1991
DOI: 10.1117/12.46702
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<title>Radiometric calibration plan for the Clouds and the Earth's Radiant Energy System scanning instruments</title>

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Cited by 10 publications
(7 citation statements)
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“…It is estimated that a 15 % underfilling ofthe CERES aperture will occur at 200 pm, but the effect cancels because the aperture stop ofthe reference detector optics is identical in size and location to the CERES sensor aperture stop. 5) In the far infrared, the FTS source intensity is about five times greater than the self-emission of the reference detector at room temperature and the CERES detectors at 3 10 K. If the FTS source energy were eliminated, an interferogram would still be produced by the detector emission because it is originating at a relayed image of the FTS field stop. This interferogram would be self-observed by the detectors under test.…”
Section: Measurement Planmentioning
confidence: 98%
“…It is estimated that a 15 % underfilling ofthe CERES aperture will occur at 200 pm, but the effect cancels because the aperture stop ofthe reference detector optics is identical in size and location to the CERES sensor aperture stop. 5) In the far infrared, the FTS source intensity is about five times greater than the self-emission of the reference detector at room temperature and the CERES detectors at 3 10 K. If the FTS source energy were eliminated, an interferogram would still be produced by the detector emission because it is originating at a relayed image of the FTS field stop. This interferogram would be self-observed by the detectors under test.…”
Section: Measurement Planmentioning
confidence: 98%
“…The sensor gains in the longwave and shortwave spectral regions are derived using the test data from various sources in the RCF 7,8 . A Fourier Transform Spectrometer (FTS) system is used for the spectral characterization of the sensors in the wavelength region beyond 3.0 micron 9 .…”
Section: Ground Calibrationsmentioning
confidence: 99%
“…During January [13][14][15][16][17][18][19][20][21][22]1998, the calibrations were conducted typically every two days. During January 4 -1 1, 1998, using the MAM, sensor solar calibrations were conducted daily.…”
Section: -Trmmjceres Sensor and Measurement Statusmentioning
confidence: 99%