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Magnetohydrodynamic waves and coronal seismology: an overview of recent results

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De Moortel, I. and Nakariakov, Valery M.. (2012) Magnetohydrodynamic waves and coronal seismology: an overview of recent results. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 370 (No. 1970). pp. 3193-3216. ISSN 1364-503X

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Official URL: http://dx.doi.org/10.1098/rsta.2011.0640

Abstract

Recent observations have revealed that magnetohydrodynamic (MHD) waves and oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a brief review of some aspects of MHD waves and coronal seismology that have recently been the focus of intense debate or are newly emerging. In particular, we focus on four topics: (i) the current controversy surrounding propagating intensity perturbations along coronal loops, (ii) the interpretation of propagating transverse loop oscillations, (iii) the ongoing search for coronal (torsional) Alfvén waves, and (iv) the rapidly developing topic of quasi-periodic pulsations in solar flares.

Item Type: Journal Article
Divisions: Faculty of Science > Physics
Journal or Publication Title: Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Publisher: The Royal Society
ISSN: 1364-503X
Date: 2012
Volume: Vol. 370
Number: No. 1970
Page Range: pp. 3193-3216
Identification Number: 10.1098/rsta.2011.0640
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
URI: http://wrap.warwick.ac.uk/id/eprint/47931

Data sourced from Thomson Reuters' Web of Knowledge

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