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Analysis of Ulysses Dust Measurements within the Asteroid Belt

Published online by Cambridge University Press:  31 July 2018

I. Mann ,
M. Wilck  and
E. Grün
I. Mann
Affiliation:
Max-Planck-Institut für Aeronomie, Postfach 20, D-37189, Katlenburg-Lindau, Germany
M. Wilck
Affiliation:
Max-Planck-Institut für Aeronomie, Postfach 20, D-37189, Katlenburg-Lindau, Germany
E. Grün
Affiliation:
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, D-69029, Heidelberg, Germany

Abstract

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Results of Ulysses impact measurements are compared to Zodiacal cloud models. We discuss the influence of radiation pressure forces on particles of different size and composition and show its relevance for the understanding of impact measurements, and give an upper estimate for the dust density in an IRAS dust band.

Type
I. Dynamics of the Interplanetary Dust Cloud
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 19 - 22
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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