Resonant MHD Waves in the Solar Atmosphere
Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introdu...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Goossens, Marcel [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2010 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2010 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 158(2010), 2-4 vom: 20. Nov., Seite 289-338 |
|---|---|
| Übergeordnetes Werk: |
volume:158 ; year:2010 ; number:2-4 ; day:20 ; month:11 ; pages:289-338 |
| Links: |
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| DOI / URN: |
10.1007/s11214-010-9702-7 |
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OLC2033697665 |
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| 520 | |a Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. | ||
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| 700 | 1 | |a Ruderman, Michael S. |4 aut | |
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10.1007/s11214-010-9702-7 doi (DE-627)OLC2033697665 (DE-He213)s11214-010-9702-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goossens, Marcel verfasserin aut Resonant MHD Waves in the Solar Atmosphere 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. Plasma Waves MHD Sun Erdélyi, Robert aut Ruderman, Michael S. aut Enthalten in Space science reviews Springer Netherlands, 1962 158(2010), 2-4 vom: 20. Nov., Seite 289-338 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:158 year:2010 number:2-4 day:20 month:11 pages:289-338 https://doi.org/10.1007/s11214-010-9702-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 158 2010 2-4 20 11 289-338 |
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10.1007/s11214-010-9702-7 doi (DE-627)OLC2033697665 (DE-He213)s11214-010-9702-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goossens, Marcel verfasserin aut Resonant MHD Waves in the Solar Atmosphere 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. Plasma Waves MHD Sun Erdélyi, Robert aut Ruderman, Michael S. aut Enthalten in Space science reviews Springer Netherlands, 1962 158(2010), 2-4 vom: 20. Nov., Seite 289-338 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:158 year:2010 number:2-4 day:20 month:11 pages:289-338 https://doi.org/10.1007/s11214-010-9702-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 158 2010 2-4 20 11 289-338 |
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10.1007/s11214-010-9702-7 doi (DE-627)OLC2033697665 (DE-He213)s11214-010-9702-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goossens, Marcel verfasserin aut Resonant MHD Waves in the Solar Atmosphere 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. Plasma Waves MHD Sun Erdélyi, Robert aut Ruderman, Michael S. aut Enthalten in Space science reviews Springer Netherlands, 1962 158(2010), 2-4 vom: 20. Nov., Seite 289-338 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:158 year:2010 number:2-4 day:20 month:11 pages:289-338 https://doi.org/10.1007/s11214-010-9702-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 158 2010 2-4 20 11 289-338 |
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10.1007/s11214-010-9702-7 doi (DE-627)OLC2033697665 (DE-He213)s11214-010-9702-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goossens, Marcel verfasserin aut Resonant MHD Waves in the Solar Atmosphere 2010 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2010 Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. Plasma Waves MHD Sun Erdélyi, Robert aut Ruderman, Michael S. aut Enthalten in Space science reviews Springer Netherlands, 1962 158(2010), 2-4 vom: 20. Nov., Seite 289-338 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:158 year:2010 number:2-4 day:20 month:11 pages:289-338 https://doi.org/10.1007/s11214-010-9702-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 158 2010 2-4 20 11 289-338 |
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Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. © Springer Science+Business Media B.V. 2010 |
| abstractGer |
Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. © Springer Science+Business Media B.V. 2010 |
| abstract_unstemmed |
Abstract The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The review starts from discussing the properties of driven resonant MHD waves. The dissipative solutions in Alfvén and slow dissipative layers are presented. The important concept of connection formulae is introduced. Next, we proceed on to non-stationary resonant MHD waves. The relation between quasi-modes of ideal MHD and eigenmodes of dissipative MHD are discussed. The solution describing the wave motion in non-stationary dissipative layers is given. It is shown that the connection formulae remain valid for non-stationary resonant MHD waves. The initial-value problem for resonant MHD waves is considered. The application of theory of resonant MHD waves to solar physics is discussed. © Springer Science+Business Media B.V. 2010 |
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Resonant MHD Waves in the Solar Atmosphere |
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Erdélyi, Robert Ruderman, Michael S. |
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