SUBROUTINE nirco2abs(ngrid,nlayer,pplay,dist_sol,nq,pq, $ mu0,fract,declin,pdtnirco2) IMPLICIT NONE c======================================================================= c subject: c -------- c Computing heating rate due to c absorption by CO2 in the near-infrared c This version includes NLTE effects c c (Scheme to be described in Forget et al., JGR, 2003) c (old Scheme described in Forget et al., JGR, 1999) c c This version updated with a new functional fit, c see NLTE correction-factor of Lopez-Valverde et al (1998) c Stephen Lewis 2000 c c jul 2011 malv+fgg New corrections for NLTE implemented c 08/2002 : correction for bug when running with diurnal=F c c author: Frederic Hourdin 1996 c ------ c Francois Forget 1999 c c input: c ----- c ngrid number of gridpoint of horizontal grid c nlayer Number of layer c dist_sol sun-Mars distance (AU) c mu0(ngridmx) c fract(ngridmx) day fraction of the time interval c declin latitude of subslar point c c output: c ------- c c pdtnirco2(ngrid,nlayer) Heating rate (K/s) c c c======================================================================= c c 0. Declarations : c ------------------ c #include "dimensions.h" #include "dimphys.h" #include "comcstfi.h" #include "callkeys.h" #include "comdiurn.h" #include "NIRdata.h" c----------------------------------------------------------------------- c Input/Output c ------------ INTEGER ngrid,nlayer REAL pplay(ngrid,nlayer) REAL dist_sol,mu0(ngridmx),fract(ngridmx),declin REAL pdtnirco2(ngrid,nlayer) c c Local variables : c ----------------- INTEGER l,ig, n, nstep,i REAL co2heat0, zmu(ngridmx) c special diurnal=F real mu0_int(ngridmx),fract_int(ngridmx),zday_int real ztim1,ztim2,ztim3,step c c local saved variables c --------------------- c p0noonlte is a pressure below which non LTE effects are significant. c REAL p0nonlte c DATA p0nonlte/7.5e-3/ c SAVE p0nonlte c parameters for CO2 heating fit real n_a, n_p0, n_b parameter (n_a=1.1956475) parameter (n_b=1.9628251) parameter (n_p0=0.0015888279) c Variables added to implement NLTE correction factor (feb 2011) real pyy(nlayer) real cor1(nlayer),oldoco2(nlayer),alfa2(nlayer) real p2011,cociente1,merge real cor0,oco2gcm integer nq real pq(ngrid,nlayer,nq) c---------------------------------------------------------------------- c Initialisation c -------------- c co2heat is the heating by CO2 at 700Pa for a zero zenithal angle. co2heat0=n_a*(1.52/dist_sol)**2/daysec c Simple calcul for a given sun incident angle (if diurnal=T) c -------------------------------------------- IF (diurnal) THEN do ig=1,ngrid zmu(ig)=sqrt(1224.*mu0(ig)*mu0(ig)+1.)/35. if(nircorr.eq.1) then do l=1,nlayer pyy(l)=pplay(ig,l) enddo call interpnir(cor1,pyy,nlayer,corgcm,pres1d,npres) call interpnir(oldoco2,pyy,nlayer,oco21d,pres1d,npres) call interpnir(alfa2,pyy,nlayer,alfa,pres1d,npres) endif do l=1,nlayer ! Calculations for the O/CO2 correction if(nircorr.eq.1) then cor0=1./(1.+n_p0/pplay(ig,l))**n_b if(pq(ig,l,1).gt.1.e-6) then oco2gcm=pq(ig,l,3)/pq(ig,l,1) else oco2gcm=1.e6 endif cociente1=oco2gcm/oldoco2(l) merge=alog10(cociente1)*alfa2(l)+alog10(cor0)* $ (1.-alfa2(l)) merge=10**merge p2011=sqrt(merge)*cor0 else if (nircorr.eq.0) then p2011=1. cor1(l)=1. endif if(fract(ig).gt.0.) pdtnirco2(ig,l)= & co2heat0*sqrt((700.*zmu(ig))/pplay(ig,l)) & /(1.+n_p0/pplay(ig,l))**n_b ! Corrections from tabulation $ * cor1(l) * p2011 c OLD SCHEME (forget et al. 1999) c s co2heat0*sqrt((700.*zmu(ig))/pplay(ig,l)) c s / (1+p0nonlte/pplay(ig,l)) enddo enddo c Averaging over diurnal cycle (if diurnal=F) c ------------------------------------------- c NIR CO2 abs is slightly non linear. To remove the diurnal c cycle, it is better to average the heating rate over 1 day rather c than using the mean mu0 computed by mucorr in physiq.F (FF, 1998) ELSE ! if (.not.diurnal) then nstep = 20 ! number of integration step /sol do n=1,nstep zday_int = (n-1)/float(nstep) ztim2=COS(declin)*COS(2.*pi*(zday_int-.5)) ztim3=-COS(declin)*SIN(2.*pi*(zday_int-.5)) CALL solang(ngrid,sinlon,coslon,sinlat,coslat, s ztim1,ztim2,ztim3, s mu0_int,fract_int) do ig=1,ngrid zmu(ig)=sqrt(1224.*mu0_int(ig)*mu0_int(ig)+1.)/35. if(nircorr.eq.1) then do l=1,nlayer pyy(l)=pplay(ig,l) enddo call interpnir(cor1,pyy,nlayer,corgcm,pres1d,npres) call interpnir(oldoco2,pyy,nlayer,oco21d,pres1d,npres) call interpnir(alfa2,pyy,nlayer,alfa,pres1d,npres) endif do l=1,nlayer if(nircorr.eq.1) then cor0=1./(1.+n_p0/pplay(ig,l))**n_b oco2gcm=pq(ig,l,3)/pq(ig,l,1) cociente1=oco2gcm/oldoco2(l) merge=alog10(cociente1)*alfa2(l)+alog10(cor0)* $ (1.-alfa2(l)) merge=10**merge p2011=sqrt(merge)*cor0 else if (nircorr.eq.0) then p2011=1. cor1(l)=1. endif if(fract_int(ig).gt.0.) pdtnirco2(ig,l)= & pdtnirco2(ig,l) + (1/float(nstep))* & co2heat0*sqrt((700.*zmu(ig))/pplay(ig,l)) & /(1.+n_p0/pplay(ig,l))**n_b ! Corrections from tabulation $ * cor1(l) * p2011 enddo enddo end do END IF return end subroutine interpnir(escout,p,nlayer,escin,pin,nl) C C subroutine to perform linear interpolation in pressure from 1D profile C escin(nl) sampled on pressure grid pin(nl) to profile C escout(nlayer) on pressure grid p(nlayer). C real escout(nlayer),p(nlayer) real escin(nl),pin(nl),wm,wp integer nl,nlayer,n1,n,nm,np do n1=1,nlayer if(p(n1) .gt. 1500. .or. p(n1) .lt. 1.0e-13) then escout(n1) = 0.0 else do n = 1,nl-1 if (p(n1).le.pin(n).and.p(n1).ge.pin(n+1)) then nm=n np=n+1 wm=abs(pin(np)-p(n1))/(pin(nm)-pin(np)) wp=1.0 - wm endif enddo escout(n1) = escin(nm)*wm + escin(np)*wp endif enddo return end