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An Infra-Red model of the zodiacal emission

✍ Scribed by J. Tigg; G. Pearce

Publisher
Springer Netherlands
Year
1988
Tongue
English
Weight
243 KB
Volume
43
Category
Article
ISSN
1573-0794

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✦ Synopsis

The Infra-Red Astronomical Satellite (IRAS) observations ofthe zodiacal dust emission are used to fit the dust grain composition and distribution in the ecliptical plane. We obtain a good fit to the data for a density distribution of black-body grains given by p = pr a 66"0s(' wR) for r > 0.87R and r < 30R.

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