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Magnetohydrodynamic waves and coronal seismology: an overview of recent results
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Recent observations have revealed that 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 which 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)doi:10.1098/rsta.2011.0640 pmid:22665899 fatcat:2qvrqgnv4jdj3jgkcsp7vljov4