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The turbulent generation of outward traveling Alfvenic fluctuations in the solar windFrom an analysis of the incompressible MHD equations, it is concluded that the frequent observation of outward propagating Alfvenic fluctuations in the solar wind can arise from early stages of in situ turbulent evolution, and need not reflect coronal processes.
Document ID
19830027714
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Matthaeus, W. H. (College of William and Mary Williamsburg, Va., United States)
Goldstein, M. L. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Montgomery, D. C. (College of William and Mary Williamsburg, Va., United States)
Date Acquired
September 4, 2013
Publication Date
July 1, 1983
Subject Category
Solar Physics
Report/Patent Number
NASA-TM-85073
NAS 1.15:85073
Accession Number
83N35985
Funding Number(s)
CONTRACT_GRANT: NSG-7416
CONTRACT_GRANT: DE-AS05-76ET-53045
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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