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Optical Models of the Three Dimensional Distribution of Interplanetary Dust

Published online by Cambridge University Press:  12 April 2016

R.H. Giese ,
G. Kinateder ,
B. Kneissel  and
U. Rittich
R.H. Giese
Affiliation:
Ruhr-Universität Bochum, Bereich Extraterrestrische Physik P.O.Box 10 21 48 4630 Bochum 1, F.R.G.
G. Kinateder
Affiliation:
Ruhr-Universität Bochum, Bereich Extraterrestrische Physik P.O.Box 10 21 48 4630 Bochum 1, F.R.G.
B. Kneissel
Affiliation:
Ruhr-Universität Bochum, Bereich Extraterrestrische Physik P.O.Box 10 21 48 4630 Bochum 1, F.R.G.
U. Rittich
Affiliation:
Ruhr-Universität Bochum, Bereich Extraterrestrische Physik P.O.Box 10 21 48 4630 Bochum 1, F.R.G.

Abstract

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Several models of three dimensional distributions of the interplanetary dust number densities are compared with observational values. It is shown that a comparatively satisfying fit can be achieved by distributions similar to the “Sombrero-Model” of Dumont and that multilobe models as recently proposed by Buitrago et al. can be rejected due to discrepancies with rocket photometry of the inner zodiacal light.

Type
IV. Optical Studies of Dust
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 255 - 259
Copyright
Copyright © Reidel 1985

References

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