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dfer |
1.1 |
function [psi,mskG,ylat] = calcEulerPsiCube(varargin); |
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% [psi,mskG,ylat] = calcEulerPsiCube(d,g,flu,rstar,blkFile,[optional]); |
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% |
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% Input arguements: |
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dfer |
1.2 |
% d [Field data] Velocity field (Mass-weighted if rstar=1): |
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% UVELMASS,VVELMASS for rstar=1 |
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% UVEL,VVEL for rstar=0 |
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dfer |
1.1 |
% g [Grid data ] drF,dxG,dyG,HFacW,HFacS |
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% flu (str) 'O' or 'A' for ocean or atmosphere |
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% rstar (int) 0 or 1 if you are using r* coordinates or not |
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% blkFile (str) Broken line file ('isoLat_cs32_59.mat') |
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% The incoming field data (d) and grid data (g) must be in a |
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% structured array format |
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% Optional parameters: |
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% mask (struct) mask (structured array including maskW and maskS) |
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% |
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% Output fields: |
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% psi Overturning (eg [61,6,nt]) |
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% mskG Land mask (eg [60,5]) |
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% ylat Latitude coordinate of psi (eg [61,1]) |
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% |
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% Description: |
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% Caculates overturning stream function (psi). For the atmosphere, data |
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% is must be in p-coordinates and the output is the mass transport psi |
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% [10^9 kg/s]. For the ocean, data should be in z-coordinates and the |
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% output is the volume transport psi [10^6 m^3/s = Sv]. If the rstar |
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% parameters is on, hu and hv are used, if off, the hfacw*.u and hfacs*.v |
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% are used (the multiplication being done inside the function). |
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% |
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% 'psi' is tabulated on broken lines at the interface between cells in |
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% the vertical. 'mskG' is for the area between broken lines and between |
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% the cell interfaces in the vertical. |
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% |
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% Defaults that can be overriden. |
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grav = 9.81; |
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masking=0; |
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% Read input parameters. |
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d = varargin{1}; |
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g = varargin{2}; |
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flu = varargin{3}; |
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rstar = varargin{4}; |
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blkFile = varargin{5}; |
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if length(varargin) == 6 |
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mask = varargin{6}; |
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masking = 1; |
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end |
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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% Prepare / reform incoming data % |
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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nc = size(g.XC,2); |
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nr = length(g.drF); |
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delM = g.drF; |
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dxg = reshape(g.dxG(1:6*nc,1:nc),[6*nc*nc,1]); |
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dyg = reshape(g.dyG(1:6*nc,1:nc),[6*nc*nc,1]); |
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if rstar |
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nt = size(d.UVELMASS,4); |
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hu = reshape(d.UVELMASS(1:6*nc,1:nc,1:nr,1:nt),[6*nc*nc,nr,nt]); |
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hv = reshape(d.VVELMASS(1:6*nc,1:nc,1:nr,1:nt),[6*nc*nc,nr,nt]); |
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else |
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nt = size(d.UVEL,4); |
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hw = reshape(g.HFacW(1:6*nc,1:nc,1:nr),[6*nc*nc,nr]); |
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hs = reshape(g.HFacS(1:6*nc,1:nc,1:nr),[6*nc*nc,nr]); |
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hu = reshape(d.UVEL(1:6*nc,1:nc,1:nr,1:nt),[6*nc*nc,nr,nt]); |
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hv = reshape(d.VVEL(1:6*nc,1:nc,1:nr,1:nt),[6*nc*nc,nr,nt]); |
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for it = 1:nt |
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hu(:,:,it) = hw.*hu(:,:,it); |
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hv(:,:,it) = hs.*hv(:,:,it); |
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end |
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end |
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mskWloc = ones(6*nc*nc,1); |
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mskSloc = ones(6*nc*nc,1); |
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if masking == 1 |
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mskWloc=reshape(mask.maskW(:,:,1),6*nc*nc,1); |
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mskSloc=reshape(mask.maskS(:,:,1),6*nc*nc,1); |
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%hu = repmat(reshape(mask.maskW,6*nc*nc,1),[1 nr nt]) .* hu; |
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%hv = repmat(reshape(mask.maskS,6*nc*nc,1),[1 nr nt]) .* hv; |
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end |
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% Load broken information. |
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% I looked at calc_psiH_CS.m, and did not find it very clear. |
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% May be you can try to see what is in |
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% MITgcm/utils/matlab/cs_grid/bk_line/use_psiLine.m |
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% it s shorter, and slightly better. |
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load(blkFile); |
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ydim = length(bkl_Ylat); |
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ylat = [-90,bkl_Ylat,90]; |
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% kMsep=1; |
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% if (nargin < 6), kfac=0; |
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% else kfac=1; end; |
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nBas=0; |
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% Prepare arrays. |
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psi = zeros(ydim+2,nr+1,1+nBas,nt); |
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mskZ = zeros(ydim+2,nr+1,1+nBas); % Mask of psi |
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mskV = zeros(ydim+2,nr,1+nBas); % Mask of the merid. transport |
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mskG = zeros(ydim+1,nr,1+nBas); % Mask of the ground |
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% The variable "bkl_Flg" is -1/1 if edge (on a given broken) has a u point |
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% and -2/2 if it has a v point. Positive/negative values contribute |
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% positively/negatively to northward heat transport (this depends on the |
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% oreientation of the cell). A zero value indicates an end of edges that |
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% contribute to a broken line. The u and v information is parced into two |
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% seperate fields, ufac and vfac (-2/2 are reduced to -1/1 for vfac). |
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ufac = zeros([size(bkl_Flg),1+nBas]); |
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vfac = zeros([size(bkl_Flg),1+nBas]); |
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ufac(:,:,1) = rem(bkl_Flg,2); |
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vfac(:,:,1) = fix(bkl_Flg/2); |
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% for jl=1:ydim, |
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% ie=bkl_Npts(jl); |
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% for b=1:nBas, |
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% ufac(1:ie,jl,1+b)=mskBw(bkl_IJuv(1:ie,jl),b).*ufac(1:ie,jl,1); |
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% vfac(1:ie,jl,1+b)=mskBs(bkl_IJuv(1:ie,jl),b).*vfac(1:ie,jl,1); |
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% end; |
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% end; |
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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% Compute mass/volume stream function % |
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
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% Compute volume transport through broken lines a hence psi. ut/vt is the |
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% velocity times the edge length it is passing through. The sum of this |
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% quantity along a broken line (vz) times the cell height is the volume |
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% transport through broken line at one layer (delM(k)*vz). psi is then |
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% the value of the volume transport through the level above subtracted |
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% from the value of psi above. |
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for it = 1:nt |
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for k = nr:-1:1 |
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ut = dyg.*hu(:,k,it).*mskWloc; |
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vt = dxg.*hv(:,k,it).*mskSloc; |
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for jl = 1:ydim |
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ie = bkl_Npts(jl); |
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for b = 1:1+nBas |
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vz = sum( ufac(1:ie,jl,b).*ut(bkl_IJuv(1:ie,jl)) ... |
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+ vfac(1:ie,jl,b).*vt(bkl_IJuv(1:ie,jl)) ); |
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psi(jl+1,k,b,it) = psi(jl+1,k+1,b,it) - delM(k)*vz; |
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end |
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end |
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end |
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end |
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psi = squeeze(psi); |
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%% For Ocean, result in Sv (10^6 m3/s) |
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%% For Atmos, results in 10^9 kg/s |
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if isequal(flu,'O'), psi = 1e-6*squeeze(psi); end |
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if isequal(flu,'A'), psi =-1e-9/grav*squeeze(psi); end |
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% % Compute the mask : |
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% if kfac == 1, |
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% ufac=abs(ufac) ; vfac=abs(vfac); |
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% for jl=1:ydim, |
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% ie=bkl_Npts(jl); |
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% hw=zeros(ie,nr); hs=zeros(ie,nr); |
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% hw=hw(bkl_IJuv(1:ie,jl),:); % Would need correction! |
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% hs=hs(bkl_IJuv(1:ie,jl),:); |
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% for b=1:1+nBas, |
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% for k=1:nr, |
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% % for ii=1:bkl_Npts(jl); |
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% % ij=bkl_IJuv(ii,jl); |
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% % mskV(jl+1,k,b)=mskV(jl+1,k,b)+ufac(ii,jl,b)*hw(ij,k)+vfac(ii,jl,b)*hs(ij,k); |
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% % end ; |
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% tmpv=ufac(1:ie,jl,b).*hw(:,k)+vfac(1:ie,jl,b).*hs(:,k); |
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% mskV(jl+1,k,b)=mskV(jl+1,k,b)+max(tmpv); |
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% end |
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% end |
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% end |
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% mskV=ceil(mskV); mskV=min(1,mskV); |
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% %- build the real mask (=mskG, ground) used to draw the continent with "surf": |
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% % position=centered , dim= ydim+1 x nr |
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% mskG=mskV(1:ydim+1,:,:)+mskV(2:ydim+2,:,:); mskG=min(1,mskG); |
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% |
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% if kMsep & nBas > 0, |
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% mskW=1+min(1,ceil(hw)); |
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% mskS=1+min(1,ceil(hs)); |
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% for b=1:nBas, |
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% bs=b; b1=1+bs; b2=2+rem(bs,nBas); |
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% if nBas == 2, bs=b+b-1; b1=2; b2=3 ; end |
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% for j=1:ydim+1, |
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% for i=1:np_Sep(bs,j), |
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% ij=ij_Sep(bs,j,i); typ=abs(tp_Sep(bs,j,i)); |
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% if typ == 1, |
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% mskG(j,:,b1)=mskG(j,:,b1).*mskW(ij,:); |
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% mskG(j,:,b2)=mskG(j,:,b2).*mskW(ij,:); |
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% elseif typ == 2, |
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% mskG(j,:,b1)=mskG(j,:,b1).*mskS(ij,:); |
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% mskG(j,:,b2)=mskG(j,:,b2).*mskS(ij,:); |
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% end |
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% end |
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% end |
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% end |
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% mskG=min(2,mskG); |
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% end |
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% |
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% %- to keep psi=0 on top & bottom |
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% mskZ(:,[2:nr+1],:)=mskV; |
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% mskZ(:,[1:nr],:)=mskZ(:,[1:nr],:)+mskV; |
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% %- to keep psi=0 on lateral boundaries : |
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% mskZ([1:ydim],:,:)=mskZ([1:ydim],:,:)+mskZ([2:ydim+1],:,:); |
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% mskZ([2:ydim+1],:,:)=mskZ([2:ydim+1],:,:)+mskZ([3:ydim+2],:,:); |
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% mskZ=ceil(mskZ); mskZ=min(1,mskZ); |
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% if kMsep & nBas > 0, |
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% mskM=zeros(ydim+2,nr,1+nBas); mskM(2:ydim+2,:,:)=min(2-mskG,1); |
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% mskM(1:ydim+1,:,:)=mskM(1:ydim+1,:,:)+mskM(2:ydim+2,:,:); |
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% mskZ(:,1:nr,:)=min(mskZ(:,1:nr,:),mskM); |
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% end |
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% %- apply the mask (and remove dim = 1) : |
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% if nt == 1, |
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% psi=squeeze(psi); mskV=squeeze(mskV); mskZ=squeeze(mskZ); |
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% psi( find(mskZ==0) )=NaN ; |
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% else |
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% for nt=1:nt, |
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% psi1=psi(:,:,:,nt); psi1( find(mskZ==0) )=NaN ; psi(:,:,:,nt)=psi1; |
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% end |
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% if nBas < 1, psi=squeeze(psi); mskV=squeeze(mskV); mskZ=squeeze(mskZ); end |
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% end |
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% else |
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% if nBas < 1 | nt == 1, psi=squeeze(psi); end |
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% end |
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