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quasi-linear theory and transport theoryThe theory of energetic particle scattering by magnetostatic fluctuations is reviewed in so far as it fails to produce the rigidity-independent mean-free-paths observed. Basic aspects of interplanetary magnetic field fluctuations are reviewed with emphasis placed on the existence of dissipation range spectra at high wavenumbers. These spectra are then incorporated into existing theories for resonant magnetostatic scattering and are shown to yield infinite mean-free-paths. Nonresonant scattering in the form of magnetic mirroring is examined and offered as a partial solution to the magnetostatic problem. In the process, mean-free-paths are obtained in good agreement with observations in the interplanetary medium at 1 AU and upstream of planetary bow shocks.
Document ID
19930055986
Document Type
Conference Paper
Authors
Smith, Charles W.
(Bartol Research Inst. Newark, DE, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93-39976 16-93)
Subject Category
PLASMA PHYSICS
Funding Number(s)
CONTRACT_GRANT: JPL-959167
CONTRACT_GRANT: NAGW-2076
CONTRACT_GRANT: NAGW-1637
Distribution Limits
Public
Copyright
Other

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IDRelationTitle19930055979Analytic PrimaryParticle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991