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Localized properties of the zodiacal dust, by comparison of IRAS and of optical observations

✍ Scribed by A.C. Levasseur-Regourd; R. Dumont

Book ID
107936289
Publisher
Elsevier Science
Year
1986
Tongue
English
Weight
282 KB
Volume
6
Category
Article
ISSN
0273-1177

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Using the Moon to occult the Sun, the Clementine spacecraft used its navigation cameras to map the inner zodiacal light at optical wavelengths over elongations of 3 ∼ < ∼ < 30 β€’ from the Sun. This surface brightness map is then used to infer the spatial distribution of interplanetary dust over helio