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Siphon flows in isolated magnetic flux tubes. II - Adiabatic flowsThis paper extends the study of steady siphon flows in isolated magnetic flux tubes surrounded by field-free gas to the case of adiabatic flows. The basic equations governing steady adiabatic siphon flows in a thin, isolated magnetic flux tube are summarized, and qualitative features of adiabatic flows in elevated, arched flux tubes are discussed. The equations are then cast in nondimensional form and the results of numerical computations of adiabatic siphon flows in arched flux tubes are presented along with comparisons between isothermal and adiabatic flows. The effects of making the interior of the flux tube hotter or colder than the surrounding atmosphere at the upstream footpoint of the arch is considered. In this case, is it found that the adiabatic flows are qualitatively similar to the isothermal flows, with adiabatic cooling producing quantitative differences. Critical flows can produce a bulge point in the rising part of the arch and a concentration of magnetic flux above the bulge point.
Document ID
19890042540
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Montesinos, Benjamin
(Oxford Univ. Oxford, United Kingdom)
Thomas, John H.
(Oxford University United Kingdom)
Date Acquired
August 14, 2013
Publication Date
February 15, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 337
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
89A29911
Funding Number(s)
CONTRACT_GRANT: NSG-7562
CONTRACT_GRANT: NAG5-934
Distribution Limits
Public
Copyright
Other

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