Nakariakov, V. M. (Valery M.). (2007) MHD oscillations in solar and stellar coronae: Current results and perspectives. ADVANCES IN SPACE RESEARCH, 39 (12). pp. 1804-1813. ISSN 0273-1177

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Abstract

Wave and oscillatory activity is observed with modern imaging and spectral instruments in the visible light, EUV, X-ray and radio bands in all parts of the solar corona. Magnetohydrodynamic (MHD) wave theory gives satisfactory interpretation of these phenomena in terms of MHD modes of coronal structures. The paper reviews the current trends in the observational study of coronal oscillations, recent development of theoretical modelling of MHD wave interaction with plasma structures, and implementation of the theoretical results for the mode identification. Also the use of MHD waves for remote diagnostics of coronal plasmas is discussed. In particular, the applicability of this method to the estimation of the coronal magnetic field is demonstrated. (c) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.

Item Type:	Journal Article
Subjects:	T Technology > TL Motor vehicles. Aeronautics. Astronautics Q Science > QB Astronomy Q Science > QE Geology Q Science > QC Physics
Journal or Publication Title:	ADVANCES IN SPACE RESEARCH
Publisher:	ELSEVIER SCI LTD
ISSN:	0273-1177
Official Date:	2007
Volume:	39
Number:	12
Number of Pages:	10
Page Range:	pp. 1804-1813
Identification Number:	10.1016/j.asr.2007.01.044
Publication Status:	Published
URI:	http://wrap.warwick.ac.uk/id/eprint/30529

Data sourced from Thomson Reuters' Web of Knowledge

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