2016
DOI: 10.3390/rs8030182
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CERES Top-of-Atmosphere Earth Radiation Budget Climate Data Record: Accounting for in-Orbit Changes in Instrument Calibration

Abstract: Abstract:The Clouds and the Earth's Radiant Energy System (CERES) project provides observations of Earth's radiation budget using measurements from CERES instruments onboard the Terra, Aqua and Suomi National Polar-orbiting Partnership (S-NPP) satellites. As the objective is to create a long-term climate data record, it is necessary to periodically reprocess the data in order to incorporate the latest calibration changes and algorithm improvements. Here, we focus on the improvements and validation of CERES Ter… Show more

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Cited by 82 publications
(65 citation statements)
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“…The Clouds and the Earth's Radiant Energy System (CERES) instrument, aboard Aqua as a part of the A-Train Earth Observing System [Wielicki et al, 1996], measures shortwave (SW) and longwave (LW) broadband radiation at top-of-atmosphere (TOA). After many years of improving instrument calibration [Loeb et al, 2016] and angular distribution model (ADM) [Loeb et al, 2005[Loeb et al, , 2007Su et al, 2015aSu et al, , 2015b, the CERES instrument gives unprecedented accuracy for TOA radiation budget estimates [Loeb et al, 2012a[Loeb et al, , 2016, and it has been widely used for examination of Earth energy imbalance and related climate changes [e.g., Loeb et al, 2012b;Trenberth et al, 2014;Allan et al, 2015]. Unlike TOA irradiance estimates, estimating surface or atmosphere radiation budget involves radiative transfer computations that require appropriate model inputs Su et al, 2005;Kato et al, 2008Kato et al, , 2011Kato et al, , 2013Wild et al, 2013;Stephens et al, 2012].…”
Section: Introductionmentioning
confidence: 99%
“…The Clouds and the Earth's Radiant Energy System (CERES) instrument, aboard Aqua as a part of the A-Train Earth Observing System [Wielicki et al, 1996], measures shortwave (SW) and longwave (LW) broadband radiation at top-of-atmosphere (TOA). After many years of improving instrument calibration [Loeb et al, 2016] and angular distribution model (ADM) [Loeb et al, 2005[Loeb et al, , 2007Su et al, 2015aSu et al, , 2015b, the CERES instrument gives unprecedented accuracy for TOA radiation budget estimates [Loeb et al, 2012a[Loeb et al, , 2016, and it has been widely used for examination of Earth energy imbalance and related climate changes [e.g., Loeb et al, 2012b;Trenberth et al, 2014;Allan et al, 2015]. Unlike TOA irradiance estimates, estimating surface or atmosphere radiation budget involves radiative transfer computations that require appropriate model inputs Su et al, 2005;Kato et al, 2008Kato et al, , 2011Kato et al, , 2013Wild et al, 2013;Stephens et al, 2012].…”
Section: Introductionmentioning
confidence: 99%
“…Such an error is assumed equal to 0.3 W m −2 , corresponding to the EEI monthly global anomaly for nonocean components, as suggested by Trenberth et al (). The instrumental error is assumed equal to 0.3 W m −2 , estimated by Loeb et al () as standard deviation of the differences of CERES measurements from different satellite platforms.…”
Section: Methodsmentioning
confidence: 99%
“…We use in this study CERES Energy Balanced and Filled Top-of-Atmosphere (EBAF-TOA) Edition 4.0 (Loeb et al, 2016), released during early 2017. This version presents improvements with respect to the previous Geophysical Research Letters 10.1002/2017GL075396 version (version 2.8) in many aspects, such as the instrument calibration and the retrieval of cloud properties.…”
Section: Ceres Ebaf Datamentioning
confidence: 99%
“…Shape and bandwidth differences of spectral response functions (SRF) must be accounted for when comparing radiances from separate instruments. The CERES project tracks calibration relative stability of multiple CERES instruments using vicarious techniques, including tropical mean and deep convective cloud comparisons referenced to the FM1 instrument [7]. CERES performs inter-satellite direct comparisons by commanding its two-axis gimbal pointing system to rotate in the azimuth direction so that observations from multiple instruments match near satellite orbit crossings.…”
Section: Introductionmentioning
confidence: 99%