Angular Distribution Models for Top-of-Atmosphere Radiative Flux Estimation from the Clouds and the Earth’s Radiant Energy System Instrument on the Terra Satellite. Part II: ValidationSource: Journal of Atmospheric and Oceanic Technology:;2007:;volume( 024 ):;issue: 004::page 564Author:Loeb, Norman G.
,
Kato, Seiji
,
Loukachine, Konstantin
,
Manalo-Smith, Natividad
,
Doelling, David R.
DOI: 10.1175/JTECH1983.1Publisher: American Meteorological Society
Abstract: Errors in top-of-atmosphere (TOA) radiative fluxes from the Clouds and the Earth?s Radiant Energy System (CERES) instrument due to uncertainties in radiance-to-flux conversion from CERES Terra angular distribution models (ADMs) are evaluated through a series of consistency tests. These tests show that the overall bias in regional monthly mean shortwave (SW) TOA flux is less than 0.2 W m?2 and the regional RMS error ranges from 0.70 to 1.4 W m?2. In contrast, SW TOA fluxes inferred using theoretical ADMs that assume clouds are plane parallel are overestimated by 3?4 W m?2 and exhibit a strong latitudinal dependence. In the longwave (LW), the bias error ranges from 0.2 to 0.4 W m?2 and regional RMS errors remain smaller than 0.7 W m?2. Global mean albedos derived from ADMs developed during the Earth Radiation Budget Experiment (ERBE) and applied to CERES measurements show a systematic increase with viewing zenith angle of 4%?8%, while albedos from the CERES Terra ADMs show a smaller increase of 1%?2%. The LW fluxes from the ERBE ADMs show a systematic decrease with viewing zenith angle of 2%?2.4%, whereas fluxes from the CERES Terra ADMs remain within 0.7%?0.8% at all angles. Based on several months of multiangle CERES along-track data, the SW TOA flux consistency between nadir- and oblique-viewing zenith angles is generally 5% (<17 W m?2) over land and ocean and 9% (26 W m?2) in polar regions, and LW TOA flux consistency is approximate 3% (7 W m?2) over all surfaces. Based on these results and a theoretically derived conversion between TOA flux consistency and TOA flux error, the best estimate of the error in CERES TOA flux due to the radiance-to-flux conversion is 3% (10 W m?2) in the SW and 1.8% (3?5 W m?2) in the LW. Monthly mean TOA fluxes based on ERBE ADMs are larger than monthly mean TOA fluxes based on CERES Terra ADMs by 1.8 and 1.3 W m?2 in the SW and LW, respectively.
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contributor author | Loeb, Norman G. | |
contributor author | Kato, Seiji | |
contributor author | Loukachine, Konstantin | |
contributor author | Manalo-Smith, Natividad | |
contributor author | Doelling, David R. | |
date accessioned | 2017-06-09T17:23:27Z | |
date available | 2017-06-09T17:23:27Z | |
date copyright | 2007/04/01 | |
date issued | 2007 | |
identifier issn | 0739-0572 | |
identifier other | ams-84367.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4227695 | |
description abstract | Errors in top-of-atmosphere (TOA) radiative fluxes from the Clouds and the Earth?s Radiant Energy System (CERES) instrument due to uncertainties in radiance-to-flux conversion from CERES Terra angular distribution models (ADMs) are evaluated through a series of consistency tests. These tests show that the overall bias in regional monthly mean shortwave (SW) TOA flux is less than 0.2 W m?2 and the regional RMS error ranges from 0.70 to 1.4 W m?2. In contrast, SW TOA fluxes inferred using theoretical ADMs that assume clouds are plane parallel are overestimated by 3?4 W m?2 and exhibit a strong latitudinal dependence. In the longwave (LW), the bias error ranges from 0.2 to 0.4 W m?2 and regional RMS errors remain smaller than 0.7 W m?2. Global mean albedos derived from ADMs developed during the Earth Radiation Budget Experiment (ERBE) and applied to CERES measurements show a systematic increase with viewing zenith angle of 4%?8%, while albedos from the CERES Terra ADMs show a smaller increase of 1%?2%. The LW fluxes from the ERBE ADMs show a systematic decrease with viewing zenith angle of 2%?2.4%, whereas fluxes from the CERES Terra ADMs remain within 0.7%?0.8% at all angles. Based on several months of multiangle CERES along-track data, the SW TOA flux consistency between nadir- and oblique-viewing zenith angles is generally 5% (<17 W m?2) over land and ocean and 9% (26 W m?2) in polar regions, and LW TOA flux consistency is approximate 3% (7 W m?2) over all surfaces. Based on these results and a theoretically derived conversion between TOA flux consistency and TOA flux error, the best estimate of the error in CERES TOA flux due to the radiance-to-flux conversion is 3% (10 W m?2) in the SW and 1.8% (3?5 W m?2) in the LW. Monthly mean TOA fluxes based on ERBE ADMs are larger than monthly mean TOA fluxes based on CERES Terra ADMs by 1.8 and 1.3 W m?2 in the SW and LW, respectively. | |
publisher | American Meteorological Society | |
title | Angular Distribution Models for Top-of-Atmosphere Radiative Flux Estimation from the Clouds and the Earth’s Radiant Energy System Instrument on the Terra Satellite. Part II: Validation | |
type | Journal Paper | |
journal volume | 24 | |
journal issue | 4 | |
journal title | Journal of Atmospheric and Oceanic Technology | |
identifier doi | 10.1175/JTECH1983.1 | |
journal fristpage | 564 | |
journal lastpage | 584 | |
tree | Journal of Atmospheric and Oceanic Technology:;2007:;volume( 024 ):;issue: 004 | |
contenttype | Fulltext |