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Jetstream Formation through Inelastic Collisions
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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