Hurlburt, N.E., Matthews, P.C. and Rucklidge, A.M. (2000) Solar magnetoconvection. Solar Physics, 192 (1-2). pp. 109-118. ISSN 1573-093XFull text available as:
Available under licence : See the attached licence file.
In recent years the study of how magnetic fields interact with thermal convection in the Sun has made significant advances. These are largely due to the rapidly increasing computer power and its application to more physically relevant parameters regimes and to more realistic physics and geometry in numerical models. Here we present a survey of recent results following one line of investigations and discuss and compare the results of these with observed phenomena.
|Copyright, Publisher and Additional Information:||Copyright © 2000 Kluwer Academic Publishers.This is an author produced version of an article published in Solar Physics. This paper has been peer-reviewed but does not include the final publisher proof-corrections or journal pagination.|
|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:||04 Jun 2014 17:24|
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