| [253] | 1 | subroutine callcorrk(icount,ngrid,nlayer,pq,nq,qsurf, & |
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| 2 | albedo,emis,mu0,pplev,pplay,pt, & |
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| 3 | tsurf,fract,dist_star,aerosol,cpp3D, & |
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| 4 | dtlw,dtsw,fluxsurf_lw, & |
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| 5 | fluxsurf_sw,fluxtop_lw,fluxabs_sw,fluxtop_dn, & |
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| 6 | reffrad,tau_col,ptime,pday,cloudfrac,totcloudfrac, & |
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| 7 | clearsky,firstcall,lastcall) |
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| 8 | |
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| 9 | use radinc_h |
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| 10 | use radcommon_h |
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| 11 | use watercommon_h |
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| 12 | use ioipsl_getincom |
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| 13 | |
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| 14 | implicit none |
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| 15 | |
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| 16 | !================================================================== |
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| 17 | ! |
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| 18 | ! Purpose |
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| 19 | ! ------- |
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| 20 | ! Solve the radiative transfer using the correlated-k method for |
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| 21 | ! the gaseous absorption and the Toon et al. (1989) method for |
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| 22 | ! scatttering due to aerosols. |
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| 23 | ! |
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| 24 | ! Authors |
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| 25 | ! ------- |
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| 26 | ! Emmanuel 01/2001, Forget 09/2001 |
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| 27 | ! Robin Wordsworth (2009) |
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| 28 | ! |
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| 29 | !================================================================== |
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| 30 | |
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| 31 | #include "dimphys.h" |
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| 32 | #include "datafile.h" |
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| 33 | #include "comcstfi.h" |
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| 34 | #include "callkeys.h" |
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| 35 | #include "tracer.h" |
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| 36 | |
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| 37 | !----------------------------------------------------------------------- |
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| 38 | ! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid |
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| 39 | ! Layer #1 is the layer near the ground. |
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| 40 | ! Layer #nlayermx is the layer at the top. |
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| 41 | |
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| 42 | ! INPUT |
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| 43 | INTEGER icount |
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| 44 | INTEGER ngrid,nlayer |
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| 45 | REAL aerosol(ngrid,nlayermx,naerkind) ! aerosol tau (kg/kg) |
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| 46 | REAL albedo(ngrid) ! SW albedo |
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| 47 | REAL emis(ngrid) ! LW emissivity |
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| 48 | REAL pplay(ngrid,nlayermx) ! pres. level in GCM mid of layer |
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| 49 | REAL pplev(ngrid,nlayermx+1) ! pres. level at GCM layer boundaries |
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| 50 | |
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| 51 | REAL pt(ngrid,nlayermx) ! air temperature (K) |
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| 52 | REAL tsurf(ngrid) ! surface temperature (K) |
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| 53 | REAL dist_star,mu0(ngrid) ! distance star-planet (AU) |
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| 54 | REAL fract(ngrid) ! fraction of day |
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| 55 | |
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| 56 | ! Globally varying aerosol optical properties on GCM grid |
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| 57 | ! Not needed everywhere so not in radcommon_h |
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| 58 | REAL :: QVISsQREF3d(ngridmx,nlayermx,L_NSPECTV,naerkind) |
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| 59 | REAL :: omegaVIS3d(ngridmx,nlayermx,L_NSPECTV,naerkind) |
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| 60 | REAL :: gVIS3d(ngridmx,nlayermx,L_NSPECTV,naerkind) |
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| 61 | |
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| 62 | REAL :: QIRsQREF3d(ngridmx,nlayermx,L_NSPECTI,naerkind) |
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| 63 | REAL :: omegaIR3d(ngridmx,nlayermx,L_NSPECTI,naerkind) |
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| 64 | REAL :: gIR3d(ngridmx,nlayermx,L_NSPECTI,naerkind) |
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| 65 | |
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| 66 | REAL :: QREFvis3d(ngridmx,nlayermx,naerkind) |
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| 67 | REAL :: QREFir3d(ngridmx,nlayermx,naerkind) |
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| 68 | |
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| 69 | ! REAL :: omegaREFvis3d(ngridmx,nlayermx,naerkind) |
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| 70 | ! REAL :: omegaREFir3d(ngridmx,nlayermx,naerkind) ! not sure of the point of these... |
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| 71 | |
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| 72 | REAL reffrad(ngrid,nlayer,naerkind) |
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| 73 | REAL nueffrad(ngrid,nlayer,naerkind) |
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| 74 | |
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| 75 | ! OUTPUT |
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| 76 | REAL dtsw(ngridmx,nlayermx) ! heating rate (K/s) due to SW |
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| 77 | REAL dtlw(ngridmx,nlayermx) ! heating rate (K/s) due to LW |
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| 78 | REAL fluxsurf_lw(ngridmx) ! incident LW flux to surf (W/m2) |
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| 79 | REAL fluxtop_lw(ngridmx) ! outgoing LW flux to space (W/m2) |
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| 80 | REAL fluxsurf_sw(ngridmx) ! incident SW flux to surf (W/m2) |
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| 81 | REAL fluxabs_sw(ngridmx) ! SW flux absorbed by planet (W/m2) |
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| 82 | REAL fluxtop_dn(ngridmx) ! incident top of atmosphere SW flux (W/m2) |
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| 83 | |
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| 84 | !----------------------------------------------------------------------- |
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| 85 | ! Declaration of the variables required by correlated-k subroutines |
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| 86 | ! Numbered from top to bottom unlike in the GCM! |
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| 87 | |
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| 88 | REAL*8 tmid(L_LEVELS),pmid(L_LEVELS) |
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| 89 | REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS) |
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| 90 | |
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| 91 | ! Optical values for the optci/cv subroutines |
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| 92 | REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV) |
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| 93 | REAL*8 dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 94 | REAL*8 dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 95 | REAL*8 cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 96 | REAL*8 cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 97 | REAL*8 wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS) |
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| 98 | REAL*8 wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS) |
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| 99 | REAL*8 tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS) |
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| 100 | REAL*8 taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS) |
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| 101 | REAL*8 taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS) |
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| 102 | |
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| 103 | REAL*8 tauaero(L_LEVELS+1,naerkind) |
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| 104 | REAL*8 nfluxtopv,nfluxtopi,nfluxtop |
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| 105 | real*8 NFLUXTOPV_nu(L_NSPECTV) |
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| 106 | real*8 NFLUXTOPI_nu(L_NSPECTI) |
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| 107 | real*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! for 1D diagnostic |
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| 108 | REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD) |
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| 109 | REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD) |
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| 110 | REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD) |
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| 111 | REAL*8 albi,albv,acosz |
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| 112 | |
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| 113 | INTEGER ig,l,k,nw,iaer,irad |
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| 114 | |
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| 115 | real fluxtoplanet |
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| 116 | real*8 taugsurf(L_NSPECTV,L_NGAUSS-1) |
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| 117 | real*8 taugsurfi(L_NSPECTI,L_NGAUSS-1) |
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| 118 | |
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| 119 | real*8 qvar(L_LEVELS) ! mixing ratio of variable component |
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| 120 | REAL pq(ngridmx,nlayer,nq) |
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| 121 | REAL qsurf(ngridmx,nqmx) ! tracer on surface (e.g. kg.m-2) |
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| 122 | integer nq |
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| 123 | |
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| 124 | ! Local aerosol optical properties for each column on RADIATIVE grid |
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| 125 | real*8 QXVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 126 | real*8 QSVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 127 | real*8 GVAER(L_LEVELS+1,L_NSPECTV,naerkind) |
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| 128 | real*8 QXIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 129 | real*8 QSIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 130 | real*8 GIAER(L_LEVELS+1,L_NSPECTI,naerkind) |
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| 131 | |
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| 132 | save qxvaer, qsvaer, gvaer |
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| 133 | save qxiaer, qsiaer, giaer |
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| 134 | save QREFvis3d, QREFir3d |
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| 135 | |
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| 136 | REAL tau_col(ngrid) ! diagnostic from aeropacity |
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| 137 | |
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| 138 | ! Misc. |
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| 139 | logical firstcall, lastcall, nantest |
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| 140 | real*8 tempv(L_NSPECTV) |
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| 141 | real*8 tempi(L_NSPECTI) |
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| 142 | real*8 temp,temp1,temp2,pweight |
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| 143 | character(len=10) :: tmp1 |
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| 144 | character(len=10) :: tmp2 |
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| 145 | |
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| 146 | ! for fixed water vapour profiles |
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| 147 | integer i_var |
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| 148 | real RH |
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| 149 | real*8 pq_temp(nlayer) |
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| 150 | real ptemp, Ttemp, qsat |
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| 151 | |
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| 152 | ! real(KIND=r8) :: pq_temp(nlayer) ! better F90 way.. DOESNT PORT TO F77!!! |
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| 153 | |
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| 154 | ! for OLR spec |
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| 155 | integer OLRcount |
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| 156 | save OLRcount |
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| 157 | integer OLRcount2 |
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| 158 | save OLRcount2 |
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| 159 | character(len=2) :: tempOLR |
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| 160 | character(len=30) :: filenomOLR |
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| 161 | real ptime, pday |
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| 162 | logical OLRz |
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| 163 | real OLR_nu(ngrid,L_NSPECTI) |
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| 164 | |
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| 165 | real GSR_nu(ngrid,L_NSPECTV) |
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| 166 | real*8 NFLUXGNDV_nu(L_NSPECTV) |
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| 167 | |
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| 168 | ! for H2O cloud fraction in aeropacity |
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| 169 | real cloudfrac(ngridmx,nlayermx) |
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| 170 | real totcloudfrac(ngridmx) |
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| 171 | logical clearsky |
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| 172 | |
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| 173 | ! Allow variations in cp with location |
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| 174 | real cpp3D(ngridmx,nlayermx) ! specific heat capacity at const. pressure |
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| 175 | |
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| 176 | ! for weird cloud test |
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| 177 | real pqtest(ngridmx,nlayer,nq) |
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| 178 | |
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| 179 | ! for Dave Crisp LBL data comparison |
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| 180 | logical crisp |
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| 181 | |
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| 182 | ! are particle radii fixed? |
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| 183 | logical radfixed |
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| 184 | real maxrad, minrad |
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| 185 | |
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| 186 | real CBRT |
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| 187 | external CBRT |
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| 188 | |
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| 189 | crisp=.false. |
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| 190 | radfixed=.false. |
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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 | call system('rm -f surf_vals_long.out') |
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| 206 | |
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| 207 | !-------------------------------------------------- |
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| 208 | ! Effective radius and variance of the aerosols |
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| 209 | |
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| 210 | ! CO2 ice: |
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| 211 | DO l=1,nlayer |
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| 212 | DO ig=1,ngrid |
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| 213 | reffrad(ig,l,1) = 1.e-4 |
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| 214 | nueffrad(ig,l,1) = 0.1 |
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| 215 | ! these values will change once the microphysics gets to work |
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| 216 | ! UNLESS tracer=.false., in which case we should be working with |
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| 217 | ! a fixed aerosol layer, and be able to define reffrad in a |
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| 218 | ! .def file. To be improved! |
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| 219 | ENDDO |
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| 220 | ENDDO |
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| 221 | |
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| 222 | ! H2O ice: |
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| 223 | if(naerkind.eq.2)then |
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| 224 | DO l=1,nlayer |
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| 225 | DO ig=1,ngrid |
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| 226 | reffrad(ig,l,naerkind) = 1.e-5 |
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| 227 | nueffrad(ig,l,naerkind) = 0.1 |
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| 228 | ENDDO |
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| 229 | ENDDO |
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| 230 | endif |
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| 231 | |
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| 232 | print*, "Correlated-k data base folder:",datafile |
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| 233 | call getin("corrkdir",corrkdir) |
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| 234 | print*, "corrkdir = ",corrkdir |
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| 235 | write( tmp1, '(i3)' ) L_NSPECTI |
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| 236 | write( tmp2, '(i3)' ) L_NSPECTV |
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| 237 | banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2)) |
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| 238 | banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir)) |
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| 239 | |
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| 240 | call sugas_corrk ! set up gaseous absorption properties |
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| 241 | call setspi ! basic infrared properties |
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| 242 | call setspv ! basic visible properties |
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| 243 | call suaer_corrk ! set up aerosol optical properties |
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| 244 | |
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| 245 | Cmk= 0.01 * 1.0 / (g * mugaz * 1.672621e-27) ! q_main=1.0 assumed |
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| 246 | |
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| 247 | if((igcm_h2o_vap.eq.0) .and. varactive)then |
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| 248 | print*,'varactive in callcorrk but no h2o_vap tracer.' |
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| 249 | stop |
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| 250 | endif |
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| 251 | |
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| 252 | firstcall=.false. |
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| 253 | |
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| 254 | end if |
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| 255 | |
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| 256 | !======================================================================= |
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| 257 | ! Initialization on every call |
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| 258 | |
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| 259 | do l=1,nlayer |
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| 260 | do ig=1,ngrid |
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| 261 | do iaer=1,naerkind |
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| 262 | nueffrad(ig,l,iaer) = 0.1 ! stays at 0.1 |
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| 263 | enddo |
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| 264 | enddo |
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| 265 | enddo |
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| 266 | |
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| 267 | |
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| 268 | if(radfixed)then |
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| 269 | do l=1,nlayer |
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| 270 | do ig=1,ngrid |
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| 271 | reffrad(ig,l,1) = 5.e-5 ! CO2 ice |
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| 272 | enddo |
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| 273 | enddo |
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| 274 | print*,'CO2 ice particle size = ',reffrad(1,1,1)/1.e-6,' um' |
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| 275 | if(naerkind.ge.2)then |
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| 276 | do l=1,nlayer |
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| 277 | do ig=1,ngrid |
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| 278 | reffrad(ig,l,2) = 2.e-5 ! H2O ice |
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| 279 | enddo |
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| 280 | enddo |
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| 281 | print*,'H2O ice particle size = ',reffrad(1,1,2)/1.e-6,' um' |
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| 282 | endif |
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| 283 | if(naerkind.eq.3)then |
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| 284 | do l=1,nlayer |
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| 285 | do ig=1,ngrid |
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| 286 | reffrad(ig,l,naerkind) = 2.e-6 ! dust |
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| 287 | enddo |
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| 288 | enddo |
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| 289 | print*,'Dust particle size = ',reffrad(1,1,naerkind)/1.e-6,' um' |
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| 290 | endif |
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| 291 | if(naerkind.gt.3)then |
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| 292 | print*,'Code not general enough to deal with naerkind > 3 yet.' |
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| 293 | call abort |
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| 294 | endif |
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| 295 | |
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| 296 | else |
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| 297 | |
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| 298 | maxrad=0.0 |
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| 299 | minrad=1.0 |
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| 300 | do l=1,nlayer |
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| 301 | do ig=1,ngrid |
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| 302 | |
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| 303 | if(tracer)then |
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| 304 | reffrad(ig,l,1) = CBRT( 3*pq(ig,l,igcm_co2_ice)/ & |
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| 305 | (4*Nmix_co2*pi*rho_co2) ) |
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| 306 | endif |
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| 307 | reffrad(ig,l,1) = max(reffrad(ig,l,1),1.e-6) |
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| 308 | reffrad(ig,l,1) = min(reffrad(ig,l,1),500.e-6) |
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| 309 | |
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| 310 | maxrad = max(reffrad(ig,l,1),maxrad) |
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| 311 | minrad = min(reffrad(ig,l,1),minrad) |
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| 312 | enddo |
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| 313 | enddo |
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| 314 | if(igcm_co2_ice.gt.0)then |
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| 315 | print*,'Max. CO2 ice particle size = ',maxrad/1.e-6,' um' |
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| 316 | print*,'Min. CO2 ice particle size = ',minrad/1.e-6,' um' |
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| 317 | endif |
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| 318 | |
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| 319 | if((naerkind.ge.2).and.water)then |
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| 320 | maxrad=0.0 |
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| 321 | minrad=1.0 |
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| 322 | do l=1,nlayer |
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| 323 | do ig=1,ngrid |
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| 324 | reffrad(ig,l,2) = CBRT( 3*pq(ig,l,igcm_h2o_ice)/ & |
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| 325 | (4*Nmix_h2o*pi*rho_ice) ) |
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| 326 | reffrad(ig,l,2) = max(reffrad(ig,l,2),1.e-6) |
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| 327 | reffrad(ig,l,2) = min(reffrad(ig,l,2),100.e-6) |
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| 328 | |
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| 329 | maxrad = max(reffrad(ig,l,2),maxrad) |
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| 330 | minrad = min(reffrad(ig,l,2),minrad) |
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| 331 | enddo |
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| 332 | enddo |
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| 333 | print*,'Max. H2O ice particle size = ',maxrad/1.e-6,' um' |
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| 334 | print*,'Min. H2O ice particle size = ',minrad/1.e-6,' um' |
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| 335 | endif |
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| 336 | |
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| 337 | if(naerkind.eq.3)then |
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| 338 | do l=1,nlayer |
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| 339 | do ig=1,ngrid |
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| 340 | reffrad(ig,l,naerkind) = 2.e-6 ! dust |
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| 341 | enddo |
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| 342 | enddo |
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| 343 | endif |
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| 344 | |
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| 345 | endif |
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| 346 | |
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| 347 | ! how much light we get |
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| 348 | fluxtoplanet=0 |
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| 349 | do nw=1,L_NSPECTV |
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| 350 | stel(nw)=stellarf(nw)/(dist_star**2) |
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| 351 | fluxtoplanet=fluxtoplanet + stel(nw) |
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| 352 | end do |
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| 353 | |
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| 354 | call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, & |
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| 355 | QVISsQREF3d,omegaVIS3d,gVIS3d, & |
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| 356 | QIRsQREF3d,omegaIR3d,gIR3d, & |
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| 357 | QREFvis3d,QREFir3d) ! get 3D aerosol optical properties |
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| 358 | |
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| 359 | call aeropacity(ngrid,nlayer,nq,pplay,pplev,pq,aerosol, & |
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| 360 | reffrad,QREFvis3d,QREFir3d, & |
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| 361 | tau_col,cloudfrac,totcloudfrac,clearsky) ! get aerosol optical depths |
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| 362 | |
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| 363 | !----------------------------------------------------------------------- |
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| 364 | ! Starting Big Loop over every GCM column |
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| 365 | do ig=1,ngridmx |
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| 366 | |
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| 367 | !======================================================================= |
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| 368 | ! Transformation of the GCM variables |
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| 369 | |
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| 370 | !----------------------------------------------------------------------- |
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| 371 | ! Aerosol optical properties Qext, Qscat and g |
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| 372 | ! The transformation in the vertical is the same as for temperature |
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| 373 | |
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| 374 | ! shortwave |
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| 375 | do iaer=1,naerkind |
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| 376 | DO nw=1,L_NSPECTV |
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| 377 | do l=1,nlayermx |
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| 378 | |
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| 379 | temp1=QVISsQREF3d(ig,nlayermx+1-l,nw,iaer) & |
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| 380 | *QREFvis3d(ig,nlayermx+1-l,iaer) |
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| 381 | |
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| 382 | temp2=QVISsQREF3d(ig,max(nlayermx-l,1),nw,iaer) & |
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| 383 | *QREFvis3d(ig,max(nlayermx-l,1),iaer) |
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| 384 | |
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| 385 | qxvaer(2*l,nw,iaer) = temp1 |
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| 386 | qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
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| 387 | |
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| 388 | temp1=temp1*omegavis3d(ig,nlayermx+1-l,nw,iaer) |
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| 389 | temp2=temp2*omegavis3d(ig,max(nlayermx-l,1),nw,iaer) |
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| 390 | |
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| 391 | qsvaer(2*l,nw,iaer) = temp1 |
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| 392 | qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
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| 393 | |
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| 394 | temp1=gvis3d(ig,nlayermx+1-l,nw,iaer) |
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| 395 | temp2=gvis3d(ig,max(nlayermx-l,1),nw,iaer) |
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| 396 | |
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| 397 | gvaer(2*l,nw,iaer) = temp1 |
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| 398 | gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
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| 399 | |
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| 400 | end do |
|---|
| 401 | |
|---|
| 402 | qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer) |
|---|
| 403 | qxvaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 404 | |
|---|
| 405 | qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer) |
|---|
| 406 | qsvaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 407 | |
|---|
| 408 | gvaer(1,nw,iaer)=gvaer(2,nw,iaer) |
|---|
| 409 | gvaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 410 | |
|---|
| 411 | end do |
|---|
| 412 | |
|---|
| 413 | |
|---|
| 414 | ! longwave |
|---|
| 415 | DO nw=1,L_NSPECTI |
|---|
| 416 | do l=1,nlayermx |
|---|
| 417 | |
|---|
| 418 | temp1=QIRsQREF3d(ig,nlayermx+1-l,nw,iaer) & |
|---|
| 419 | *QREFir3d(ig,nlayermx+1-l,iaer) |
|---|
| 420 | |
|---|
| 421 | temp2=QIRsQREF3d(ig,max(nlayermx-l,1),nw,iaer) & |
|---|
| 422 | *QREFir3d(ig,max(nlayermx-l,1),iaer) |
|---|
| 423 | |
|---|
| 424 | qxiaer(2*l,nw,iaer) = temp1 |
|---|
| 425 | qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 426 | |
|---|
| 427 | temp1=temp1*omegair3d(ig,nlayermx+1-l,nw,iaer) |
|---|
| 428 | temp2=temp2*omegair3d(ig,max(nlayermx-l,1),nw,iaer) |
|---|
| 429 | |
|---|
| 430 | qsiaer(2*l,nw,iaer) = temp1 |
|---|
| 431 | qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 432 | |
|---|
| 433 | temp1=gir3d(ig,nlayermx+1-l,nw,iaer) |
|---|
| 434 | temp2=gir3d(ig,max(nlayermx-l,1),nw,iaer) |
|---|
| 435 | |
|---|
| 436 | giaer(2*l,nw,iaer) = temp1 |
|---|
| 437 | giaer(2*l+1,nw,iaer)=(temp1+temp2)/2 |
|---|
| 438 | |
|---|
| 439 | end do |
|---|
| 440 | |
|---|
| 441 | qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer) |
|---|
| 442 | qxiaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 443 | |
|---|
| 444 | qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer) |
|---|
| 445 | qsiaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 446 | |
|---|
| 447 | giaer(1,nw,iaer)=giaer(2,nw,iaer) |
|---|
| 448 | giaer(2*nlayermx+1,nw,iaer)=0. |
|---|
| 449 | |
|---|
| 450 | end do |
|---|
| 451 | end do |
|---|
| 452 | |
|---|
| 453 | |
|---|
| 454 | ! test / correct for freaky s. s. albedo values |
|---|
| 455 | do iaer=1,naerkind |
|---|
| 456 | do k=1,L_LEVELS+1 |
|---|
| 457 | |
|---|
| 458 | do nw=1,L_NSPECTV |
|---|
| 459 | if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then |
|---|
| 460 | print*,'Serious problems with qsvaer values in callcorrk' |
|---|
| 461 | call abort |
|---|
| 462 | endif |
|---|
| 463 | if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then |
|---|
| 464 | qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer) |
|---|
| 465 | endif |
|---|
| 466 | end do |
|---|
| 467 | |
|---|
| 468 | do nw=1,L_NSPECTI |
|---|
| 469 | if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then |
|---|
| 470 | print*,'Serious problems with qsiaer values in callcorrk' |
|---|
| 471 | call abort |
|---|
| 472 | endif |
|---|
| 473 | if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then |
|---|
| 474 | qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer) |
|---|
| 475 | endif |
|---|
| 476 | end do |
|---|
| 477 | |
|---|
| 478 | end do |
|---|
| 479 | end do |
|---|
| 480 | |
|---|
| 481 | !----------------------------------------------------------------------- |
|---|
| 482 | ! Aerosol optical depths |
|---|
| 483 | |
|---|
| 484 | do iaer=1,naerkind ! a bug was here |
|---|
| 485 | do k=0,nlayer-1 |
|---|
| 486 | |
|---|
| 487 | pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ & |
|---|
| 488 | (pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1)) |
|---|
| 489 | |
|---|
| 490 | temp=aerosol(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer) |
|---|
| 491 | |
|---|
| 492 | tauaero(2*k+2,iaer)=max(temp*pweight,0.0) |
|---|
| 493 | tauaero(2*k+3,iaer)=max(temp-tauaero(2*k+2,iaer),0.0) |
|---|
| 494 | ! |
|---|
| 495 | end do |
|---|
| 496 | ! boundary conditions |
|---|
| 497 | tauaero(1,iaer) = tauaero(2,iaer) |
|---|
| 498 | tauaero(L_LEVELS+1,iaer) = tauaero(L_LEVELS,iaer) |
|---|
| 499 | !tauaero(1,iaer) = 0. |
|---|
| 500 | !tauaero(L_LEVELS+1,iaer) = 0. |
|---|
| 501 | end do |
|---|
| 502 | !print*,'Note changed tauaero BCs in callcorrk!' |
|---|
| 503 | |
|---|
| 504 | ! Albedo and emissivity |
|---|
| 505 | albi=1-emis(ig) ! longwave |
|---|
| 506 | albv=albedo(ig) ! shortwave |
|---|
| 507 | |
|---|
| 508 | if(noradsurf.and.(albv.gt.0.0))then |
|---|
| 509 | print*,'For open lower boundary in callcorrk must' |
|---|
| 510 | print*,'have surface albedo set to zero!' |
|---|
| 511 | call abort |
|---|
| 512 | endif |
|---|
| 513 | |
|---|
| 514 | if(ngridmx.eq.1) then ! fixed zenith angle in 1D |
|---|
| 515 | acosz = cos(pi*szangle/180.0) |
|---|
| 516 | !acosz=mu0(ig) |
|---|
| 517 | !print*,'oned SZ angle OVERRIDE in callcorrk' |
|---|
| 518 | print*,'acosz=',acosz,', szangle=',szangle |
|---|
| 519 | else |
|---|
| 520 | acosz=mu0(ig) ! cosine of sun incident angle |
|---|
| 521 | endif |
|---|
| 522 | |
|---|
| 523 | !----------------------------------------------------------------------- |
|---|
| 524 | ! Water vapour (to be generalised / ignored for other planets) |
|---|
| 525 | |
|---|
| 526 | if(varactive) then |
|---|
| 527 | |
|---|
| 528 | i_var=igcm_h2o_vap |
|---|
| 529 | |
|---|
| 530 | do l=1,nlayer |
|---|
| 531 | |
|---|
| 532 | qvar(2*l) = pq(ig,nlayer+1-l,i_var) |
|---|
| 533 | qvar(2*l+1) = (pq(ig,nlayer+1-l,i_var)+pq(ig,max(nlayer-l,1),i_var))/2 |
|---|
| 534 | ! Average approximation as for temperature... |
|---|
| 535 | |
|---|
| 536 | end do |
|---|
| 537 | qvar(1)=qvar(2) |
|---|
| 538 | qvar(2*nlayermx+1)=qsurf(ig,i_var) |
|---|
| 539 | |
|---|
| 540 | elseif(varfixed)then |
|---|
| 541 | |
|---|
| 542 | do l=1,nlayermx ! here we will assign fixed water vapour profiles globally |
|---|
| 543 | RH = satval * ((pplay(ig,l)/pplev(ig,1) - 0.02) / 0.98) |
|---|
| 544 | if(RH.lt.0.0) RH=0.0 |
|---|
| 545 | |
|---|
| 546 | ptemp=pplay(ig,l) |
|---|
| 547 | Ttemp=pt(ig,l) |
|---|
| 548 | call watersat(Ttemp,ptemp,qsat) |
|---|
| 549 | |
|---|
| 550 | !pq_temp(l) = qsat ! fully saturated everywhere |
|---|
| 551 | pq_temp(l) = RH * qsat ! ~realistic profile (e.g. 80% saturation at ground) |
|---|
| 552 | end do |
|---|
| 553 | |
|---|
| 554 | do l=1,nlayer |
|---|
| 555 | qvar(2*l) = pq_temp(nlayer+1-l) |
|---|
| 556 | qvar(2*l+1) = (pq_temp(nlayer+1-l)+pq_temp(max(nlayer-l,1)))/2 |
|---|
| 557 | end do |
|---|
| 558 | qvar(1)=qvar(2) |
|---|
| 559 | |
|---|
| 560 | ! Lowest layer of atmosphere |
|---|
| 561 | RH = satval * (1 - 0.02) / 0.98 |
|---|
| 562 | if(RH.lt.0.0) RH=0.0 |
|---|
| 563 | |
|---|
| 564 | ptemp = pplev(ig,1) |
|---|
| 565 | Ttemp = tsurf(ig) |
|---|
| 566 | call watersat(Ttemp,ptemp,qsat) |
|---|
| 567 | |
|---|
| 568 | !qvar(2*nlayermx+1)=qsat ! fully saturated everywhere |
|---|
| 569 | qvar(2*nlayermx+1)= RH * qsat ! ~realistic profile (e.g. 80% saturation at ground) |
|---|
| 570 | |
|---|
| 571 | else |
|---|
| 572 | do k=1,L_LEVELS |
|---|
| 573 | qvar(k) = 1.0D-7 |
|---|
| 574 | end do |
|---|
| 575 | end if |
|---|
| 576 | |
|---|
| 577 | ! Now convert from kg/kg to mol/mol |
|---|
| 578 | do k=1,L_LEVELS |
|---|
| 579 | qvar(k) = qvar(k)/epsi |
|---|
| 580 | end do |
|---|
| 581 | |
|---|
| 582 | ! Keep values inside limits for which we have radiative transfer coefficients |
|---|
| 583 | if(L_REFVAR.gt.1)then ! there was a bug here! |
|---|
| 584 | do k=1,L_LEVELS |
|---|
| 585 | if(qvar(k).lt.wrefvar(1))then |
|---|
| 586 | qvar(k)=wrefvar(1)+1.0e-8 |
|---|
| 587 | elseif(qvar(k).gt.wrefvar(L_REFVAR))then |
|---|
| 588 | qvar(k)=wrefvar(L_REFVAR)-1.0e-8 |
|---|
| 589 | endif |
|---|
| 590 | end do |
|---|
| 591 | endif |
|---|
| 592 | |
|---|
| 593 | !----------------------------------------------------------------------- |
|---|
| 594 | ! Pressure and temperature |
|---|
| 595 | |
|---|
| 596 | DO l=1,nlayer |
|---|
| 597 | plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep |
|---|
| 598 | plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep |
|---|
| 599 | tlevrad(2*l) = pt(ig,nlayer+1-l) |
|---|
| 600 | tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2 |
|---|
| 601 | END DO |
|---|
| 602 | |
|---|
| 603 | plevrad(1) = 0 |
|---|
| 604 | plevrad(2) = max(pgasmin,0.0001*plevrad(3)) |
|---|
| 605 | |
|---|
| 606 | tlevrad(1) = tlevrad(2) |
|---|
| 607 | tlevrad(2*nlayermx+1)=tsurf(ig) |
|---|
| 608 | |
|---|
| 609 | |
|---|
| 610 | if(crisp)then |
|---|
| 611 | open(111,file='/u/rwlmd/CrispLBL/p.dat') |
|---|
| 612 | open(112,file='/u/rwlmd/CrispLBL/T.dat') |
|---|
| 613 | do k=1,L_LEVELS |
|---|
| 614 | read(111,*) plevrad(k) |
|---|
| 615 | read(112,*) tlevrad(k) |
|---|
| 616 | plevrad(k)=plevrad(k)*1000.0 |
|---|
| 617 | enddo |
|---|
| 618 | close(111) |
|---|
| 619 | close(112) |
|---|
| 620 | endif |
|---|
| 621 | |
|---|
| 622 | tmid(1) = tlevrad(2) |
|---|
| 623 | tmid(2) = tlevrad(2) |
|---|
| 624 | pmid(1) = plevrad(2) |
|---|
| 625 | pmid(2) = plevrad(2) |
|---|
| 626 | |
|---|
| 627 | DO l=1,L_NLAYRAD-1 |
|---|
| 628 | tmid(2*l+1) = tlevrad(2*l+1) |
|---|
| 629 | tmid(2*l+2) = tlevrad(2*l+1) |
|---|
| 630 | pmid(2*l+1) = plevrad(2*l+1) |
|---|
| 631 | pmid(2*l+2) = plevrad(2*l+1) |
|---|
| 632 | END DO |
|---|
| 633 | pmid(L_LEVELS) = plevrad(L_LEVELS) |
|---|
| 634 | tmid(L_LEVELS) = tlevrad(L_LEVELS) |
|---|
| 635 | |
|---|
| 636 | |
|---|
| 637 | ! test for out-of-bounds pressure |
|---|
| 638 | if(plevrad(3).lt.pgasmin)then |
|---|
| 639 | print*,'Minimum pressure is outside the radiative' |
|---|
| 640 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 641 | call abort |
|---|
| 642 | elseif(plevrad(L_LEVELS).gt.pgasmax)then |
|---|
| 643 | print*,'Maximum pressure is outside the radiative' |
|---|
| 644 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 645 | call abort |
|---|
| 646 | endif |
|---|
| 647 | |
|---|
| 648 | ! test for out-of-bounds temperature |
|---|
| 649 | do k=1,L_LEVELS |
|---|
| 650 | if(tlevrad(k).lt.tgasmin)then |
|---|
| 651 | print*,'Minimum temperature is outside the radiative' |
|---|
| 652 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 653 | !print*,'WARNING, OVERRIDING FOR TEST' |
|---|
| 654 | call abort |
|---|
| 655 | elseif(tlevrad(k).gt.tgasmax)then |
|---|
| 656 | print*,'Maximum temperature is outside the radiative' |
|---|
| 657 | print*,'transfer kmatrix bounds, exiting.' |
|---|
| 658 | !print*,'WARNING, OVERRIDING FOR TEST' |
|---|
| 659 | call abort |
|---|
| 660 | endif |
|---|
| 661 | enddo |
|---|
| 662 | |
|---|
| 663 | !======================================================================= |
|---|
| 664 | ! Calling the main radiative transfer subroutines |
|---|
| 665 | |
|---|
| 666 | |
|---|
| 667 | !----------------------------------------------------------------------- |
|---|
| 668 | ! Shortwave |
|---|
| 669 | |
|---|
| 670 | if(fract(ig) .ge. 1.0e-4) then ! only during daylight! |
|---|
| 671 | |
|---|
| 672 | fluxtoplanet=0. |
|---|
| 673 | |
|---|
| 674 | if((ngridmx.eq.1).and.(.not.(diurnal.or.tlocked)))then |
|---|
| 675 | do nw=1,L_NSPECTV |
|---|
| 676 | stel_fract(nw)= stel(nw) * 0.25 / acosz |
|---|
| 677 | fluxtoplanet=fluxtoplanet + stel_fract(nw) |
|---|
| 678 | ! globally averaged = divide by 4 |
|---|
| 679 | ! but we correct for solar zenith angle |
|---|
| 680 | end do |
|---|
| 681 | else |
|---|
| 682 | do nw=1,L_NSPECTV |
|---|
| 683 | stel_fract(nw)= stel(nw) * fract(ig) |
|---|
| 684 | fluxtoplanet=fluxtoplanet + stel_fract(nw) |
|---|
| 685 | end do |
|---|
| 686 | endif |
|---|
| 687 | |
|---|
| 688 | call optcv(dtauv,tauv,taucumv,plevrad, & |
|---|
| 689 | qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, & |
|---|
| 690 | tmid,pmid,taugsurf,qvar) |
|---|
| 691 | |
|---|
| 692 | |
|---|
| 693 | call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, & |
|---|
| 694 | acosz,stel_fract,gweight,nfluxtopv,nfluxgndv_nu, & |
|---|
| 695 | fmnetv,fluxupv,fluxdnv,fzerov,taugsurf) |
|---|
| 696 | |
|---|
| 697 | else ! during the night, fluxes = 0 |
|---|
| 698 | nfluxtopv=0.0 |
|---|
| 699 | do l=1,L_NLAYRAD |
|---|
| 700 | fmnetv(l)=0.0 |
|---|
| 701 | fluxupv(l)=0.0 |
|---|
| 702 | fluxdnv(l)=0.0 |
|---|
| 703 | end do |
|---|
| 704 | end if |
|---|
| 705 | |
|---|
| 706 | !print*,'taugsurf=',taugsurf(:,L_NGAUSS-1) |
|---|
| 707 | |
|---|
| 708 | |
|---|
| 709 | !----------------------------------------------------------------------- |
|---|
| 710 | ! Longwave |
|---|
| 711 | |
|---|
| 712 | call optci(plevrad,tlevrad,dtaui,taucumi, & |
|---|
| 713 | qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, & |
|---|
| 714 | taugsurfi,qvar) |
|---|
| 715 | |
|---|
| 716 | call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, & |
|---|
| 717 | wnoi,dwni,cosbi,wbari,gweight,nfluxtopi,nfluxtopi_nu, & |
|---|
| 718 | fmneti,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi) |
|---|
| 719 | |
|---|
| 720 | !----------------------------------------------------------------------- |
|---|
| 721 | ! Transformation of the correlated-k code outputs |
|---|
| 722 | ! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw) |
|---|
| 723 | |
|---|
| 724 | ! Flux incident at the top of the atmosphere |
|---|
| 725 | fluxtop_dn(ig)=fluxdnv(1) |
|---|
| 726 | |
|---|
| 727 | fluxtop_lw(ig) = real(nfluxtopi) |
|---|
| 728 | fluxabs_sw(ig) = real(-nfluxtopv) |
|---|
| 729 | fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD)) |
|---|
| 730 | fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD)) |
|---|
| 731 | |
|---|
| 732 | if(fluxtop_dn(ig).lt.0.0)then |
|---|
| 733 | print*,'Achtung! fluxtop_dn has lost the plot!' |
|---|
| 734 | print*,'fluxtop_dn=',fluxtop_dn(ig) |
|---|
| 735 | print*,'acosz=',acosz |
|---|
| 736 | print*,'aerosol=',aerosol(ig,:,:) |
|---|
| 737 | print*,'temp= ',pt(ig,:) |
|---|
| 738 | print*,'pplay= ',pplay(ig,:) |
|---|
| 739 | call abort |
|---|
| 740 | endif |
|---|
| 741 | |
|---|
| 742 | if(crisp)then |
|---|
| 743 | open(111,file='/u/rwlmd/CrispLBL/GCMfluxdn.dat') |
|---|
| 744 | open(112,file='/u/rwlmd/CrispLBL/GCMfluxup.dat') |
|---|
| 745 | do k=1,L_NLAYRAD |
|---|
| 746 | write(111,*) fluxdni(k) |
|---|
| 747 | write(112,*) fluxupi(k) |
|---|
| 748 | enddo |
|---|
| 749 | close(111) |
|---|
| 750 | close(112) |
|---|
| 751 | print*,'fluxdni',fluxdni |
|---|
| 752 | print*,'fluxupi',fluxupi |
|---|
| 753 | call abort |
|---|
| 754 | endif |
|---|
| 755 | |
|---|
| 756 | ! Spectral output, for exoplanet observational comparison |
|---|
| 757 | if(specOLR)then |
|---|
| 758 | do nw=1,L_NSPECTI |
|---|
| 759 | OLR_nu(ig,nw)=nfluxtopi_nu(nw) |
|---|
| 760 | end do |
|---|
| 761 | do nw=1,L_NSPECTV |
|---|
| 762 | GSR_nu(ig,nw)=nfluxgndv_nu(nw) |
|---|
| 763 | end do |
|---|
| 764 | endif |
|---|
| 765 | |
|---|
| 766 | ! Finally, the heating rates |
|---|
| 767 | if(nonideal)then |
|---|
| 768 | |
|---|
| 769 | DO l=2,L_NLAYRAD |
|---|
| 770 | dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) & |
|---|
| 771 | *g/(cpp3D(ig,L_NLAYRAD+1-l) & |
|---|
| 772 | *scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 773 | dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) & |
|---|
| 774 | *g/(cpp3D(ig,L_NLAYRAD+1-l) & |
|---|
| 775 | *scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 776 | END DO |
|---|
| 777 | |
|---|
| 778 | ! These are values at top of atmosphere |
|---|
| 779 | dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) & |
|---|
| 780 | *g/(cpp3D(ig,L_NLAYRAD)*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 781 | dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) & |
|---|
| 782 | *g/(cpp3D(ig,L_NLAYRAD)*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 783 | |
|---|
| 784 | else |
|---|
| 785 | |
|---|
| 786 | DO l=2,L_NLAYRAD |
|---|
| 787 | dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) & |
|---|
| 788 | *g/(cpp*scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 789 | dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) & |
|---|
| 790 | *g/(cpp*scalep*(plevrad(2*l+1)-plevrad(2*l-1))) |
|---|
| 791 | END DO |
|---|
| 792 | |
|---|
| 793 | ! These are values at top of atmosphere |
|---|
| 794 | dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) & |
|---|
| 795 | *g/(cpp*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 796 | dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) & |
|---|
| 797 | *g/(cpp*scalep*(plevrad(3)-plevrad(1))) |
|---|
| 798 | |
|---|
| 799 | endif |
|---|
| 800 | |
|---|
| 801 | ! --------------------------------------------------------------- |
|---|
| 802 | end do ! end of big loop over every GCM column (ig = 1:ngrid) |
|---|
| 803 | |
|---|
| 804 | |
|---|
| 805 | !----------------------------------------------------------------------- |
|---|
| 806 | ! Additional diagnostics |
|---|
| 807 | |
|---|
| 808 | ! IR spectral output, for exoplanet observational comparison |
|---|
| 809 | if(specOLR)then |
|---|
| 810 | if(ngrid.ne.1)then |
|---|
| 811 | call writediagspec(ngrid,"OLR3D","OLR(lon,lat,band)","W m^-2",3,OLR_nu) |
|---|
| 812 | ! call writediagspec(ngrid,"OSR3D","OSR(lon,lat,band)","W m^-2",3,OSR_nu) |
|---|
| 813 | endif |
|---|
| 814 | endif |
|---|
| 815 | |
|---|
| 816 | if(ngrid.eq.1)then |
|---|
| 817 | open(113,file='surf_vals_long.out',ACCESS='append') |
|---|
| 818 | write(113,*) tsurf(1),fluxtop_dn(1), & |
|---|
| 819 | real(-nfluxtopv),real(nfluxtopi) |
|---|
| 820 | close(113) |
|---|
| 821 | endif |
|---|
| 822 | |
|---|
| 823 | !if(kastprof)then ! for kasthop only |
|---|
| 824 | |
|---|
| 825 | if(ngrid.eq.1)then |
|---|
| 826 | |
|---|
| 827 | print*,'Saving tsurf,psurf in surf_vals.out...' |
|---|
| 828 | open(116,file='surf_vals.out') |
|---|
| 829 | write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), & |
|---|
| 830 | real(-nfluxtopv),real(nfluxtopi) |
|---|
| 831 | close(116) |
|---|
| 832 | |
|---|
| 833 | if(specOLR)then |
|---|
| 834 | open(117,file='OLRnu.out') |
|---|
| 835 | do nw=1,L_NSPECTI |
|---|
| 836 | write(117,*) OLR_nu(1,nw) |
|---|
| 837 | enddo |
|---|
| 838 | close(117) |
|---|
| 839 | |
|---|
| 840 | open(127,file='GSRnu.out') |
|---|
| 841 | do nw=1,L_NSPECTV |
|---|
| 842 | write(127,*) GSR_nu(1,nw) |
|---|
| 843 | enddo |
|---|
| 844 | close(127) |
|---|
| 845 | endif |
|---|
| 846 | |
|---|
| 847 | ! mixing ratio: CO2 ice particles |
|---|
| 848 | if(igcm_co2_ice.ne.0)then |
|---|
| 849 | open(122,file='qCO2ice.out') |
|---|
| 850 | do l=1,L_NLAYRAD |
|---|
| 851 | write(122,*) pq(1,l,igcm_co2_ice) |
|---|
| 852 | enddo |
|---|
| 853 | close(122) |
|---|
| 854 | endif |
|---|
| 855 | |
|---|
| 856 | ! mixing ratio: H2O vapour |
|---|
| 857 | if(igcm_h2o_vap.ne.0)then |
|---|
| 858 | open(123,file='qH2Ovap.out') |
|---|
| 859 | do l=1,L_NLAYRAD |
|---|
| 860 | write(123,*) pq(1,l,igcm_h2o_vap) |
|---|
| 861 | enddo |
|---|
| 862 | close(123) |
|---|
| 863 | endif |
|---|
| 864 | |
|---|
| 865 | ! OLR vs altitude: do it as a .txt file |
|---|
| 866 | OLRz=.false. |
|---|
| 867 | if(OLRz)then |
|---|
| 868 | print*,'saving IR vertical flux for OLRz...' |
|---|
| 869 | open(118,file='OLRz_plevs.out') |
|---|
| 870 | open(119,file='OLRz.out') |
|---|
| 871 | do l=1,L_NLAYRAD |
|---|
| 872 | write(118,*) plevrad(2*l) |
|---|
| 873 | do nw=1,L_NSPECTI |
|---|
| 874 | write(119,*) fluxupi_nu(l,nw) |
|---|
| 875 | enddo |
|---|
| 876 | enddo |
|---|
| 877 | close(118) |
|---|
| 878 | close(119) |
|---|
| 879 | endif |
|---|
| 880 | endif |
|---|
| 881 | |
|---|
| 882 | !endif |
|---|
| 883 | |
|---|
| 884 | end subroutine callcorrk |
|---|
