Physics
Scientific paper
Mar 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1635z&link_type=abstract
Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 635.
Physics
Zodiacal Light, Stratosphere, Clementine Spacecraft, Star Trackers, Ccd Cameras, Image Analysis, Calibrating, Hot Electrons, Pixels, Satellite Imagery, Brightness Distribution
Scientific paper
The zodiacal light, due to sunlight reflected off interplanetary dust grains, is a measure of their spatial density as a function of heliocentric distance and latitude. We have developed procedures to photometrically correct the brightness variations in the Clementine Corona and Zodiacal Light (CZL) photographs to true image brightnesses. The processing steps follow generally along the path described by Berry (1994); however, there are additional processing steps involved for the Clementine images. Careful corrections are necessary because of the dimness of the features that we wish to observe.
Cooper Lauren B.
Potter Andrew E.
Zook Herbert A.
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