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The Three-Dimenstional Solar Wind at Solar Activity MinimumIn late 1997, the Ulysses spacecraft completed its first orbit around the Sun, observing the properties of the heliosphere at all latitudes between 80 degrees South and 80 degrees North. Because the mission occurred during a period of near-minimum solar activity, the configuration of the solar wind and interplanetary magnetic field were particularly simple, thus allowing confident comparisons between the properties of the polar corona observed by instruments of the Spartan and SOHO spacecraft and the resulting properties of the solar wind.
Document ID
20060034698
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Neugebauer, M.
Date Acquired
August 23, 2013
Publication Date
May 5, 1998
Publication Information
Publication: Reviews of Geophysics
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Other
Keywords
Solar Wind Ulysses Solar Activity polar corona

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