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Title: Shortwave Spectrometer (SWS) zenith radiance swsrad.b1 v3 and higher

Abstract

Hyperspectral zenith radiances from the SWS instrument reported at 1 Hz. This data stream contains calibrated, dark-subtracted, radiances from two grating array spectrometers: a Si-detector based spectrometer denoted by SW and an InGaAs based detector denoted by LW. Spectra from both spectrometers are calibrated based on the spectral responsivity determined by reference against NIST-traceable light sources are reported independently as separate arrays having the same time record but wavelength dimension specified for each detector. Because the LW spectrometer is more susceptible to temperature-induced changes, a scale factor adjustment is applied the the LW spectra to yield agreement with the SW spectra over the wavelength range where they overlap. The final radiances incorporate QC to flag saturated values, periods where house-keeping fields fall outside acceptable bounds, and to flag pixels for which the spectral responsivity is not acceptable.

Authors:
Publication Date:
DOE Contract Number:  
AC05-00OR22725
Research Org.:
Atmospheric Radiation Measurement User Facility
Sponsoring Org.:
USDOE Office of Science (SC), Biological and Environmental Research (BER)
Collaborations:
PNNL, BNL, ANL, ORNL
Subject:
54 ENVIRONMENTAL SCIENCES; shortwave; hyperspectral; zenith radiance; SWS
OSTI Identifier:
1602611
DOI:
https://doi.org/10.5439/1602611

Citation Formats

Flynn, Connor. Shortwave Spectrometer (SWS) zenith radiance swsrad.b1 v3 and higher. United States: N. p., 2026. Web. doi:10.5439/1602611.
Flynn, Connor. Shortwave Spectrometer (SWS) zenith radiance swsrad.b1 v3 and higher. United States. doi:https://doi.org/10.5439/1602611
Flynn, Connor. 2026. "Shortwave Spectrometer (SWS) zenith radiance swsrad.b1 v3 and higher". United States. doi:https://doi.org/10.5439/1602611. https://www.osti.gov/servlets/purl/1602611. Pub date:Tue Jan 13 19:00:00 EST 2026
@article{osti_1602611,
title = {Shortwave Spectrometer (SWS) zenith radiance swsrad.b1 v3 and higher},
author = {Flynn, Connor},
abstractNote = {Hyperspectral zenith radiances from the SWS instrument reported at 1 Hz. This data stream contains calibrated, dark-subtracted, radiances from two grating array spectrometers: a Si-detector based spectrometer denoted by SW and an InGaAs based detector denoted by LW. Spectra from both spectrometers are calibrated based on the spectral responsivity determined by reference against NIST-traceable light sources are reported independently as separate arrays having the same time record but wavelength dimension specified for each detector. Because the LW spectrometer is more susceptible to temperature-induced changes, a scale factor adjustment is applied the the LW spectra to yield agreement with the SW spectra over the wavelength range where they overlap. The final radiances incorporate QC to flag saturated values, periods where house-keeping fields fall outside acceptable bounds, and to flag pixels for which the spectral responsivity is not acceptable.},
doi = {10.5439/1602611},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Tue Jan 13 19:00:00 EST 2026},
month = {Tue Jan 13 19:00:00 EST 2026}
}