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Interplanetary Dust Close to the Sun

Published online by Cambridge University Press:  12 April 2016

Ingrid Mann
Ingrid Mann*
Affiliation:
Ruhr-Universität Bochum*) D 4630 Bochum, RFA

Abstract

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The optical and infrared brightness of the Fraunhofer-corona is produced by light scattering at the zodiacal dust particles and by their thermal emission (see Koutchmy and Lamy 1985). It is modelled within the ecliptic (4 Ro ≤ ε ≤ 15 Ro)taking into account investigations of the global zodiacal dust cloud due to remote sensing and in situ experiments. The input of near solar dust to the corona brightness is discussed.

Type
Interplanetary Dust: Zodiacal Light and Optical Studies
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 187 - 190
Copyright
Copyright © Kluwer 1991

References

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