module spetru !----------------------------------------------------------------------- ! ! Purpose: Spectrally truncate initial data fields. ! ! Method: Truncate one or a few fields at a time, to minimize the ! memory requirements ! ! Original version: J. Rosinski ! Standardized: J. Rosinski, June 1992 ! Reviewed: B. Boville, J. Hack, August 1992 ! Modified to implement processing of subsets of fields: P. Worley, May 2003 ! !----------------------------------------------------------------------- use shr_kind_mod, only: r8 => shr_kind_r8 use pmgrid, only: plon, plev, plat use pspect, only: psp, pspt, ptrn, pmmax use comspe, only: alp, nlen, nstart, dalp use rgrid, only: nlon, nmmax use commap, only: w, xm use physconst, only: rearth, ra use sld_control_mod, only : pcray, trig, ifax implicit none ! ! By default make data and interfaces to this module private ! private ! ! Public interfaces ! public spetru_phis ! Spectrally truncate PHIS public spetru_ps ! Spectrally truncate PS public spetru_3d_scalar ! Spectrally truncate 3D scalar fields public spetru_uv ! Spectrally truncate winds (U and V) ! ! Private module data ! integer, parameter :: plondfft = plon + 2 ! Size of longitude needed for FFT's ! !======================================================================= contains !************************************************************************ subroutine spetru_phis (phis, phis_hires, phisl, phism, phi_out) !----------------------------------------------------------------------- ! ! Purpose: ! ! Method: ! Spectrally truncate PHIS input field. ! ! Author: ! Original version: J. Rosinski ! Standardized: J. Rosinski, June 1992 ! Reviewed: B. Boville, J. Hack, August 1992 ! Modified: P. Worley, May 2003 ! Modified: J. Olson, Apr 2004 ! !----------------------------------------------------------------------- use pmgrid, only: plon, plat ! ! Input/Output arguments ! real(r8), intent(inout) :: phis(plon,plat) ! Fourier -> spec. coeffs. for sfc geo. logical, intent(in) :: phis_hires ! true => PHIS came from hi res topo file real(r8), intent(out), optional :: phisl(plon,plat) ! Spectrally trunc d(phis)/d(longitude) real(r8), intent(out), optional :: phism(plon,plat) ! Spectrally trunc d(phis)/d(latitude) real(r8), intent(out), optional :: phi_out(2,psp/2) ! used in spectral truncation of phis ! !---------------------------Local workspace----------------------------- ! real(r8), pointer :: phis_tmp(:,:) ! Temporary to compute Phis of size needed for FFT real(r8), pointer :: phisl_tmp(:,:) ! Temporary to compute phisl of size needed for FFT real(r8), pointer :: phism_tmp(:,:) ! Temporary to compute phism of size needed for FFT real(r8) tmp1 ! vector temporary real(r8) tmp2 ! vector temporary real(r8) phialpr,phialpi ! phi*alp (real and imaginary) real(r8) phdalpr,phdalpi ! phi*dalp (real and imaginary) real(r8) zwalp ! zw*alp real(r8) zw ! w**2 real(r8) filtlim ! filter function real(r8) ft ! filter multiplier for spectral coefficients real(r8) phi(2,psp/2) ! used in spectral truncation of phis #if ( ! defined USEFFTLIB ) real(r8) work((plon+1)*plev) ! Workspace for fft #else real(r8) work((plon+1)*pcray) ! Workspace for fft #endif integer i ! longitude index integer irow ! latitude pair index integer latm,latp ! symmetric latitude indices integer lat integer m ! longitudinal wavenumber index integer n ! latitudinal wavenumber index integer nspec integer mr ! spectral indices ! !----------------------------------------------------------------------- ! ! Zero spectral array ! phi(:,:) = 0._r8 ! ! Transform grid -> fourier ! allocate(phis_tmp(plondfft,plat)) phis_tmp(:plon,:) = phis(:plon,:) do lat=1,plat irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 call fft991(phis_tmp(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,-1) end do ! lat=1,plat ! ! Loop over latitude pairs ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 zw = w(irow)*2._r8 do i=1,2*nmmax(irow) ! ! Compute symmetric and antisymmetric components ! tmp1 = 0.5_r8*(phis_tmp(i,latm) - phis_tmp(i,latp)) tmp2 = 0.5_r8*(phis_tmp(i,latm) + phis_tmp(i,latp)) phis_tmp(i,latm) = tmp1 phis_tmp(i,latp) = tmp2 end do ! ! Compute phi*mn ! do m=1,nmmax(irow) mr = nstart(m) do n=1,nlen(m),2 zwalp = zw*alp(mr+n,irow) phi(1,mr+n) = phi(1,mr+n) + zwalp*phis_tmp(2*m-1,latp) phi(2,mr+n) = phi(2,mr+n) + zwalp*phis_tmp(2*m ,latp) end do do n=2,nlen(m),2 zwalp = zw*alp(mr+n,irow) phi(1,mr+n) = phi(1,mr+n) + zwalp*phis_tmp(2*m-1,latm) phi(2,mr+n) = phi(2,mr+n) + zwalp*phis_tmp(2*m ,latm) end do end do enddo ! irow=1,plat/2 ! if (phis_hires) then ! ! Apply spectral filter to phis ! filter is a function of n ! if n < filter limit then ! spectral_coeff = spectral_coeff * (1. - (real(n,r8)/filtlim)**2) ! else ! spectral_coeff = 0. ! endif ! where filter limit = 1.4*PTRN ! filtlim = real(int(1.4_r8*real(ptrn,r8)),r8) do m=1,pmmax mr = nstart(m) do n=1,nlen(m) nspec=m-1+n ft = 1._r8 - (real(nspec,r8)/filtlim)**2 if (real(nspec,r8) .ge. filtlim) ft = 0._r8 phi(1,mr+n) = phi(1,mr+n)*ft phi(2,mr+n) = phi(2,mr+n)*ft end do end do call hordif1(rearth,phi) end if ! ! Compute grid point values of phi*. ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! phis_tmp(:,latm) = 0._r8 phis_tmp(:,latp) = 0._r8 ! ! Compute(phi*)m ! do m=1,nmmax(irow) mr = nstart(m) do n=1,nlen(m),2 phialpr = phi(1,mr+n)*alp(mr+n,irow) phialpi = phi(2,mr+n)*alp(mr+n,irow) phis_tmp(2*m-1,latm) = phis_tmp(2*m-1,latm) + phialpr phis_tmp(2*m ,latm) = phis_tmp(2*m ,latm) + phialpi end do end do do m=1,nmmax(irow) mr = nstart(m) do n=2,nlen(m),2 phialpr = phi(1,mr+n)*alp(mr+n,irow) phialpi = phi(2,mr+n)*alp(mr+n,irow) phis_tmp(2*m-1,latp) = phis_tmp(2*m-1,latp) + phialpr phis_tmp(2*m ,latp) = phis_tmp(2*m ,latp) + phialpi end do end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = phis_tmp(i,latm) + phis_tmp(i,latp) tmp2 = phis_tmp(i,latm) - phis_tmp(i,latp) phis_tmp(i,latm) = tmp1 phis_tmp(i,latp) = tmp2 end do enddo ! irow=1,plat/2 if(present(phisl)) then allocate(phisl_tmp(plondfft,plat)) do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! phisl_tmp(:,latm) = 0._r8 phisl_tmp(:,latp) = 0._r8 ! ! Compute(phi*)m ! do m=1,nmmax(irow) mr = nstart(m) do n=1,nlen(m),2 phialpr = phi(1,mr+n)*alp(mr+n,irow) phialpi = phi(2,mr+n)*alp(mr+n,irow) phisl_tmp(2*m-1,latm) = phisl_tmp(2*m-1,latm) - phialpi*ra phisl_tmp(2*m ,latm) = phisl_tmp(2*m ,latm) + phialpr*ra end do end do do m=1,nmmax(irow) mr = nstart(m) do n=2,nlen(m),2 phialpr = phi(1,mr+n)*alp(mr+n,irow) phialpi = phi(2,mr+n)*alp(mr+n,irow) phisl_tmp(2*m-1,latp) = phisl_tmp(2*m-1,latp) - phialpi*ra phisl_tmp(2*m ,latp) = phisl_tmp(2*m ,latp) + phialpr*ra end do end do ! ! d(Phi)/d(lamda) ! do m=1,nmmax(irow) phisl_tmp(2*m-1,latm) = xm(m)*phisl_tmp(2*m-1,latm) phisl_tmp(2*m ,latm) = xm(m)*phisl_tmp(2*m ,latm) phisl_tmp(2*m-1,latp) = xm(m)*phisl_tmp(2*m-1,latp) phisl_tmp(2*m ,latp) = xm(m)*phisl_tmp(2*m ,latp) end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = phisl_tmp(i,latm) + phisl_tmp(i,latp) tmp2 = phisl_tmp(i,latm) - phisl_tmp(i,latp) phisl_tmp(i,latm) = tmp1 phisl_tmp(i,latp) = tmp2 end do enddo ! irow=1,plat/2 end if if(present(phism)) then allocate(phism_tmp(plondfft,plat)) do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! phism_tmp(:,latm) = 0._r8 phism_tmp(:,latp) = 0._r8 ! ! Compute(phi*)m ! do m=1,nmmax(irow) mr = nstart(m) do n=1,nlen(m),2 phdalpr = phi(1,mr+n)*dalp(mr+n,irow) phdalpi = phi(2,mr+n)*dalp(mr+n,irow) phism_tmp(2*m-1,latp) = phism_tmp(2*m-1,latp) + phdalpr*ra phism_tmp(2*m ,latp) = phism_tmp(2*m ,latp) + phdalpi*ra end do end do do m=1,nmmax(irow) mr = nstart(m) do n=2,nlen(m),2 phdalpr = phi(1,mr+n)*dalp(mr+n,irow) phdalpi = phi(2,mr+n)*dalp(mr+n,irow) phism_tmp(2*m-1,latm) = phism_tmp(2*m-1,latm) + phdalpr*ra phism_tmp(2*m ,latm) = phism_tmp(2*m ,latm) + phdalpi*ra end do end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = phism_tmp(i,latm) + phism_tmp(i,latp) tmp2 = phism_tmp(i,latm) - phism_tmp(i,latp) phism_tmp(i,latm) = tmp1 phism_tmp(i,latp) = tmp2 end do enddo ! irow=1,plat/2 end if ! do lat=1,plat ! ! Transform Fourier -> grid, obtaining spectrally truncated ! grid point values. ! irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 call fft991(phis_tmp(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,+1) phis(:nlon(lat),lat) = phis_tmp(:nlon(lat),lat) if(present(phisl)) then call fft991 (phisl_tmp(1,lat),work ,trig(1,irow),ifax(1,irow),1 , & plondfft ,nlon(lat),1 ,+1 ) phisl(:nlon(lat),lat) = phisl_tmp(:nlon(lat),lat) end if if(present(phism)) then call fft991 (phism_tmp(1,lat),work ,trig(1,irow),ifax(1,irow),1 , & plondfft ,nlon(lat),1 ,+1 ) phism(:nlon(lat),lat) = phism_tmp(:nlon(lat),lat) end if enddo deallocate( phis_tmp ) if ( present(phisl) ) deallocate( phisl_tmp ) if ( present(phism) ) deallocate( phism_tmp ) if(present(phi_out)) then phi_out(:,:) = phi(:,:) end if return end subroutine spetru_phis !************************************************************************ subroutine spetru_ps(ps ,dpsl ,dpsm) !----------------------------------------------------------------------- ! ! Purpose: ! ! Method: ! Spectrally truncate PS input field. ! ! Author: ! Original version: J. Rosinski ! Standardized: J. Rosinski, June 1992 ! Reviewed: B. Boville, J. Hack, August 1992 ! Modified: P. Worley, May 2003 ! Modified: J. Olson, Apr 2004 ! !----------------------------------------------------------------------- use pmgrid, only: plon, plat ! ! Input/Output arguments ! real(r8), intent(inout) :: ps(plon,plat) ! Fourier -> spec. coeffs. for ln(ps) ! ! Output arguments ! real(r8), intent(out) :: dpsl(plon,plat) ! Spectrally trunc d(ln(ps))/d(longitude) real(r8), intent(out) :: dpsm(plon,plat) ! Spectrally trunc d(ln(ps))/d(latitude) ! !---------------------------Local workspace----------------------------- ! real(r8), pointer :: log_ps(:,:) ! log(ps) real(r8), pointer :: dpsm_tmp(:,:) ! Temporary to compute dpsm of size needed for FFT real(r8), pointer :: dpsl_tmp(:,:) ! Temporary to compute dpsl of size needed for FFT real(r8) alps_tmp(psp) ! used in spectral truncation of phis real(r8) tmp1 ! vector temporary real(r8) tmp2 ! vector temporary real(r8) zwalp ! zw*alp real(r8) psdalpr,psdalpi ! alps (real and imaginary)*dalp real(r8) psalpr,psalpi ! alps (real and imaginary)*alp real(r8) zw ! w**2 #if ( ! defined USEFFTLIB ) real(r8) work((plon+1)*plev) ! Workspace for fft #else real(r8) work((plon+1)*pcray) ! Workspace for fft #endif integer ir,ii ! indices complex coeffs. of spec. arrs. integer i,k ! longitude, level indices integer irow ! latitude pair index integer latm,latp ! symmetric latitude indices integer lat integer m ! longitudinal wavenumber index integer n ! latitudinal wavenumber index integer nspec integer mr,mc ! spectral indices ! !----------------------------------------------------------------------- ! ! Zero spectral array ! alps_tmp(:) = 0._r8 ! ! Compute the 2D quantities which are transformed to spectral space: ! ps= ln(ps). ! allocate( log_ps(plondfft,plat) ) do lat=1,plat irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 do i=1,nlon(lat) log_ps(i,lat) = log(ps(i,lat)) end do ! ! Transform grid -> fourier ! call fft991(log_ps(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,-1) end do ! lat=1,plat allocate( dpsl_tmp(plondfft,plat) ) allocate( dpsm_tmp(plondfft,plat) ) ! ! Loop over latitude pairs ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 zw = w(irow)*2._r8 do i=1,2*nmmax(irow) ! ! Compute symmetric and antisymmetric components ! tmp1 = 0.5_r8*(log_ps(i,latm) - log_ps(i,latp)) tmp2 = 0.5_r8*(log_ps(i,latm) + log_ps(i,latp)) log_ps(i,latm) = tmp1 log_ps(i,latp) = tmp2 end do ! ! Compute ln(p*)mn ! do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 zwalp = zw*alp(mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 alps_tmp(ir) = alps_tmp(ir) + zwalp*log_ps(2*m-1,latp) alps_tmp(ii) = alps_tmp(ii) + zwalp*log_ps(2*m ,latp) end do do n=2,nlen(m),2 zwalp = zw*alp(mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 alps_tmp(ir) = alps_tmp(ir) + zwalp*log_ps(2*m-1,latm) alps_tmp(ii) = alps_tmp(ii) + zwalp*log_ps(2*m ,latm) end do end do enddo ! irow=1,plat/2 ! ! Compute grid point values of:ln(p*) and grad(ln(p*)). ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! log_ps(:,latm) = 0._r8 log_ps(:,latp) = 0._r8 dpsl_tmp(:,latm) = 0._r8 dpsl_tmp(:,latp) = 0._r8 dpsm_tmp(:,latm) = 0._r8 dpsm_tmp(:,latp) = 0._r8 ! ! Compute(ln(p*),grad(ln(p*)))m ! do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 psalpr = alps_tmp(ir)*alp(mr+n,irow) psalpi = alps_tmp(ii)*alp(mr+n,irow) ! log_ps(2*m-1,latm) = log_ps(2*m-1,latm) + psalpr log_ps(2*m ,latm) = log_ps(2*m ,latm) + psalpi dpsl_tmp(2*m-1,latm) = dpsl_tmp(2*m-1,latm) - psalpi*ra dpsl_tmp(2*m ,latm) = dpsl_tmp(2*m ,latm) + psalpr*ra ! psdalpr = alps_tmp(ir)*dalp(mr+n,irow) psdalpi = alps_tmp(ii)*dalp(mr+n,irow) ! dpsm_tmp(2*m-1,latp) = dpsm_tmp(2*m-1,latp) + psdalpr*ra dpsm_tmp(2*m ,latp) = dpsm_tmp(2*m ,latp) + psdalpi*ra end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 psalpr = alps_tmp(ir)*alp(mr+n,irow) psalpi = alps_tmp(ii)*alp(mr+n,irow) ! log_ps(2*m-1,latp) = log_ps(2*m-1,latp) + psalpr log_ps(2*m ,latp) = log_ps(2*m ,latp) + psalpi dpsl_tmp(2*m-1,latp) = dpsl_tmp(2*m-1,latp) - psalpi*ra dpsl_tmp(2*m ,latp) = dpsl_tmp(2*m ,latp) + psalpr*ra ! psdalpr = alps_tmp(ir)*dalp(mr+n,irow) psdalpi = alps_tmp(ii)*dalp(mr+n,irow) ! dpsm_tmp(2*m-1,latm) = dpsm_tmp(2*m-1,latm) + psdalpr*ra dpsm_tmp(2*m ,latm) = dpsm_tmp(2*m ,latm) + psdalpi*ra end do end do do m=1,nmmax(irow) dpsl_tmp(2*m-1,latm) = xm(m)*dpsl_tmp(2*m-1,latm) dpsl_tmp(2*m ,latm) = xm(m)*dpsl_tmp(2*m ,latm) dpsl_tmp(2*m-1,latp) = xm(m)*dpsl_tmp(2*m-1,latp) dpsl_tmp(2*m ,latp) = xm(m)*dpsl_tmp(2*m ,latp) end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 ! tmp1 = log_ps(i,latm) + log_ps(i,latp) tmp2 = log_ps(i,latm) - log_ps(i,latp) log_ps(i,latm) = tmp1 log_ps(i,latp) = tmp2 ! tmp1 = dpsl_tmp(i,latm) + dpsl_tmp(i,latp) tmp2 = dpsl_tmp(i,latm) - dpsl_tmp(i,latp) dpsl_tmp(i,latm) = tmp1 dpsl_tmp(i,latp) = tmp2 ! tmp1 = dpsm_tmp(i,latm) + dpsm_tmp(i,latp) tmp2 = dpsm_tmp(i,latm) - dpsm_tmp(i,latp) dpsm_tmp(i,latm) = tmp1 dpsm_tmp(i,latp) = tmp2 end do ! enddo ! irow=1,plat/2 ! do lat=1,plat ! ! Transform Fourier -> grid, obtaining spectrally truncated ! grid point values. ! irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 call fft991(log_ps(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,+1) call fft991(dpsl_tmp(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,+1) call fft991(dpsm_tmp(1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),1,+1) ! ! Convert from ln(ps) to ps, copy temporaries to input arrays ! do i=1,nlon(lat) ps(i,lat) = exp(log_ps(i,lat)) dpsl(i,lat) = dpsl_tmp(i,lat) dpsm(i,lat) = dpsm_tmp(i,lat) end do ! enddo deallocate( log_ps ) deallocate( dpsm_tmp ) deallocate( dpsl_tmp ) return end subroutine spetru_ps !************************************************************************ subroutine spetru_3d_scalar(x3, dl, dm) !----------------------------------------------------------------------- ! ! Purpose: ! ! Method: ! Spectrally truncate 3-D scalar field. ! ! Author: ! Original version: J. Rosinski ! Standardized: J. Rosinski, June 1992 ! Reviewed: B. Boville, J. Hack, August 1992 ! Modified: P. Worley, May 2003 ! Modified: J. Olson, Apr 2004 ! !----------------------------------------------------------------------- use pmgrid, only: plon, plat ! ! Input/Output arguments ! real(r8), intent(inout) :: x3(plon,plev,plat) ! Fourier -> spec. coeffs. for X real(r8), intent(out), optional :: dl(plon,plev,plat) ! Spectrally trunc d(X)/d(longitude) real(r8), intent(out), optional :: dm(plon,plev,plat) ! Spectrally trunc d(X)/d(latitude) ! !---------------------------Local workspace----------------------------- ! real(r8), pointer :: x3_tmp(:,:,:) ! Temporary to compute x3 of size needed for FFT real(r8), pointer :: dl_tmp(:,:,:) ! Temporary to compute dl of size needed for FFT real(r8), pointer :: dm_tmp(:,:,:) ! Temporary to compute dm of size needed for FFT real(r8) t_tmp(psp) ! used in spectral truncation of t real(r8) tmp1 ! vector temporary real(r8) tmp2 ! vector temporary real(r8) tmpr ! vector temporary (real) real(r8) tmpi ! vector temporary (imaginary) real(r8) zwalp ! zw*alp real(r8) zw ! w**2 #if ( ! defined USEFFTLIB ) real(r8) work((plon+1)*plev) ! Workspace for fft #else real(r8) work((plon+1)*pcray) ! Workspace for fft #endif integer ir,ii ! indices complex coeffs. of spec. arrs. integer i,k ! longitude, level indices integer irow ! latitude pair index integer latm,latp ! symmetric latitude indices integer lat integer m ! longitudinal wavenumber index integer n ! latitudinal wavenumber index integer nspec integer mr,mc ! spectral indices ! !----------------------------------------------------------------------- ! ! Transform grid -> fourier ! allocate( x3_tmp(plondfft,plev,plat) ) if(present(dm)) allocate( dm_tmp(plondfft,plev,plat) ) if(present(dl)) allocate( dl_tmp(plondfft,plev,plat) ) do lat=1,plat irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 x3_tmp(:nlon(lat),:,lat) = x3(:nlon(lat),:,lat) call fft991(x3_tmp(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,-1) end do ! lat=1,plat ! ! Loop over vertical levels ! do k=1,plev ! ! Zero spectral array ! t_tmp(:) = 0._r8 ! ! Loop over latitude pairs ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 zw = w(irow)*2._r8 ! ! Multi-level field: T ! do i=1,2*nmmax(irow) tmp1 = 0.5_r8*(x3_tmp(i,k,latm) - x3_tmp(i,k,latp)) tmp2 = 0.5_r8*(x3_tmp(i,k,latm) + x3_tmp(i,k,latp)) x3_tmp(i,k,latm) = tmp1 x3_tmp(i,k,latp) = tmp2 end do ! ! Compute tmn ! do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 zwalp = zw*alp (mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 t_tmp(ir) = t_tmp(ir) + zwalp*x3_tmp(2*m-1,k,latp) t_tmp(ii) = t_tmp(ii) + zwalp*x3_tmp(2*m ,k,latp) end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 zwalp = zw*alp (mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 t_tmp(ir) = t_tmp(ir) + zwalp*x3_tmp(2*m-1,k,latm) t_tmp(ii) = t_tmp(ii) + zwalp*x3_tmp(2*m ,k,latm) end do end do enddo ! irow=1,plat/2 ! ! Compute grid point values of:t. ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! x3_tmp(:,k,latm) = 0._r8 x3_tmp(:,k,latp) = 0._r8 do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*alp(mr+n,irow) tmpi = t_tmp(ii)*alp(mr+n,irow) x3_tmp(2*m-1,k,latm) = x3_tmp(2*m-1,k,latm) + tmpr x3_tmp(2*m ,k,latm) = x3_tmp(2*m ,k,latm) + tmpi end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*alp(mr+n,irow) tmpi = t_tmp(ii)*alp(mr+n,irow) x3_tmp(2*m-1,k,latp) = x3_tmp(2*m-1,k,latp) + tmpr x3_tmp(2*m ,k,latp) = x3_tmp(2*m ,k,latp) + tmpi end do end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = x3_tmp(i,k,latm) + x3_tmp(i,k,latp) tmp2 = x3_tmp(i,k,latm) - x3_tmp(i,k,latp) x3_tmp(i,k,latm) = tmp1 x3_tmp(i,k,latp) = tmp2 end do enddo ! irow=1,plat/2 if(present(dl)) then do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! dl_tmp(:,k,latm) = 0._r8 dl_tmp(:,k,latp) = 0._r8 do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*alp(mr+n,irow) tmpi = t_tmp(ii)*alp(mr+n,irow) dl_tmp(2*m-1,k,latm) = dl_tmp(2*m-1,k,latm) - tmpi*ra dl_tmp(2*m ,k,latm) = dl_tmp(2*m ,k,latm) + tmpr*ra end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*alp(mr+n,irow) tmpi = t_tmp(ii)*alp(mr+n,irow) dl_tmp(2*m-1,k,latp) = dl_tmp(2*m-1,k,latp) - tmpi*ra dl_tmp(2*m ,k,latp) = dl_tmp(2*m ,k,latp) + tmpr*ra end do end do ! ! d(T)/d(lamda) ! do m=1,nmmax(irow) dl_tmp(2*m-1,k,latm) = xm(m)*dl_tmp(2*m-1,k,latm) dl_tmp(2*m ,k,latm) = xm(m)*dl_tmp(2*m ,k,latm) dl_tmp(2*m-1,k,latp) = xm(m)*dl_tmp(2*m-1,k,latp) dl_tmp(2*m ,k,latp) = xm(m)*dl_tmp(2*m ,k,latp) end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = dl_tmp(i,k,latm) + dl_tmp(i,k,latp) tmp2 = dl_tmp(i,k,latm) - dl_tmp(i,k,latp) dl_tmp(i,k,latm) = tmp1 dl_tmp(i,k,latp) = tmp2 end do enddo ! irow=1,plat/2 end if if(present(dm)) then do irow=1,plat/2 latp = irow latm = plat - irow + 1 ! ! Zero fourier fields ! dm_tmp(:,k,latm) = 0._r8 dm_tmp(:,k,latp) = 0._r8 do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*dalp(mr+n,irow) tmpi = t_tmp(ii)*dalp(mr+n,irow) dm_tmp(2*m-1,k,latp) = dm_tmp(2*m-1,k,latp) + tmpr*ra dm_tmp(2*m ,k,latp) = dm_tmp(2*m ,k,latp) + tmpi*ra end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 tmpr = t_tmp(ir)*dalp(mr+n,irow) tmpi = t_tmp(ii)*dalp(mr+n,irow) dm_tmp(2*m-1,k,latm) = dm_tmp(2*m-1,k,latm) + tmpr*ra dm_tmp(2*m ,k,latm) = dm_tmp(2*m ,k,latm) + tmpi*ra end do end do ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = dm_tmp(i,k,latm) + dm_tmp(i,k,latp) tmp2 = dm_tmp(i,k,latm) - dm_tmp(i,k,latp) dm_tmp(i,k,latm) = tmp1 dm_tmp(i,k,latp) = tmp2 end do enddo ! irow=1,plat/2 end if enddo ! k=1,plev ! do lat=1,plat ! ! Transform Fourier -> grid, obtaining spectrally truncated ! grid point values. irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 call fft991(x3_tmp(1,1,lat) ,work ,trig(1,irow),ifax(1,irow),1 , & plondfft ,nlon(lat),plev ,+1) x3(:nlon(lat),:,lat) = x3_tmp(:nlon(lat),:,lat) if(present(dl)) then call fft991(dl_tmp(1,1,lat) ,work ,trig(1,irow),ifax(1,irow),1 , & plondfft ,nlon(lat),plev ,+1 ) dl(:nlon(lat),:,lat) = dl_tmp(:nlon(lat),:,lat) end if if(present(dm)) then call fft991(dm_tmp(1,1,lat) ,work ,trig(1,irow),ifax(1,irow),1 , & plondfft ,nlon(lat),plev ,+1 ) dm(:nlon(lat),:,lat) = dm_tmp(:nlon(lat),:,lat) end if end do deallocate( x3_tmp ) if ( present(dm) ) deallocate( dm_tmp ) if ( present(dl) ) deallocate( dl_tmp ) return end subroutine spetru_3d_scalar !*********************************************************************** subroutine spetru_uv(u3 ,v3 ,div ,vort ) !----------------------------------------------------------------------- ! ! Purpose: ! ! Method: ! Spectrally truncate U, V input fields. ! ! Author: ! Original version: J. Rosinski ! Standardized: J. Rosinski, June 1992 ! Reviewed: B. Boville, J. Hack, August 1992 ! Modified: P. Worley, May 2003 ! Modified: J. Olson, Apr 2004 ! !----------------------------------------------------------------------- use pmgrid, only: plon, plat use commap, only: rsq, cs use physconst,only: ez ! ! Input/Output arguments ! real(r8), intent(inout) :: u3(plon,plev,plat) ! Fourier -> spec. coeffs. for u-wind real(r8), intent(inout) :: v3(plon,plev,plat) ! Fourier -> spec. coeffs. for v-wind ! ! Output arguments ! real(r8), intent(out), optional :: div (plon,plev,plat) ! Spectrally truncated divergence real(r8), intent(out), optional :: vort(plon,plev,plat) ! Spectrally truncated vorticity ! !---------------------------Local workspace----------------------------- ! real(r8), pointer :: u_cosphi(:,:,:) ! u3*cos(phi) real(r8), pointer :: v_cosphi(:,:,:) ! v3*cos(phi) real(r8), pointer :: div_tmp(:,:,:) ! Temporary to compute div of size needed for FFT real(r8), pointer :: vort_tmp(:,:,:) ! Temporary to compute vort of size needed for FFT real(r8) d_tmp(psp) ! used in spectral truncation of div real(r8) vz_tmp(psp) ! used in spectral truncation of vort real(r8) alpn(pspt) ! alp*rsq*xm*ra real(r8) dalpn(pspt) ! dalp*rsq*ra real(r8) tmp1 ! vector temporary real(r8) tmp2 ! vector temporary real(r8) tmpr ! vector temporary (real) real(r8) tmpi ! vector temporary (imaginary) real(r8) zcor ! correction for absolute vorticity real(r8) zwalp ! zw*alp real(r8) zwdalp ! zw*dalp real(r8) zrcsj ! ra/(cos**2 latitude) real(r8) zw ! w**2 #if ( ! defined USEFFTLIB ) real(r8) work((plon+1)*plev) ! Workspace for fft #else real(r8) work((plon+1)*pcray) ! Workspace for fft #endif real(r8) zsqcs integer ir,ii ! indices complex coeffs. of spec. arrs. integer i,k ! longitude, level indices integer irow ! latitude pair index integer latm,latp ! symmetric latitude indices integer lat integer m ! longitudinal wavenumber index integer n ! latitudinal wavenumber index integer nspec integer mr,mc ! spectral indices ! !----------------------------------------------------------------------- ! ! Compute the quantities which are transformed to spectral space: ! 1. u = u*sqrt(1-mu*mu), u * cos(phi) ! 2. v = v*sqrt(1-mu*mu), v * cos(phi) ! allocate( u_cosphi(plondfft,plev,plat) ) allocate( v_cosphi(plondfft,plev,plat) ) do lat=1,plat irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 zsqcs = sqrt(cs(irow)) do k=1,plev do i=1,nlon(lat) u_cosphi(i,k,lat) = u3(i,k,lat)*zsqcs v_cosphi(i,k,lat) = v3(i,k,lat)*zsqcs end do end do ! ! Transform grid -> fourier ! 1st transform: U,V,T: note contiguity assumptions ! 2nd transform: LN(PS). 3rd transform: surface geopotential ! call fft991(u_cosphi(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,-1) call fft991(v_cosphi(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,-1) end do ! lat=1,plat ! ! Multi-level fields: U, V ! if ( present(div) ) allocate( div_tmp(plondfft,plev,plat) ) if ( present(vort) ) allocate( vort_tmp(plondfft,plev,plat) ) do k=1,plev ! ! Zero spectral arrays ! vz_tmp(:) = 0._r8 d_tmp(:) = 0._r8 ! ! Loop over latitude pairs ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 zrcsj = ra/cs(irow) zw = w(irow)*2._r8 do i=1,2*nmmax(irow) tmp1 = 0.5_r8*(u_cosphi(i,k,latm) - u_cosphi(i,k,latp)) tmp2 = 0.5_r8*(u_cosphi(i,k,latm) + u_cosphi(i,k,latp)) u_cosphi(i,k,latm) = tmp1 u_cosphi(i,k,latp) = tmp2 tmp1 = 0.5_r8*(v_cosphi(i,k,latm) - v_cosphi(i,k,latp)) tmp2 = 0.5_r8*(v_cosphi(i,k,latm) + v_cosphi(i,k,latp)) v_cosphi(i,k,latm) = tmp1 v_cosphi(i,k,latp) = tmp2 end do ! ! Compute vzmn and dmn ! do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 zwdalp = zw*dalp(mr+n,irow) zwalp = zw*alp (mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 d_tmp(ir) = d_tmp(ir) - (zwdalp*v_cosphi(2*m-1,k,latm) + & xm(m)*zwalp*u_cosphi(2*m ,k,latp))*zrcsj d_tmp(ii) = d_tmp(ii) - (zwdalp*v_cosphi(2*m ,k,latm) - & xm(m)*zwalp*u_cosphi(2*m-1,k,latp))*zrcsj vz_tmp(ir) = vz_tmp(ir) + (zwdalp*u_cosphi(2*m-1,k,latm) - & xm(m)*zwalp*v_cosphi(2*m ,k,latp))*zrcsj vz_tmp(ii) = vz_tmp(ii) + (zwdalp*u_cosphi(2*m ,k,latm) + & xm(m)*zwalp*v_cosphi(2*m-1,k,latp))*zrcsj end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 zwdalp = zw*dalp(mr+n,irow) zwalp = zw*alp (mr+n,irow) ir = mc + 2*n - 1 ii = ir + 1 d_tmp(ir) = d_tmp(ir) - (zwdalp*v_cosphi(2*m-1,k,latp) + & xm(m)*zwalp*u_cosphi(2*m ,k,latm))*zrcsj d_tmp(ii) = d_tmp(ii) - (zwdalp*v_cosphi(2*m ,k,latp) - & xm(m)*zwalp*u_cosphi(2*m-1,k,latm))*zrcsj vz_tmp(ir) = vz_tmp(ir) + (zwdalp*u_cosphi(2*m-1,k,latp) - & xm(m)*zwalp*v_cosphi(2*m ,k,latm))*zrcsj vz_tmp(ii) = vz_tmp(ii) + (zwdalp*u_cosphi(2*m ,k,latp) + & xm(m)*zwalp*v_cosphi(2*m-1,k,latm))*zrcsj end do end do enddo ! irow=1,plat/2 ! ! Compute grid point values of:u,v,vz, and d. ! do irow=1,plat/2 latp = irow latm = plat - irow + 1 zcor = ez*alp(2,irow) ! ! Compute(u,v,vz,d)m ! do m=1,nmmax(irow) mr = nstart(m) do n=1,nlen(m) ! ! These statements will likely not be bfb since xm*ra is now a scalar ! alpn (mr+n) = alp(mr+n,irow)*rsq(n+m-1)*xm(m)*ra dalpn(mr+n) = dalp(mr+n,irow)*rsq(n+m-1) *ra end do end do ! ! Zero fourier fields ! u_cosphi(:,k,latm) = 0._r8 u_cosphi(:,k,latp) = 0._r8 v_cosphi(:,k,latm) = 0._r8 v_cosphi(:,k,latp) = 0._r8 if(present(vort)) then vort_tmp(:,k,latm) = 0._r8 vort_tmp(:,k,latp) = 0._r8 end if if(present(div)) then div_tmp(:,k,latm) = 0._r8 div_tmp(:,k,latp) = 0._r8 end if do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=1,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 ! tmpr = d_tmp(ir)*alpn(mr+n) tmpi = d_tmp(ii)*alpn(mr+n) u_cosphi(2*m-1,k,latm) = u_cosphi(2*m-1,k,latm) + tmpi u_cosphi(2*m ,k,latm) = u_cosphi(2*m ,k,latm) - tmpr ! tmpr = d_tmp(ir)*dalpn(mr+n) tmpi = d_tmp(ii)*dalpn(mr+n) v_cosphi(2*m-1,k,latp) = v_cosphi(2*m-1,k,latp) - tmpr v_cosphi(2*m ,k,latp) = v_cosphi(2*m ,k,latp) - tmpi ! tmpr = vz_tmp(ir)*dalpn(mr+n) tmpi = vz_tmp(ii)*dalpn(mr+n) u_cosphi(2*m-1,k,latp) = u_cosphi(2*m-1,k,latp) + tmpr u_cosphi(2*m ,k,latp) = u_cosphi(2*m ,k,latp) + tmpi ! tmpr = vz_tmp(ir)*alpn(mr+n) tmpi = vz_tmp(ii)*alpn(mr+n) v_cosphi(2*m-1,k,latm) = v_cosphi(2*m-1,k,latm) + tmpi v_cosphi(2*m ,k,latm) = v_cosphi(2*m ,k,latm) - tmpr ! if(present(div)) then tmpr = d_tmp(ir)*alp(mr+n,irow) tmpi = d_tmp(ii)*alp(mr+n,irow) div_tmp(2*m-1,k,latm) = div_tmp(2*m-1,k,latm) + tmpr div_tmp(2*m ,k,latm) = div_tmp(2*m ,k,latm) + tmpi end if ! if(present(vort)) then tmpr = vz_tmp(ir)*alp(mr+n,irow) tmpi = vz_tmp(ii)*alp(mr+n,irow) vort_tmp(2*m-1,k,latm) = vort_tmp(2*m-1,k,latm) + tmpr vort_tmp(2*m ,k,latm) = vort_tmp(2*m ,k,latm) + tmpi end if end do end do do m=1,nmmax(irow) mr = nstart(m) mc = 2*mr do n=2,nlen(m),2 ir = mc + 2*n - 1 ii = ir + 1 ! tmpr = d_tmp(ir)*alpn(mr+n) tmpi = d_tmp(ii)*alpn(mr+n) u_cosphi(2*m-1,k,latp) = u_cosphi(2*m-1,k,latp) + tmpi u_cosphi(2*m ,k,latp) = u_cosphi(2*m ,k,latp) - tmpr ! tmpr = d_tmp(ir)*dalpn(mr+n) tmpi = d_tmp(ii)*dalpn(mr+n) v_cosphi(2*m-1,k,latm) = v_cosphi(2*m-1,k,latm) - tmpr v_cosphi(2*m ,k,latm) = v_cosphi(2*m ,k,latm) - tmpi ! tmpr = vz_tmp(ir)*dalpn(mr+n) tmpi = vz_tmp(ii)*dalpn(mr+n) u_cosphi(2*m-1,k,latm) = u_cosphi(2*m-1,k,latm) + tmpr u_cosphi(2*m ,k,latm) = u_cosphi(2*m ,k,latm) + tmpi ! tmpr = vz_tmp(ir)*alpn(mr+n) tmpi = vz_tmp(ii)*alpn(mr+n) v_cosphi(2*m-1,k,latp) = v_cosphi(2*m-1,k,latp) + tmpi v_cosphi(2*m ,k,latp) = v_cosphi(2*m ,k,latp) - tmpr ! if(present(div)) then tmpr = d_tmp(ir)*alp(mr+n,irow) tmpi = d_tmp(ii)*alp(mr+n,irow) div_tmp(2*m-1,k,latp) = div_tmp(2*m-1,k,latp) + tmpr div_tmp(2*m ,k,latp) = div_tmp(2*m ,k,latp) + tmpi end if ! if(present(vort)) then tmpr = vz_tmp(ir)*alp(mr+n,irow) tmpi = vz_tmp(ii)*alp(mr+n,irow) vort_tmp(2*m-1,k,latp) = vort_tmp(2*m-1,k,latp) + tmpr vort_tmp(2*m ,k,latp) = vort_tmp(2*m ,k,latp) + tmpi end if end do end do ! ! Correction to get the absolute vorticity. ! if(present(vort)) then vort_tmp(1,k,latp) = vort_tmp(1,k,latp) + zcor end if ! ! Recompute real fields from symmetric and antisymmetric parts ! do i=1,nlon(latm)+2 tmp1 = u_cosphi(i,k,latm) + u_cosphi(i,k,latp) tmp2 = u_cosphi(i,k,latm) - u_cosphi(i,k,latp) u_cosphi(i,k,latm) = tmp1 u_cosphi(i,k,latp) = tmp2 ! tmp1 = v_cosphi(i,k,latm) + v_cosphi(i,k,latp) tmp2 = v_cosphi(i,k,latm) - v_cosphi(i,k,latp) v_cosphi(i,k,latm) = tmp1 v_cosphi(i,k,latp) = tmp2 ! if(present(vort)) then tmp1 = vort_tmp(i,k,latm) + vort_tmp(i,k,latp) tmp2 = vort_tmp(i,k,latm) - vort_tmp(i,k,latp) vort_tmp(i,k,latm) = tmp1 vort_tmp(i,k,latp) = tmp2 end if ! if(present(div)) then tmp1 = div_tmp(i,k,latm) + div_tmp(i,k,latp) tmp2 = div_tmp(i,k,latm) - div_tmp(i,k,latp) div_tmp(i,k,latm) = tmp1 div_tmp(i,k,latp) = tmp2 end if end do enddo ! irow=1,plat/2 enddo ! k=1,plev ! do lat=1,plat ! ! Transform Fourier -> grid, obtaining spectrally truncated ! grid point values. ! irow = lat if (lat.gt.plat/2) irow = plat - lat + 1 call fft991(u_cosphi(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,+1) call fft991(v_cosphi(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,+1) if(present(vort)) then call fft991(vort_tmp(1,1,lat),work,trig(1,irow),ifax(1,irow),1, & plondfft,nlon(lat),plev,+1) vort(:nlon(lat),:,lat) = vort_tmp(:nlon(lat),:,lat) end if if(present(div)) then call fft991(div_tmp(1,1,lat),work,trig(1,irow),ifax(1,irow),1,plondfft, & nlon(lat),plev,+1) div(:nlon(lat),:,lat) = div_tmp(:nlon(lat),:,lat) end if ! ! Convert U,V to u,v ! zsqcs = sqrt(cs(irow)) do k=1,plev do i=1,nlon(lat) u3(i,k,lat) = u_cosphi(i,k,lat)/zsqcs v3(i,k,lat) = v_cosphi(i,k,lat)/zsqcs end do end do enddo deallocate( u_cosphi ) deallocate( v_cosphi ) if ( present(div) ) deallocate( div_tmp ) if ( present(vort) ) deallocate( vort_tmp ) return end subroutine spetru_uv end module spetru