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Axisymmetric ideal MHD stellar wind flowThe ideal MHD equations are reduced to a single equation under the assumption of axisymmetric flow. A variational principle from which the equation is derivable is given. The characteristics of the equation are briefly discussed. The equation is used to rederive the theorem of Gussenhoven and Carovillano.
Document ID
19780057145
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Heinemann, M. (Boston College Chestnut Hill, Mass., United States)
Olbert, S. (MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
June 1, 1978
Publication Information
Publication: Journal of Geophysical Research
Volume: 83
Subject Category
Astrophysics
Accession Number
78A41054
Funding Number(s)
CONTRACT_GRANT: NSF ATM-77-11690
CONTRACT_GRANT: NGL-22-009-015
Distribution Limits
Public
Copyright
Other

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