Observations of Solar Type II bursts at frequencies 10–30 MHz
Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wave...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Mel'nik, V.N. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2004 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2004 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 222(2004), 1 vom: Juli, Seite 151-166 |
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| Übergeordnetes Werk: |
volume:222 ; year:2004 ; number:1 ; month:07 ; pages:151-166 |
| Links: |
|---|
| DOI / URN: |
10.1023/B:SOLA.0000036854.66380.a4 |
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| Katalog-ID: |
OLC2033596958 |
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| 520 | |a Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. | ||
| 650 | 4 | |a Fine Structure | |
| 650 | 4 | |a Drift Rate | |
| 650 | 4 | |a Radio Telescope | |
| 650 | 4 | |a Radio Burst | |
| 650 | 4 | |a Frequency Drift | |
| 700 | 1 | |a Konovalenko, A.A. |4 aut | |
| 700 | 1 | |a Rucker, H.O. |4 aut | |
| 700 | 1 | |a Stanislavsky, A.A. |4 aut | |
| 700 | 1 | |a Abranin, E.P. |4 aut | |
| 700 | 1 | |a Lecacheux, A. |4 aut | |
| 700 | 1 | |a Mann, G. |4 aut | |
| 700 | 1 | |a Warmuth, A. |4 aut | |
| 700 | 1 | |a Zaitsev, V.V. |4 aut | |
| 700 | 1 | |a Boudjada, M.Y. |4 aut | |
| 700 | 1 | |a Dorovskii, V.V. |4 aut | |
| 700 | 1 | |a Zaharenko, V.V. |4 aut | |
| 700 | 1 | |a Lisachenko, V.N. |4 aut | |
| 700 | 1 | |a Rosolen, C. |4 aut | |
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10.1023/B:SOLA.0000036854.66380.a4 doi (DE-627)OLC2033596958 (DE-He213)B:SOLA.0000036854.66380.a4-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel'nik, V.N. verfasserin aut Observations of Solar Type II bursts at frequencies 10–30 MHz 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. Fine Structure Drift Rate Radio Telescope Radio Burst Frequency Drift Konovalenko, A.A. aut Rucker, H.O. aut Stanislavsky, A.A. aut Abranin, E.P. aut Lecacheux, A. aut Mann, G. aut Warmuth, A. aut Zaitsev, V.V. aut Boudjada, M.Y. aut Dorovskii, V.V. aut Zaharenko, V.V. aut Lisachenko, V.N. aut Rosolen, C. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 151-166 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:151-166 https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 151-166 |
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10.1023/B:SOLA.0000036854.66380.a4 doi (DE-627)OLC2033596958 (DE-He213)B:SOLA.0000036854.66380.a4-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel'nik, V.N. verfasserin aut Observations of Solar Type II bursts at frequencies 10–30 MHz 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. Fine Structure Drift Rate Radio Telescope Radio Burst Frequency Drift Konovalenko, A.A. aut Rucker, H.O. aut Stanislavsky, A.A. aut Abranin, E.P. aut Lecacheux, A. aut Mann, G. aut Warmuth, A. aut Zaitsev, V.V. aut Boudjada, M.Y. aut Dorovskii, V.V. aut Zaharenko, V.V. aut Lisachenko, V.N. aut Rosolen, C. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 151-166 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:151-166 https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 151-166 |
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10.1023/B:SOLA.0000036854.66380.a4 doi (DE-627)OLC2033596958 (DE-He213)B:SOLA.0000036854.66380.a4-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel'nik, V.N. verfasserin aut Observations of Solar Type II bursts at frequencies 10–30 MHz 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. Fine Structure Drift Rate Radio Telescope Radio Burst Frequency Drift Konovalenko, A.A. aut Rucker, H.O. aut Stanislavsky, A.A. aut Abranin, E.P. aut Lecacheux, A. aut Mann, G. aut Warmuth, A. aut Zaitsev, V.V. aut Boudjada, M.Y. aut Dorovskii, V.V. aut Zaharenko, V.V. aut Lisachenko, V.N. aut Rosolen, C. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 151-166 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:151-166 https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 151-166 |
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10.1023/B:SOLA.0000036854.66380.a4 doi (DE-627)OLC2033596958 (DE-He213)B:SOLA.0000036854.66380.a4-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel'nik, V.N. verfasserin aut Observations of Solar Type II bursts at frequencies 10–30 MHz 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. Fine Structure Drift Rate Radio Telescope Radio Burst Frequency Drift Konovalenko, A.A. aut Rucker, H.O. aut Stanislavsky, A.A. aut Abranin, E.P. aut Lecacheux, A. aut Mann, G. aut Warmuth, A. aut Zaitsev, V.V. aut Boudjada, M.Y. aut Dorovskii, V.V. aut Zaharenko, V.V. aut Lisachenko, V.N. aut Rosolen, C. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 151-166 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:151-166 https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 151-166 |
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10.1023/B:SOLA.0000036854.66380.a4 doi (DE-627)OLC2033596958 (DE-He213)B:SOLA.0000036854.66380.a4-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel'nik, V.N. verfasserin aut Observations of Solar Type II bursts at frequencies 10–30 MHz 2004 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2004 Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. Fine Structure Drift Rate Radio Telescope Radio Burst Frequency Drift Konovalenko, A.A. aut Rucker, H.O. aut Stanislavsky, A.A. aut Abranin, E.P. aut Lecacheux, A. aut Mann, G. aut Warmuth, A. aut Zaitsev, V.V. aut Boudjada, M.Y. aut Dorovskii, V.V. aut Zaharenko, V.V. aut Lisachenko, V.N. aut Rosolen, C. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 222(2004), 1 vom: Juli, Seite 151-166 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:222 year:2004 number:1 month:07 pages:151-166 https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 222 2004 1 07 151-166 |
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Observations of Solar Type II bursts at frequencies 10–30 MHz |
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Mel'nik, V.N. |
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Solar physics |
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Solar physics |
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eng |
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500 - Science |
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2004 |
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151 |
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Mel'nik, V.N. Konovalenko, A.A. Rucker, H.O. Stanislavsky, A.A. Abranin, E.P. Lecacheux, A. Mann, G. Warmuth, A. Zaitsev, V.V. Boudjada, M.Y. Dorovskii, V.V. Zaharenko, V.V. Lisachenko, V.N. Rosolen, C. |
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Mel'nik, V.N. |
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10.1023/B:SOLA.0000036854.66380.a4 |
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530 |
| title_sort |
observations of solar type ii bursts at frequencies 10–30 mhz |
| title_auth |
Observations of Solar Type II bursts at frequencies 10–30 MHz |
| abstract |
Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. © Kluwer Academic Publishers 2004 |
| abstractGer |
Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. © Kluwer Academic Publishers 2004 |
| abstract_unstemmed |
Abstract We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz $ s^{−1} $. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed. © Kluwer Academic Publishers 2004 |
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| title_short |
Observations of Solar Type II bursts at frequencies 10–30 MHz |
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https://doi.org/10.1023/B:SOLA.0000036854.66380.a4 |
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Konovalenko, A.A. Rucker, H.O. Stanislavsky, A.A. Abranin, E.P. Lecacheux, A. Mann, G. Warmuth, A. Zaitsev, V.V. Boudjada, M.Y. Dorovskii, V.V. Zaharenko, V.V. Lisachenko, V.N. Rosolen, C. |
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Konovalenko, A.A. Rucker, H.O. Stanislavsky, A.A. Abranin, E.P. Lecacheux, A. Mann, G. Warmuth, A. Zaitsev, V.V. Boudjada, M.Y. Dorovskii, V.V. Zaharenko, V.V. Lisachenko, V.N. Rosolen, C. |
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