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Zodiacal Light and the Spatial Density of Interplanetary Grains

Published online by Cambridge University Press:  12 April 2016

P.L. Lamy  and
J.M. Perrin
P.L. Lamy
Affiliation:
Laboratoire d’Astronomie Spatiale Marseille, France
J.M. Perrin
Affiliation:
Laboratoire d’Astronomie Spatiale Marseille, France

Abstract

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Using our model of light scattering by large rough grains, the compatibility of the observed properties of the zodiacal light with models of the spatial density of interplanetary grains is investigated. The agreement is not yet satisfactory and probably calls for further revision of the density distribution function. Our previous conclusion that submicronic grains gives a non-negligible contribution (Lamy and Perrin, 1980) is confirmed.

Type
IV. Optical Studies of Dust
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 239 - 243
Copyright
Copyright © Reidel 1985

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