An Infra-Red model of the zodiacal emiss
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J. Tigg; G. Pearce
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Article
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1988
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Springer Netherlands
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English
โ 243 KB
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