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An Estimate of Solar Wind Velocity Profiles in a Coronal Hole and Coronal Streamer Area (6-40R)Using the total electron content data obtained by the Ulysses Solar Corona Experiment during the first solar conjunction in summer 1991 (Bird et al., 1994), an estimate is presented of solar wind velocity profiles in a coronal hole and a coronal streamer area in the range between 6 and 40 solar radii.
Document ID
20060042050
Acquisition Source
Jet Propulsion Laboratory
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 Wind

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