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Interplanetary Dust Close to the Sun
Published online by Cambridge University Press: 12 April 2016
Abstract
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