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Jetstream Formation through Inelastic Collisions

Published online by Cambridge University Press:  12 April 2016

David C. Baxter  and
William B. Thompson
David C. Baxter
Affiliation:
University of California, San Diego
William B. Thompson
Affiliation:
University of California, San Diego

Abstract

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An inelastic collision integral is used in a Boltzmann-type equation for a distribution of particles in Kepler orbits. A Fokker-Planck equation is found that leads to radial density clustering.

Type
Part II-Origin of Asteroids Interrelations with Comets, Meteorites, and Meteors
Information
International Astronomical Union Colloquium , Volume 12: Physical Studies of Minor Planets , 1971 , pp. 319 - 326
Copyright
Copyright © NASA 1971

References

Alfvén, H. 1970, Jet Streams in Space. Astrophys. Space Sci. 6, 161.CrossRefGoogle Scholar
Jeans, I.H. 1944, The Universe Around Us, pp. 237–238. Fourth ed., Cambridge Univ. Press. London.Google Scholar