Theoretical aspects of MHD coronal seismology

V. M. Nakariakov

Theoretical aspects of MHD coronal seismology

V. M. Nakariakov

Research output: Contribution to journal › Conference article › peer-review

2 Citations (Scopus)

Abstract

The revolutionary breakthrough in observational detection of propagating and standing quasi-periodic disturbances of coronal plasma parameters, made in the EUV band with SOHO and TRACE mission instruments, together with confident interpretation of these phenomena in terms of magnetohydrodynamic (MHD) waves, has given rise to MHD coronal seismology. This review presents the theoretical background of these studies and reflects current trends in the development of the theory. Solar corona, loop oscillations, MHD waves.

Original language	English
Pages (from-to)	407-416
Number of pages	10
Journal	European Space Agency, (Special Publication) ESA SP
Issue number	547
Publication status	Published - 2004
Event	Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE - Balearic Islands, Spain Duration: 29 Sept 2003 → 3 Oct 2003

Cite this

@article{a5974c55dae94061b744948c4957cb29,

title = "Theoretical aspects of MHD coronal seismology",

abstract = "The revolutionary breakthrough in observational detection of propagating and standing quasi-periodic disturbances of coronal plasma parameters, made in the EUV band with SOHO and TRACE mission instruments, together with confident interpretation of these phenomena in terms of magnetohydrodynamic (MHD) waves, has given rise to MHD coronal seismology. This review presents the theoretical background of these studies and reflects current trends in the development of the theory. Solar corona, loop oscillations, MHD waves.",

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

note = "Copyright: Copyright 2008 Elsevier B.V., All rights reserved.; Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE ; Conference date: 29-09-2003 Through 03-10-2003",

year = "2004",

language = "English",

pages = "407--416",

journal = "European Space Agency, (Special Publication) ESA SP",

issn = "0379-6566",

publisher = "European Space Agency",

number = "547",

}

TY - JOUR

T1 - Theoretical aspects of MHD coronal seismology

AU - Nakariakov, V. M.

PY - 2004

Y1 - 2004

N2 - The revolutionary breakthrough in observational detection of propagating and standing quasi-periodic disturbances of coronal plasma parameters, made in the EUV band with SOHO and TRACE mission instruments, together with confident interpretation of these phenomena in terms of magnetohydrodynamic (MHD) waves, has given rise to MHD coronal seismology. This review presents the theoretical background of these studies and reflects current trends in the development of the theory. Solar corona, loop oscillations, MHD waves.

AB - The revolutionary breakthrough in observational detection of propagating and standing quasi-periodic disturbances of coronal plasma parameters, made in the EUV band with SOHO and TRACE mission instruments, together with confident interpretation of these phenomena in terms of magnetohydrodynamic (MHD) waves, has given rise to MHD coronal seismology. This review presents the theoretical background of these studies and reflects current trends in the development of the theory. Solar corona, loop oscillations, MHD waves.

UR - https://www.scopus.com/pages/publications/18644368323

M3 - Conference article

AN - SCOPUS:18644368323

SN - 0379-6566

SP - 407

EP - 416

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

IS - 547

T2 - Proceedings of the Conference SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE

Y2 - 29 September 2003 through 3 October 2003

ER -

Theoretical aspects of MHD coronal seismology

Abstract

Other files and links

Fingerprint

Cite this