Decameter Type III-Like Bursts
Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Mel’nik, V. N. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2008 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2008 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Springer Netherlands, 1967, 250(2008), 1 vom: 13. Juni, Seite 133-145 |
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| Übergeordnetes Werk: |
volume:250 ; year:2008 ; number:1 ; day:13 ; month:06 ; pages:133-145 |
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| DOI / URN: |
10.1007/s11207-008-9166-z |
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| 520 | |a Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. | ||
| 650 | 4 | |a Decameter type III-like bursts | |
| 650 | 4 | |a Active regions | |
| 650 | 4 | |a Frequency drift rates | |
| 650 | 4 | |a Group velocity | |
| 700 | 1 | |a Konovalenko, A. A. |4 aut | |
| 700 | 1 | |a Rucker, H. O. |4 aut | |
| 700 | 1 | |a Rutkevych, B. P. |4 aut | |
| 700 | 1 | |a Dorovskyy, V. V. |4 aut | |
| 700 | 1 | |a Abranin, E. P. |4 aut | |
| 700 | 1 | |a Brazhenko, A. I. |4 aut | |
| 700 | 1 | |a Stanislavskii, A. A. |4 aut | |
| 700 | 1 | |a Lecacheux, A. |4 aut | |
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10.1007/s11207-008-9166-z doi (DE-627)OLC2033604020 (DE-He213)s11207-008-9166-z-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel’nik, V. N. verfasserin aut Decameter Type III-Like Bursts 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. Decameter type III-like bursts Active regions Frequency drift rates Group velocity Konovalenko, A. A. aut Rucker, H. O. aut Rutkevych, B. P. aut Dorovskyy, V. V. aut Abranin, E. P. aut Brazhenko, A. I. aut Stanislavskii, A. A. aut Lecacheux, A. aut Enthalten in Solar physics Springer Netherlands, 1967 250(2008), 1 vom: 13. Juni, Seite 133-145 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:250 year:2008 number:1 day:13 month:06 pages:133-145 https://doi.org/10.1007/s11207-008-9166-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 250 2008 1 13 06 133-145 |
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10.1007/s11207-008-9166-z doi (DE-627)OLC2033604020 (DE-He213)s11207-008-9166-z-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel’nik, V. N. verfasserin aut Decameter Type III-Like Bursts 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. Decameter type III-like bursts Active regions Frequency drift rates Group velocity Konovalenko, A. A. aut Rucker, H. O. aut Rutkevych, B. P. aut Dorovskyy, V. V. aut Abranin, E. P. aut Brazhenko, A. I. aut Stanislavskii, A. A. aut Lecacheux, A. aut Enthalten in Solar physics Springer Netherlands, 1967 250(2008), 1 vom: 13. Juni, Seite 133-145 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:250 year:2008 number:1 day:13 month:06 pages:133-145 https://doi.org/10.1007/s11207-008-9166-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 250 2008 1 13 06 133-145 |
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10.1007/s11207-008-9166-z doi (DE-627)OLC2033604020 (DE-He213)s11207-008-9166-z-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Mel’nik, V. N. verfasserin aut Decameter Type III-Like Bursts 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. Decameter type III-like bursts Active regions Frequency drift rates Group velocity Konovalenko, A. A. aut Rucker, H. O. aut Rutkevych, B. P. aut Dorovskyy, V. V. aut Abranin, E. P. aut Brazhenko, A. I. aut Stanislavskii, A. A. aut Lecacheux, A. aut Enthalten in Solar physics Springer Netherlands, 1967 250(2008), 1 vom: 13. Juni, Seite 133-145 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:250 year:2008 number:1 day:13 month:06 pages:133-145 https://doi.org/10.1007/s11207-008-9166-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 AR 250 2008 1 13 06 133-145 |
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Mel’nik, V. N. Konovalenko, A. A. Rucker, H. O. Rutkevych, B. P. Dorovskyy, V. V. Abranin, E. P. Brazhenko, A. I. Stanislavskii, A. A. Lecacheux, A. |
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Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. © Springer Science+Business Media B.V. 2008 |
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Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. © Springer Science+Business Media B.V. 2008 |
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Abstract We report the first observations of Type III-like bursts at frequencies 10 – 30 MHz. More than 1000 such bursts during 2002 – 2004 have been analyzed. The frequency drift of these bursts is several times that of decameter Type III bursts. A typical duration of the Type III-like bursts is 1 – 2 s. These bursts are mainly observed when the source active region is located within a few days from the central meridian. The drift rate of the Type III-like bursts can take a large value by considering the velocity of Type III electrons and the group velocity of generated electromagnetic waves. © Springer Science+Business Media B.V. 2008 |
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Decameter Type III-Like Bursts |
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Konovalenko, A. A. Rucker, H. O. Rutkevych, B. P. Dorovskyy, V. V. Abranin, E. P. Brazhenko, A. I. Stanislavskii, A. A. Lecacheux, A. |
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Konovalenko, A. A. Rucker, H. O. Rutkevych, B. P. Dorovskyy, V. V. Abranin, E. P. Brazhenko, A. I. Stanislavskii, A. A. Lecacheux, A. |
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