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Electron heating in quasi-perpendicular shocks - A Monte Carlo simulationTo study the problem of electron heating in quasi-perpendicular shocks, under the combined effects of 'reversible' motion, in the shock electric potential and magnetic field, and wave-particle interactions a diffusion equation was derived, in the drift (adiabatic) approximation and it was solved by using a Monte Carlo method. The results show that most of the observations can be explained within this framework. The simulation has also definitively shown that the electron parallel temperature is determined by the dc electromagnetic field and not by any wave particle induced heating. Wave-particle interactions are effective in smoothing out the large gradients in phase space produced by the 'reversible' motion of the electrons, thus producing a 'cooling' of the electrons. Some constraints on the wave-particle interaction process may be obtained from a detailed comparison between the simulation and observations. In particular, it appears that the adiabatic approximation must be violated in order to explain the observed evolution of the perpendicular temperature.
Document ID
19900063364
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Veltri, Pierluigi
(Calabria, Universita Arcavacata di Rende, Italy)
Mangeney, Andre
(Paris Observatoire, Meudon, France)
Scudder, Jack D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1990
Publication Information
Publication: Journal of Geophysical Research
Volume: 95
ISSN: 0148-0227
Subject Category
Plasma Physics
Accession Number
90A50419
Distribution Limits
Public
Copyright
Other

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