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Solar Wind Speed Structure in the Inner Corona at 3-12R(sub)OEstimates of solar wind speed obtained by Armstrong et al. [1986] based on 1983 VLA multiple-station intensity scintillation measurements inside 12 R(sub)O have been compared with white light coronagraph measurements.
Document ID
20060036922
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/29141
Authors
Woo, R.
Date Acquired
August 23, 2013
Publication Date
May 1, 1995
Publication Information
Publication: EOS
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
solar wind corona radio astronomy

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