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Spatial Distribution and Orbital Properties of Zodiacal Dust

Published online by Cambridge University Press:  12 April 2016

Bernhard Kneißel  and
Ingrid Mann
Bernhard Kneißel
Affiliation:
Ruhr-Universität Bochum, D 4630 Bochum, RFA
Ingrid Mann
Affiliation:
Ruhr-Universität Bochum, D 4630 Bochum, RFA

Abstract

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Within the recent years the spatial distribution of Zodiacal dust has been subject to a variety of modelling approaches. Whereas models derived from observations in the visual range tend to demand for an increase of interplanetary matter above the solar poles (bulges), models based on infrared measurements and extended to small r seem to favor a decrease there (holes). The models are reviewed, and the dynamical structure implicated in the models is outlined.

Type
Interplanetary Dust: Zodiacal Light and Optical Studies
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 139 - 146
Copyright
Copyright © Kluwer 1991

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