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Commit 04f6935d authored by Joe Taylor's avatar Joe Taylor
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Initial commit of RU sample code into public user repo

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*.nc filter=lfs diff=lfs merge=lfs -text
*.mat filter=lfs diff=lfs merge=lfs -text
RU/.gitattributes 0 → 100644
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*.nc filter=lfs diff=lfs merge=lfs -text
RU/Ep_approx.m 0 → 100644
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function E_p = Ep_approx(prpt,alph,delta_ext,L_cbb,L_hbb,B_ssm,L,d_cbb,d_hbb)
%
% function E_p = Ep_approx(prpt,alph,delta_ext,L_cbb,L_hbb,B_ssm,L,d_cbb,d_hbb)
%
% The SSM and sensor act like a polarizer-analyzer pair. This function calculates
% the approximate radiance error generated by the polarizer-analyzer pair
%
% Inputs
% prpt: p_r * p_t for sensor + SSM (unitless) [nchan x 1]
% alph: analyzer angle alpha for sensor (radians) [scalar]
% delta_ext: polarizer angle for N scene views (radians) [1 x N]
% L_cbb: Radiance for cold cal reference (Rad units)) [nChan x N]
% L_hbb: Radiance for hot cal reference (Rad units)) [nChan x 1]
% B_ssm: Planck radiance for scene mirror temp (Rad units)) [nChan x 1]
% L: Scene radiance for N scene views (Rad units)) [nChan x 1] or [nChan x N]
% d_cbb: polarizer angle for CBB view (radians) [scalar]
% d_hbb: polarizer angle for HBB view (radians) [scalar]
%
% Outputs
% E_p calibration bias due to polarization (Rad units) [nChan x N]
%
% 2020-08-19 JKT
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
if size(L,2) == 1
L = repmat(L,1,length(delta_ext));
elseif size(L,2) ~= length(delta_ext)
fprintf(1, 'Ep_approx: ERROR Invalid scene radiance dimensions\n');
end
if abs(d_cbb) > 2*pi
fprintf(1, 'Ep_approx: ERROR delta CBB out of range, should be in units of radians\n')
return
end
if abs(d_hbb) > 2*pi
fprintf('Ep_approx: ERROR delta HBB out of range, should be in units of radians\n')
return
end
E_p = NaN*ones(length(L_cbb),length(delta_ext)); % N_{d.wn} x N_{d.delta_ext}
for ii = 1:length(delta_ext)
d_ext = delta_ext(ii);
L_ext = L(:,ii);
% approximate equation
term1 = prpt.*(L_ext*cos(2*(d_ext - alph)));
term2 = -prpt.*(L_hbb.*((L_ext - L_cbb)./(L_hbb - L_cbb))*cos(2*(d_hbb - alph)));
term3 = -prpt.*(L_cbb.*((L_hbb - L_ext)./(L_hbb - L_cbb))*cos(2*(d_cbb - alph)));
term4 = -B_ssm.*prpt.*(cos(2*(d_ext - alph)));
term5 = +B_ssm.*prpt.*(((L_ext - L_cbb)./(L_hbb - L_cbb))*cos(2*(d_hbb - alph)));
term6 = +B_ssm.*prpt.*(((L_hbb - L_ext)./(L_hbb - L_cbb))*cos(2*(d_cbb - alph)));
E_p(:,ii) = term1 + term2 + term3 + term4 + term5 + term6;
end
return
RU/ICTradModelRU_L1b_aux.m 0 → 100644
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function B = ICTradModelRU_L1b_aux(sensor,T_ICT,T_CRIS,ICT_Param,ru_term,ru_value)
%
% function B = ICTradModelRU_L1b_aux(sensor,T_ICT,T_CRIS,ICT_Param,ru_term,ru_value)
%
% Compute ICT predicted radiance using ICT radiometric model prescribed by ATBD
% with perturbation to a single term
%
% Inputs
% sensor sparse spectral params structure
% .band
% .v
% .output_range
% T_ICT ICT Temperature
% T_CRIS CrIS temperature struct
% ICT_Param ICT radiometric model parameters
% ru_term string indicating ru_term to perturb
% ru_value size of perturbation
%
% Outputs
% B Structure of predicted ICT radiance variables
% .emitted emitted radiance
% .wn wavenumber scale
% .SSM_Baffle SSM Baffle term reflected radiance
% .ICT_baffle ICT baffle term reflected radiance
% .OMA OMA term reflected radiance
% .BS_warm BS_warm term reflected radiance
% .BS_cold BS_cold term reflected radiance
% .Space Earth/Space term reflected radiance
% .reflected total reflected radiance
% .total total radiance (emitted and reflected)
% .V view factors (struct)
% .e emissivities (struct)
% .r reflectivies (.SSM)
% .T temperatures (struct)
% .e_ICT ICT emissivity
% .T_ICT ICT temperature
% .ru_term RU term to perturb
% .ru_value value of perturbation
% .no_perturb_val
% .perturbed_val
%
% 2020-08-19 JKT
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
wn = sensor.v_onaxis;
ICT_wnum = ICT_Param.(sprintf('%s_ICT_wnum',lower(sensor.band)));
ICT_emiss = ICT_Param.(sprintf('%s_ICT_emiss',lower(sensor.band)));
ICT_Baffle_emiss = ICT_Param.(sprintf('%s_ICT_Baffle_emiss',lower(sensor.band)));
Housing_emiss = ICT_Param.(sprintf('%s_Housing_emiss',lower(sensor.band)));
ScanBaffle_emiss = ICT_Param.(sprintf('%s_ScanBaffle_emiss',lower(sensor.band)));
ScanMirror_emiss = ICT_Param.(sprintf('%s_ScanMirror_emiss',lower(sensor.band)));
Earth_emiss = ICT_Param.(sprintf('%s_Earth_emiss',lower(sensor.band)));
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% ICT emissivity interpolation to wavenumber grid
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% Interpolate 4-min-EP emissivity to the on-axis sensor grid.
%% The wavenumber values corresponding to the emissivity values in the engineering packet are on the normal spectral resolution and on user grid
e_ICT = interp1(ICT_wnum,ICT_emiss,wn,'nearest','extrap');
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% Temperature, emissivity and view factor init
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% SSM
%%----------
%r.SSM = 1-ICT_Param.Band(iband).Emissivity.ScanMirrorPts;
r.SSM = 1-ScanMirror_emiss;
%% SSM_Baffle
%%----------
%e.SSM_Baffle = ICT_Param.Band(iband).Emissivity.ScanBafflePts;
e.SSM_Baffle = ScanBaffle_emiss;
T.SSM_Baffle = T_CRIS.ssm_baffle_temp + T_CRIS.ssm_baffle_corr_temp;
T.SSM_Baffle(isnan(T.SSM_Baffle)) = 0;
V.SSM_Baffle = ICT_Param.View_Factor.ScanBaffle;
%% ICT_baffle
%%----------
%e.ICT_baffle = ICT_Param.Band(iband).Emissivity.ICT_BafflePts;
e.ICT_baffle = ICT_Baffle_emiss;
T.ICT_baffle = T_ICT;
V.ICT_baffle = ICT_Param.View_Factor.ICTBaffle;
%% OMA + Frame + Other
%%----------
%e.OMA = ICT_Param.Band(iband).Emissivity.HousingPts;
e.OMA = Housing_emiss;
T.OMA = mean(0.5*T_CRIS.oma_struct_temp_1 + 0.5*T_CRIS.oma_struct_temp_2);
V.OMA = ICT_Param.View_Factor.OMAandFrame;
%% BS_warm
%%----------
e.BS_warm = e.OMA;
T.BS_warm = T.OMA;
V.BS_warm = ICT_Param.View_Factor.BeamSplitterWarm;
%% BS_cold
%%----------
T.BS_cold = T_ICT;
V.BS_cold = ICT_Param.View_Factor.BeamSplitterCold;
%% Space/Earth Reflected
%%----------
e.Space = Earth_emiss;
T.Space = ICT_Param.Earth_Temperature;
V.Space = ICT_Param.View_Factor.Space;
no_perturb_val = []; % initialize, will remain at this value for no perturbation
perturbed_val = []; % initialize, will remain at this value for no perturbation
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% Perturbation
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
switch ru_term
case 'e_ICT'
no_perturb_val = e_ICT;
e_ICT = e_ICT*(1-ru_value);
e_ICT(e_ICT > 1) = 1;
e_ICT(e_ICT < 0) = 0;
perturbed_val = e_ICT;
case 'T_ICT'
no_perturb_val = T_ICT;
T_ICT = T_ICT + ru_value;
perturbed_val = T_ICT;
case 'SSM_scan_mirror_baffle'
no_perturb_val = T.SSM_Baffle;
T.SSM_Baffle = T.SSM_Baffle + ru_value;
perturbed_val = T.SSM_Baffle;
case 'T_ScanBaffleCorrection'
no_perturb_val = T.SSM_Baffle;
T.SSM_Baffle = T.SSM_Baffle + ru_value;
perturbed_val = T.SSM_Baffle;
case 'T_ICT_baffle'
no_perturb_val = T.ICT_baffle;
T.ICT_baffle = T.ICT_baffle + ru_value;
perturbed_val = T.ICT_baffle;
case 'T_OMA' % OMA + Frame + Other
no_perturb_val = T.OMA;
T.OMA = T.OMA + ru_value;
perturbed_val = T.OMA;
case 'T_Frame' % no longer used
no_perturb_val = T.Frame;
T.Frame = T.Frame + ru_value;
perturbed_val = T.Frame;
case 'T_BS_warm'
no_perturb_val = T.BS_warm;
T.BS_warm = T.BS_warm + ru_value;
perturbed_val = T.BS_warm;
case 'T_BS_cold'
no_perturb_val = T.BS_cold;
T.BS_cold = T.BS_cold + ru_value;
perturbed_val = T.BS_cold;
case 'T_Space'
no_perturb_val = T.Space;
T.Space = T.Space + ru_value;
perturbed_val = T.Space;
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% ICT emission
% (ref: eq 75 in 474-00032, Rev C)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
B.emitted = e_ICT .* bt2rad(wn,T_ICT);
B.wn = wn;
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Reflected term 1: SSM Baffle
% (ref: eq 76 in 474-00032, Rev C)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
if V.SSM_Baffle == 0
B.SSM_Baffle = zeros(size(B.wn));
else
B.SSM_Baffle = (1 - e_ICT) .* e.SSM_Baffle * V.SSM_Baffle .* bt2rad(wn,T.SSM_Baffle);
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Reflected term 2: ICT Baffle
% (ref: eq 78a in 474-00032, Rev C)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
if V.ICT_baffle == 0
B.ICT_baffle = zeros(size(B.wn));
else
B.ICT_baffle = (1 - e_ICT) .* e.ICT_baffle * V.ICT_baffle .* bt2rad(wn,T.ICT_baffle);
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Reflected term 3a,b,c: OMA, frame, other, Beamsplitter Warm
% (ref: eq 77 in 474-00032, Rev C)
% V = 0.214 for OMA, Other, Frame terms in ATBD (= 0.0590 + 0.0100 + 0.1450)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% OMA
%%----------
if V.OMA == 0
B.OMA = zeros(size(B.wn));
else
B.OMA = (1 - e_ICT) .* e.OMA * r.SSM * V.OMA .* bt2rad(wn,T.OMA);
end
%% BS_Warm
%%----------
if V.BS_warm == 0
B.BS_warm = zeros(size(B.wn));;
else
B.BS_warm = (1 - e_ICT) .* e.BS_warm * r.SSM * V.BS_warm .* bt2rad(wn,T.BS_warm);
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Reflected term 4: Beamsplitter Cold
% (ref: eq 78b in 474-00032, Rev C)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
if V.BS_cold == 1
B.BS_cold = (1 - e_ICT) .* r.SSM^2 .* 0.5 * V.BS_cold .* bt2rad(wn,T.BS_cold); % Consistent with ATBD
else
B.BS_cold = (1 - e_ICT) .* r.SSM^2 .* 0.5 * V.BS_cold .* bt2rad(wn,T.BS_cold); % SNPP
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Reflected term 5: Space/Earth View
% (ref: eq 78c in 474-00032, Rev C)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
if V.Space == 0
B.Space = zeros(size(B.wn));;
else
B.Space = (1 - e_ICT) .* V.Space .* e.Space .* bt2rad(wn,T.Space);
end
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% total reflected radiance into ICT cavity
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
V.Total = V.SSM_Baffle + V.ICT_baffle + V.OMA + V.BS_warm + V.BS_cold + V.Space; % should total 1, for check only
B.reflected = B.SSM_Baffle + B.ICT_baffle + B.OMA + B.BS_warm + B.BS_cold + B.Space;
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Total radiance from ICT
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
B.total = B.emitted + B.reflected;
B.wn = wn;
B.V = V;
B.e = e;
B.r = r;
B.T = T;
B.e_ICT = e_ICT;
B.T_ICT = T_ICT;
B.ru_term = ru_term;
B.ru_value = ru_value;
B.no_perturb_val = no_perturb_val;
B.perturbed_val = perturbed_val;
return
RU/J1_L1B_ru_tool_param_file.nc 0 → 100644 LFS
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RU/SNPP_L1B_ru_tool_param_file.nc 0 → 100644 LFS
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RU/TEST_INPUT/SNDR.J1.CRIS.20191031T0012.m06.g003.L1B.std.v03_08.G.201204050506.nc 0 → 100644 LFS
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RU/bt2rad.m 0 → 100644
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function radiance = bt2rad(freq,bt);
%
% function radiance = bt2rad(freq,bt);
%
% compute radiance given wavenumbers and brightness temperature.
%
% Inputs:
% freq wavenumbers (Nx1) in 1/cm
% bt brightnes temperature (Nx1) in Kelvin
% Outputs:
% radiance Planck radiances (Nx1) in mW/(m^2 sr. 1/cm)
%
% see also RADTOT.M, RAD2BT.M, TTORAD.M
%
% DCT 11/11-99
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
%
% fundamental constants:
% (Cohen, E.R. and B.N. Taylor, The 1986 CODATA recommended values
% of the fundamental physical constants, Journal of Research of
% the National Bureau of Standard, 92(2), March-April 1987.)
h = 6.6260755E-34; % Planck constant in Js
c = 2.99792458E8; % photon speed in m/s
k = 1.380658E-23; % Boltzmann constant in J/K
c1 = 2*h*c*c*1e8;
c2 = h*c/k*1e2;
radiance = 1e3 * c1.*(freq.*freq.*freq)./(exp((c2.*freq)./bt)-1);
ind = find(bt < 0);
if length(ind) ~= 0
radiance = nan*real(radiance);
disp('WARNING: negative inputs to BT2RAD')
end
ind = find(~isreal(bt));
if length(ind) ~= 0
radiance = nan*real(radiance);
disp('WARNING: imaginary inputs to BT2RAD')
end
ind = find(isnan(bt));
if length(ind) ~= 0
radiance = nan*real(radiance);
disp('WARNING: NaN inputs to BT2RAD')
end
ind = find(isinf(bt));
if length(ind) ~= 0
radiance = nan*real(radiance);
disp('WARNING: Inf inputs to BT2RAD')
end
return
RU/convert_anc_to_structs.m 0 → 100644
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function [ICT_Param,RU,nonlin,polcorr_param] = convert_anc_to_structs(nc_struct);
%
% function [ICT_Param,RU,nonlin,polcorr_param] = convert_anc_to_structs(nc_struct);
%
% This function converts the contents from the CrIS L1b RU ancillary file
% to ICT_Param, RU, nonlin, and polcorr structures for use in the RU calculations
%
% Input
% nc_struct structure of vars read from CrIS L1b RU ancillary file
%
% Output
% ICT_Param ICT ancillary parameters [struct]
% RU Radiometric Uncertainty ancillary parameters [struct]
% nonlin nonlinearity corretion ancillary parameters [struct]
% polcorr_param polarization correction ancillary parameters [struct]
%
% JKT 2021-Aug-26
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
ICT_Param.Earth_Temperature = nc_struct.ICT_Param_Earth_Temperature;
ICT_Param.lw_ICT_wnum = nc_struct.wnum_lw;
ICT_Param.lw_ICT_emiss = nc_struct.ICT_Param_lw_ICT_emiss;
ICT_Param.lw_ICT_Baffle_emiss = nc_struct.ICT_Param_lw_ICT_Baffle_emiss;
ICT_Param.lw_Housing_emiss = nc_struct.ICT_Param_lw_Housing_emiss;
ICT_Param.lw_ScanBaffle_emiss = nc_struct.ICT_Param_lw_ScanBaffle_emiss;
ICT_Param.lw_ScanMirror_emiss = nc_struct.ICT_Param_lw_ScanMirror_emiss;
ICT_Param.lw_Earth_emiss = nc_struct.ICT_Param_lw_Earth_emiss;
ICT_Param.mw_ICT_wnum = nc_struct.wnum_mw;
ICT_Param.mw_ICT_emiss = nc_struct.ICT_Param_mw_ICT_emiss;
ICT_Param.mw_ICT_Baffle_emiss = nc_struct.ICT_Param_mw_ICT_Baffle_emiss;
ICT_Param.mw_Housing_emiss = nc_struct.ICT_Param_mw_Housing_emiss;
ICT_Param.mw_ScanBaffle_emiss = nc_struct.ICT_Param_mw_ScanBaffle_emiss;
ICT_Param.mw_ScanMirror_emiss = nc_struct.ICT_Param_mw_ScanMirror_emiss;
ICT_Param.mw_Earth_emiss = nc_struct.ICT_Param_mw_Earth_emiss;
ICT_Param.sw_ICT_wnum = nc_struct.wnum_sw;
ICT_Param.sw_ICT_emiss = nc_struct.ICT_Param_sw_ICT_emiss;
ICT_Param.sw_ICT_Baffle_emiss = nc_struct.ICT_Param_sw_ICT_Baffle_emiss;
ICT_Param.sw_Housing_emiss = nc_struct.ICT_Param_sw_Housing_emiss;
ICT_Param.sw_ScanBaffle_emiss = nc_struct.ICT_Param_sw_ScanBaffle_emiss;
ICT_Param.sw_ScanMirror_emiss = nc_struct.ICT_Param_sw_ScanMirror_emiss;
ICT_Param.sw_Earth_emiss = nc_struct.ICT_Param_sw_Earth_emiss;
ICT_Param.View_Factor.Space = nc_struct.ICT_Param_A_Space;
ICT_Param.View_Factor.BeamSplitterCold = nc_struct.ICT_Param_A_BeamSplitterCold;
ICT_Param.View_Factor.BeamSplitterWarm = nc_struct.ICT_Param_A_BeamSplitterWarm;
ICT_Param.View_Factor.OMAandFrame = nc_struct.ICT_Param_A_OMAandFrame;
ICT_Param.View_Factor.ICTBaffle = nc_struct.ICT_Param_A_ICTBaffle;
ICT_Param.View_Factor.ScanBaffle = nc_struct.ICT_Param_A_ScanBaffle;
RU.dT_ict = nc_struct.RU_dT_ict;
RU.de_ict = nc_struct.RU_de_ict;
RU.dT_ict_ref_meas = nc_struct.RU_dT_ict_ref_meas;
RU.dT_ict_ref_model = nc_struct.RU_dT_ict_ref_model;
RU.dprpt = nc_struct.RU_dprpt;
RU.dalpha = nc_struct.RU_dalpha;
RU.lw_da2 = nc_struct.RU_lw_da2;
RU.mw_da2 = nc_struct.RU_mw_da2;
RU.sw_da2 = nc_struct.RU_sw_da2;
nonlin.lw_a2 = nc_struct.nonlin_lw_a2;
nonlin.mw_a2 = nc_struct.nonlin_mw_a2;
nonlin.sw_a2 = nc_struct.nonlin_sw_a2;
polcorr_param.delta_SSM = nc_struct.polcorr_delta_SSM;
polcorr_param.lw_wn = repmat(nc_struct.wnum_lw(:),1,9);
polcorr_param.lw_prpt = nc_struct.polcorr_lw_prpt;
polcorr_param.lw_alph = nc_struct.polcorr_lw_alph;
polcorr_param.lw_delta_cbb = nc_struct.polcorr_delta_cbb;
polcorr_param.lw_delta_hbb = nc_struct.polcorr_delta_hbb;
polcorr_param.mw_wn = repmat(nc_struct.wnum_mw(:),1,9);
polcorr_param.mw_prpt = nc_struct.polcorr_mw_prpt;
polcorr_param.mw_alph = nc_struct.polcorr_mw_alph;
polcorr_param.mw_delta_cbb = nc_struct.polcorr_delta_cbb;
polcorr_param.mw_delta_hbb = nc_struct.polcorr_delta_hbb;
polcorr_param.sw_wn = repmat(nc_struct.wnum_sw,1,9);
polcorr_param.sw_prpt = nc_struct.polcorr_sw_prpt;
polcorr_param.sw_alph = nc_struct.polcorr_sw_alph;
polcorr_param.sw_delta_cbb = nc_struct.polcorr_delta_cbb;
polcorr_param.sw_delta_hbb = nc_struct.polcorr_delta_hbb;
return
RU/cris_calbudget_1gran_nc_wrapper.m 0 → 100644
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% This is a wrapper script for testing the generation of the CrIS NASA L1b for a single L1b granule
% and utilizes the netcdf4 formatted parameter files
% The user must set the following (within USER INPUT section of script)
%
% sat_name satellite name ('J1' or 'SNPP')
% l1b_fname L1b granule name (including path if not in same directory as code)
% saveTotalRU_FLAG set to 1 if you want to save the RSS RU to a mat file
%
% The primary contributors to the CrIS radiometric uncertainty are
% ICT temperature uncertainty
% ICT emissivity uncertainty
% uncertainty in the the other temperatures in the ICT radiometric model (modeled and measured)
% uncertainty in the quadratic coefficient NLC coefficient (a2)
% polarization correction uncertainty
% (sensor polarization angle alpha, and combined SSM and sensor polarization prpt)
%
% RU term 1: e_ict ICT rad model, emitted radiance
% RU term 2: T_ict ICT rad model, emitted radiance
% RU term 3: T_SSM_scan_mirror_baffle ICT rad model, reflected radiance (measured T)
% RU term 4: T_ScanBaffleCorrection ICT rad model, reflected radiance (modeled T)
% RU term 5: T_ICT_baffle ICT rad model, reflected radiance (measured T)
% RU term 6a: T_OMA, T_Frame ICT rad model, reflected radiance (measured T)
% RU term 6b: T_BS_warm ICT rad model, reflected radiance (measured T)
% RU term 7: T_BS_cold ICT rad model, reflected radiance (measured T)
% RU term 8: T_Space ICT rad model, reflected radiance (modeled T)
% RU term 9: prpt polarization correction
% RU term 10: alpha polarization correction
% RU term 11: a2 nonlinearity correction
%
% Refer to the NASA CrIS L1b RU document and ATBD for details on the ICT radiometric model
% Each reflected term in the ICT radiometric model also has a view factor and emissivity, but the uncertainty
% in those quantities produce negligible contributions to the CrIS radiometric uncertainty and are not perturbed for the RU estimate
% J1 has an improved ICT emissivity, and the view factors of some of the reflected terms are set to zero as a result
%
% JKT 2020-Sep-13
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% START: USER INPUT
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
sat_name = 'SNPP'; % set to 'J1' or 'SNPP'
l1b_fname = 'SNDR.SNPP.CRIS.20191031T0012.m06.g003.L1B.std.v03_08.G.201219125854.nc'; % set to file name of v3 L1b granule
%sat_name = 'J1'; % set to 'J1' or 'SNPP'
%l1b_fname = 'SNDR.J1.CRIS.20191031T0012.m06.g003.L1B.std.v03_08.G.201204050506.nc'; % set to file name of v3 L1b granule
l1b_pname = '/Users/joet/git/cris_l1b_user/RU/TEST_INPUT'; % set to path to v3 L1b granule
ru_code_pname = pwd; % set to path of the RU code
saveTotalRU_FLAG = 1; % set to 1 if you want to save the RSS RU to a mat file
pname_out = fullfile(pwd,'RU_OUT_NC'); % set to path for RU output files
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%% END: USER INPUT
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
mkdir(pname_out)
addpath(ru_code_pname);
RU = cris_gran_RU_ncparam(sat_name,fullfile(l1b_pname,l1b_fname),saveTotalRU_FLAG,pname_out);
RU/cris_gran_RU_ncparam.m 0 → 100644
View file @ 04f6935d
function RU = cris_gran_RU_ncparam(sat_name,l1b_fname,saveTotalRU_FLAG,pname_out);
%
% function RU = cris_gran_RU_ncparam(sat_name,l1b_fname,saveTotalRU_FLAG,pname_out);
%
% This is a function for generation of the CrIS NASA L1b for a single L1b granule
% and utilizes the netcdf4 formatted parameter files
%
% Inputs
% sat_name satellite name ('J1' or 'SNPP')
% l1b_fname L1b granule name (including path if not in same directory as code)
% saveTotalRU_FLAG set to 1 if you want to save the RSS RU to a mat file
% pname_out output directory
%
% JKT 2021-Aug-26
% University of Wisconsin-Madison Space Science and Engineering Center (UW-SSEC)
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% code will loop over bands
bands{1} = 'lw';
bands{2} = 'mw';
bands{3} = 'sw';
%%============================================================
%% RU STEP 1a: Load ancillary data from static file (satellite dependent)
%%============================================================
switch sat_name
case 'J1'
% J1
jnk = rd_nc4('J1_L1B_ru_tool_param_file.nc');
case 'SNPP'
% SNPP
jnk = rd_nc4('SNPP_L1B_ru_tool_param_file.nc');
end
%%============================================================
%% RU STEP 1b: separate .nc param file contents into ICT_Param, RU,
%% nonlin, polcorr_param structures used in this code package
%%============================================================
[ICT_Param,RU,nonlin,polcorr_param] = convert_anc_to_structs(jnk);
%%============================================================
%% RU STEP 1c: copy data from anc file to expected var names for this code package
%%============================================================
dT_ict = RU.dT_ict;
de_ict = RU.de_ict;
dT_ict_ref_meas = RU.dT_ict_ref_meas;
dT_ict_ref_model = RU.dT_ict_ref_model;
dprpt = RU.dprpt;
dalpha = RU.dalpha;
da2.lw = RU.lw_da2;
da2.mw = RU.mw_da2;
da2.sw = RU.sw_da2;
sensor_all.lw.a2_now = nonlin.lw_a2;
sensor_all.mw.a2_now = nonlin.mw_a2;
sensor_all.sw.a2_now = nonlin.sw_a2;
%%%%%%%%%%
%% create an opts structure
%% not needed to calc RU estimate, but used here to record configuration options
%%%%%%%%%%
opts.extraFLAG = 1;
opts.l1b_fname = l1b_fname;
opts.bands = bands;
opts.sat_name = sat_name;
%%%%%%%%%%
% create output file name
% not required to calc RU estimate, but used here for optional output
%%%%%%%%%%
[~,fname_out,~] = fileparts(l1b_fname);
fname_out = sprintf('%s_RU',fname_out);
%%============================================================
%% RU STEP 2: Load v3 L1b data
%%============================================================
l1b_dat = read_l1b_for_RU(l1b_fname);
%%%%%%%%%%
%% save opts params
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