write(*,*) "szangle = ",szangle |
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| 263 | endif |
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| 264 | endif |
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| 265 | |
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| 266 | end if ! of if (firstcall) |
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| 267 | |
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| 268 | !======================================================================= |
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| 269 | ! Initialization on every call |
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| 270 | |
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| 271 | !-------------------------------------------------- |
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| 272 | ! Effective radius and variance of the aerosols |
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| 273 | do iaer=1,naerkind |
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| 274 | |
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| 275 | if ((iaer.eq.iaero_co2).and.tracer.and.(igcm_co2_ice.gt.0)) then ! treat condensed co2 particles. |
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| 276 | call co2_reffrad(ngrid,nlayer,nq,pq,reffrad(1,1,iaero_co2)) |
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| 277 | print*,'Max. CO2 ice particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um' |
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| 278 | print*,'Min. CO2 ice particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um' |
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| 279 | end if |
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| 280 | if ((iaer.eq.iaero_h2o).and.water) then ! treat condensed water particles. to be generalized for other aerosols |
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| 281 | call h2o_reffrad(ngrid,nlayer,pq(1,1,igcm_h2o_ice),pt, & |
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| 282 | reffrad(1,1,iaero_h2o),nueffrad(1,1,iaero_h2o)) |
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| 283 | print*,'Max. H2O cloud particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um' |
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| 284 | print*,'Min. H2O cloud particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um' |
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| 285 | endif |
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| 286 | if(iaer.eq.iaero_dust)then |
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| 287 | call dust_reffrad(ngrid,nlayer,reffrad(1,1,iaero_dust)) |
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| 288 | print*,'Dust particle size = ',reffrad(1,1,iaer)/1.e-6,' um' |
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| 289 | endif |
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| 290 | if(iaer.eq.iaero_h2so4)then |
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| 291 | call h2so4_reffrad(ngrid,nlayer,reffrad(1,1,iaero_h2so4)) |
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| 292 | print*,'H2SO4 particle size =',reffrad(1,1,iaer)/1.e-6,' um' |
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| 293 | endif |
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| 294 | if(iaer.eq.iaero_back2lay)then |
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| 295 | call back2lay_reffrad(ngrid,reffrad(1,1,iaero_back2lay),nlayer,pplev) |
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| 296 | endif |
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| 297 | end do !iaer=1,naerkind |
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| 298 | |
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| 299 | |
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| 300 | ! how much light we get |
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| 301 | do nw=1,L_NSPECTV |
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| 302 | stel(nw)=stellarf(nw)/(dist_star**2) |
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| 303 | end do |
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| 304 | |
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| 305 | call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, & |
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| 306 | QVISsQREF3d,omegaVIS3d,gVIS3d, & |
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| 307 | QIRsQREF3d,omegaIR3d,gIR3d, & |
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| 308 | QREFvis3d,QREFir3d) ! get 3D aerosol optical properties |
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| 309 | |
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| 310 | call aeropacity(ngrid,nlayer,nq,pplay,pplev,pq,aerosol, & |
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| 311 | reffrad,QREFvis3d,QREFir3d, & |
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| 312 | tau_col,cloudfrac,totcloudfrac,clearsky) ! get aerosol optical depths |
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| 313 | |
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| 314 | !----------------------------------------------------------------------- |
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| 315 | ! Starting Big Loop over every GCM column |
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| 316 | do ig=1,ngrid |
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| 317 | |
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| 318 | !======================================================================= |
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| 319 | ! Transformation of the GCM variables |
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| 320 | |
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| 321 | !----------------------------------------------------------------------- |
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| 322 | ! Aerosol optical properties Qext, Qscat and g |
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| 323 | ! The transformation in the vertical is the same as for temperature |
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| 324 | |
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| 325 | ! shortwave |
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| 326 | do iaer=1,naerkind |
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| 327 | DO nw=1,L_NSPECTV |
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| 328 | do l=1,nlayer |
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| 329 | |
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| 330 | temp1=QVISsQREF3d(ig,nlayer+1-l,nw,iaer) & |
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| 331 | *QREFvis3d(ig,nlayer+1-l,iaer) |
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| 332 | |
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| 333 | temp2=QVISsQREF3d(ig,max(nlayer-l,1),nw,iaer) & |
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| 334 | *QREFvis3d(ig,max(nlayer-l,1),iaer) |
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| 335 | |
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| 336 | qxvaer(2*l,nw,iaer) = temp1 |
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| 337 | qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
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| 338 | |
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| 339 | temp1=temp1*omegavis3d(ig,nlayer+1-l,nw,iaer) |
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| 340 | temp2=temp2*omegavis3d(ig,max(nlayer-l,1),nw,iaer) |
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| 341 | |
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| 342 | qsvaer(2*l,nw,iaer) = temp1 |
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| 343 | qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
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| 344 | |
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| 345 | temp1=gvis3d(ig,nlayer+1-l,nw,iaer) |
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| 346 | temp2=gvis3d(ig,max(nlayer-l,1),nw,iaer) |
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| 347 | |
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| 348 | gvaer(2*l,nw,iaer) = temp1 |
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| 349 | gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 350 | |
|---|
| 351 | end do |
|---|
| 352 | |
|---|
| 353 | qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer) |
|---|
| 354 | qxvaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 355 | |
|---|
| 356 | qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer) |
|---|
| 357 | qsvaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 358 | |
|---|
| 359 | gvaer(1,nw,iaer)=gvaer(2,nw,iaer) |
|---|
| 360 | gvaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 361 | |
|---|
| 362 | end do |
|---|
| 363 | |
|---|
| 364 | ! longwave |
|---|
| 365 | DO nw=1,L_NSPECTI |
|---|
| 366 | do l=1,nlayer |
|---|
| 367 | |
|---|
| 368 | temp1=QIRsQREF3d(ig,nlayer+1-l,nw,iaer) & |
|---|
| 369 | *QREFir3d(ig,nlayer+1-l,iaer) |
|---|
| 370 | |
|---|
| 371 | temp2=QIRsQREF3d(ig,max(nlayer-l,1),nw,iaer) & |
|---|
| 372 | *QREFir3d(ig,max(nlayer-l,1),iaer) |
|---|
| 373 | |
|---|
| 374 | qxiaer(2*l,nw,iaer) = temp1 |
|---|
| 375 | qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 376 | |
|---|
| 377 | temp1=temp1*omegair3d(ig,nlayer+1-l,nw,iaer) |
|---|
| 378 | temp2=temp2*omegair3d(ig,max(nlayer-l,1),nw,iaer) |
|---|
| 379 | |
|---|
| 380 | qsiaer(2*l,nw,iaer) = temp1 |
|---|
| 381 | qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 382 | |
|---|
| 383 | temp1=gir3d(ig,nlayer+1-l,nw,iaer) |
|---|
| 384 | temp2=gir3d(ig,max(nlayer-l,1),nw,iaer) |
|---|
| 385 | |
|---|
| 386 | giaer(2*l,nw,iaer) = temp1 |
|---|
| 387 | giaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 388 | |
|---|
| 389 | end do |
|---|
| 390 | |
|---|
| 391 | qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer) |
|---|
| 392 | qxiaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 393 | |
|---|
| 394 | qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer) |
|---|
| 395 | qsiaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 396 | |
|---|
| 397 | giaer(1,nw,iaer)=giaer(2,nw,iaer) |
|---|
| 398 | giaer(2*nlayer+1,nw,iaer)=0. |
|---|
| 399 | |
|---|
| 400 | end do |
|---|
| 401 | end do |
|---|
| 402 | |
|---|
| 403 | ! test / correct for freaky s. s. albedo values |
|---|
| 404 | do iaer=1,naerkind |
|---|
| 405 | do k=1,L_LEVELS+1 |
|---|
| 406 | |
|---|
| 407 | do nw=1,L_NSPECTV |
|---|
| 408 | if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then |
|---|
| 409 | print*,'Serious problems with qsvaer values' |
|---|
| 410 | print*,'in callcorrk' |
|---|
| 411 | call abort |
|---|
| 412 | endif |
|---|
| 413 | if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then |
|---|
| 414 | qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer) |
|---|
| 415 | endif |
|---|
| 416 | end do |
|---|
| 417 | |
|---|
| 418 | do nw=1,L_NSPECTI |
|---|
| 419 | if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then |
|---|
| 420 | print*,'Serious problems with qsiaer values' |
|---|
| 421 | print*,'in callcorrk' |
|---|
| 422 | call abort |
|---|
| 423 | endif |
|---|
| 424 | if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then |
|---|
| 425 | qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer) |
|---|
| 426 | endif |
|---|
| 427 | end do |
|---|
| 428 | |
|---|
| 429 | end do |
|---|
| 430 | end do |
|---|
| 431 | |
|---|
| 432 | !----------------------------------------------------------------------- |
|---|
| 433 | ! Aerosol optical depths |
|---|
| 434 | |
|---|
| 435 | do iaer=1,naerkind ! a bug was here |
|---|
| 436 | do k=0,nlayer-1 |
|---|
| 437 | |
|---|
| 438 | pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ & |
|---|
| 439 | (pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1)) |
|---|
| 440 | |
|---|
| 441 | temp=aerosol(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer) |
|---|
| 442 | |
|---|
| 443 | tauaero(2*k+2,iaer)=max(temp*pweight,0.d0) |
|---|
| 444 | tauaero(2*k+3,iaer)=max(temp-tauaero(2*k+2,iaer),0.d0) |
|---|
| 445 | ! |
|---|
| 446 | end do |
|---|
| 447 | ! boundary conditions |
|---|
| 448 | tauaero(1,iaer) = tauaero(2,iaer) |
|---|
| 449 | tauaero(L_LEVELS+1,iaer) = tauaero(L_LEVELS,iaer) |
|---|
| 450 | !tauaero(1,iaer) = 0. |
|---|
| 451 | !tauaero(L_LEVELS+1,iaer) = 0. |
|---|
| 452 | end do |
|---|
| 453 | |
|---|
| 454 | ! Albedo and emissivity |
|---|
| 455 | albi=1-emis(ig) ! Longwave. |
|---|
| 456 | DO nw=1,L_NSPECTV ! Shortwave loop. |
|---|
| 457 | albv(nw)=albedo(ig,nw) |
|---|
| 458 | ENDDO |
|---|
| 459 | |
|---|
| 460 | if (nosurf) then |
|---|
| 461 | DO nw=1,L_NSPECTV |
|---|
| 462 | if(albv(nw).gt.0.0) then |
|---|
| 463 | print*,'For open lower boundary in callcorrk must' |
|---|
| 464 | print*,'have spectral surface band albedos all set to zero!' |
|---|
| 465 | call abort |
|---|
| 466 | endif |
|---|
| 467 | ENDDO |
|---|
| 468 | endif |
|---|
| 469 | |
|---|
| 470 | if ((ngrid.eq.1).and.(global1d)) then ! fixed zenith angle 'szangle' in 1D simulations w/ globally-averaged sunlight |
|---|
| 471 | acosz = cos(pi*szangle/180.0) |
|---|
| 472 | print*,'acosz=',acosz,', szangle=',szangle |
|---|
| 473 | else |
|---|
| 474 | acosz=mu0(ig) ! cosine of sun incident angle : 3D simulations or local 1D simulations using latitude |
|---|
| 475 | endif |
|---|
| 476 | |
|---|
| 477 | !!! JL13: in the following, I changed some indices in the interpolations so that the model rsults are less dependent on the number of layers |
|---|
| 478 | !!! the older verions are commented with the commetn !JL13index |
|---|
| 479 | |
|---|
| 480 | |
|---|
| 481 | !----------------------------------------------------------------------- |
|---|
| 482 | ! Water vapour (to be generalised for other gases eventually) |
|---|
| 483 | |
|---|
| 484 | if(varactive)then |
|---|
| 485 | |
|---|
| 486 | i_var=igcm_h2o_vap |
|---|
| 487 | do l=1,nlayer |
|---|
| 488 | qvar(2*l) = pq(ig,nlayer+1-l,i_var) |
|---|
| 489 | qvar(2*l+1) = pq(ig,nlayer+1-l,i_var) |
|---|
| 490 | !JL13index qvar(2*l+1) = (pq(ig,nlayer+1-l,i_var)+pq(ig,max(nlayer-l,1),i_var))/2 |
|---|
| 491 | !JL13index ! Average approximation as for temperature... |
|---|
| 492 | end do |
|---|
| 493 | qvar(1)=qvar(2) |
|---|
| 494 | |
|---|
| 495 | elseif(varfixed)then |
|---|
| 496 | |
|---|
| 497 | do l=1,nlayer ! here we will assign fixed water vapour profiles globally |
|---|
| 498 | RH = satval * ((pplay(ig,l)/pplev(ig,1) - 0.02) / 0.98) |
|---|
| 499 | if(RH.lt.0.0) RH=0.0 |
|---|
| 500 | |
|---|
| 501 | ptemp=pplay(ig,l) |
|---|
| 502 | Ttemp=pt(ig,l) |
|---|
| 503 | call watersat(Ttemp,ptemp,qsat) |
|---|
| 504 | |
|---|
| 505 | !pq_temp(l) = qsat ! fully saturated everywhere |
|---|
| 506 | pq_temp(l) = RH * qsat ! ~realistic profile (e.g. 80% saturation at ground) |
|---|
| 507 | end do |
|---|
| 508 | |
|---|
| 509 | do l=1,nlayer |
|---|
| 510 | qvar(2*l) = pq_temp(nlayer+1-l) |
|---|
| 511 | qvar(2*l+1) = (pq_temp(nlayer+1-l)+pq_temp(max(nlayer-l,1)))/2 |
|---|
| 512 | end do |
|---|
| 513 | qvar(1)=qvar(2) |
|---|
| 514 | |
|---|
| 515 | ! Lowest layer of atmosphere |
|---|
| 516 | RH = satval * (1 - 0.02) / 0.98 |
|---|
| 517 | if(RH.lt.0.0) RH=0.0 |
|---|
| 518 | |
|---|
| 519 | ! ptemp = pplev(ig,1) |
|---|
| 520 | ! Ttemp = tsurf(ig) |
|---|
| 521 | ! call watersat(Ttemp,ptemp,qsat) |
|---|
| 522 | |
|---|
| 523 | qvar(2*nlayer+1)= RH * qsat ! ~realistic profile (e.g. 80% saturation at ground) |
|---|
| 524 | |
|---|
| 525 | else |
|---|
| 526 | do k=1,L_LEVELS |
|---|
| 527 | qvar(k) = 1.0D-7 |
|---|
| 528 | end do |
|---|
| 529 | end if |
|---|
| 530 | |
|---|
| 531 | if(.not.kastprof)then |
|---|
| 532 | ! IMPORTANT: Now convert from kg/kg to mol/mol |
|---|
| 533 | do k=1,L_LEVELS |
|---|
| 534 | qvar(k) = qvar(k)/(epsi+qvar(k)*(1.-epsi)) |
|---|
| 535 | end do |
|---|
| 536 | end if |
|---|
| 537 | |
|---|
| 538 | !----------------------------------------------------------------------- |
|---|
| 539 | ! kcm mode only |
|---|
| 540 | if(kastprof)then |
|---|
| 541 | |
|---|
| 542 | ! initial values equivalent to mugaz |
|---|
| 543 | DO l=1,nlayer |
|---|
| 544 | muvarrad(2*l) = mugaz |
|---|
| 545 | muvarrad(2*l+1) = mugaz |
|---|
| 546 | END DO |
|---|
| 547 | |
|---|
| 548 | if(ngasmx.gt.1)then |
|---|
| 549 | |
|---|
| 550 | DO l=1,nlayer |
|---|
| 551 | muvarrad(2*l) = muvar(ig,nlayer+2-l) |
|---|
| 552 | muvarrad(2*l+1) = (muvar(ig,nlayer+2-l) + & |
|---|
| 553 | muvar(ig,max(nlayer+1-l,1)))/2 |
|---|
| 554 | END DO |
|---|
| 555 | |
|---|
| 556 | muvarrad(1) = muvarrad(2) |
|---|
| 557 | muvarrad(2*nlayer+1)=muvar(ig,1) |
|---|
| 558 | |
|---|
| 559 | print*,'Recalculating qvar with VARIABLE epsi for kastprof' |
|---|
| 560 | print*,'Assumes that the variable gas is H2O!!!' |
|---|
| 561 | print*,'Assumes that there is only one tracer' |
|---|
| 562 | !i_var=igcm_h2o_vap |
|---|
| 563 | i_var=1 |
|---|
| 564 | if(nq.gt.1)then |
|---|
| 565 | print*,'Need 1 tracer only to run kcm1d.e' |
|---|
| 566 | stop |
|---|
| 567 | endif |
|---|
| 568 | do l=1,nlayer |
|---|
| 569 | vtmp(l)=pq(ig,l,i_var)/(epsi+pq(ig,l,i_var)*(1.-epsi)) |
|---|
| 570 | !vtmp(l)=pq(ig,l,i_var)*muvar(ig,l+1)/mH2O !JL to be changed |
|---|
| 571 | end do |
|---|
| 572 | |
|---|
| 573 | do l=1,nlayer |
|---|
| 574 | qvar(2*l) = vtmp(nlayer+1-l) |
|---|
| 575 | qvar(2*l+1) = vtmp(nlayer+1-l) |
|---|
| 576 | ! qvar(2*l+1) = ( vtmp(nlayer+1-l) + vtmp(max(nlayer-l,1)) )/2 |
|---|
| 577 | end do |
|---|
| 578 | qvar(1)=qvar(2) |
|---|
| 579 | |
|---|
| 580 | print*,'Warning: reducing qvar in callcorrk.' |
|---|
| 581 | print*,'Temperature profile no longer consistent ', & |
|---|
| 582 | 'with saturated H2O. qsat=',satval |
|---|
| 583 | do k=1,L_LEVELS |
|---|
| 584 | qvar(k) = qvar(k)*satval |
|---|
| 585 | end do |
|---|
| 586 | |
|---|
| 587 | endif |
|---|
| 588 | else ! if kastprof |
|---|
| 589 | DO l=1,nlayer |
|---|
| 590 | muvarrad(2*l) = muvar(ig,nlayer+2-l) |
|---|
| 591 | muvarrad(2*l+1) = (muvar(ig,nlayer+2-l)+muvar(ig,max(nlayer+1-l,1)))/2 |
|---|
| 592 | END DO |
|---|
| 593 | |
|---|
| 594 | muvarrad(1) = muvarrad(2) |
|---|
| 595 | muvarrad(2*nlayer+1)=muvar(ig,1) |
|---|
| 596 | endif |
|---|
| 597 | |
|---|
| 598 | ! Keep values inside limits for which we have radiative transfer coefficients |
|---|
| 599 | if(L_REFVAR.gt.1)then ! there was a bug here! |
|---|
| 600 | do k=1,L_LEVELS |
|---|
| 601 | if(qvar(k).lt.wrefvar(1))then |
|---|
| 602 | qvar(k)=wrefvar(1)+1.0e-8 |
|---|
| 603 | elseif(qvar(k).gt.wrefvar(L_REFVAR))then |
|---|
| 604 | qvar(k)=wrefvar(L_REFVAR)-1.0e-8 |
|---|
| 605 | endif |
|---|
| 606 | end do |
|---|
| 607 | endif |
|---|
| 608 | |
|---|
| 609 | !----------------------------------------------------------------------- |
|---|
| 610 | ! Pressure and temperature |
|---|
| 611 | |
|---|
| 612 | DO l=1,nlayer |
|---|
| 613 | plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep |
|---|
| 614 | plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep |
|---|
| 615 | tlevrad(2*l) = pt(ig,nlayer+1-l) |
|---|
| 616 | tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2 |
|---|
| 617 | END DO |
|---|
| 618 | |
|---|
| 619 | plevrad(1) = 0. |
|---|
| 620 | plevrad(2) = 0. !! Trick to have correct calculations of fluxes in gflux(i/v).F, |
|---|
| 621 | !! but the pmid levels are not impacted by this change. |
|---|
| 622 | |
|---|
| 623 | tlevrad(1) = tlevrad(2) |
|---|
| 624 | tlevrad(2*nlayer+1)=tsurf(ig) |
|---|
| 625 | |
|---|
| 626 | pmid(1) = max(pgasmin,0.0001*plevrad(3)) |
|---|
| 627 | pmid(2) = pmid(1) |
|---|
| 628 | |
|---|
| 629 | tmid(1) = tlevrad(2) |
|---|
| 630 | tmid(2) = tmid(1) |
|---|
| 631 | |
|---|
| 632 | DO l=1,L_NLAYRAD-1 |
|---|
| 633 | tmid(2*l+1) = tlevrad(2*l+1) |
|---|
| 634 | tmid(2*l+2) = tlevrad(2*l+1) |
|---|
| 635 | pmid(2*l+1) = plevrad(2*l+1) |
|---|
| 636 | pmid(2*l+2) = plevrad(2*l+1) |
|---|
| 637 | END DO |
|---|
| 638 | pmid(L_LEVELS) = plevrad(L_LEVELS) |
|---|
| 639 | tmid(L_LEVELS) = tlevrad(L_LEVELS) |
|---|
| 640 | |
|---|
| 641 | !!Alternative interpolation: |
|---|
| 642 | ! pmid(3) = pmid(1) |
|---|
| 643 | ! pmid(4) = pmid(1) |
|---|
| 644 | ! tmid(3) = tmid(1) |
|---|
| 645 | ! tmid(4) = tmid(1) |
|---|
| 646 | ! DO l=2,L_NLAYRAD-1 |
|---|
| 647 | ! tmid(2*l+1) = tlevrad(2*l) |
|---|
| 648 | ! tmid(2*l+2) = tlevrad(2*l) |
|---|
| 649 | ! pmid(2*l+1) = plevrad(2*l) |
|---|
| 650 | ! pmid(2*l+2) = plevrad(2*l) |
|---|
| 651 | ! END DO |
|---|
| 652 | ! pmid(L_LEVELS) = plevrad(L_LEVELS-1) |
|---|
| 653 | ! tmid(L_LEVELS) = tlevrad(L_LEVELS-1) |
|---|
| 654 | |
|---|
| 655 | ! test for out-of-bounds pressure |
|---|
| 656 | if(plevrad(3).lt.pgasmin)then |
|---|
| 657 | print*,'Minimum pressure is outside the radiative' |
|---|
| 658 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 659 | call abort |
|---|
| 660 | elseif(plevrad(L_LEVELS).gt.pgasmax)then |
|---|
| 661 | print*,'Maximum pressure is outside the radiative' |
|---|
| 662 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 663 | call abort |
|---|
| 664 | endif |
|---|
| 665 | |
|---|
| 666 | ! test for out-of-bounds temperature |
|---|
| 667 | do k=1,L_LEVELS |
|---|
| 668 | if(tlevrad(k).lt.tgasmin)then |
|---|
| 669 | print*,'Minimum temperature is outside the radiative' |
|---|
| 670 | print*,'transfer kmatrix bounds' |
|---|
| 671 | print*,"k=",k," tlevrad(k)=",tlevrad(k) |
|---|
| 672 | print*,"tgasmin=",tgasmin |
|---|
| 673 | if (strictboundcorrk) then |
|---|
| 674 | call abort |
|---|
| 675 | else |
|---|
| 676 | print*,'***********************************************' |
|---|
| 677 | print*,'we allow model to continue with tlevrad=tgasmin' |
|---|
| 678 | print*,' ... we assume we know what you are doing ... ' |
|---|
| 679 | print*,' ... but do not let this happen too often ... ' |
|---|
| 680 | print*,'***********************************************' |
|---|
| 681 | !tlevrad(k)=tgasmin |
|---|
| 682 | endif |
|---|
| 683 | elseif(tlevrad(k).gt.tgasmax)then |
|---|
| 684 | print*,'Maximum temperature is outside the radiative' |
|---|
| 685 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 686 | print*,"k=",k," tlevrad(k)=",tlevrad(k) |
|---|
| 687 | print*,"tgasmax=",tgasmax |
|---|
| 688 | if (strictboundcorrk) then |
|---|
| 689 | call abort |
|---|
| 690 | else |
|---|
| 691 | print*,'***********************************************' |
|---|
| 692 | print*,'we allow model to continue with tlevrad=tgasmax' |
|---|
| 693 | print*,' ... we assume we know what you are doing ... ' |
|---|
| 694 | print*,' ... but do not let this happen too often ... ' |
|---|
| 695 | print*,'***********************************************' |
|---|
| 696 | !tlevrad(k)=tgasmax |
|---|
| 697 | endif |
|---|
| 698 | endif |
|---|
| 699 | enddo |
|---|
| 700 | do k=1,L_NLAYRAD+1 |
|---|
| 701 | if(tmid(k).lt.tgasmin)then |
|---|
| 702 | print*,'Minimum temperature is outside the radiative' |
|---|
| 703 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 704 | print*,"k=",k," tmid(k)=",tmid(k) |
|---|
| 705 | print*,"tgasmin=",tgasmin |
|---|
| 706 | if (strictboundcorrk) then |
|---|
| 707 | call abort |
|---|
| 708 | else |
|---|
| 709 | print*,'***********************************************' |
|---|
| 710 | print*,'we allow model to continue with tmid=tgasmin' |
|---|
| 711 | print*,' ... we assume we know what you are doing ... ' |
|---|
| 712 | print*,' ... but do not let this happen too often ... ' |
|---|
| 713 | print*,'***********************************************' |
|---|
| 714 | tmid(k)=tgasmin |
|---|
| 715 | endif |
|---|
| 716 | elseif(tmid(k).gt.tgasmax)then |
|---|
| 717 | print*,'Maximum temperature is outside the radiative' |
|---|
| 718 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 719 | print*,"k=",k," tmid(k)=",tmid(k) |
|---|
| 720 | print*,"tgasmax=",tgasmax |
|---|
| 721 | if (strictboundcorrk) then |
|---|
| 722 | call abort |
|---|
| 723 | else |
|---|
| 724 | print*,'***********************************************' |
|---|
| 725 | print*,'we allow model to continue with tmid=tgasmin' |
|---|
| 726 | print*,' ... we assume we know what you are doing ... ' |
|---|
| 727 | print*,' ... but do not let this happen too often ... ' |
|---|
| 728 | print*,'***********************************************' |
|---|
| 729 | tmid(k)=tgasmax |
|---|
| 730 | endif |
|---|
| 731 | endif |
|---|
| 732 | enddo |
|---|
| 733 | |
|---|
| 734 | !======================================================================= |
|---|
| 735 | ! Calling the main radiative transfer subroutines |
|---|
| 736 | |
|---|
| 737 | |
|---|
| 738 | Cmk= 0.01 * 1.0 / (glat(ig) * mugaz * 1.672621e-27) ! q_main=1.0 assumed |
|---|
| 739 | glat_ig=glat(ig) |
|---|
| 740 | |
|---|
| 741 | !----------------------------------------------------------------------- |
|---|
| 742 | ! Shortwave |
|---|
| 743 | |
|---|
| 744 | if(fract(ig) .ge. 1.0e-4) then ! only during daylight! |
|---|
| 745 | if((ngrid.eq.1).and.(global1d))then |
|---|
| 746 | do nw=1,L_NSPECTV |
|---|
| 747 | stel_fract(nw)= stel(nw)* 0.25 / acosz |
|---|
| 748 | ! globally averaged = divide by 4 |
|---|
| 749 | ! but we correct for solar zenith angle |
|---|
| 750 | end do |
|---|
| 751 | else |
|---|
| 752 | do nw=1,L_NSPECTV |
|---|
| 753 | stel_fract(nw)= stel(nw) * fract(ig) |
|---|
| 754 | end do |
|---|
| 755 | endif |
|---|
| 756 | call optcv(dtauv,tauv,taucumv,plevrad, & |
|---|
| 757 | qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, & |
|---|
| 758 | tmid,pmid,taugsurf,qvar,muvarrad) |
|---|
| 759 | |
|---|
| 760 | call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, & |
|---|
| 761 | acosz,stel_fract,gweight, & |
|---|
| 762 | nfluxtopv,fluxtopvdn,nfluxoutv_nu,nfluxgndv_nu, & |
|---|
| 763 | fmnetv,fluxupv,fluxdnv,fzerov,taugsurf) |
|---|
| 764 | |
|---|
| 765 | else ! during the night, fluxes = 0 |
|---|
| 766 | nfluxtopv = 0.0d0 |
|---|
| 767 | fluxtopvdn = 0.0d0 |
|---|
| 768 | nfluxoutv_nu(:) = 0.0d0 |
|---|
| 769 | nfluxgndv_nu(:) = 0.0d0 |
|---|
| 770 | do l=1,L_NLAYRAD |
|---|
| 771 | fmnetv(l)=0.0d0 |
|---|
| 772 | fluxupv(l)=0.0d0 |
|---|
| 773 | fluxdnv(l)=0.0d0 |
|---|
| 774 | end do |
|---|
| 775 | end if |
|---|
| 776 | |
|---|
| 777 | |
|---|
| 778 | ! Equivalent Albedo Calculation. MT2015 |
|---|
| 779 | if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight. |
|---|
| 780 | DO nw=1,L_NSPECTV |
|---|
| 781 | albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw) |
|---|
| 782 | ENDDO |
|---|
| 783 | albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/sum(nfluxgndv_nu(1:L_NSPECTV)) |
|---|
| 784 | albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV)) |
|---|
| 785 | else |
|---|
| 786 | albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0. |
|---|
| 787 | endif |
|---|
| 788 | |
|---|
| 789 | |
|---|
| 790 | !----------------------------------------------------------------------- |
|---|
| 791 | ! Longwave |
|---|
| 792 | |
|---|
| 793 | call optci(plevrad,tlevrad,dtaui,taucumi, & |
|---|
| 794 | qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, & |
|---|
| 795 | taugsurfi,qvar,muvarrad) |
|---|
| 796 | |
|---|
| 797 | call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, & |
|---|
| 798 | wnoi,dwni,cosbi,wbari,gweight,nfluxtopi,nfluxtopi_nu, & |
|---|
| 799 | fmneti,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi) |
|---|
| 800 | |
|---|
| 801 | !----------------------------------------------------------------------- |
|---|
| 802 | ! Transformation of the correlated-k code outputs |
|---|
| 803 | ! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw) |
|---|
| 804 | |
|---|
| 805 | ! Flux incident at the top of the atmosphere |
|---|
| 806 | fluxtop_dn(ig)=fluxtopvdn |
|---|
| 807 | |
|---|
| 808 | fluxtop_lw(ig) = real(nfluxtopi) |
|---|
| 809 | fluxabs_sw(ig) = real(-nfluxtopv) |
|---|
| 810 | fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD)) |
|---|
| 811 | fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD)) |
|---|
| 812 | |
|---|
| 813 | ! Flux absorbed by the surface. By MT2015. |
|---|
| 814 | fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig)) |
|---|
| 815 | |
|---|
| 816 | if(fluxtop_dn(ig).lt.0.0)then |
|---|
| 817 | print*,'Achtung! fluxtop_dn has lost the plot!' |
|---|
| 818 | print*,'fluxtop_dn=',fluxtop_dn(ig) |
|---|
| 819 | print*,'acosz=',acosz |
|---|
| 820 | print*,'aerosol=',aerosol(ig,:,:) |
|---|
| 821 | print*,'temp= ',pt(ig,:) |
|---|
| 822 | print*,'pplay= ',pplay(ig,:) |
|---|
| 823 | call abort |
|---|
| 824 | endif |
|---|
| 825 | |
|---|
| 826 | ! Spectral output, for exoplanet observational comparison |
|---|
| 827 | if(specOLR)then |
|---|
| 828 | do nw=1,L_NSPECTI |
|---|
| 829 | OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth |
|---|
| 830 | end do |
|---|
| 831 | do nw=1,L_NSPECTV |
|---|
| 832 | !GSR_nu(ig,nw)=nfluxgndv_nu(nw) |
|---|
| 833 | OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth |
|---|
| 834 | end do |
|---|
| 835 | endif |
|---|
| 836 | |
|---|
| 837 | ! Finally, the heating rates |
|---|
| 838 | |
|---|
| 839 | DO l=2,L_NLAYRAD |
|---|
| 840 | dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) & |
|---|
| 841 | *glat(ig)/(cpp*scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 842 | dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) & |
|---|
| 843 | *glat(ig)/(cpp*scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 844 | END DO |
|---|
| 845 | |
|---|
| 846 | ! These are values at top of atmosphere |
|---|
| 847 | dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) & |
|---|
| 848 | *glat(ig)/(cpp*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 849 | dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) & |
|---|
| 850 | *glat(ig)/(cpp*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 851 | |
|---|
| 852 | ! --------------------------------------------------------------- |
|---|
| 853 | end do ! end of big loop over every GCM column (ig = 1:ngrid) |
|---|
| 854 | |
|---|
| 855 | |
|---|
| 856 | !----------------------------------------------------------------------- |
|---|
| 857 | ! Additional diagnostics |
|---|
| 858 | |
|---|
| 859 | ! IR spectral output, for exoplanet observational comparison |
|---|
| 860 | |
|---|
| 861 | |
|---|
| 862 | if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12 |
|---|
| 863 | |
|---|
| 864 | print*,'Saving scalar quantities in surf_vals.out...' |
|---|
| 865 | print*,'psurf = ', pplev(1,1),' Pa' |
|---|
| 866 | open(116,file='surf_vals.out') |
|---|
| 867 | write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), & |
|---|
| 868 | real(-nfluxtopv),real(nfluxtopi) |
|---|
| 869 | close(116) |
|---|
| 870 | |
|---|
| 871 | ! I am useful, please don`t remove me! |
|---|
| 872 | ! if(specOLR)then |
|---|
| 873 | ! open(117,file='OLRnu.out') |
|---|
| 874 | ! do nw=1,L_NSPECTI |
|---|
| 875 | ! write(117,*) OLR_nu(1,nw) |
|---|
| 876 | ! enddo |
|---|
| 877 | ! close(117) |
|---|
| 878 | ! |
|---|
| 879 | ! open(127,file='OSRnu.out') |
|---|
| 880 | ! do nw=1,L_NSPECTV |
|---|
| 881 | ! write(127,*) OSR_nu(1,nw) |
|---|
| 882 | ! enddo |
|---|
| 883 | ! close(127) |
|---|
| 884 | ! endif |
|---|
| 885 | |
|---|
| 886 | ! OLR vs altitude: do it as a .txt file |
|---|
| 887 | OLRz=.false. |
|---|
| 888 | if(OLRz)then |
|---|
| 889 | print*,'saving IR vertical flux for OLRz...' |
|---|
| 890 | open(118,file='OLRz_plevs.out') |
|---|
| 891 | open(119,file='OLRz.out') |
|---|
| 892 | do l=1,L_NLAYRAD |
|---|
| 893 | write(118,*) plevrad(2*l) |
|---|
| 894 | do nw=1,L_NSPECTI |
|---|
| 895 | write(119,*) fluxupi_nu(l,nw) |
|---|
| 896 | enddo |
|---|
| 897 | enddo |
|---|
| 898 | close(118) |
|---|
| 899 | close(119) |
|---|
| 900 | endif |
|---|
| 901 | |
|---|
| 902 | endif |
|---|
| 903 | |
|---|
| 904 | ! see physiq.F for explanations about CLFvarying. This is temporary. |
|---|
| 905 | if (lastcall .and. .not.CLFvarying) then |
|---|
| 906 | IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi ) |
|---|
| 907 | IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv ) |
|---|
| 908 | !$OMP BARRIER |
|---|
| 909 | !$OMP MASTER |
|---|
| 910 | IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref ) |
|---|
| 911 | IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref ) |
|---|
| 912 | IF( ALLOCATED( wrefvar ) ) DEALLOCATE( wrefvar ) |
|---|
| 913 | IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref ) |
|---|
| 914 | !$OMP END MASTER |
|---|
| 915 | !$OMP BARRIER |
|---|
| 916 | IF ( ALLOCATED(reffrad)) DEALLOCATE(reffrad) |
|---|
| 917 | IF ( ALLOCATED(nueffrad)) DEALLOCATE(nueffrad) |
|---|
| 918 | endif |
|---|
| 919 | |
|---|
| 920 | |
|---|
| 921 | end subroutine callcorrk |
|---|
