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An Estimate of Solar Wind Velocity Profiles in a Coronal Hole and a Coronal Streamer Area (6-40 R(radius symbol)Total electron content data obtained from the Ulysses Solar Corona Experiment (SCE) in 1991 were used to select two data sets, one associated with a coronal hole and the other with coronal streamer crossings. (This is largely equatorial data shortly after solar maximum.) The solar wind velocity profile is estimated for these areas.
Document ID
20060037421
Document Type
Conference Paper
External Source(s)
Authors
Patzold, M.
Tsurutani, B. T.
Bird, M. K.
Date Acquired
August 23, 2013
Publication Date
January 1, 1995
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar corona solar wind coronal streamer Ulysses