Magnetohydrodynamic waves and coronal seismology: an overview of recent results
De Moortel, I. and Nakariakov, V. M. (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 1364-503XFull text not available from this repository.
Official URL: http://dx.doi.org/10.1098/rsta.2011.0640
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|
|Page Range:||pp. 3193-3216|
|Access rights to Published version:||Restricted or Subscription Access|
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