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Coronal dynamics

By V. M. (Valery M.) Nakariakov

Abstract

The lectures present the foundation of solar coronal physics with the main emphasis on the MHD theory and on wave and oscillatory phenomena. We discuss major challenges of the modem coronal physics; the main plasma structures observed in the corona and the conditions for their equilibrium; phenomenology of large scale long period oscillatory coronal phenomena and their theoretical modelling as MHD waves. The possibility of the remote diagnostics of coronal plasmas with the use of MHD oscillations is demonstrated

Topics: QC
Publisher: American Institute of Physics
OAI identifier: oai:wrap.warwick.ac.uk:31028
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