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An Estimate of Solar Wind Density and Velocity Profiles in a Coronal Hole and a Coronal StreamerUsing the total electron content data obtained by the Ulysses Solar Corona Experiment (SCE) during the first solar conjunction in summer 1991, two data sets were selected, one associated with a coronal hole and the other associated with coronal streamer crossings. In order to determine coronal streamer density profiles, the electron content of the tracking passes embedded in a coronal streamer were corrected for the contributions from coronal hole densities.
Document ID
20060036859
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Patzold, M.
Tsurutani, B. T.
Bird, M. K.
Date Acquired
August 23, 2013
Publication Date
January 1, 1996
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
coronal density coronal velocity velocity profiles solar conjunction

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