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Title: On the emergence of toroidal flux tubes: general dynamics and comparisons with the cylinder model
Authors: MacTaggart, David
Hood, Alan W.
Affiliation: University of Abertay Dundee. School of Computing & Engineering Systems
Keywords: Magnetic fields
Magnetohydrodynamics (MHD)
Numerical simulation
Flux emergence
Issue Date: Nov-2009
Publisher: EDP Sciences
Type: Journal Article
Refereed: peer-reviewed
Rights: This is the published version of this article. Reproduced with permission from the publisher. Published version (c)EDP Sciences, available from http://dx.doi.org/10.1051/0004-6361/200912930 and http://www.aanda.org/
Citation: MacTaggart, D. and Hood, A.W. 2009. On the emergence of toroidal flux tubes: general dynamics and comparisons with the cylinder model. Astronomy and Astrophysics. 507(2): pp.995-1004. Available from http://dx.doi.org/10.1051/0004-6361/200912930
Abstract: Aims. In this paper we study the dynamics of toroidal flux tubes emerging from the solar interior, through the photosphere and into the corona. Many previous theoretical studies of flux emergence use a twisted cylindrical tube in the solar interior as the initial condition. Important insights can be gained from this model, however, it does have shortcomings. The axis of the tube never fully emerges as dense plasma becomes trapped in magnetic dips and restrains its ascent. Also, since the entire tube is buoyant, the main photospheric footpoints (sunspots) continually drift apart. These problems make it difficult to produce a convincing sunspot pair.We aim to address these problems by considering a different initial condition, namely a toroidal flux tube. Methods. We perform numerical experiments and solve the 3D MHD equations. The dynamics are investigated through a range of initial field strengths and twists. Results. The experiments demonstrate that the emergence of toroidal flux tubes is highly dynamic and exhibits a rich variety of behaviour. In answer to the aims, however, if the initial field strength is strong enough, the axis of the tube can fully emerge. Also, the sunspot pair does not continually drift apart. Instead, its maximum separation is the diameter of the original toroidal tube.
URI: http://hdl.handle.net/10373/1156
ISSN: 0004-6361
Appears in Collections:Computing & Engineering Systems Collection

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