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22 September 2009RapidEye constellation relative radiometric accuracy measurement using lunar images
The RapidEye constellation includes five identical satellites in Low Earth Orbit (LEO). Each satellite has a 5-band
(blue, green, red, red-edge and near infrared (NIR)) multispectral imager at 6.5m GSD. A three-axes attitude control
system allows pointing the imager of each satellite at the Moon during lunations. It is therefore possible to image the
Moon from near identical viewing geometry within a span of 80 minutes with each one of the imagers. Comparing the
radiometrically corrected images obtained from each band and each satellite allows a near instantaneous relative
radiometric accuracy measurement and determination of relative gain changes between the five imagers. A more
traditional terrestrial vicarious radiometric calibration program has also been completed by MDA on RapidEye. The two
components of this program provide for spatial radiometric calibration ensuring that detector-to-detector response
remains flat, while a temporal radiometric calibration approach has accumulated images of specific dry dessert
calibration sites. These images are used to measure the constellation relative radiometric response and make on-ground
gain and offset adjustments in order to maintain the relative accuracy of the constellation within ±2.5%. A quantitative
comparison between the gain changes measured by the lunar method and the terrestrial temporal radiometric calibration
method is performed and will be presented.
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Joe Steyn, George Tyc, Keith Beckett, Yoshi Hashida, "RapidEye constellation relative radiometric accuracy measurement using lunar images," Proc. SPIE 7474, Sensors, Systems, and Next-Generation Satellites XIII, 74740Y (22 September 2009); https://doi.org/10.1117/12.829728