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Heliospheric Plasma Sheet and Coronal StreamersIn-situ measurements of solar wind plasma and magnetic field between 0.3 and 1 AU are used to investigate the structure of the heliospheric plasma sheet, namely the region of enhanced plasma density that surrounds the helioshperic current sheet.
Document ID
20060041666
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bavassano, B.
Woo, R.
Bruno, R.
Date Acquired
August 23, 2013
Publication Date
January 1, 1997
Publication Information
Publication: Geophysical Research Letters
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar wind

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