Data Quality Reports for Session: 110013 User: srrb Completed: 01/18/2008


TABLE OF CONTENTS

DQR IDSubjectData Streams Affected
D040209.1SGP/MFRSR/E9 - Shadowband FailuresgpmfrsrE9.00, sgpmfrsrE9.b1, sgpmfrsrlangleyE9.c1, sgpmfrsrlangplotE9.c1,
sgpmfrsrod1barnmichE9.c1
D040427.3SGP/MFRSR/E9 - Shadowband MisalignedsgpmfrsrE9.b1, sgpmfrsrlangleyE9.c1, sgpmfrsrlangplotE9.c1, sgpmfrsrod1barnmichE9.c1


DQRID : D040209.1
Start DateStart TimeEnd DateEnd Time
02/02/2004130002/12/20042359
Subject:
SGP/MFRSR/E9 - Shadowband Failure
DataStreams:sgpmfrsrE9.00, sgpmfrsrE9.b1, sgpmfrsrlangleyE9.c1, sgpmfrsrlangplotE9.c1,
sgpmfrsrod1barnmichE9.c1
Description:
The shadowband of this instrument failed 20040202 - 20040212. All direct and diffuse 
measurements are incorrect during this time period.
Measurements:sgpmfrsrE9.b1:
  • Diffuse Hemispheric Broadband Irradiance (Approximate), MFRSR(diffuse_hemisp_broadband)
  • Direct Normal Narrowband Irradiance, Filter 2, offset corrected(direct_normal_narrowband_filter2)
  • Direct Normal Broadband Irradiance, broadband scale applied(direct_normal_broadband)
  • Direct Normal Narrowband Irradiance, Filter 1, offset corrected(direct_normal_narrowband_filter1)
  • Direct Normal Narrowband Irradiance, Filter 5, offset corrected(direct_normal_narrowband_filter5)
  • Direct Normal Narrowband Irradiance, Filter 6, offset corrected(direct_normal_narrowband_filter6)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 2(diffuse_hemisp_narrowband_filter2)
  • Direct Normal Narrowband Irradiance, Filter 3, offset corrected(direct_normal_narrowband_filter3)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 4(diffuse_hemisp_narrowband_filter4)
  • Direct Normal Narrowband Irradiance, Filter 4, offset corrected(direct_normal_narrowband_filter4)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 1(diffuse_hemisp_narrowband_filter1)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 3(diffuse_hemisp_narrowband_filter3)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 5(diffuse_hemisp_narrowband_filter5)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 6(diffuse_hemisp_narrowband_filter6)

sgpmfrsrE9.00:
  • Raw data stream - documentation not supported(Raw data stream - documentation not supported)

sgpmfrsrod1barnmichE9.c1:
  • aerosol optical depth filter 5(aerosol_optical_depth_filter5)
  • Angstrom exponent(angstrom_exponent)
  • aerosol optical depth filter 4(aerosol_optical_depth_filter4)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter4)
  • totaloptical depth direct narrowband filter 2(total_optical_depth_filter2)
  • total optical depth direct narrowband filter 1(total_optical_depth_filter1)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter2)
  • Rayleigh optical thickness computed for filter 5(Rayleigh_optical_thickness_filter5)
  • Rayleigh optical thickness computed for filter 2(Rayleigh_optical_thickness_filter2)
  • Rayleigh optical thickness computed for filter 1(Rayleigh_optical_thickness_filter1)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter3)
  • Optical depth from TOMS satellite(TOMS_optical_depth)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter5)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter1)
  • Rayleigh optical thickness computed for filter 3(Rayleigh_optical_thickness_filter3)
  • Rayleigh optical thickness computed for filter 4(Rayleigh_optical_thickness_filter4)
  • aerosol optical depth filter 3(aerosol_optical_depth_filter3)
  • aerosol optical depth filter 2(aerosol_optical_depth_filter2)
  • Ozone absorption coefficient used for filter 2(Ozone_absorption_coefficient_filter2)
  • surface pressure(surface_pressure)
  • Indicator of optical depth stability(optical_depth_stability_flag)
  • Airmasses(airmass)
  • Ozone absorption coefficient used for filter 5(Ozone_absorption_coefficient_filter5)
  • total optical depth direct narrowband filter 4(total_optical_depth_filter4)
  • Ozone absorption coefficient used for filter 4(Ozone_absorption_coefficient_filter4)
  • total optical depth direct narrowband filter 3(total_optical_depth_filter3)
  • Ozone absorption coefficient used for filter 3(Ozone_absorption_coefficient_filter3)
  • aerosol optical depth filter 1(aerosol_optical_depth_filter1)
  • Ozone absorption coefficient used for filter 1(Ozone_absorption_coefficient_filter1)
  • total optical depth direct narrowband filter 5(total_optical_depth_filter5)

sgpmfrsrlangplotE9.c1:
  • airmass(michalsky_airmass)
  • log(irradiance) for the Direct Narrowband Filter6, Michalsky(michalsky_lnI_filter6)
  • rejected points for the final fit for the Direct Narrowband Filter2, Barnard(barnard_rejected_filter2)
  • log(irradiance) for the Direct Narrowband Filter5, Barnard(barnard_lnI_filter5)
  • rejected points for the final fit for the Direct Narrowband Filter1, Barnard(barnard_rejected_filter1)
  • log(irradiance) for the Direct Narrowband Filter4, Barnard(barnard_lnI_filter4)
  • rejected points for the final fit for the Direct Broadband, Michalsky(michalsky_rejected_broadband)
  • rejected points for the final fit for the Direct Narrowband Filter4, Barnard(barnard_rejected_filter4)
  • log(irradiance) for the Direct Narrowband Filter5, Michalsky(michalsky_lnI_filter5)
  • log(irradiance) for the Direct Narrowband Filter4, Michalsky(michalsky_lnI_filter4)
  • rejected points for the final fit for the Direct Narrowband Filter5, Barnard(barnard_rejected_filter5)
  • rejected points for the final fit for the Direct Broadband, Barnard(barnard_rejected_broadband)
  • rejected points for the final fit for the Direct Narrowband Filter6, Barnard(barnard_rejected_filter6)
  • log(irradiance) for the Direct Narrowband Filter1, Michalsky(michalsky_lnI_filter1)
  • rejected points for the final fit for the Direct Narrowband Filter5, Michalsky(michalsky_rejected_filter5)
  • log(irradiance) for the Direct Narrowband Filter6, Barnard(barnard_lnI_filter6)
  • log(irradiance) for the Direct Broadband, Barnard(barnard_lnI_broadband)
  • log(irradiance) for the Direct Narrowband Filter1, Barnard(barnard_lnI_filter1)
  • rejected points for the final fit for the Direct Narrowband Filter6, Michalsky(michalsky_rejected_filter6)
  • rejected points for the final fit for the Direct Narrowband Filter3, Barnard(barnard_rejected_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter2, Michalsky(michalsky_rejected_filter2)
  • log(irradiance) for the Direct Broadband, Michalsky(michalsky_lnI_broadband)
  • log(irradiance) for the Direct Narrowband Filter2, Barnard(barnard_lnI_filter2)
  • log(irradiance) for the Direct Narrowband Filter3, Barnard(barnard_lnI_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter1, Michalsky(michalsky_rejected_filter1)
  • airmass(barnard_airmass)
  • log(irradiance) for the Direct Narrowband Filter3, Michalsky(michalsky_lnI_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter3, Michalsky(michalsky_rejected_filter3)
  • log(irradiance) for the Direct Narrowband Filter2, Michalsky(michalsky_lnI_filter2)
  • rejected points for the final fit for the Direct Narrowband Filter4, Michalsky(michalsky_rejected_filter4)

sgpmfrsrlangleyE9.c1:
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter5(barnard_error_slope_filter5)
  • Langley regression Io, Michalsky, Direct Narrowband Filter6(michalsky_solar_constant_filter6)
  • rejection flag for Direct Broadband(barnard_badflag_broadband)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter3(barnard_error_slope_filter3)
  • optical depth for the Direct Narrowband Filter3(barnard_optical_depth_filter3)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct BroadBand(barnard_solar_constant_sdist_broadband)
  • rejection flag for Direct Broadband(michalsky_badflag_broadband)
  • rejection flag for Direct Narrowband Filter6(barnard_badflag_filter6)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter1(barnard_error_slope_filter1)
  • error in final linear fit for the Direct Narrowband Filter5(barnard_error_fit_filter5)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter6(barnard_error_slope_filter6)
  • solar constant corrected for solar distance for the Direct Narrowband Filter3(michalsky_solar_constant_sdist_filter3)
  • error in final linear fit for the Direct Narrowband Filter4(barnard_error_fit_filter4)
  • percentage of initial points used in final linear fit for the Direct Broadband(michalsky_good_fraction_broadband)
  • Angstrom exponent(barnard_angstrom_exponent)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter2(barnard_solar_constant_sdist_filter2)
  • solar constant corrected for solar distance for the Direct Broadband(michalsky_solar_constant_sdist_broadband)
  • rejection flag for Direct Narrowband Filter5(barnard_badflag_filter5)
  • rejection flag for Direct Narrowband Filter4(barnard_badflag_filter4)
  • rejection flag for Direct Narrowband Filter6(michalsky_badflag_filter6)
  • error in optical depth (slope) of final linear fit for the Direct Broadband(barnard_error_slope_broadband)
  • Langley regression Io, Michalsky, Direct BroadBand(michalsky_solar_constant_broadband)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter4(barnard_solar_constant_sdist_filter4)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter1(barnard_solar_constant_sdist_filter1)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter2(barnard_error_slope_filter2)
  • percentage of initial points used in final linear fit for the Direct Broadband(barnard_good_fraction_broadband)
  • solar constant corrected for solar distance for the Direct Narrowband Filter6(barnard_solar_constant_sdist_filter6)
  • rejection flag for Direct Narrowband Filter5(michalsky_badflag_filter5)
  • optical depth for the Direct Narrowband Filter1(barnard_optical_depth_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter2(michalsky_good_fraction_filter2)
  • error in final linear fit for the Direct Narrowband Filter3(barnard_error_fit_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter1(michalsky_standard_deviation_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter1(michalsky_good_fraction_filter1)
  • optical depth for the Direct BroadBand(michalsky_optical_depth_broadband)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter4(barnard_error_slope_filter4)
  • Langley regression Io, Michalsky, Direct Narrowband Filter4(michalsky_solar_constant_filter4)
  • error in final linear fit for the Direct Narrowband Filter6(barnard_error_fit_filter6)
  • optical depth for the Direct Narrowband Filter2(barnard_optical_depth_filter2)
  • Langley regression Io, Michalsky, Direct Narrowband Filter5(michalsky_solar_constant_filter5)
  • solar constant corrected for solar distance for the Direct Narrowband Filter2(michalsky_solar_constant_sdist_filter2)
  • rejection flag for Direct Narrowband Filter1(michalsky_badflag_filter1)
  • standard deviation around regression line for the Direct Narrowband Filter4(michalsky_standard_deviation_filter4)
  • Langley regression Io, Michalsky, Direct Narrowband Filter2(michalsky_solar_constant_filter2)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter3(barnard_solar_constant_sdist_filter3)
  • Langley regression Io, Michalsky, Direct Narrowband Filter3(michalsky_solar_constant_filter3)
  • optical depth for the Direct Narrowband Filter4(barnard_optical_depth_filter4)
  • optical depth for the Direct BroadBand(barnard_optical_depth_broadband)
  • number of points used in final linear fit for the Direct Narrowband Filter3(barnard_number_points_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter5(michalsky_standard_deviation_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter5(michalsky_good_fraction_filter5)
  • standard deviation around regression line for the Direct Narrowband Filter2(michalsky_standard_deviation_filter2)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter6(barnard_good_fraction_filter6)
  • number of points used in final linear fit for the Direct Broadband(barnard_number_points_broadband)
  • rejection flag for Direct Narrowband Filter3(michalsky_badflag_filter3)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter2(barnard_good_fraction_filter2)
  • Langley regression Io, Michalsky, Direct Narrowband Filter1(michalsky_solar_constant_filter1)
  • number of points used in final linear fit for the Direct Narrowband Filter1(barnard_number_points_filter1)
  • rejection flag for Direct Narrowband Filter4(michalsky_badflag_filter4)
  • optical depth for the Direct Narrowband Filter1(michalsky_optical_depth_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter3(michalsky_good_fraction_filter3)
  • number of points used in final linear fit for the Direct Narrowband Filter2(barnard_number_points_filter2)
  • optical depth for the Direct Narrowband Filter6(michalsky_optical_depth_filter6)
  • rejection flag for Direct Narrowband Filter1(barnard_badflag_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter4(barnard_good_fraction_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter2(michalsky_number_points_filter2)
  • solar constant corrected for solar distance for the Direct Narrowband Filter6(michalsky_solar_constant_sdist_filter6)
  • optical depth for the Direct Narrowband Filter3(michalsky_optical_depth_filter3)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter5(barnard_solar_constant_sdist_filter5)
  • optical depth for the Direct Narrowband Filter4(michalsky_optical_depth_filter4)
  • solar constant corrected for solar distance for the Direct Narrowband Filter1(michalsky_solar_constant_sdist_filter1)
  • rejection flag for Direct Narrowband Filter2(michalsky_badflag_filter2)
  • number of points used in final linear fit for the Direct Narrowband Filter4(michalsky_number_points_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter4(barnard_number_points_filter4)
  • standard deviation around regression line for the Direct Narrowband Filter3(michalsky_standard_deviation_filter3)
  • number of points used in final linear fit for the Direct Broadband(michalsky_number_points_broadband)
  • number of points used in final linear fit for the Direct Narrowband Filter5(barnard_number_points_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter1(barnard_good_fraction_filter1)
  • rejection flag for Direct Narrowband Filter2(barnard_badflag_filter2)
  • number of points used in final linear fit for the Direct Narrowband Filter1(michalsky_number_points_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter6(michalsky_good_fraction_filter6)
  • optical depth for the Direct Narrowband Filter5(barnard_optical_depth_filter5)
  • optical depth for the Direct Narrowband Filter2(michalsky_optical_depth_filter2)
  • optical depth for the Direct Narrowband Filter6(barnard_optical_depth_filter6)
  • error in final linear fit for the Direct Narrowband Filter2(barnard_error_fit_filter2)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter5(barnard_good_fraction_filter5)
  • error in final linear fit for the Direct Narrowband Filter1(barnard_error_fit_filter1)
  • rejection flag for Direct Narrowband Filter3(barnard_badflag_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter6(michalsky_standard_deviation_filter6)
  • number of points used in final linear fit for the Direct Narrowband Filter3(michalsky_number_points_filter3)
  • Angstrom exponent(michalsky_angstrom_exponent)
  • number of points used in final linear fit for the Direct Narrowband Filter6(michalsky_number_points_filter6)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter3(barnard_good_fraction_filter3)
  • number of points used in final linear fit for the Direct Narrowband Filter5(michalsky_number_points_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter4(michalsky_good_fraction_filter4)
  • optical depth for the Direct Narrowband Filter5(michalsky_optical_depth_filter5)
  • error in final linear fit for the Direct BroadBand(barnard_error_fit_broadband)
  • standard deviation around regression line for the Direct BroadBand(michalsky_standard_deviation_broadband)
  • solar constant corrected for solar distance for the Direct Narrowband Filter5(michalsky_solar_constant_sdist_filter5)
  • solar constant corrected for solar distance for the Direct Narrowband Filter4(michalsky_solar_constant_sdist_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter6(barnard_number_points_filter6)


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DQRID : D040427.3
Start DateStart TimeEnd DateEnd Time
02/13/2004235903/11/20041845
Subject:
SGP/MFRSR/E9 - Shadowband Misaligned
DataStreams:sgpmfrsrE9.b1, sgpmfrsrlangleyE9.c1, sgpmfrsrlangplotE9.c1, sgpmfrsrod1barnmichE9.c1
Description:
The shadowband was misaligned following replacement.  Data in the afternoon should be used 
with caution.
Measurements:sgpmfrsrE9.b1:
  • Diffuse Hemispheric Broadband Irradiance (Approximate), MFRSR(diffuse_hemisp_broadband)
  • Direct Normal Narrowband Irradiance, Filter 2, offset corrected(direct_normal_narrowband_filter2)
  • Direct Normal Broadband Irradiance, broadband scale applied(direct_normal_broadband)
  • Direct Normal Narrowband Irradiance, Filter 1, offset corrected(direct_normal_narrowband_filter1)
  • Direct Normal Narrowband Irradiance, Filter 5, offset corrected(direct_normal_narrowband_filter5)
  • Direct Normal Narrowband Irradiance, Filter 6, offset corrected(direct_normal_narrowband_filter6)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 2(diffuse_hemisp_narrowband_filter2)
  • Direct Normal Narrowband Irradiance, Filter 3, offset corrected(direct_normal_narrowband_filter3)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 4(diffuse_hemisp_narrowband_filter4)
  • Direct Normal Narrowband Irradiance, Filter 4, offset corrected(direct_normal_narrowband_filter4)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 1(diffuse_hemisp_narrowband_filter1)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 3(diffuse_hemisp_narrowband_filter3)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 5(diffuse_hemisp_narrowband_filter5)
  • Narrowband Diffuse Hemispheric Irradiance, Filter 6(diffuse_hemisp_narrowband_filter6)

sgpmfrsrod1barnmichE9.c1:
  • aerosol optical depth filter 5(aerosol_optical_depth_filter5)
  • Angstrom exponent(angstrom_exponent)
  • aerosol optical depth filter 4(aerosol_optical_depth_filter4)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter4)
  • totaloptical depth direct narrowband filter 2(total_optical_depth_filter2)
  • total optical depth direct narrowband filter 1(total_optical_depth_filter1)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter2)
  • Rayleigh optical thickness computed for filter 5(Rayleigh_optical_thickness_filter5)
  • Rayleigh optical thickness computed for filter 2(Rayleigh_optical_thickness_filter2)
  • Rayleigh optical thickness computed for filter 1(Rayleigh_optical_thickness_filter1)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter3)
  • Optical depth from TOMS satellite(TOMS_optical_depth)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter5)
  • extraterrestrial spectral irradiance used for optical depth calculations,
    corrected for eccentricity of earth\'s orbit(io_filter1)
  • Rayleigh optical thickness computed for filter 3(Rayleigh_optical_thickness_filter3)
  • Rayleigh optical thickness computed for filter 4(Rayleigh_optical_thickness_filter4)
  • aerosol optical depth filter 3(aerosol_optical_depth_filter3)
  • aerosol optical depth filter 2(aerosol_optical_depth_filter2)
  • Ozone absorption coefficient used for filter 2(Ozone_absorption_coefficient_filter2)
  • surface pressure(surface_pressure)
  • Indicator of optical depth stability(optical_depth_stability_flag)
  • Airmasses(airmass)
  • Ozone absorption coefficient used for filter 5(Ozone_absorption_coefficient_filter5)
  • total optical depth direct narrowband filter 4(total_optical_depth_filter4)
  • Ozone absorption coefficient used for filter 4(Ozone_absorption_coefficient_filter4)
  • total optical depth direct narrowband filter 3(total_optical_depth_filter3)
  • Ozone absorption coefficient used for filter 3(Ozone_absorption_coefficient_filter3)
  • aerosol optical depth filter 1(aerosol_optical_depth_filter1)
  • Ozone absorption coefficient used for filter 1(Ozone_absorption_coefficient_filter1)
  • total optical depth direct narrowband filter 5(total_optical_depth_filter5)

sgpmfrsrlangplotE9.c1:
  • airmass(michalsky_airmass)
  • log(irradiance) for the Direct Narrowband Filter6, Michalsky(michalsky_lnI_filter6)
  • rejected points for the final fit for the Direct Narrowband Filter2, Barnard(barnard_rejected_filter2)
  • log(irradiance) for the Direct Narrowband Filter5, Barnard(barnard_lnI_filter5)
  • rejected points for the final fit for the Direct Narrowband Filter1, Barnard(barnard_rejected_filter1)
  • log(irradiance) for the Direct Narrowband Filter4, Barnard(barnard_lnI_filter4)
  • rejected points for the final fit for the Direct Broadband, Michalsky(michalsky_rejected_broadband)
  • rejected points for the final fit for the Direct Narrowband Filter4, Barnard(barnard_rejected_filter4)
  • log(irradiance) for the Direct Narrowband Filter5, Michalsky(michalsky_lnI_filter5)
  • log(irradiance) for the Direct Narrowband Filter4, Michalsky(michalsky_lnI_filter4)
  • rejected points for the final fit for the Direct Narrowband Filter5, Barnard(barnard_rejected_filter5)
  • rejected points for the final fit for the Direct Broadband, Barnard(barnard_rejected_broadband)
  • rejected points for the final fit for the Direct Narrowband Filter6, Barnard(barnard_rejected_filter6)
  • log(irradiance) for the Direct Narrowband Filter1, Michalsky(michalsky_lnI_filter1)
  • rejected points for the final fit for the Direct Narrowband Filter5, Michalsky(michalsky_rejected_filter5)
  • log(irradiance) for the Direct Narrowband Filter6, Barnard(barnard_lnI_filter6)
  • log(irradiance) for the Direct Broadband, Barnard(barnard_lnI_broadband)
  • log(irradiance) for the Direct Narrowband Filter1, Barnard(barnard_lnI_filter1)
  • rejected points for the final fit for the Direct Narrowband Filter6, Michalsky(michalsky_rejected_filter6)
  • rejected points for the final fit for the Direct Narrowband Filter3, Barnard(barnard_rejected_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter2, Michalsky(michalsky_rejected_filter2)
  • log(irradiance) for the Direct Broadband, Michalsky(michalsky_lnI_broadband)
  • log(irradiance) for the Direct Narrowband Filter2, Barnard(barnard_lnI_filter2)
  • log(irradiance) for the Direct Narrowband Filter3, Barnard(barnard_lnI_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter1, Michalsky(michalsky_rejected_filter1)
  • airmass(barnard_airmass)
  • log(irradiance) for the Direct Narrowband Filter3, Michalsky(michalsky_lnI_filter3)
  • rejected points for the final fit for the Direct Narrowband Filter3, Michalsky(michalsky_rejected_filter3)
  • log(irradiance) for the Direct Narrowband Filter2, Michalsky(michalsky_lnI_filter2)
  • rejected points for the final fit for the Direct Narrowband Filter4, Michalsky(michalsky_rejected_filter4)

sgpmfrsrlangleyE9.c1:
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter5(barnard_error_slope_filter5)
  • Langley regression Io, Michalsky, Direct Narrowband Filter6(michalsky_solar_constant_filter6)
  • rejection flag for Direct Broadband(barnard_badflag_broadband)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter3(barnard_error_slope_filter3)
  • optical depth for the Direct Narrowband Filter3(barnard_optical_depth_filter3)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct BroadBand(barnard_solar_constant_sdist_broadband)
  • rejection flag for Direct Broadband(michalsky_badflag_broadband)
  • rejection flag for Direct Narrowband Filter6(barnard_badflag_filter6)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter1(barnard_error_slope_filter1)
  • error in final linear fit for the Direct Narrowband Filter5(barnard_error_fit_filter5)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter6(barnard_error_slope_filter6)
  • solar constant corrected for solar distance for the Direct Narrowband Filter3(michalsky_solar_constant_sdist_filter3)
  • error in final linear fit for the Direct Narrowband Filter4(barnard_error_fit_filter4)
  • percentage of initial points used in final linear fit for the Direct Broadband(michalsky_good_fraction_broadband)
  • Angstrom exponent(barnard_angstrom_exponent)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter2(barnard_solar_constant_sdist_filter2)
  • solar constant corrected for solar distance for the Direct Broadband(michalsky_solar_constant_sdist_broadband)
  • rejection flag for Direct Narrowband Filter5(barnard_badflag_filter5)
  • rejection flag for Direct Narrowband Filter4(barnard_badflag_filter4)
  • rejection flag for Direct Narrowband Filter6(michalsky_badflag_filter6)
  • error in optical depth (slope) of final linear fit for the Direct Broadband(barnard_error_slope_broadband)
  • Langley regression Io, Michalsky, Direct BroadBand(michalsky_solar_constant_broadband)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter4(barnard_solar_constant_sdist_filter4)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter1(barnard_solar_constant_sdist_filter1)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter2(barnard_error_slope_filter2)
  • percentage of initial points used in final linear fit for the Direct Broadband(barnard_good_fraction_broadband)
  • solar constant corrected for solar distance for the Direct Narrowband Filter6(barnard_solar_constant_sdist_filter6)
  • rejection flag for Direct Narrowband Filter5(michalsky_badflag_filter5)
  • optical depth for the Direct Narrowband Filter1(barnard_optical_depth_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter2(michalsky_good_fraction_filter2)
  • error in final linear fit for the Direct Narrowband Filter3(barnard_error_fit_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter1(michalsky_standard_deviation_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter1(michalsky_good_fraction_filter1)
  • optical depth for the Direct BroadBand(michalsky_optical_depth_broadband)
  • error in optical depth (slope) of final linear fit for the Direct Narrowband
    Filter4(barnard_error_slope_filter4)
  • Langley regression Io, Michalsky, Direct Narrowband Filter4(michalsky_solar_constant_filter4)
  • error in final linear fit for the Direct Narrowband Filter6(barnard_error_fit_filter6)
  • optical depth for the Direct Narrowband Filter2(barnard_optical_depth_filter2)
  • Langley regression Io, Michalsky, Direct Narrowband Filter5(michalsky_solar_constant_filter5)
  • solar constant corrected for solar distance for the Direct Narrowband Filter2(michalsky_solar_constant_sdist_filter2)
  • rejection flag for Direct Narrowband Filter1(michalsky_badflag_filter1)
  • standard deviation around regression line for the Direct Narrowband Filter4(michalsky_standard_deviation_filter4)
  • Langley regression Io, Michalsky, Direct Narrowband Filter2(michalsky_solar_constant_filter2)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter3(barnard_solar_constant_sdist_filter3)
  • Langley regression Io, Michalsky, Direct Narrowband Filter3(michalsky_solar_constant_filter3)
  • optical depth for the Direct Narrowband Filter4(barnard_optical_depth_filter4)
  • optical depth for the Direct BroadBand(barnard_optical_depth_broadband)
  • number of points used in final linear fit for the Direct Narrowband Filter3(barnard_number_points_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter5(michalsky_standard_deviation_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter5(michalsky_good_fraction_filter5)
  • standard deviation around regression line for the Direct Narrowband Filter2(michalsky_standard_deviation_filter2)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter6(barnard_good_fraction_filter6)
  • number of points used in final linear fit for the Direct Broadband(barnard_number_points_broadband)
  • rejection flag for Direct Narrowband Filter3(michalsky_badflag_filter3)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter2(barnard_good_fraction_filter2)
  • Langley regression Io, Michalsky, Direct Narrowband Filter1(michalsky_solar_constant_filter1)
  • number of points used in final linear fit for the Direct Narrowband Filter1(barnard_number_points_filter1)
  • rejection flag for Direct Narrowband Filter4(michalsky_badflag_filter4)
  • optical depth for the Direct Narrowband Filter1(michalsky_optical_depth_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter3(michalsky_good_fraction_filter3)
  • number of points used in final linear fit for the Direct Narrowband Filter2(barnard_number_points_filter2)
  • optical depth for the Direct Narrowband Filter6(michalsky_optical_depth_filter6)
  • rejection flag for Direct Narrowband Filter1(barnard_badflag_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter4(barnard_good_fraction_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter2(michalsky_number_points_filter2)
  • solar constant corrected for solar distance for the Direct Narrowband Filter6(michalsky_solar_constant_sdist_filter6)
  • optical depth for the Direct Narrowband Filter3(michalsky_optical_depth_filter3)
  • Langley regression Io, adjusted to 1AU, Barnard, Direct Narrowband Filter5(barnard_solar_constant_sdist_filter5)
  • optical depth for the Direct Narrowband Filter4(michalsky_optical_depth_filter4)
  • solar constant corrected for solar distance for the Direct Narrowband Filter1(michalsky_solar_constant_sdist_filter1)
  • rejection flag for Direct Narrowband Filter2(michalsky_badflag_filter2)
  • number of points used in final linear fit for the Direct Narrowband Filter4(michalsky_number_points_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter4(barnard_number_points_filter4)
  • standard deviation around regression line for the Direct Narrowband Filter3(michalsky_standard_deviation_filter3)
  • number of points used in final linear fit for the Direct Broadband(michalsky_number_points_broadband)
  • number of points used in final linear fit for the Direct Narrowband Filter5(barnard_number_points_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter1(barnard_good_fraction_filter1)
  • rejection flag for Direct Narrowband Filter2(barnard_badflag_filter2)
  • number of points used in final linear fit for the Direct Narrowband Filter1(michalsky_number_points_filter1)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter6(michalsky_good_fraction_filter6)
  • optical depth for the Direct Narrowband Filter5(barnard_optical_depth_filter5)
  • optical depth for the Direct Narrowband Filter2(michalsky_optical_depth_filter2)
  • optical depth for the Direct Narrowband Filter6(barnard_optical_depth_filter6)
  • error in final linear fit for the Direct Narrowband Filter2(barnard_error_fit_filter2)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter5(barnard_good_fraction_filter5)
  • error in final linear fit for the Direct Narrowband Filter1(barnard_error_fit_filter1)
  • rejection flag for Direct Narrowband Filter3(barnard_badflag_filter3)
  • standard deviation around regression line for the Direct Narrowband Filter6(michalsky_standard_deviation_filter6)
  • number of points used in final linear fit for the Direct Narrowband Filter3(michalsky_number_points_filter3)
  • Angstrom exponent(michalsky_angstrom_exponent)
  • number of points used in final linear fit for the Direct Narrowband Filter6(michalsky_number_points_filter6)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter3(barnard_good_fraction_filter3)
  • number of points used in final linear fit for the Direct Narrowband Filter5(michalsky_number_points_filter5)
  • percentage of initial points used in final linear fit for the Direct Narrowband
    Filter4(michalsky_good_fraction_filter4)
  • optical depth for the Direct Narrowband Filter5(michalsky_optical_depth_filter5)
  • error in final linear fit for the Direct BroadBand(barnard_error_fit_broadband)
  • standard deviation around regression line for the Direct BroadBand(michalsky_standard_deviation_broadband)
  • solar constant corrected for solar distance for the Direct Narrowband Filter5(michalsky_solar_constant_sdist_filter5)
  • solar constant corrected for solar distance for the Direct Narrowband Filter4(michalsky_solar_constant_sdist_filter4)
  • number of points used in final linear fit for the Direct Narrowband Filter6(barnard_number_points_filter6)


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