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Coronal dynamics

  • V. M. Nakariakov

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

1 Citation (Scopus)

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 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.

Original languageEnglish
Title of host publicationKODAI SCHOOL ON SOLAR PHYSICS
Pages214-244
Number of pages31
DOIs
Publication statusPublished - 2007
EventKODAI SCHOOL ON SOLAR PHYSICS - Kodaikanal, India
Duration: 10 Dec 200622 Dec 2006

Publication series

NameAIP Conference Proceedings
Volume919
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceKODAI SCHOOL ON SOLAR PHYSICS
Country/TerritoryIndia
CityKodaikanal
Period10/12/0622/12/06

Keywords

  • Magnetohydrodynamic instabilities
  • Magnetohydrodynamic waves
  • Magnetohydrodynamics
  • Solar corona

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