MHD oscillations in solar and stellar coronae: Current results and perspectives
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 0273-1177Full text not available from this repository.
Official URL: http://dx.doi.org/10.1016/j.asr.2007.01.044
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|
|Number of Pages:||10|
|Page Range:||pp. 1804-1813|
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