Pulsations of type IV solar radio emission: The bounce-resonance effects
Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be fo...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Meerson, B. I. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1978 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1978 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 58(1978), 1 vom: Juni, Seite 165-179 |
|---|---|
| Übergeordnetes Werk: |
volume:58 ; year:1978 ; number:1 ; month:06 ; pages:165-179 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00152562 |
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| Katalog-ID: |
OLC2033544354 |
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| 520 | |a Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. | ||
| 650 | 4 | |a Flare | |
| 650 | 4 | |a Dense Plasma | |
| 650 | 4 | |a Periodic Modulation | |
| 650 | 4 | |a Radio Emission | |
| 650 | 4 | |a Rate Dependence | |
| 700 | 1 | |a Sasorov, P. V. |4 aut | |
| 700 | 1 | |a Stepanov, A. V. |4 aut | |
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10.1007/BF00152562 doi (DE-627)OLC2033544354 (DE-He213)BF00152562-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meerson, B. I. verfasserin aut Pulsations of type IV solar radio emission: The bounce-resonance effects 1978 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1978 Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. Flare Dense Plasma Periodic Modulation Radio Emission Rate Dependence Sasorov, P. V. aut Stepanov, A. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 58(1978), 1 vom: Juni, Seite 165-179 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:58 year:1978 number:1 month:06 pages:165-179 https://doi.org/10.1007/BF00152562 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 58 1978 1 06 165-179 |
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10.1007/BF00152562 doi (DE-627)OLC2033544354 (DE-He213)BF00152562-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meerson, B. I. verfasserin aut Pulsations of type IV solar radio emission: The bounce-resonance effects 1978 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1978 Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. Flare Dense Plasma Periodic Modulation Radio Emission Rate Dependence Sasorov, P. V. aut Stepanov, A. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 58(1978), 1 vom: Juni, Seite 165-179 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:58 year:1978 number:1 month:06 pages:165-179 https://doi.org/10.1007/BF00152562 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 58 1978 1 06 165-179 |
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10.1007/BF00152562 doi (DE-627)OLC2033544354 (DE-He213)BF00152562-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meerson, B. I. verfasserin aut Pulsations of type IV solar radio emission: The bounce-resonance effects 1978 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1978 Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. Flare Dense Plasma Periodic Modulation Radio Emission Rate Dependence Sasorov, P. V. aut Stepanov, A. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 58(1978), 1 vom: Juni, Seite 165-179 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:58 year:1978 number:1 month:06 pages:165-179 https://doi.org/10.1007/BF00152562 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 58 1978 1 06 165-179 |
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10.1007/BF00152562 doi (DE-627)OLC2033544354 (DE-He213)BF00152562-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meerson, B. I. verfasserin aut Pulsations of type IV solar radio emission: The bounce-resonance effects 1978 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1978 Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. Flare Dense Plasma Periodic Modulation Radio Emission Rate Dependence Sasorov, P. V. aut Stepanov, A. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 58(1978), 1 vom: Juni, Seite 165-179 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:58 year:1978 number:1 month:06 pages:165-179 https://doi.org/10.1007/BF00152562 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 58 1978 1 06 165-179 |
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10.1007/BF00152562 doi (DE-627)OLC2033544354 (DE-He213)BF00152562-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Meerson, B. I. verfasserin aut Pulsations of type IV solar radio emission: The bounce-resonance effects 1978 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1978 Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. Flare Dense Plasma Periodic Modulation Radio Emission Rate Dependence Sasorov, P. V. aut Stepanov, A. V. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 58(1978), 1 vom: Juni, Seite 165-179 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:58 year:1978 number:1 month:06 pages:165-179 https://doi.org/10.1007/BF00152562 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4305 GBV_ILN_4306 AR 58 1978 1 06 165-179 |
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Meerson, B. I. |
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pulsations of type iv solar radio emission: the bounce-resonance effects |
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Pulsations of type IV solar radio emission: The bounce-resonance effects |
| abstract |
Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. © D. Reidel Publishing Company 1978 |
| abstractGer |
Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. © D. Reidel Publishing Company 1978 |
| abstract_unstemmed |
Abstract A mechanism of excitation of radial oscillations of a ‘magnetic tube’ is proposed for the interpretation of a periodic modulation of type IV radio burst intensity in the meter and decimeter range. After the flare a configuration with denser plasma extended along the magnetic field can be formed in the corona. Eigenoscillations of such a system are damped by MHD-wave emission into the external coronal plasma. However, if high energy protons with β ≳ 0.2 are trapped by this configuration, the damping of oscillations can be made up for by an amplification due to bounce-resonant plasma instability. The regularity of the pulse period is explained by presence of a maximum in the wave growth rate dependence on the frequency. © D. Reidel Publishing Company 1978 |
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Pulsations of type IV solar radio emission: The bounce-resonance effects |
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Sasorov, P. V. Stepanov, A. V. |
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