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Title: csphothybv3: A hybrid sky radiance scan scenario version 3 data

Abstract

This hybrid scan starts at the position of the Sun and first follows the great circle that is orthogonal to the Principal Plane until it reaches a viewing zenith angle of 75 degrees and then follows the almucantar keep that viewing zenith angle constant. The scan is then repeated in the opposite azimuth direction. This mode was designed to optimize the range of scattering angles and significantly improves the retrieval of inversion parameters especially at low solar zenith angles.

Authors:
;
Publication Date:
DOE Contract Number:  
DE-AC05-00OR22725
Research Org.:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Atmospheric Radiation Measurement (ARM) Archive; Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Atmospheric Radiation Measurement (ARM) Data Center
Sponsoring Org.:
USDOE Office of Science (SC), Biological and Environmental Research (BER)
Collaborations:
PNNL, BNL, ANL, ORNL
Subject:
54 Environmental Sciences
Keywords:
Sky radiance in Hybrid mode for varying scattering angle.
OSTI Identifier:
1877106
DOI:
https://doi.org/10.5439/1877106

Citation Formats

Ma, Lynn, and Wagener, Richard. csphothybv3: A hybrid sky radiance scan scenario version 3 data. United States: N. p., 2022. Web. doi:10.5439/1877106.
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Ma, Lynn, & Wagener, Richard. csphothybv3: A hybrid sky radiance scan scenario version 3 data. United States. doi:https://doi.org/10.5439/1877106
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Ma, Lynn, and Wagener, Richard. 2022. "csphothybv3: A hybrid sky radiance scan scenario version 3 data". United States. doi:https://doi.org/10.5439/1877106. https://www.osti.gov/servlets/purl/1877106. Pub date:Wed Aug 31 00:00:00 EDT 2022
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@article{osti_1877106,
title = {csphothybv3: A hybrid sky radiance scan scenario version 3 data},
author = {Ma, Lynn and Wagener, Richard},
abstractNote = {This hybrid scan starts at the position of the Sun and first follows the great circle that is orthogonal to the Principal Plane until it reaches a viewing zenith angle of 75 degrees and then follows the almucantar keep that viewing zenith angle constant. The scan is then repeated in the opposite azimuth direction. This mode was designed to optimize the range of scattering angles and significantly improves the retrieval of inversion parameters especially at low solar zenith angles.},
doi = {10.5439/1877106},
journal = {},
number = ,
volume = ,
place = {United States},
year = {2022},
month = {8}
}
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Dataset:
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DOI: https://doi.org/10.5439/1877106
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