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Monte Carlo simulation of collisionless shocks showing preferential acceleration of high A/Z particlesA collisionless quasi-parallel shock is simulated by Monte Carlo techniques. The scattering of all velocity particles from thermal to high energy is assumed to occur so that the mean free path is directly proportional to velocity times the mass-to-charge-ratio, and inversely proporational to the plasma density. The shock profile and velocity spectra are obtained, showing preferential acceleration of high A/Z particles relative to protons. The inclusion of the back pressure of the scattering particles on the inflowing plasma produces a smoothing of the shock profile, which implies that the spectra are steeper than for a discontinuous shock.
Document ID
19820035288
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ellison, D. C.
(NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics, Greenbelt, MD; Catholic University of America, Washington, , United States)
Jones, F. C.
(NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics, Greenbelt, MD, United States)
Eichler, D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1981
Subject Category
Space Radiation
Accession Number
82A18823
Funding Number(s)
CONTRACT_GRANT: NSF AST-80-02673
Distribution Limits
Public
Copyright
Other

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