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Zodiacal Light Models with a Bimodal Population

Published online by Cambridge University Press:  14 August 2015

P.L. Lamy
Affiliation:
Laboratoire d'Astronomie Spatiale, Marseille, France
J.M. Perrin
Affiliation:
Laboratoire d'Astronomie Spatiale, Marseille, France

Abstract

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The compatibility of the observed properties of the zodiacal light with a model made of two populations is investigated. It is shown that a population of submicron grains may play a non-negligible role.

Type
I: Zodiacal Light - Measurements and Models
Copyright
Copyright © Reidel 1980 

References

Bourrely, C., Chiappetta, P.: 1979, submitted to Astron. Astrophys. Google Scholar
Brownlee, D.E., Hörz, F., Tormandl’, D.A., Hodge, P.W.: 1976, NASA SP-393, p.962 CrossRefGoogle Scholar
Cook, A.F.: 1978, Icarus 33 p.349 Google Scholar
Fechtig, H., Gentner, W., Hartung, J.B., Nagel, K., Neukum, G., Schneider, E., and Storzer, D.: 1974, Proc. Soviet American Conf. Cosmochemistry Moon and Planets, Moscow (NASA SP-370, 1976), pp.585604 Google Scholar
Fried, J.W.: 1978, Astron. Astrophys. 68 p.259 Google Scholar
Giese, R.M., Grün, F.: 1976, Lecture Notes in Physics 48 p.135 Google Scholar
Giese, R.M., Weiss, K., Zerull, R.H., Ono, T.: 1978, Astron. Astrophys. Google Scholar
Johnson, T.V., Fanale, F.P.: J. Geophys. Res. 78 p.8507 Google Scholar
Leinert, C., Link, H., Pitz, E., Giese, R.H.: 1976, Astron. Astrophys. 47 p.221 Google Scholar
Le Sergeant, L.B., Lamy, P.L.: 1978, Nature 276 p.800 CrossRefGoogle Scholar
Morrison, D.A., Zinner, E.: 1977, Proc. Lunar Sci. Conf. VIII, p.841 Google Scholar