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Ion isotropy and fluctuations in the solar windThe effects of measured fluctuations, with only general considerations as to their source, are considered. Data from interplanetary scintillations and fluctuations in plasma density provided data on electric fields, while fluctuations in magnetic fields are measured directly. Data from the unified radio and plasma experiment (URAP) on Ulysses is used to fill in higher frequency ranges, to assess the variations in the fluctuations with time and space, and to help to identify wave modes. It is shown that electric field fluctuations are of the right order of magnitude to maintain ion isotropy.
Document ID
19990056461
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Kellogg, Paul J.
(Minnesota Univ. Minneapolis, MN United States)
Lin, Naiguo
(Minnesota Univ. Minneapolis, MN United States)
Date Acquired
August 19, 2013
Publication Date
December 1, 1997
Publication Information
Publication: Proceedings of the 31st ESALB Symposium on Correlated Phenomena at the Sun, in the Heliosphere and in Geospace
Subject Category
Solar Physics
Funding Number(s)
CONTRACT_GRANT: NAS5-32994
Distribution Limits
Public
Copyright
Other
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