Beat structure in pulsating type IV solar radio bursts and a possible mechanism
Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two l...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Li, H. -W. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1987 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1987 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 111(1987), 1 vom: März, Seite 137-142 |
|---|---|
| Übergeordnetes Werk: |
volume:111 ; year:1987 ; number:1 ; month:03 ; pages:137-142 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00145446 |
|---|
| Katalog-ID: |
OLC2033562018 |
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| 520 | |a Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. | ||
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10.1007/BF00145446 doi (DE-627)OLC2033562018 (DE-He213)BF00145446-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Li, H. -W. verfasserin aut Beat structure in pulsating type IV solar radio bursts and a possible mechanism 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. Soliton Pulsation Frequency Radio Burst Large Depth Magnetic Loop Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 137-142 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:137-142 https://doi.org/10.1007/BF00145446 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 111 1987 1 03 137-142 |
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10.1007/BF00145446 doi (DE-627)OLC2033562018 (DE-He213)BF00145446-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Li, H. -W. verfasserin aut Beat structure in pulsating type IV solar radio bursts and a possible mechanism 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. Soliton Pulsation Frequency Radio Burst Large Depth Magnetic Loop Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 137-142 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:137-142 https://doi.org/10.1007/BF00145446 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 111 1987 1 03 137-142 |
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10.1007/BF00145446 doi (DE-627)OLC2033562018 (DE-He213)BF00145446-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Li, H. -W. verfasserin aut Beat structure in pulsating type IV solar radio bursts and a possible mechanism 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. Soliton Pulsation Frequency Radio Burst Large Depth Magnetic Loop Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 137-142 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:137-142 https://doi.org/10.1007/BF00145446 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 111 1987 1 03 137-142 |
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10.1007/BF00145446 doi (DE-627)OLC2033562018 (DE-He213)BF00145446-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Li, H. -W. verfasserin aut Beat structure in pulsating type IV solar radio bursts and a possible mechanism 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. Soliton Pulsation Frequency Radio Burst Large Depth Magnetic Loop Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 137-142 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:137-142 https://doi.org/10.1007/BF00145446 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 111 1987 1 03 137-142 |
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Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. © D. Reidel Publishing Company 1987 |
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Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. © D. Reidel Publishing Company 1987 |
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Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. The large depth of pulsation is also explained in this model. © D. Reidel Publishing Company 1987 |
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Reidel Publishing Company 1987</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Pulsating type IV solar radio bursts with beat structure are presented and analysed in this paper. Based upon the theory of whistler soliton emission we interpret the beat structure by the combination of two components with different pulsation frequencies due to radial oscillations of two legs of the magnetic loop. 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