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The Source of Alfven Waves That Heat the Solar CoronaWe suggest a source for high-frequency Alfven waves invoked in coronal heating and acceleration of the solar wind. The source is associated with small-scale magnetic loops in the chromospheric network.
Document ID
20060041108
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/18986
Authors
Ruzmaikin, A.
Berger, M. A.
Date Acquired
August 23, 2013
Publication Date
January 1, 1998
Publication Information
Publication: Geophysical Research Letters
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
Alfven Waves Heat Solar Corona solar wind solar wind

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