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Hydromagnetic wave dissipation in molecular cloudsThe damping of long wavelength, hydromagnetic waves in molecular cloud environments is studied with the aim of determining whether the supersonic motions observed in such clouds are likely to be due to the waves. It is found that Alfven waves propagating parallel to the average magnetic field are the longest lived wave modes. Such waves can typically survive for as long as one-million years if the wavelength is as long as a few tenths of a pc and the magnetic field is 0.1-1 milligauss. Nonlinear steepening of the waves followed by ion-neutral friction in the steepened wave profiles appears to be the most effective damping mechanism.
Document ID
19830060401
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Zweibel, E. G.
(Colorado, University Boulder, CO; California, University, Berkeley, CA, United States)
Josafatsson, K.
(Colorado, University Boulder, CO, United States)
Date Acquired
August 11, 2013
Publication Date
July 15, 1983
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 270
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
83A41619
Funding Number(s)
CONTRACT_GRANT: NSG-7626
CONTRACT_GRANT: NAS5-26535
Distribution Limits
Public
Copyright
Other

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