!********************************************************************** ! Copyright 1998,1999,2000,2001,2002,2005,2007,2008,2009,2010 * ! Andreas Stohl, Petra Seibert, A. Frank, Gerhard Wotawa, * ! Caroline Forster, Sabine Eckhardt, John Burkhart, Harald Sodemann * ! * ! This file is part of FLEXPART. * ! * ! FLEXPART is free software: you can redistribute it and/or modify * ! it under the terms of the GNU General Public License as published by* ! the Free Software Foundation, either version 3 of the License, or * ! (at your option) any later version. * ! * ! FLEXPART is distributed in the hope that it will be useful, * ! but WITHOUT ANY WARRANTY; without even the implied warranty of * ! MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * ! GNU General Public License for more details. * ! * ! You should have received a copy of the GNU General Public License * ! along with FLEXPART. If not, see . * !********************************************************************** subroutine calcpv_nests(l,n,uuhn,vvhn,pvhn) ! i i i i o !***************************************************************************** ! * ! Calculation of potential vorticity on 3-d nested grid * ! * ! Author: P. James * ! 22 February 2000 * ! * !***************************************************************************** ! * ! Variables: * ! n temporal index for meteorological fields (1 to 2) * ! l index of current nest * ! * ! Constants: * ! * !***************************************************************************** use par_mod use com_mod implicit none integer :: n,ix,jy,i,j,k,kl,ii,jj,klvrp,klvrm,klpt,kup,kdn,kch integer :: jyvp,jyvm,ixvp,ixvm,jumpx,jumpy,jux,juy,ivrm,ivrp,ivr integer :: nlck,l real :: vx(2),uy(2),phi,tanphi,cosphi,dvdx,dudy,f real :: theta,thetap,thetam,dthetadp,dt1,dt2,dt real :: ppml(0:nxmaxn-1,0:nymaxn-1,nuvzmax),ppmk(0:nxmaxn-1,0:nymaxn-1,nuvzmax) real :: thup,thdn real,parameter :: eps=1.e-5,p0=101325 real :: uuhn(0:nxmaxn-1,0:nymaxn-1,nuvzmax,maxnests) real :: vvhn(0:nxmaxn-1,0:nymaxn-1,nuvzmax,maxnests) real :: pvhn(0:nxmaxn-1,0:nymaxn-1,nuvzmax,maxnests) ! Set number of levels to check for adjacent theta nlck=nuvz/3 ! ! Loop over entire grid !********************** do kl=1,nuvz do jy=0,nyn(l)-1 do ix=0,nxn(l)-1 ppml(ix,jy,kl)=akz(kl)+bkz(kl)*psn(ix,jy,1,n,l) enddo enddo enddo ppmk=(100000./ppml)**kappa do jy=0,nyn(l)-1 phi = (ylat0n(l) + jy * dyn(l)) * pi / 180. f = 0.00014585 * sin(phi) tanphi = tan(phi) cosphi = cos(phi) ! Provide a virtual jy+1 and jy-1 in case we are on domain edge (Lat) jyvp=jy+1 jyvm=jy-1 if (jy.eq.0) jyvm=0 if (jy.eq.nyn(l)-1) jyvp=nyn(l)-1 ! Define absolute gap length jumpy=2 if (jy.eq.0.or.jy.eq.nyn(l)-1) jumpy=1 juy=jumpy ! do ix=0,nxn(l)-1 ! Provide a virtual ix+1 and ix-1 in case we are on domain edge (Long) ixvp=ix+1 ixvm=ix-1 jumpx=2 if (ix.eq.0) ixvm=0 if (ix.eq.nxn(l)-1) ixvp=nxn(l)-1 ivrp=ixvp ivrm=ixvm ! Define absolute gap length if (ix.eq.0.or.ix.eq.nxn(l)-1) jumpx=1 jux=jumpx ! ! Loop over the vertical !*********************** do kl=1,nuvz theta=tthn(ix,jy,kl,n,l)*ppmk(ix,jy,kl) klvrp=kl+1 klvrm=kl-1 klpt=kl ! If top or bottom level, dthetadp is evaluated between the current ! level and the level inside, otherwise between level+1 and level-1 ! if (klvrp.gt.nuvz) klvrp=nuvz if (klvrm.lt.1) klvrm=1 thetap=tthn(ix,jy,klvrp,n,l)*ppmk(ix,jy,klvrp) thetam=tthn(ix,jy,klvrm,n,l)*ppmk(ix,jy,klvrm) dthetadp=(thetap-thetam)/(ppml(ix,jy,klvrp)-ppml(ix,jy,klvrm)) ! Compute vertical position at pot. temperature surface on subgrid ! and the wind at that position !***************************************************************** ! a) in x direction ii=0 do i=ixvm,ixvp,jumpx ivr=i ii=ii+1 ! Search adjacent levels for current theta value ! Spiral out from current level for efficiency kup=klpt-1 kdn=klpt kch=0 40 continue ! Upward branch kup=kup+1 if (kch.ge.nlck) goto 21 ! No more levels to check, ! ! and no values found if (kup.ge.nuvz) goto 41 kch=kch+1 k=kup thdn=tthn(ivr,jy,k,n,l)*ppmk(ivr,jy,k) thup=tthn(ivr,jy,k+1,n,l)*ppmk(ivr,jy,k+1) if (((thdn.ge.theta).and.(thup.le.theta)).or. & ((thdn.le.theta).and.(thup.ge.theta))) then dt1=abs(theta-thdn) dt2=abs(theta-thup) dt=dt1+dt2 if (dt.lt.eps) then ! Avoid division by zero error dt1=0.5 ! G.W., 10.4.1996 dt2=0.5 dt=1.0 endif vx(ii)=(vvhn(ivr,jy,k,l)*dt2+vvhn(ivr,jy,k+1,l)*dt1)/dt goto 20 endif 41 continue ! Downward branch kdn=kdn-1 if (kdn.lt.1) goto 40 kch=kch+1 k=kdn thdn=tthn(ivr,jy,k,n,l)*ppmk(ivr,jy,k) thup=tthn(ivr,jy,k+1,n,l)*ppmk(ivr,jy,k+1) if (((thdn.ge.theta).and.(thup.le.theta)).or. & ((thdn.le.theta).and.(thup.ge.theta))) then dt1=abs(theta-thdn) dt2=abs(theta-thup) dt=dt1+dt2 if (dt.lt.eps) then ! Avoid division by zero error dt1=0.5 ! G.W., 10.4.1996 dt2=0.5 dt=1.0 endif vx(ii)=(vvhn(ivr,jy,k,l)*dt2+vvhn(ivr,jy,k+1,l)*dt1)/dt goto 20 endif goto 40 ! This section used when no values were found 21 continue ! Must use vv at current level and long. jux becomes smaller by 1 vx(ii)=vvhn(ix,jy,kl,l) jux=jux-1 ! Otherwise OK 20 continue end do if (jux.gt.0) then dvdx=(vx(2)-vx(1))/real(jux)/(dxn(l)*pi/180.) else dvdx=vvhn(ivrp,jy,kl,l)-vvhn(ivrm,jy,kl,l) dvdx=dvdx/real(jumpx)/(dxn(l)*pi/180.) ! Only happens if no equivalent theta value ! can be found on either side, hence must use values ! from either side, same pressure level. end if ! b) in y direction jj=0 do j=jyvm,jyvp,jumpy jj=jj+1 ! Search adjacent levels for current theta value ! Spiral out from current level for efficiency kup=klpt-1 kdn=klpt kch=0 70 continue ! Upward branch kup=kup+1 if (kch.ge.nlck) goto 51 ! No more levels to check, ! ! and no values found if (kup.ge.nuvz) goto 71 kch=kch+1 k=kup thdn=tthn(ix,j,k,n,l)*ppmk(ix,j,k) thup=tthn(ix,j,k+1,n,l)*ppmk(ix,j,k+1) if (((thdn.ge.theta).and.(thup.le.theta)).or. & ((thdn.le.theta).and.(thup.ge.theta))) then dt1=abs(theta-thdn) dt2=abs(theta-thup) dt=dt1+dt2 if (dt.lt.eps) then ! Avoid division by zero error dt1=0.5 ! G.W., 10.4.1996 dt2=0.5 dt=1.0 endif uy(jj)=(uuhn(ix,j,k,l)*dt2+uuhn(ix,j,k+1,l)*dt1)/dt goto 50 endif 71 continue ! Downward branch kdn=kdn-1 if (kdn.lt.1) goto 70 kch=kch+1 k=kdn thdn=tthn(ix,j,k,n,l)*ppmk(ix,j,k) thup=tthn(ix,j,k+1,n,l)*ppmk(ix,j,k+1) if (((thdn.ge.theta).and.(thup.le.theta)).or. & ((thdn.le.theta).and.(thup.ge.theta))) then dt1=abs(theta-thdn) dt2=abs(theta-thup) dt=dt1+dt2 if (dt.lt.eps) then ! Avoid division by zero error dt1=0.5 ! G.W., 10.4.1996 dt2=0.5 dt=1.0 endif uy(jj)=(uuhn(ix,j,k,l)*dt2+uuhn(ix,j,k+1,l)*dt1)/dt goto 50 endif goto 70 ! This section used when no values were found 51 continue ! Must use uu at current level and lat. juy becomes smaller by 1 uy(jj)=uuhn(ix,jy,kl,l) juy=juy-1 ! Otherwise OK 50 continue end do if (juy.gt.0) then dudy=(uy(2)-uy(1))/real(juy)/(dyn(l)*pi/180.) else dudy=uuhn(ix,jyvp,kl,l)-uuhn(ix,jyvm,kl,l) dudy=dudy/real(jumpy)/(dyn(l)*pi/180.) end if ! pvhn(ix,jy,kl,l)=dthetadp*(f+(dvdx/cosphi-dudy & +uuhn(ix,jy,kl,l)*tanphi)/r_earth)*(-1.e6)*9.81 ! ! Resest jux and juy jux=jumpx juy=jumpy end do end do end do ! end subroutine calcpv_nests