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Comments on the photospheric dynamo model of Henoux and SomovA detailed model for a photospheric dynamo has been presented by Henoux and Somov (1987), who used the three-fluid model to treat the properties of the weakly ionized plasma. Only the equations for the two ionized components were solved. The equation for the neutral component is considered, and it is argued that the model is unacceptable becaused of an implied impossibly large unbalanced stress on the neutral gas. It is argued more generally that all existing photospheric dynamo models are untenable.
Document ID
19890064572
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Melrose, D. B.
(Sydney Univ. Australia)
Khan, J. I.
(Sydney, University Australia)
Date Acquired
August 14, 2013
Publication Date
July 1, 1989
Publication Information
Publication: Astronomy and Astrophysics
Volume: 219
Issue: 2-Jan
ISSN: 0004-6361
Subject Category
Solar Physics
Accession Number
89A51943
Funding Number(s)
CONTRACT_GRANT: NAGW-864
CONTRACT_GRANT: NSF ATM-86-19853
Distribution Limits
Public
Copyright
Other

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