Abstract
The need for long term global data sets to enable quantitative studies of changes in the Earth’s climate leads directly to a requirement for a radiometric calibration source that is stable over several decades (and possibly several centuries) to levels of better than one part in a thousand, that can be readily used on-orbit and that is suitable for inter-comparison of a wide variety of imagng radiometers. For the visible through shortwave-infrared portion of the electromagnetic spectrum the moon meets this requirement. It’s surface is stable over thousands of years, the sun’s illumination is well characterized, and, if care is taken to account for changes in phase and libration, it can be used for radiometric calibration, calibration transfer and intercomparison of sensors.
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© 2006 Tsinghua University Press, Beijing and Springer-Verlag GmbH Berlin Heidelberg
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Barnes, W., Xiong, X., Eplee, R., Sun, J., Lyu, CH. (2006). Use of the Moon for Calibration and Characterization of MODIS, SeaWiFS, and VIRS. In: Qu, J.J., Gao, W., Kafatos, M., Murphy, R.E., Salomonson, V.V. (eds) Earth Science Satellite Remote Sensing. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-37294-3_6
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DOI: https://doi.org/10.1007/978-3-540-37294-3_6
Publisher Name: Springer, Berlin, Heidelberg
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