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Computer simulation of Alfven resonance in a cylindrical, axially bounded flux tubeThe resonant absorption of Alfven waves in an axially bounded cylindrical flux tube is investigated in a dissipative MHD simulation. It is found that in an axially bounded flux tube, in contrast to an infinite periodic model, the resonant frequency is nearly independent of the poloidal component of the magnetic field. This is a consequence of the 'ballooning' structure of the resonant Alfven waves. The scaling with resistivity and viscosity of the width of the resonance layer, the dissipation rate, and the time for steady state absorption to occur, are all in agreement with theory.
Document ID
19900029195
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Strauss, H. R.
(New York Univ. New York, NY, United States)
Lawson, William S.
(New York University NY, United States)
Date Acquired
August 14, 2013
Publication Date
November 15, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 346
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
90A16250
Funding Number(s)
CONTRACT_GRANT: NAGW-781
Distribution Limits
Public
Copyright
Other

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