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Corotating shock structuresConsideration of observed interplanetary shocks leads to the conclusion that a corotating forward shock has not been unambiguously identified at 1 AU. A reverse shock identified in September 1967 is a likely candidate for a corotating structure.
Document ID
19730002069
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ogilvie, K. W. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Publication Information
Publication: Solar Wind
Subject Category
Space Radiation
Accession Number
73N10796
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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