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The Optical Properties of Interplanetary Dust

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Origin and Evolution of Interplanetary Dust

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 173))

Abstract

After briefly evaluating the observations of the Zodiacal Light and F-corona, we review the laboratory results on the light scattering by dust particles and the various theories which have been recently proposed. We then discuss the optical properties of the dust with emphasis on the phase function, the polarization, the color, the albedo and the local enhancement in the Gegenschein.

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© 1991 Springer Science+Business Media Dordrecht

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Lamy, P.L., Perrin, J.M. (1991). The Optical Properties of Interplanetary Dust. In: Levasseur-Regourd, A.C., Hasegawa, H. (eds) Origin and Evolution of Interplanetary Dust. Astrophysics and Space Science Library, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3640-2_34

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  • DOI: https://doi.org/10.1007/978-94-011-3640-2_34

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5616-8

  • Online ISBN: 978-94-011-3640-2

  • eBook Packages: Springer Book Archive

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