Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections
Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phen...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bazilevskaya, G. A. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. |
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| Übergeordnetes Werk: |
Enthalten in: Geomagnetism and aeronomy - Pleiades Publishing, 1961, 61(2021), 5 vom: Sept., Seite 773-779 |
|---|---|
| Übergeordnetes Werk: |
volume:61 ; year:2021 ; number:5 ; month:09 ; pages:773-779 |
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10.1134/S0016793221050030 |
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OLC2128149916 |
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| 520 | |a Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. | ||
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10.1134/S0016793221050030 doi (DE-627)OLC2128149916 (DE-He213)S0016793221050030-p DE-627 ger DE-627 rakwb eng 550 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. Logachev, Yu. I. aut Daibog, E. I. aut Vlasova, N. A. aut Ginzburg, E. A. aut Ishkov, V. N. aut Lazutin, L. L. aut Nguyen, M. D. aut Surova, G. M. aut Yakovchuk, O. S. aut Enthalten in Geomagnetism and aeronomy Pleiades Publishing, 1961 61(2021), 5 vom: Sept., Seite 773-779 (DE-627)129365564 (DE-600)161523-3 (DE-576)014739321 0016-7932 nnns volume:61 year:2021 number:5 month:09 pages:773-779 https://doi.org/10.1134/S0016793221050030 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GEO SSG-OPC-GGO AR 61 2021 5 09 773-779 |
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10.1134/S0016793221050030 doi (DE-627)OLC2128149916 (DE-He213)S0016793221050030-p DE-627 ger DE-627 rakwb eng 550 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. Logachev, Yu. I. aut Daibog, E. I. aut Vlasova, N. A. aut Ginzburg, E. A. aut Ishkov, V. N. aut Lazutin, L. L. aut Nguyen, M. D. aut Surova, G. M. aut Yakovchuk, O. S. aut Enthalten in Geomagnetism and aeronomy Pleiades Publishing, 1961 61(2021), 5 vom: Sept., Seite 773-779 (DE-627)129365564 (DE-600)161523-3 (DE-576)014739321 0016-7932 nnns volume:61 year:2021 number:5 month:09 pages:773-779 https://doi.org/10.1134/S0016793221050030 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GEO SSG-OPC-GGO AR 61 2021 5 09 773-779 |
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10.1134/S0016793221050030 doi (DE-627)OLC2128149916 (DE-He213)S0016793221050030-p DE-627 ger DE-627 rakwb eng 550 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. Logachev, Yu. I. aut Daibog, E. I. aut Vlasova, N. A. aut Ginzburg, E. A. aut Ishkov, V. N. aut Lazutin, L. L. aut Nguyen, M. D. aut Surova, G. M. aut Yakovchuk, O. S. aut Enthalten in Geomagnetism and aeronomy Pleiades Publishing, 1961 61(2021), 5 vom: Sept., Seite 773-779 (DE-627)129365564 (DE-600)161523-3 (DE-576)014739321 0016-7932 nnns volume:61 year:2021 number:5 month:09 pages:773-779 https://doi.org/10.1134/S0016793221050030 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GEO SSG-OPC-GGO AR 61 2021 5 09 773-779 |
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10.1134/S0016793221050030 doi (DE-627)OLC2128149916 (DE-He213)S0016793221050030-p DE-627 ger DE-627 rakwb eng 550 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. Logachev, Yu. I. aut Daibog, E. I. aut Vlasova, N. A. aut Ginzburg, E. A. aut Ishkov, V. N. aut Lazutin, L. L. aut Nguyen, M. D. aut Surova, G. M. aut Yakovchuk, O. S. aut Enthalten in Geomagnetism and aeronomy Pleiades Publishing, 1961 61(2021), 5 vom: Sept., Seite 773-779 (DE-627)129365564 (DE-600)161523-3 (DE-576)014739321 0016-7932 nnns volume:61 year:2021 number:5 month:09 pages:773-779 https://doi.org/10.1134/S0016793221050030 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GEO SSG-OPC-GGO AR 61 2021 5 09 773-779 |
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10.1134/S0016793221050030 doi (DE-627)OLC2128149916 (DE-He213)S0016793221050030-p DE-627 ger DE-627 rakwb eng 550 VZ 16,13 ssgn Bazilevskaya, G. A. verfasserin aut Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. Logachev, Yu. I. aut Daibog, E. I. aut Vlasova, N. A. aut Ginzburg, E. A. aut Ishkov, V. N. aut Lazutin, L. L. aut Nguyen, M. D. aut Surova, G. M. aut Yakovchuk, O. S. aut Enthalten in Geomagnetism and aeronomy Pleiades Publishing, 1961 61(2021), 5 vom: Sept., Seite 773-779 (DE-627)129365564 (DE-600)161523-3 (DE-576)014739321 0016-7932 nnns volume:61 year:2021 number:5 month:09 pages:773-779 https://doi.org/10.1134/S0016793221050030 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GEO SSG-OPC-GGO AR 61 2021 5 09 773-779 |
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Bazilevskaya, G. A. Logachev, Yu. I. Daibog, E. I. Vlasova, N. A. Ginzburg, E. A. Ishkov, V. N. Lazutin, L. L. Nguyen, M. D. Surova, G. M. Yakovchuk, O. S. |
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Bazilevskaya, G. A. |
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10.1134/S0016793221050030 |
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550 |
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statistical links between solar cosmic rays, type-ii radio emission, and coronal mass ejections |
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Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections |
| abstract |
Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. |
| abstractGer |
Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. |
| abstract_unstemmed |
Abstract Type-II radio emission often accompanies events in solar cosmic rays and is an indicator of the propagation of a shock wave in the solar corona. Conversely, the shock wave associated with coronal mass ejections plays an important role in the acceleration of solar protons. Both of these phenomena can occur unaccompanied by solar cosmic rays, while not all solar cosmic ray events are accompanied by type-II radio emission. The statistical relationships between these phenomena are considered based on the catalogs of solar proton events for the 23rd and 24th solar-activity cycles. It is shown that the events of solar cosmic rays accompanied by type-II radio emissions are among the most powerful in terms of both particle characteristics and source characteristics. © Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 5, pp. 773–779. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 5, pp. 672–679. |
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Statistical Links between Solar Cosmic Rays, Type-II Radio Emission, and Coronal Mass Ejections |
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Logachev, Yu. I. Daibog, E. I. Vlasova, N. A. Ginzburg, E. A. Ishkov, V. N. Lazutin, L. L. Nguyen, M. D. Surova, G. M. Yakovchuk, O. S. |
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Logachev, Yu. I. Daibog, E. I. Vlasova, N. A. Ginzburg, E. A. Ishkov, V. N. Lazutin, L. L. Nguyen, M. D. Surova, G. M. Yakovchuk, O. S. |
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