subroutine interpolateN2N2(wn,temp,pres,abcoef,firstcall,ind) !================================================================== ! ! Purpose ! ------- ! Calculates the N2-N2 CIA opacity, using a lookup table from ! HITRAN (2011) ! ! Authors ! ------- ! R. Wordsworth (2011) ! !================================================================== use datafile_mod, only: datadir implicit none ! input double precision wn ! wavenumber (cm^-1) double precision temp ! temperature (Kelvin) double precision pres ! pressure (Pascals) integer :: ind ! output double precision abcoef ! absorption coefficient (m^-1) integer nS,nT parameter(nS=582) parameter(nT=10) double precision, parameter :: losch = 2.6867774e19 ! Loschmit's number (molecule cm^-3 at STP) ! converts cm^5 molecule^-2 --> cm^-1 amagat^-2 ! see Richard et al. 2011, JQSRT for details double precision amagat double precision wn_arr(nS) double precision temp_arr(nT) double precision abs_arr(nS,nT) integer k,iT logical firstcall save wn_arr, temp_arr, abs_arr !read by master character*100 dt_file integer strlen,ios character(LEN=*), parameter :: fmat1 = "(A20,F10.3,F10.3,I7,F7.1,E10.3,F5.3)" character*20 bleh double precision blah, Ttemp integer nres if(temp.gt.400)then print*,'Your temperatures are too high for this N2-N2 CIA dataset.' print*,'Currently, HITRAN provides data for this pair in the range 40-400 K.' stop endif amagat = (273.15/temp)*(pres/101325.0) if(firstcall)then ! called by sugas_corrk only print*,'----------------------------------------------------' print*,'Initialising N2-N2 continuum from HITRAN database...' ! 1.1 Open the ASCII files dt_file=TRIM(datadir)//'/continuum_data/N2-N2_2011.cia' !$OMP MASTER open(33,file=dt_file,form='formatted',status='old',iostat=ios) if (ios.ne.0) then ! file not found write(*,*) 'Error from interpolateN2N2' write(*,*) 'Data file ',trim(dt_file),' not found.' write(*,*) 'Check that your path to datagcm:',trim(datadir) write(*,*) 'is correct. You can change it in callphys.def with:' write(*,*) 'datadir = /absolute/path/to/datagcm' write(*,*) 'Also check that the continuum data continuum_data/N2-N2_norm_2011.cia is there.' call abort else do iT=1,nT read(33,fmat1) bleh,blah,blah,nres,Ttemp if(nS.ne.nres)then print*,'Resolution given in file: ',trim(dt_file) print*,'is ',nres,', which does not match nS.' print*,'Please adjust nS value in interpolateN2N2.F90' stop endif temp_arr(iT)=Ttemp do k=1,nS read(33,*) wn_arr(k),abs_arr(k,it) end do end do endif close(33) !$OMP END MASTER !$OMP BARRIER print*,'interpolateN2N2: At wavenumber ',wn,' cm^-1' print*,' temperature ',temp,' K' print*,' pressure ',pres,' Pa' endif call bilinearbig(nS,nT,wn_arr,temp_arr,abs_arr,wn,temp,abcoef,ind) ! print*,'the absorption is ',abcoef,' cm^5 molecule^-2' ! print*,'or ',abcoef*losch**2,' cm^-1 amagat^-2' abcoef=abcoef*losch**2*100.0*amagat**2 ! convert to m^-1 ! abcoef=0. ! print*,'We have ',amagat,' amagats of N2' ! print*,'So the absorption is ',abcoef,' m^-1' ! unlike for Rayleigh scattering, we do not currently weight by the BB function ! however our bands are normally thin, so this is no big deal. return end subroutine interpolateN2N2