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The Solar Wind-Inner HeliosphereThe Solar wind in the inner heliosphere, inside approximately 5 AU, has been almost fully characterized by the addition of the high heliographic latitude Ulysses mission to the many low latitude inner heliosphere missions that preceded it. The two major omissions are the high latitude solar wind at solar maximum, which will be measured during the second Ulysses polar passages, and the solar wind near the Sun, which could be analyzed by a Solar Probe mission. Here, existing knowledge of the global solar wind in the inner heliosphere is summarized in the context of the new results from Ulysses.
Document ID
19990017745
Acquisition Source
Marshall Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Suess, S. T.
(NASA Marshall Space Flight Center Huntsville, AL United States)
Phillips, J. L.
(Los Alamos National Lab. NM United States)
McComas, D. J.
(Los Alamos National Lab. NM United States)
Goldstein, B. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Neugebauer, M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Nerney, S.
(Ohio Univ. Lancaster, OH United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1998
Publication Information
Publication: Space Science Reviews
Publisher: Kluwer Academic Publishers
Volume: 83
ISSN: 0038-6308
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-6308
Distribution Limits
Public
Copyright
Other

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