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 ... file shaes.f c c this file contains code and documentation for subroutines c shaes and shaesi c c ... files which must be loaded with shaes.f c c sphcom.f, hrfft.f c c subroutine shaes(nlat,nlon,isym,nt,g,idg,jdg,a,b,mdab,ndab, c + wshaes,lshaes,work,lwork,ierror) c c subroutine shaes performs the spherical harmonic analysis c on the array g and stores the result in the arrays a and b. c the analysis is performed on an equally spaced grid. the c associated legendre functions are stored rather than recomputed c as they are in subroutine shaec. the analysis is described c below at output parameters a,b. c c sphcom.f, hrfft.f c 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 londitude 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 or equal to 4. the efficiency of the computation is c improved when nlon is a product of small prime numbers. c c isym = 0 no symmetries exist about the equator. the analysis c is performed on the entire sphere. i.e. on the c array g(i,j) for i=1,...,nlat and j=1,...,nlon. c (see description of g below) c c = 1 g is antisymmetric about the equator. the analysis c is performed on the northern hemisphere only. i.e. c if nlat is odd the analysis is performed on the c array g(i,j) for i=1,...,(nlat+1)/2 and j=1,...,nlon. c if nlat is even the analysis is performed on the c array g(i,j) for i=1,...,nlat/2 and j=1,...,nlon. c c c = 2 g is symmetric about the equator. the analysis is c performed on the northern hemisphere only. i.e. c if nlat is odd the analysis is performed on the c array g(i,j) for i=1,...,(nlat+1)/2 and j=1,...,nlon. c if nlat is even the analysis is performed on the c array g(i,j) for i=1,...,nlat/2 and j=1,...,nlon. c c nt the number of analyses. in the program that calls shaes, c the arrays g,a and b can be three dimensional in which c case multiple analyses will be performed. the third c index is the analysis index which assumes the values c k=1,...,nt. for a single analysis set nt=1. the c discription of the remaining parameters is simplified c by assuming that nt=1 or that the arrays g,a and b c have only two dimensions. c c g a two or three dimensional array (see input parameter c nt) that contains the discrete function to be analyzed. c g(i,j) contains the value of the function at the colatitude c point theta(i) = (i-1)*pi/(nlat-1) and longitude point c phi(j) = (j-1)*2*pi/nlon. the index ranges are defined c above at the input parameter isym. c c c idg the first dimension of the array g as it appears in the c program that calls shaes. if isym equals zero then idg c must be at least nlat. if isym is nonzero then idg c must be at least nlat/2 if nlat is even or at least c (nlat+1)/2 if nlat is odd. c c jdg the second dimension of the array g as it appears in the c program that calls shaes. jdg must be at least nlon. c c mdab the first dimension of the arrays a and b as it appears c in the program that calls shaes. mdab must be at least c 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 shaes. ndab must be at least nlat c c wshaes an array which must be initialized by subroutine shaesi. c once initialized, wshaes can be used repeatedly by shaes c as long as nlon and nlat remain unchanged. wshaes must c not be altered between calls of shaes. c c lshaes the dimension of the array wshaes as it appears in the c program that calls shaes. define 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 lshaes must be at least c c (l1*l2*(nlat+nlat-l1+1))/2+nlon+15 c c work a work array that does not have to be saved. c c lwork the dimension of the array work as it appears in the c program that calls shaes. define c c l2 = nlat/2 if nlat is even or c l2 = (nlat+1)/2 if nlat is odd c c if isym is zero then lwork must be at least c (nt+1)*nlat*nlon. if isym is not zero then c lwork must be at least (nt+1)*l2*nlon. c c c ************************************************************** c c output parameters c c a,b both a,b are two or three dimensional arrays (see input c parameter nt) that contain the spherical harmonic c coefficients in the representation of g(i,j) given in the c discription of subroutine shses. for isym=0, a(m,n) and c b(m,n) are given by the equations listed below. symmetric c versions are used when isym is greater than zero. c c c c definitions c c 1. the normalized associated legendre functions c c pbar(m,n,theta) = sqrt((2*n+1)*factorial(n-m)/(2*factorial(n+m))) c *sin(theta)**m/(2**n*factorial(n)) times the c (n+m)th derivative of (x**2-1)**n with respect c to x=cos(theta) c c 2. the normalized z functions for m even c c zbar(m,n,theta) = 2/(nlat-1) times the sum from k=0 to k=nlat-1 of c the integral from tau = 0 to tau = pi of c cos(k*theta)*cos(k*tau)*pbar(m,n,tau)*sin(tau) c (first and last terms in this sum are divided c by 2) c c 3. the normalized z functions for m odd c c zbar(m,n,theta) = 2/(nlat-1) times the sum from k=0 to k=nlat-1 of c of the integral from tau = 0 to tau = pi of c sin(k*theta)*sin(k*tau)*pbar(m,n,tau)*sin(tau) c c 4. the fourier transform of g(i,j). c c c(m,i) = 2/nlon times the sum from j=1 to j=nlon c of g(i,j)*cos((m-1)*(j-1)*2*pi/nlon) c (the first and last terms in this sum c are divided by 2) c c s(m,i) = 2/nlon times the sum from j=2 to j=nlon c of g(i,j)*sin((m-1)*(j-1)*2*pi/nlon) c c 5. the maximum (plus one) longitudinal wave number c c mmax = min0(nlat,(nlon+2)/2) if nlon is even or c mmax = min0(nlat,(nlon+1)/2) if nlon is odd. c c then for m=0,...,mmax-1 and n=m,...,nlat-1 the arrays a,b are c given by c c a(m+1,n+1) = the sum from i=1 to i=nlat of c c(m+1,i)*zbar(m,n,theta(i)) c (first and last terms in this sum are c divided by 2) c c b(m+1,n+1) = the sum from i=1 to i=nlat of c s(m+1,i)*zbar(m,n,theta(i)) c c c ierror = 0 no errors c = 1 error in the specification of nlat c = 2 error in the specification of nlon c = 3 error in the specification of isym c = 4 error in the specification of nt c = 5 error in the specification of idg c = 6 error in the specification of jdg c = 7 error in the specification of mdab c = 8 error in the specification of ndab c = 9 error in the specification of lshaes c = 10 error in the specification of lwork c c c **************************************************************** c subroutine shaesi(nlat,nlon,wshaes,lshaes,work,lwork,dwork, c + ldwork,ierror) c c subroutine shaesi initializes the array wshaes which can then c be used repeatedly by subroutine shaes 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 londitude 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 or equal to 4. the efficiency of the computation is c improved when nlon is a product of small prime numbers. c c lshaes the dimension of the array wshaes as it appears in the c program that calls shaesi. define 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 lshaes must be at least c c (l1*l2*(nlat+nlat-l1+1))/2+nlon+15 c c work a real work array that does not have to be saved. c c lwork the dimension of the array work as it appears in the c program that calls shaesi. define 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 lwork must be at least c c 5*nlat*l2+3*((l1-2)*(nlat+nlat-l1-1))/2 c c c dwork a double precision work array that does not have to be saved. c c ldwork the dimension of the array dwork as it appears in the c program that calls shaesi. ldwork must be at least nlat+1 c c c output parameters c c wshaes an array which is initialized for use by subroutine shaes. c once initialized, wshaes can be used repeatedly by shaes c as long as nlon and nlat remain unchanged. wshaes must c not be altered between calls of shaes. c c ierror = 0 no errors c = 1 error in the specification of nlat c = 2 error in the specification of nlon c = 3 error in the specification of lshaes c = 4 error in the specification of lwork c = 5 error in the specification of ldwork c c c **************************************************************** subroutine shaes(nlat,nlon,isym,nt,g,idg,jdg,a,b,mdab,ndab, 1 wshaes,lshaes,work,lwork,ierror) dimension g(idg,jdg,1),a(mdab,ndab,1),b(mdab,ndab,1),wshaes(1), 1 work(1) 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 if((isym.eq.0 .and. idg.lt.nlat) .or. 1 (isym.ne.0 .and. idg.lt.(nlat+1)/2)) return ierror = 6 if(jdg .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 idz = (mmax*(nlat+nlat-mmax+1))/2 lzimn = idz*imid if(lshaes .lt. lzimn+nlon+15) return ierror = 10 ls = nlat if(isym .gt. 0) ls = imid nln = nt*ls*nlon if(lwork .lt. nln+ls*nlon) return ierror = 0 ist = 0 if(isym .eq. 0) ist = imid call shaes1(nlat,isym,nt,g,idg,jdg,a,b,mdab,ndab,wshaes,idz, 1 ls,nlon,work,work(ist+1),work(nln+1),wshaes(lzimn+1)) return end subroutine shaes1(nlat,isym,nt,g,idgs,jdgs,a,b,mdab,ndab,z,idz, 1 idg,jdg,ge,go,work,whrfft) dimension g(idgs,jdgs,1),a(mdab,ndab,1),b(mdab,ndab,1),z(idz,1), 1 ge(idg,jdg,1),go(idg,jdg,1),work(1),whrfft(1) ls = idg nlon = jdg mmax = min0(nlat,nlon/2+1) mdo = mmax if(mdo+mdo-1 .gt. nlon) mdo = mmax-1 nlp1 = nlat+1 tsn = 2./nlon fsn = 4./nlon imid = (nlat+1)/2 modl = mod(nlat,2) imm1 = imid if(modl .ne. 0) imm1 = imid-1 if(isym .ne. 0) go to 15 do 5 k=1,nt do 5 i=1,imm1 do 5 j=1,nlon ge(i,j,k) = tsn*(g(i,j,k)+g(nlp1-i,j,k)) go(i,j,k) = tsn*(g(i,j,k)-g(nlp1-i,j,k)) 5 continue go to 30 15 do 20 k=1,nt do 20 i=1,imm1 do 20 j=1,nlon ge(i,j,k) = fsn*g(i,j,k) 20 continue if(isym .eq. 1) go to 27 30 if(modl .eq. 0) go to 27 do 25 k=1,nt do 25 j=1,nlon ge(imid,j,k) = tsn*g(imid,j,k) 25 continue 27 do 35 k=1,nt call hrfftf(ls,nlon,ge(1,1,k),ls,whrfft,work) if(mod(nlon,2) .ne. 0) go to 35 do 36 i=1,ls ge(i,nlon,k) = .5*ge(i,nlon,k) 36 continue 35 continue do 40 k=1,nt do 40 mp1=1,mmax do 40 np1=mp1,nlat a(mp1,np1,k) = 0. b(mp1,np1,k) = 0. 40 continue if(isym .eq. 1) go to 145 do 110 k=1,nt do 110 i=1,imid do 110 np1=1,nlat,2 a(1,np1,k) = a(1,np1,k)+z(np1,i)*ge(i,1,k) 110 continue ndo = nlat if(mod(nlat,2) .eq. 0) ndo = nlat-1 do 120 mp1=2,mdo m = mp1-1 mb = m*(nlat-1)-(m*(m-1))/2 do 120 k=1,nt do 120 i=1,imid do 120 np1=mp1,ndo,2 a(mp1,np1,k) = a(mp1,np1,k)+z(np1+mb,i)*ge(i,2*mp1-2,k) b(mp1,np1,k) = b(mp1,np1,k)+z(np1+mb,i)*ge(i,2*mp1-1,k) 120 continue if(mdo .eq. mmax .or. mmax .gt. ndo) go to 135 mb = mdo*(nlat-1)-(mdo*(mdo-1))/2 do 130 k=1,nt do 130 i=1,imid do 130 np1=mmax,ndo,2 a(mmax,np1,k) = a(mmax,np1,k)+z(np1+mb,i)*ge(i,2*mmax-2,k) 130 continue 135 if(isym .eq. 2) return 145 do 150 k=1,nt do 150 i=1,imm1 do 150 np1=2,nlat,2 a(1,np1,k) = a(1,np1,k)+z(np1,i)*go(i,1,k) 150 continue ndo = nlat if(mod(nlat,2) .ne. 0) ndo = nlat-1 do 160 mp1=2,mdo m = mp1-1 mp2 = mp1+1 mb = m*(nlat-1)-(m*(m-1))/2 do 160 k=1,nt do 160 i=1,imm1 do 160 np1=mp2,ndo,2 a(mp1,np1,k) = a(mp1,np1,k)+z(np1+mb,i)*go(i,2*mp1-2,k) b(mp1,np1,k) = b(mp1,np1,k)+z(np1+mb,i)*go(i,2*mp1-1,k) 160 continue mp2 = mmax+1 if(mdo .eq. mmax .or. mp2 .gt. ndo) return mb = mdo*(nlat-1)-(mdo*(mdo-1))/2 do 170 k=1,nt do 170 i=1,imm1 do 170 np1=mp2,ndo,2 a(mmax,np1,k) = a(mmax,np1,k)+z(np1+mb,i)*go(i,2*mmax-2,k) 170 continue return end subroutine shaesi(nlat,nlon,wshaes,lshaes,work,lwork,dwork, + ldwork,ierror) dimension wshaes(*),work(*) double precision dwork(*) c c length of wshaes is (l*(l+1)*imid)/2+nlon+15 c length of work is 5*l*imid + 3*((l-3)*l+2)/2 c ierror = 1 if(nlat.lt.3) return ierror = 2 if(nlon.lt.4) return ierror = 3 mmax = min0(nlat,nlon/2+1) imid = (nlat+1)/2 lzimn = (imid*mmax*(nlat+nlat-mmax+1))/2 if(lshaes .lt. lzimn+nlon+15) return ierror = 4 labc = 3*((mmax-2)*(nlat+nlat-mmax-1))/2 if(lwork .lt. 5*nlat*imid + labc) return ierror = 5 if (ldwork .lt. nlat+1) return ierror = 0 iw1 = 3*nlat*imid+1 idz = (mmax*(nlat+nlat-mmax+1))/2 call sea1(nlat,nlon,imid,wshaes,idz,work,work(iw1),dwork) call hrffti(nlon,wshaes(lzimn+1)) return end