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5.5 Temperature Distribution and Lifetime of Interplanetary Ice Grains

Published online by Cambridge University Press:  12 April 2016

Ph. Lamy  and
M.F. Jousselme
Ph. Lamy
Affiliation:
Laboratoire d’Astronomie Spatiale, Marseille
M.F. Jousselme
Affiliation:
Laboratoire d’Astronomie Spatiale, Marseille

Abstract

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An improved solution of the temperature distribution of interplanetary ice grains is presented using the refractive index measured at 100° K. The efficiency factors for absorption are obtained from Mie theory and the calculation is carried out for micronic and submicronic grains at 50, 100 and 150° K; corresponding lifetimes are given.

Type
5 Dynamics and Evolution
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 443 - 447
Copyright
Copyright © Springer-Verlag 1976

References

Allen, C.W. 1973, Astrophysical Quantities, third Edition, The Athlone Press, London.Google Scholar
Irvine, W.M. and Pollack, J.B. 1968, Icarus 8, 324.CrossRefGoogle Scholar
Isobe, S. 1971, Ann. Tokyo Astron. Obs. 12, 263.Google Scholar
Jancso, G., Pupezin, J. and Van Hook, W.A. 1970, J. Phys. Chem. 74, 2984.CrossRefGoogle Scholar
Labs, D. and Neckel, H. 1968, Z. Astrophys. 69, 1.Google Scholar
Lamy, Ph.L. 1974, Astron. Astrophys. 35, 197.Google Scholar
Mukai, T. and Mukai, S. 1973, Publ. Astron. Soc. Japan 25, 481.Google Scholar