Pascoe, D. J. (David J.) (2014) Numerical simulations for MHD coronal seismology. Research in Astronomy and Astrophysics, Volume 14 (Number 7). pp. 805-830. doi:10.1088/1674-4527/14/7/004 ISSN 1674-4527.

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Abstract

Magnetohydrodynamic (MHD) processes are important for the transfer of energy over large scales in plasmas and so are essential to understanding most forms of dynamical activity in the solar atmosphere. The introduction of transverse structuring into models for the corona modifies the behavior of MHD waves through processes such as dispersion and mode coupling. Exploiting our understanding of MHD waves with the diagnostic tool of coronal seismology relies upon the development of sufficiently detailed models to account for all the features in observations. The development of realistic models appropriate for highly structured and dynamical plasmas is often beyond the domain of simple mathematical analysis and so numerical methods are employed. This paper reviews recent numerical results for seismology of the solar corona using MHD.

Item Type:	Journal Article
Divisions:	Faculty of Science, Engineering and Medicine > Science > Physics
Journal or Publication Title:	Research in Astronomy and Astrophysics
Publisher:	IoP Publishing
ISSN:	1674-4527
Official Date:	July 2014
Dates:	Date Event July 2014 Published 14 April 2014 Accepted 16 March 2014 Submitted
Volume:	Volume 14
Number:	Number 7
Page Range:	pp. 805-830
DOI:	10.1088/1674-4527/14/7/004
Status:	Peer Reviewed
Publication Status:	Published
Access rights to Published version:	Restricted or Subscription Access

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