Coronal waves and oscillations

Valery M. Nakariakov

doi:10.1017/S174392130600250X

Coronal waves and oscillations

Valery M. Nakariakov

Research output: Contribution to journal › Article › peer-review

3 Citations (Scopus)

Abstract

Wave and oscillatory activity of the solar corona is confidently observed with modern imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and interpreted in terms of magnetohydrodynamic (MHD) wave theory. The review reflects the current trends in the observational study of coronal waves and oscillations, theoretical modelling of interaction of MHD waves with plasma structures, and implementation of the theoretical results for the mode identification. Also the use of MHD waves for remote diagnostics of coronal plasma, - MHD coronal seismology - is discussed.

Original language	English
Pages (from-to)	464-471
Number of pages	8
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	233
DOIs	https://doi.org/10.1017/S174392130600250X
Publication status	Published - Mar 2006

Keywords

(Magnetohydrodynamics:) MHD
Sun: corona
Sun: flares
Sun: magnetic fields
Sun: oscillations
Waves

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10.1017/S174392130600250X

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title = "Coronal waves and oscillations",

abstract = "Wave and oscillatory activity of the solar corona is confidently observed with modern imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and interpreted in terms of magnetohydrodynamic (MHD) wave theory. The review reflects the current trends in the observational study of coronal waves and oscillations, theoretical modelling of interaction of MHD waves with plasma structures, and implementation of the theoretical results for the mode identification. Also the use of MHD waves for remote diagnostics of coronal plasma, - MHD coronal seismology - is discussed.",

keywords = "(Magnetohydrodynamics:) MHD, Sun: corona, Sun: flares, Sun: magnetic fields, Sun: oscillations, Waves",

author = "Nakariakov, \{Valery M.\}",

year = "2006",

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doi = "10.1017/S174392130600250X",

language = "English",

volume = "2",

pages = "464--471",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

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TY - JOUR

T1 - Coronal waves and oscillations

AU - Nakariakov, Valery M.

PY - 2006/3

Y1 - 2006/3

N2 - Wave and oscillatory activity of the solar corona is confidently observed with modern imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and interpreted in terms of magnetohydrodynamic (MHD) wave theory. The review reflects the current trends in the observational study of coronal waves and oscillations, theoretical modelling of interaction of MHD waves with plasma structures, and implementation of the theoretical results for the mode identification. Also the use of MHD waves for remote diagnostics of coronal plasma, - MHD coronal seismology - is discussed.

AB - Wave and oscillatory activity of the solar corona is confidently observed with modern imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and interpreted in terms of magnetohydrodynamic (MHD) wave theory. The review reflects the current trends in the observational study of coronal waves and oscillations, theoretical modelling of interaction of MHD waves with plasma structures, and implementation of the theoretical results for the mode identification. Also the use of MHD waves for remote diagnostics of coronal plasma, - MHD coronal seismology - is discussed.

KW - (Magnetohydrodynamics:) MHD

KW - Sun: corona

KW - Sun: flares

KW - Sun: magnetic fields

KW - Sun: oscillations

KW - Waves

UR - https://www.scopus.com/pages/publications/33750684353

U2 - 10.1017/S174392130600250X

DO - 10.1017/S174392130600250X

M3 - Article

AN - SCOPUS:33750684353

SN - 1743-9213

VL - 2

SP - 464

EP - 471

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - 233

ER -

Coronal waves and oscillations

Abstract

Keywords

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