SUBROUTINE SFLUXI(PLEV,TLEV,DTAUI,TAUCUMI,UBARI,RSFI,WNOI,DWNI, * COSBI,WBARI,GWEIGHT,NFLUXTOPI,NFLUXTOPI_nu, * FMNETI,fluxupi,fluxdni,fluxupi_nu, * FZEROI,TAUGSURF) use radinc_h use radcommon_h, only: planckir, tlimit,sigma use comcstfi_mod, only: pi implicit none integer NLEVRAD, L, NW, NG, NTS, NTT real*8 TLEV(L_LEVELS), PLEV(L_LEVELS) real*8 TAUCUMI(L_LEVELS,L_NSPECTI,L_NGAUSS) real*8 FMNETI(L_NLAYRAD) real*8 WNOI(L_NSPECTI), DWNI(L_NSPECTI) real*8 DTAUI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) real*8 FMUPI(L_NLEVRAD), FMDI(L_NLEVRAD) real*8 COSBI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) real*8 WBARI(L_NLAYRAD,L_NSPECTI,L_NGAUSS) real*8 GWEIGHT(L_NGAUSS), NFLUXTOPI real*8 NFLUXTOPI_nu(L_NSPECTI) real*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) real*8 FTOPUP real*8 UBARI, RSFI, TSURF, BSURF, TTOP, BTOP, TAUTOP real*8 PLANCK, PLTOP real*8 fluxupi(L_NLAYRAD), fluxdni(L_NLAYRAD) real*8 FZEROI(L_NSPECTI) real*8 taugsurf(L_NSPECTI,L_NGAUSS-1), fzero real*8 fup_tmp(L_NSPECTI),fdn_tmp(L_NSPECTI) real*8 PLANCKSUM,PLANCKREF C======================================================================C NLEVRAD = L_NLEVRAD C ZERO THE NET FLUXES NFLUXTOPI = 0.0D0 DO NW=1,L_NSPECTI NFLUXTOPI_nu(NW) = 0.0D0 DO L=1,L_NLAYRAD FLUXUPI_nu(L,NW) = 0.0D0 fup_tmp(nw)=0.0D0 fdn_tmp(nw)=0.0D0 END DO END DO DO L=1,L_NLAYRAD FMNETI(L) = 0.0D0 FLUXUPI(L) = 0.0D0 FLUXDNI(L) = 0.0D0 END DO C WE NOW ENTER A MAJOR LOOP OVER SPECTRAL INTERVALS IN THE INFRARED C TO CALCULATE THE NET FLUX IN EACH SPECTRAL INTERVAL TTOP = TLEV(2) ! JL12 why not (1) ??? TSURF = TLEV(L_LEVELS) NTS = int(TSURF*NTfac)-NTstar+1 NTT = int(TTOP *NTfac)-NTstar+1 !JL12 corrects the surface planck function so that its integral is equal to sigma Tsurf^4 !JL12 this ensure that no flux is lost due to: !JL12 -truncation of the planck function at high/low wavenumber !JL12 -numerical error during first spectral integration !JL12 -discrepancy between Tsurf and NTS/NTfac PLANCKSUM=0.d0 PLANCKREF=TSURF*TSURF PLANCKREF=sigma*PLANCKREF*PLANCKREF DO NW=1,L_NSPECTI PLANCKSUM=PLANCKSUM+PLANCKIR(NW,NTS)*DWNI(NW) ENDDO PLANCKSUM=PLANCKREF/(PLANCKSUM*Pi) !JL12 DO 501 NW=1,L_NSPECTI C SURFACE EMISSIONS - INDEPENDENT OF GAUSS POINTS BSURF = (1.-RSFI)*PLANCKIR(NW,NTS)*PLANCKSUM !JL12 plancksum see above PLTOP = PLANCKIR(NW,NTT) C If FZEROI(NW) = 1, then the k-coefficients are zero - skip to the C special Gauss point at the end. FZERO = FZEROI(NW) IF(FZERO.ge.0.99) goto 40 DO NG=1,L_NGAUSS-1 if(TAUGSURF(NW,NG).lt. TLIMIT) then fzero = fzero + (1.0D0-FZEROI(NW))*GWEIGHT(NG) goto 30 end if C SET UP THE UPPER AND LOWER BOUNDARY CONDITIONS ON THE IR C CALCULATE THE DOWNWELLING RADIATION AT THE TOP OF THE MODEL C OR THE TOP LAYER WILL COOL TO SPACE UNPHYSICALLY ! TAUTOP = DTAUI(1,NW,NG)*PLEV(2)/(PLEV(4)-PLEV(2)) TAUTOP = TAUCUMI(2,NW,NG) BTOP = (1.0D0-EXP(-TAUTOP/UBARI))*PLTOP C WE CAN NOW SOLVE FOR THE COEFFICIENTS OF THE TWO STREAM C CALL A SUBROUTINE THAT SOLVES FOR THE FLUX TERMS C WITHIN EACH INTERVAL AT THE MIDPOINT WAVENUMBER CALL GFLUXI(NLEVRAD,TLEV,NW,DWNI(NW),DTAUI(1,NW,NG), * TAUCUMI(1,NW,NG), * WBARI(1,NW,NG),COSBI(1,NW,NG),UBARI,RSFI,BTOP, * BSURF,FTOPUP,FMUPI,FMDI) C NOW CALCULATE THE CUMULATIVE IR NET FLUX NFLUXTOPI = NFLUXTOPI+FTOPUP*DWNI(NW)*GWEIGHT(NG)* * (1.0D0-FZEROI(NW)) c and same thing by spectral band... (RDW) NFLUXTOPI_nu(NW) = NFLUXTOPI_nu(NW) * +FTOPUP*DWNI(NW)*GWEIGHT(NG)*(1.0D0-FZEROI(NW)) DO L=1,L_NLEVRAD-1 C CORRECT FOR THE WAVENUMBER INTERVALS FMNETI(L) = FMNETI(L)+(FMUPI(L)-FMDI(L))*DWNI(NW)* * GWEIGHT(NG)*(1.0D0-FZEROI(NW)) FLUXUPI(L) = FLUXUPI(L) + FMUPI(L)*DWNI(NW)*GWEIGHT(NG)* * (1.0D0-FZEROI(NW)) FLUXDNI(L) = FLUXDNI(L) + FMDI(L)*DWNI(NW)*GWEIGHT(NG)* * (1.0D0-FZEROI(NW)) c and same thing by spectral band... (RW) FLUXUPI_nu(L,NW) = FLUXUPI_nu(L,NW) + * FMUPI(L)*DWNI(NW)*GWEIGHT(NG)*(1.0D0-FZEROI(NW)) END DO 30 CONTINUE END DO !End NGAUSS LOOP 40 CONTINUE C SPECIAL 17th Gauss point NG = L_NGAUSS ! TAUTOP = DTAUI(1,NW,NG)*PLEV(2)/(PLEV(4)-PLEV(2)) TAUTOP = TAUCUMI(2,NW,NG) BTOP = (1.0D0-EXP(-TAUTOP/UBARI))*PLTOP C WE CAN NOW SOLVE FOR THE COEFFICIENTS OF THE TWO STREAM C CALL A SUBROUTINE THAT SOLVES FOR THE FLUX TERMS C WITHIN EACH INTERVAL AT THE MIDPOINT WAVENUMBER CALL GFLUXI(NLEVRAD,TLEV,NW,DWNI(NW),DTAUI(1,NW,NG), * TAUCUMI(1,NW,NG), * WBARI(1,NW,NG),COSBI(1,NW,NG),UBARI,RSFI,BTOP, * BSURF,FTOPUP,FMUPI,FMDI) C NOW CALCULATE THE CUMULATIVE IR NET FLUX NFLUXTOPI = NFLUXTOPI+FTOPUP*DWNI(NW)*FZERO c and same thing by spectral band... (RW) NFLUXTOPI_nu(NW) = NFLUXTOPI_nu(NW) * +FTOPUP*DWNI(NW)*FZERO DO L=1,L_NLEVRAD-1 C CORRECT FOR THE WAVENUMBER INTERVALS FMNETI(L) = FMNETI(L)+(FMUPI(L)-FMDI(L))*DWNI(NW)*FZERO FLUXUPI(L) = FLUXUPI(L) + FMUPI(L)*DWNI(NW)*FZERO FLUXDNI(L) = FLUXDNI(L) + FMDI(L)*DWNI(NW)*FZERO c and same thing by spectral band... (RW) FLUXUPI_nu(L,NW) = FLUXUPI_nu(L,NW) + FMUPI(L)*DWNI(NW)*FZERO END DO 501 CONTINUE !End Spectral Interval LOOP C *** END OF MAJOR SPECTRAL INTERVAL LOOP IN THE INFRARED**** RETURN END