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Origins of the Slow and the Ubiquitous Fast Solar WindWe present in this letter the first coordinated radio occultation measurements and ultraviolet observations of the inner corona below 5.5 Rs, obtained during the Galileo solar conjunction in January 1997, to establish the origin of the slow wind.
Document ID
20060041718
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/22453
Authors
Korendyke, Noci C.
Habbal, S. R.
Date Acquired
August 23, 2013
Publication Date
July 23, 1997
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
Solar Wind

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