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The Latitudinal Distribution of Solar Wind Magnetic HolesUsing the fast latitude scan period of the Ulysses spacecraft, the occurrence of magnetic holes in the solar wind is investigated from -80 degrees to +80 degrees helio-latitude.
Document ID
20060032635
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/14291
Authors
Winterhalter, D.
Smith, E.
Neugebauer, M.
Goldstein, B.
Tsurutani, B.
Date Acquired
August 23, 2013
Publication Date
January 1, 2000
Publication Information
Publication: Geophysical Research Letters
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
Solar Wind Plasma

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