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A Statistical Study of CME Plasma FlowsMany studies of the interplanetary manifestations of coronal mass ejections (CMEs) have focused on the shock driver gas or on the regions that display a flux-rope magnetic topology. Somewhat less attention has been paid to investigating how the solar wind returns to its ambient, pre-CME condition.
Document ID
20060041730
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Goldstein, R.
Neugebauer, M.
Clay, D.
Date Acquired
August 23, 2013
Publication Date
November 1, 1997
Subject Category
Plasma Physics
Distribution Limits
Public
Copyright
Other
Keywords
Coronal Mass Ejections Flux-rope Plasma Flows

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