Coronal dynamics

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Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..919..214n&link_type=abstract

KODAI SCHOOL ON SOLAR PHYSICS. AIP Conference Proceedings, Volume 919, pp. 214-244 (2007).

Physics

1

Corona, Magnetohydrodynamics And Plasmas

Scientific paper

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 modern 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.

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