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% [] = compute_JBz(SNAPSHOT) |
% [JBz] = compute_JBz(SNAPSHOT) |
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% |
% |
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% Here we compute the PV flux due to diabatic processes as |
% Here we compute the PV flux due to diabatic processes as |
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% JFz = - alpha * f * Qnet / MLD / Cw |
% JFz = - alpha * f * Qnet / MLD / Cw |
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% alpha = 2.5*E-4 1/K is the thermal expansion coefficient |
% alpha = 2.5*E-4 1/K is the thermal expansion coefficient |
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% f = 2*OMEGA*sin(LAT) is the Coriolis parameter |
% f = 2*OMEGA*sin(LAT) is the Coriolis parameter |
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% Qnet is the net surface heat flux (W/m^2), positive downward |
% Qnet is the net surface heat flux (W/m^2), positive downward |
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% MLD is the mixed layer depth (m) |
% MLD is the mixed layer depth (m, positive) |
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% Cw = 4187 J/kg/K is the specific heat of seawater |
% Cw = 4187 J/kg/K is the specific heat of seawater |
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% |
% |
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% Files names are: |
% Files names are: |
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% 06/27/06 |
% 06/27/06 |
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% gmaze@mit.edu |
% gmaze@mit.edu |
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function compute_JBz(snapshot) |
function varargout = compute_JBz(snapshot) |
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global sla toshow |
global sla toshow |
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global netcdf_suff netcdf_domain |
global netcdf_suff netcdf_domain |
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nc{'Z'}.long_name = ncchar('depth'); |
nc{'Z'}.long_name = ncchar('depth'); |
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nc{'Z'}.gridtype = nclong(0); |
nc{'Z'}.gridtype = nclong(0); |
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nc{'Z'}.units = ncchar('m'); |
nc{'Z'}.units = ncchar('m'); |
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nc{'Z'}(:) = Qdpt; |
nc{'Z'}(:) = Qdpt(1); |
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% And main field: |
% And main field: |
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nc{ncid} = ncfloat('Z', 'Y', 'X'); |
nc{ncid} = ncfloat('Z', 'Y', 'X'); |
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nc{ncid}(:,:,:) = JBz; |
nc{ncid}(:,:,:) = JBz; |
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nc=close(nc); |
nc=close(nc); |
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close(ncQ); |
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close(ncMLD); |
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% Output: |
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output = struct('JBz',JBz,'lat',Qlat,'lon',Qlon); |
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switch nargout |
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case 1 |
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varargout(1) = {output}; |
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end |