subroutine blendrad(ngrid, nlayer, pplay, & zdtsw, zdtlw, zdtnirco2, zdtnlte, dtrad) c c Combine radiative tendencies. LTE contributions (zdtsw and zdtlw) c have been calculated for the first NLAYLTE layers, zdtnirco2 and c zdtnlte have been calculated for all nlayer layers (but zdtnlte may c be zero low down). zdtlw is phased out in favour of zdtnlte with c height; zdtsw is also phased out to remove possible spurious heating c at low pressures. The pressure at which the transition occurs and c the scale over which this happens are set in the nlteparams.h file. c Above layer NLAYLTE the tendency is purely the sum of NLTE contributions. c (Note : nlaylte is calculated by "nlthermeq" and stored in common "yomlw.h") c Stephen Lewis 6/2000 FF c implicit none #include "dimensions.h" #include "dimphys.h" #include "dimradmars.h" #include "nlteparams.h" #include "yomlw.h" c Input: integer ngrid, nlayer real pplay(ngrid, nlayer) real zdtlw(ngrid, nlayer) real zdtsw(ngrid, nlayer) real zdtnirco2(ngrid, nlayer) real zdtnlte(ngrid, nlayer) c c Output: real dtrad(ngrid, nlayer) c c Local: integer l, ig real alpha c c This is split into two loops to minimize number of calculations, c but for vector machines it may be faster to perform one big c loop from 1 to nlayer and remove the second loop. c c Loop over layers for which zdtsw/lw have been calculated. do l = 1,nlaylte do ig = 1, ngrid c alpha is actually 0.5*(1+tanh((z-ztrans)/zw)) c written here in a simpler form, with z=-ln(p) and zwi=2/zw alpha = 1./(1.+(pplay(ig,l)/ptrans)**zwi) dtrad(ig,l) = (1.-alpha)*(zdtsw(ig,l)+zdtlw(ig,l)) & + zdtnirco2(ig,l) + alpha*zdtnlte(ig,l) enddo enddo c c Faster loop over any remaining layers. do l = nlaylte+1, nlayer do ig = 1, ngrid dtrad(ig,l) = zdtnirco2(ig,l) + zdtnlte(ig,l) enddo enddo c return end