Botha, GJJ, Rucklidge, AM and Hurlburt, NE (2004) Dynamics of convection around axisymmetric magnetic flux tubes. In: 31st EPS Conference on Plasma Physics, 28 Jun - 02 Jul 2004, London.
Abstract
Pores and sunspots are some of the magnetic features observed on the surface of the solar photosphere. In this presentation numerical models are used to study idealised pores and sunspots. Vertical flux tubes are placed in a compressable convecting photosphere in an axisymmetric cylindrical box with radius up to 4 times its depth [1].
Metadata
Item Type: | Conference or Workshop Item |
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Authors/Creators: |
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Keywords: | Pores; sunspots. |
Dates: |
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Institution: | The University of Leeds |
Academic Units: | The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds) |
Depositing User: | Symplectic Publications |
Date Deposited: | 29 Jul 2019 10:11 |
Last Modified: | 29 Jul 2019 10:11 |
Published Version: | http://epsppd.epfl.ch/London/pdf/P2_062.pdf |
Status: | Published |
Publisher: | Dynamics of convection around axisymmetric magnetc flux tubes |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:84734 |