c c . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . c . . c . copyright (c) 1998 by UCAR . c . . c . University Corporation for Atmospheric Research . c . . c . all rights reserved . c . . c . . c . SPHEREPACK . c . . c . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . c c c c c ... file slapes.f c c this file includes documentation and code for c subroutine slapes i c c ... files which must be loaded with slapec.f c c sphcom.f, hrfft.f, shaes.f, shses.f c c c c subroutine slapes(nlat,nlon,isym,nt,slap,ids,jds,a,b,mdab,ndab, c + wshses,lshses,work,lwork,ierror) c c c given the scalar spherical harmonic coefficients a and b, precomputed c by subroutine shaes for a scalar field sf, subroutine slapes computes c the laplacian of sf in the scalar array slap. slap(i,j) is the c laplacian of sf at the colatitude c c theta(i) = (i-1)*pi/(nlat-1) c c and east longitude c c lambda(j) = (j-1)*2*pi/nlon c c on the sphere. i.e. c c slap(i,j) = c c 2 2 c [1/sint*d (sf(i,j)/dlambda + d(sint*d(sf(i,j))/dtheta)/dtheta]/sint c c c where sint = sin(theta(i)). the scalar laplacian in slap has the c same symmetry or absence of symmetry about the equator as the scalar c field sf. the input parameters isym,nt,mdab,ndab must have the c same values used by shaes to compute a and b for sf. the associated c legendre functions are stored rather than recomputed as they are c in subroutine slapec. c c input parameters c c nlat the number of colatitudes on the full sphere including the c poles. for example, nlat = 37 for a five degree grid. c nlat determines the grid increment in colatitude as c pi/(nlat-1). if nlat is odd the equator is located at c grid point i=(nlat+1)/2. if nlat is even the equator is c located half way between points i=nlat/2 and i=nlat/2+1. c nlat must be at least 3. note: on the half sphere, the c number of grid points in the colatitudinal direction is c nlat/2 if nlat is even or (nlat+1)/2 if nlat is odd. c c nlon the number of distinct longitude points. nlon determines c the grid increment in longitude as 2*pi/nlon. for example c nlon = 72 for a five degree grid. nlon must be greater c than zero. the axisymmetric case corresponds to nlon=1. c the efficiency of the computation is improved when nlon c is a product of small prime numbers. c c isym this parameter should have the same value input to subroutine c shaes to compute the coefficients a and b for the scalar field c sf. isym is set as follows: c c = 0 no symmetries exist in sf about the equator. scalar c synthesis is used to compute slap on the entire sphere. c i.e., in the array slap(i,j) for i=1,...,nlat and c j=1,...,nlon. c c = 1 sf and slap are antisymmetric about the equator. the c synthesis used to compute slap is performed on the c northern hemisphere only. if nlat is odd, slap(i,j) is c computed for i=1,...,(nlat+1)/2 and j=1,...,nlon. if c nlat is even, slap(i,j) is computed for i=1,...,nlat/2 c and j=1,...,nlon. c c c = 2 sf and slap are symmetric about the equator. the c synthesis used to compute slap is performed on the c northern hemisphere only. if nlat is odd, slap(i,j) is c computed for i=1,...,(nlat+1)/2 and j=1,...,nlon. if c nlat is even, slap(i,j) is computed for i=1,...,nlat/2 c and j=1,...,nlon. c c c nt the number of analyses. in the program that calls slapes c the arrays slap,a, and b can be three dimensional in which c case multiple synthesis will be performed. the third index c is the synthesis index which assumes the values k=1,...,nt. c for a single analysis set nt=1. the description of the c remaining parameters is simplified by assuming that nt=1 c or that all the arrays are two dimensional. c c ids the first dimension of the array slap as it appears in the c program that calls slapes. if isym = 0 then ids must be at c least nlat. if isym > 0 and nlat is even then ids must be c at least nlat/2. if isym > 0 and nlat is odd then ids must c be at least (nlat+1)/2. c c jds the second dimension of the array slap as it appears in the c program that calls slapes. jds must be at least nlon. c c c a,b two or three dimensional arrays (see input parameter nt) c that contain scalar spherical harmonic coefficients c of the scalar field sf as computed by subroutine shaes. c *** a,b must be computed by shaes prior to calling slapes. c c c mdab the first dimension of the arrays a and b as it appears c in the program that calls slapes. mdab must be at c least min0(nlat,(nlon+2)/2) if nlon is even or at least c min0(nlat,(nlon+1)/2) if nlon is odd. c c ndab the second dimension of the arrays a and b as it appears c in the program that calls slapes. ndbc must be at least c least nlat. c c mdab,ndab should have the same values input to shaes to c compute the coefficients a and b. c c c wshses an array which must be initialized by subroutine shsesi c before calling slapes. once initialized, wshses c can be used repeatedly by slapes as long as nlat and nlon c remain unchanged. wshses must not be altered between calls c of slapes. c c lshses the dimension of the array wshses as it appears in the c program that calls slapes. let c c l1 = min0(nlat,(nlon+2)/2) if nlon is even or c l1 = min0(nlat,(nlon+1)/2) if nlon is odd c c and c c l2 = nlat/2 if nlat is even or c l2 = (nlat+1)/2 if nlat is odd c c then lshses must be greater than or equal to c c (l1*l2*(nlat+nlat-l1+1))/2+nlon+15. c c c work a work array that does not have to be saved. c c c lwork the dimension of the array work as it appears in the c program that calls slapes. define c c l2 = nlat/2 if nlat is even or c l2 = (nlat+1)/2 if nlat is odd c l1 = min0(nlat,(nlon+2)/2) if nlon is even or c l1 = min0(nlat,(nlon+1)/2) if nlon is odd c c if isym is zero then lwork must be at least c c (nt+1)*nlat*nlon + nlat*(2*nt*l1+1) c c if isym is nonzero lwork must be at least c c (nt+1)*l2*nlon + nlat*(2*nt*l1+1) c c ************************************************************** c c output parameters c c c slap a two or three dimensional arrays (see input parameter nt) that c contain the scalar laplacian of the scalar field sf. slap(i,j) c is the scalar laplacian at the colatitude c c theta(i) = (i-1)*pi/(nlat-1) c c and longitude c c lambda(j) = (j-1)*2*pi/nlon c c for i=1,...,nlat and j=1,...,nlon. c c c ierror a parameter which flags errors in input parameters as follows: c c = 0 no errors detected c c = 1 error in the specification of nlat c c = 2 error in the specification of nlon c c = 3 error in the specification of ityp c c = 4 error in the specification of nt c c = 5 error in the specification of ids c c = 6 error in the specification of jds c c = 7 error in the specification of mdbc c c = 8 error in the specification of ndbc c c = 9 error in the specification of lshses c c = 10 error in the specification of lwork c c c ********************************************************************** c c end of documentation for slapes c c ********************************************************************** c subroutine slapes(nlat,nlon,isym,nt,slap,ids,jds,a,b,mdab,ndab, + wshses,lshses,work,lwork,ierror) dimension slap(ids,jds,nt),a(mdab,ndab,nt),b(mdab,ndab,nt) dimension wshses(lshses),work(lwork) c c check input parameters c ierror = 1 if(nlat .lt. 3) return ierror = 2 if(nlon .lt. 4) return ierror = 3 if (isym.lt.0 .or. isym.gt.2) return ierror = 4 if(nt .lt. 0) return ierror = 5 imid = (nlat+1)/2 if((isym.eq.0 .and. ids.lt.nlat) .or. 1 (isym.gt.0 .and. ids.lt.imid)) return ierror = 6 if(jds .lt. nlon) return ierror = 7 mmax = min0(nlat,nlon/2+1) if(mdab .lt. mmax) return ierror = 8 if(ndab .lt. nlat) return ierror = 9 imid = (nlat+1)/2 lpimn = (imid*mmax*(nlat+nlat-mmax+1))/2 if(lshses .lt. lpimn+nlon+15) return ierror = 10 c c set and verify unsaved work space length c ls = nlat if(isym .gt. 0) ls = imid nln = nt*ls*nlon mn = mmax*nlat*nt c lwkmin = nln+ls*nlon+2*mn+nlat c if (lwork .lt. lwkmin) return l2 = (nlat+1)/2 l1 = min0(nlat,nlon/2+1) if (isym.eq.0) then lwkmin = (nt+1)*nlat*nlon + nlat*(2*nt*l1+1) else lwkmin = (nt+1)*l2*nlon + nlat*(2*nt*l1+1) end if if (lwork .lt. lwkmin) return ierror = 0 c c set work space pointers c ia = 1 ib = ia+mn ifn = ib+mn iwk = ifn+nlat lwk = lwork-2*mn-nlat call slapes1(nlat,nlon,isym,nt,slap,ids,jds,a,b,mdab,ndab, +work(ia),work(ib),mmax,work(ifn),wshses,lshses,work(iwk),lwk, +ierror) return end subroutine slapes1(nlat,nlon,isym,nt,slap,ids,jds,a,b,mdab,ndab, + alap,blap,mmax,fnn,wsave,lsave,wk,lwk,ierror) dimension slap(ids,jds,nt),a(mdab,ndab,nt),b(mdab,ndab,nt) dimension alap(mmax,nlat,nt),blap(mmax,nlat,nt),fnn(nlat) dimension wsave(lsave),wk(lwk) c c set coefficient multiplyers c do 1 n=2,nlat fn = float(n-1) fnn(n) = fn*(fn+1.) 1 continue c c compute scalar laplacian coefficients for each vector field c do 2 k=1,nt do 3 n=1,nlat do 4 m=1,mmax alap(m,n,k) = 0.0 blap(m,n,k) = 0.0 4 continue 3 continue c c compute m=0 coefficients c do 5 n=2,nlat alap(1,n,k) = -fnn(n)*a(1,n,k) blap(1,n,k) = -fnn(n)*b(1,n,k) 5 continue c c compute m>0 coefficients c do 6 m=2,mmax do 7 n=m,nlat alap(m,n,k) = -fnn(n)*a(m,n,k) blap(m,n,k) = -fnn(n)*b(m,n,k) 7 continue 6 continue 2 continue c c synthesize alap,blap into slap c call shses(nlat,nlon,isym,nt,slap,ids,jds,alap,blap, + mmax,nlat,wsave,lsave,wk,lwk,ierror) return end