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Spatial Distribution and Orbital Properties of Zodiacal Dust
Published online by Cambridge University Press: 12 April 2016
Abstract
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