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The structure of untwisted magnetic flux tubesWhile most previous investigations have concentrated on slender flux tubes, the present study of the equilibrium structure of an axisymmetric magnetic flux tube, confined by an external pressure that varies along the length of the tube, explores the properties of thick tubes in order to establish the degree to which slender tube theory is valid. It is found that slender flux tube results may in some cases give no indication of thick tube behavior in a nonuniform atmosphere. Depending on boundary conditions applied at the ends of the tube, it may expand or contract upon entering a region of increasing pressure. Rather than expanding indefinitely, the tube surface may form a cusped shape when a point of external pressure on the tube surface falls to equality with the internal pressure. Numerical solutions for an initially uniform tube give smaller expansions than would be expected from slender tube theory.
Document ID
19830031766
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Browning, P. K.
(Saint Andrew's Univ. United Kingdom)
Priest, E. R.
(St. Andrews, University St. Andrews, United Kingdom)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Publication Information
Publication: Geophysical and Astrophysical Fluid Dynamics
Volume: 21
Issue: 3-4,
Subject Category
Solar Physics
Accession Number
83A12984
Funding Number(s)
CONTRACT_GRANT: NAGW-76
Distribution Limits
Public
Copyright
Other

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