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Alfven solitons in the solar windA nonlinear Alfven soliton solution of the MHD equations is presented. This solution represents the final state of modulationally unstable Alfven waves. A model of the expected turbulent spectrum due to a collection of such solitons is briefly described.
Document ID
19840005007
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ovenden, C. (London Univ.)
Schwartz, S. J. (London Univ.)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: JPL Solar Wind Five
Subject Category
Solar Physics
Accession Number
84N13075
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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