Validation of Point Spread Functions of CERES Radiometers by the Use of Lunar Observations

Kory J. Priestley NASA Langley Research Center, Hampton, Virginia

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Susan Thomas Science Systems Applications, Inc., Hampton, Virginia

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G. Louis Smith National Institute for Aerospace, Hampton, Virginia

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Abstract

The Clouds and the Earth’s Radiant Energy System (CERES) scanning radiometers have been operating to make raster scans of the moon on a quarterly basis to validate the point response function for the three channels of flight models 1–4 aboard the Terra and Aqua spacecraft. Instrument pointing accuracy was verified by this method to 0.2° for the total channel of FM-3. The point response functions were computed from the lunar observations and were found to be nominal with the exception of the FM-2 window channel, which was found to have a region of high sensitivity. This anomaly is attributed to a delamination of the detector flake from the heat sink in that region. The influence of this anomaly is accounted for by the in-flight calibration and has no adverse effect on the application of the data.

Corresponding author address: G. Louis Smith, Mail Stop 420, Langley Research Center, Hampton, VA 23681. Email: g.louis.smith@nasa.gov

Abstract

The Clouds and the Earth’s Radiant Energy System (CERES) scanning radiometers have been operating to make raster scans of the moon on a quarterly basis to validate the point response function for the three channels of flight models 1–4 aboard the Terra and Aqua spacecraft. Instrument pointing accuracy was verified by this method to 0.2° for the total channel of FM-3. The point response functions were computed from the lunar observations and were found to be nominal with the exception of the FM-2 window channel, which was found to have a region of high sensitivity. This anomaly is attributed to a delamination of the detector flake from the heat sink in that region. The influence of this anomaly is accounted for by the in-flight calibration and has no adverse effect on the application of the data.

Corresponding author address: G. Louis Smith, Mail Stop 420, Langley Research Center, Hampton, VA 23681. Email: g.louis.smith@nasa.gov

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