Development of structure in pores and sunspots: flows around axisymmetric magnetic flux tubes

Hurlburt, N.E. and Rucklidge, A.M. (2000) Development of structure in pores and sunspots: flows around axisymmetric magnetic flux tubes. Monthly Notices of the Royal Astronomical Society, 314 (4). pp. 793-806. ISSN 0035-8711

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Authors/Creators:
  • Hurlburt, N.E.
  • Rucklidge, A.M.
Copyright, Publisher and Additional Information: Copyright © 2000 Royal Astronomical Society. This is an author produced version of an article published in Monthly Notices of the Royal Astronomical Society. This paper has been peer-reviewed but does not include the final publisher proof-corrections or journal pagination.The definitive version is available at www.blackwell-synergy.com.
Keywords: convection, MHD, sun, interior, magnetic fields, sunspots
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Maths and Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: A. M. Rucklidge
Date Deposited: 10 Feb 2006
Last Modified: 27 Oct 2016 16:40
Published Version: http://www.blackwell-synergy.com/doi/abs/10.1046/j...
Status: Published
Refereed: Yes
Identification Number: https://doi.org/10.1046/j.1365-8711.2000.03407.x

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