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Shock drift accelerationThis is a review of the fundamental physics of the interactions of charged particles treated individually while they interact with fast mode magnetohydrodynamic shocks. Numerical simulation and analytical theory are used to develop predictions of the expected characteristics of this process strong upstream anisotropies directed along the magnetic field and downstream anisotropies tending to be peaked more perpendicular to the field; relatively more of the enhancement of higher-energy particles occurring upstream; sensitive dependence on shock normal to magnetic field angle of the efficiency of energization. Observations which display all of the above characteristics are reviewed. Also discussed is the relationship of shock drift acceleration to the models for stochastic transport of charged particles in the vicinity of shocks. Extensions of this work in both the observational and theoretical approaches are discussed.
Document ID
19870038071
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Armstrong, Thomas P.
(Kansas, University Lawrence, United States)
Pesses, Mark E.
(NASA Goddard Space Flight Center Greenbelt; Applied Research Corp., Landover, MD, United States)
Decker, Robert B.
(Johns Hopkins University Laurel, MD, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1985
Subject Category
Astrophysics
Accession Number
87A25345
Funding Number(s)
CONTRACT_GRANT: NAS5-28407
CONTRACT_GRANT: NSF ATM-83-05537
Distribution Limits
Public
Copyright
Other

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