Articles | Volume 8, issue 2
https://doi.org/10.5194/amt-8-611-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/amt-8-611-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Next-generation angular distribution models for top-of-atmosphere radiative flux calculation from CERES instruments: methodology
W. Su
CORRESPONDING AUTHOR
MS420, NASA Langley Research Center, Hampton, Virginia, USA
J. Corbett
Science Systems & Applications, Inc., Hampton, Virginia, USA
Z. Eitzen
Science Systems & Applications, Inc., Hampton, Virginia, USA
L. Liang
Science Systems & Applications, Inc., Hampton, Virginia, USA
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Short summary
The top-of-atmosphere (TOA) radiative fluxes are critical components to advancing our understanding of the Earth's radiative energy balance. The Clouds and Earth's Radiant Energy System (CERES) instruments provide broadband shortwave and longwave radiance measurements. These radiances are converted to fluxes by using scene-type-dependent angular distribution models (ADMs). This paper describes the next-generation CERES ADMs that are developed for TOA radiative flux inversion.
The top-of-atmosphere (TOA) radiative fluxes are critical components to advancing our...