subroutine setspi !================================================================== ! ! Purpose ! ------- ! Set up spectral intervals and Planck function in the longwave. ! ! Authors ! ------- ! Adapted from setspi in the NASA Ames radiative code by ! Robin Wordsworth (2009). ! ! Called by ! --------- ! callcorrk.F ! ! Calls ! ----- ! none ! !================================================================== use radinc_h, only: L_NSPECTI,corrkdir,banddir,NTstart,NTstop,NTfac use radcommon_h, only: BWNI,BLAMI,WNOI,DWNI,WAVEI,planckir,sigma use datafile_mod, only: datadir use comcstfi_mod, only: pi implicit none logical file_ok integer nw, nt, m, mm, file_entries real*8 a, b, ans, y, bpa, bma, T, dummy character(len=30) :: temp1 character(len=200) :: file_id character(len=200) :: file_path ! C1 and C2 values from Goody and Yung (2nd edition) MKS units ! These values lead to a "sigma" (sigma*T^4) of 5.67032E-8 W m^-2 K^-4 real*8 :: c1 = 3.741832D-16 ! W m^-2 real*8 :: c2 = 1.438786D-2 ! m K real*8 :: lastband(2), plancksum !! used to count lines integer :: nb integer :: ierr logical forceEC, planckcheck real*8 :: x(12) = [ -0.981560634246719D0, -0.904117256370475D0, & -0.769902674194305D0, -0.587317954286617D0, & -0.367831498998180D0, -0.125233408511469D0, & 0.125233408511469D0, 0.367831498998180D0, & 0.587317954286617D0, 0.769902674194305D0, & 0.904117256370475D0, 0.981560634246719D0 ] real*8 :: w(12) = [ 0.047175336386512D0, 0.106939325995318D0, & 0.160078328543346D0, 0.203167426723066D0, & 0.233492536538355D0, 0.249147045813403D0, & 0.249147045813403D0, 0.233492536538355D0, & 0.203167426723066D0, 0.160078328543346D0, & 0.106939325995318D0, 0.047175336386512D0 ] mm=0 forceEC=.true. planckcheck=.true. !======================================================================= ! Set up spectral bands - wavenumber [cm^(-1)]. Go from smaller to ! larger wavenumbers. write(temp1,'(i2.2)') L_NSPECTI !file_id='/corrk_data/' // corrkdir(1:LEN_TRIM(corrkdir)) // '/narrowbands_IR.in' file_id='/corrk_data/'//trim(adjustl(banddir))//'/narrowbands_IR.in' file_path=TRIM(datadir)//TRIM(file_id) ! check that the file exists inquire(FILE=file_path,EXIST=file_ok) if(.not.file_ok) then write(*,*)'The file ',TRIM(file_path) write(*,*)'was not found by setspi.F90, exiting.' write(*,*)'Check that your path to datagcm:',trim(datadir) write(*,*)' is correct. You can change it in callphys.def with:' write(*,*)' datadir = /absolute/path/to/datagcm' write(*,*)'Also check that the corrkdir you chose in callphys.def exists.' call abort endif !$OMP MASTER nb=0 ierr=0 ! check that the file contains the right number of bands open(131,file=file_path,form='formatted') read(131,*,iostat=ierr) file_entries do while (ierr==0) read(131,*,iostat=ierr) dummy ! write(*,*) 'setspi: file_entries:',dummy,'ierr=',ierr if (ierr==0) nb=nb+1 enddo close(131) write(*,*) 'setspi: L_NSPECTI = ',L_NSPECTI, 'in the model ' write(*,*) ' there are ',nb, 'entries in ',TRIM(file_path) if(nb.ne.L_NSPECTI) then write(*,*) 'MISMATCH !! I stop here' call abort endif ! load and display the data open(111,file=file_path,form='formatted') read(111,*) do M=1,L_NSPECTI-1 read(111,*) BWNI(M) end do read(111,*) lastband close(111) BWNI(L_NSPECTI) =lastband(1) BWNI(L_NSPECTI+1)=lastband(2) !$OMP END MASTER !$OMP BARRIER print*,'' print*,'setspi: IR band limits:' do M=1,L_NSPECTI+1 print*,m,'-->',BWNI(M),' cm^-1' end do ! Set up mean wavenumbers and wavenumber deltas. Units of ! wavenumbers is cm^(-1); units of wavelengths is microns. do M=1,L_NSPECTI WNOI(M) = 0.5D0*(BWNI(M+1)+BWNI(M)) DWNI(M) = BWNI(M+1)-BWNI(M) WAVEI(M) = 1.0D+4/WNOI(M) BLAMI(M) = 0.01D0/BWNI(M) end do BLAMI(M) = 0.01D0/BWNI(M) ! note M=L_NSPECTI+1 after loop due to Fortran bizarreness !======================================================================= ! For each IR wavelength interval, compute the integral of B(T), the ! Planck function, divided by the wavelength interval, in cm-1. The ! integration is in MKS units, the final answer is the same as the ! original planck.f; W m^-2 wavenumber^-1, where wavenumber is in CM^-1. print*,'' print*,'setspi: Current Planck integration range:' print*,'T = ',dble(NTstart)/NTfac, ' to ',dble(NTstop)/NTfac,' K.' IF(.NOT.ALLOCATED(planckir)) ALLOCATE(planckir(L_NSPECTI,NTstop-NTstart+1)) do NW=1,L_NSPECTI a = 1.0D-2/BWNI(NW+1) b = 1.0D-2/BWNI(NW) bpa = (b+a)/2.0D0 bma = (b-a)/2.0D0 ! if (nw .eq. 25) then !LT debug ! print*, "a = ",a ! print*, "b= ",b ! print*,"bpa = ",bpa ! print*, "bma = ",bma ! endif do nt=NTstart,NTstop T = dble(NT)/NTfac ans = 0.0D0 do mm=1,12 y = bma*x(mm)+bpa !to avoid floating overflow when T is low and optical wavelength if ((c2/(y*T)) .lt. 700.0D0) then ans = ans + w(mm)*c1/(y**5*(exp(c2/(y*T))-1.0D0)) else ans = ans +0.0D0 endif end do planckir(NW,nt-NTstart+1) = ans*bma/(PI*DWNI(NW)) end do end do ! force planck=sigma*eps*T^4 for each temperature in array if(forceEC)then print*,'setspi: Force F=sigma*eps*T^4 for all values of T!' do nt=NTstart,NTstop plancksum=0.0D0 T=dble(NT)/NTfac do NW=1,L_NSPECTI plancksum=plancksum+ & planckir(NW,nt-NTstart+1)*DWNI(NW)*pi end do do NW=1,L_NSPECTI planckir(NW,nt-NTstart+1)= & planckir(NW,nt-NTstart+1)* & sigma*(dble(nt)/NTfac)**4/plancksum end do end do endif if(planckcheck)then ! check energy conservation at lower temperature boundary plancksum=0.0D0 nt=NTstart do NW=1,L_NSPECTI plancksum=plancksum+planckir(NW,nt-NTstart+1)*DWNI(NW)*pi end do print*,'setspi: At lower limit:' print*,'in model sig*T^4 = ',plancksum,' W m^-2' print*,'actual sig*T^4 = ',sigma*(dble(nt)/NTfac)**4,' W m^-2' ! check energy conservation at upper temperature boundary plancksum=0.0D0 nt=NTstop do NW=1,L_NSPECTI plancksum=plancksum+planckir(NW,nt-NTstart+1)*DWNI(NW)*pi end do print*,'setspi: At upper limit:' print*,'in model sig*T^4 = ',plancksum,' W m^-2' print*,'actual sig*T^4 = ',sigma*(dble(nt)/NTfac)**4,' W m^-2' print*,'' endif return end subroutine setspi