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Please use this identifier to cite or link to this item: http://hdl.handle.net/10373/1163

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Title: 3D MHD flux emergence experiments: idealised models and coronal interactions:
Authors: Hood, Alan W.
Archontis, Vasilis
MacTaggart, David
Affiliation: University of Abertay Dundee. School of Computing & Engineering Systems
Keywords: Magnetohydrodynamics (MHD)
Flux emergence
Numerical simulation
Solar corona
Issue Date: 2012
Publisher: Springer Verlag
Type: Journal Article
Refereed: peer-reviewed
Rights: Published version (c)Springer Verlag, available from http://dx.doi.org/10.1007/s11207-011-9745-2. The original publication is available at www.springerlink.com
Citation: Hood, A.W., Archontis, V. and MacTaggart, D. 2012. 3D MHD flux emergence experiments: idealised models and coronal interactions. Solar Physics. 278(1): pp.3-31. Available from http://dx.doi.org/10.1007/s11207-011-9745-2
Abstract: This paper reviews some of the many 3D numerical experiments of the emergence of magnetic fields from the solar interior and the subsequent interaction with the pre-existing coronal magnetic field. The models described here are idealised, in the sense that the internal energy equation only involves the adiabatic, Ohmic and viscous shock heating terms. However, provided the main aim is to investigate the dynamical evolution, this is adequate. Many interesting observational phenomena are explained by these models in a self-consistent manner.
URI: http://hdl.handle.net/10373/1163
ISSN: 0038-0938
Appears in Collections:Computing & Engineering Systems Collection

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