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The role of drifts in diffusive shock accelerationThe role played by shock-associated drifts during the diffusive acceleration of charged particles at collisionless MHD shocks is evaluated. In the rest frame of the shock, the total energy gained by a particle is shown to result from two coupled acceleration mechanisms, the usual first-order Fermi mechanism and the drift mechanism. When averaged over a distribution of particles, the ratio of the drift-associated energy gain to the total energy is found to be independent of the total energy at a given theta1 (the angle between the shock normal and the unperturbed upstream magnetic field) in agreement with theoretical predictions. No evidence is found for drift-associated deceleration, suggesting that drifts always augment acceleration.
Document ID
19880036616
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Decker, R. B.
(Johns Hopkins University Laurel, MD, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 324
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
88A23843
Funding Number(s)
CONTRACT_GRANT: NAG5-782
CONTRACT_GRANT: N00024-85-C-5301
CONTRACT_GRANT: NSG-7055
Distribution Limits
Public
Copyright
Other

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