Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016
Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite ap...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Astapov, I. I. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2018 |
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| Schlagwörter: |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2018 |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - Pleiades Publishing, 1993, 81(2018), 9 vom: Dez., Seite 1370-1373 |
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| Übergeordnetes Werk: |
volume:81 ; year:2018 ; number:9 ; month:12 ; pages:1370-1373 |
| Links: |
|---|
| DOI / URN: |
10.1134/S106377881809003X |
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OLC204993050X |
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| 520 | |a Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. | ||
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| 700 | 1 | |a Borog, V. V. |4 aut | |
| 700 | 1 | |a Veselovsky, I. S. |4 aut | |
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| 700 | 1 | |a Gvishiani, A. D. |4 aut | |
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| 700 | 1 | |a Solov’ev, A. A. |4 aut | |
| 700 | 1 | |a Shutenko, V. V. |4 aut | |
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10.1134/S106377881809003X doi (DE-627)OLC204993050X (DE-He213)S106377881809003X-p DE-627 ger DE-627 rakwb eng 530 VZ Astapov, I. I. verfasserin aut Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. hodoscope muon detector muon flux coronal mass ejections the Sun Barbashina, N. S. aut Bogoutdinov, Sh. R. aut Borog, V. V. aut Veselovsky, I. S. aut Getmanov, V. G. aut Gvishiani, A. D. aut Dmitrieva, A. N. aut Mishutina, Yu. N. aut Osetrova, N. V. aut Petrukhin, A. A. aut Sidorov, R. V. aut Solov’ev, A. A. aut Shutenko, V. V. aut Yashin, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1370-1373 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1370-1373 https://doi.org/10.1134/S106377881809003X lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1370-1373 |
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10.1134/S106377881809003X doi (DE-627)OLC204993050X (DE-He213)S106377881809003X-p DE-627 ger DE-627 rakwb eng 530 VZ Astapov, I. I. verfasserin aut Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. hodoscope muon detector muon flux coronal mass ejections the Sun Barbashina, N. S. aut Bogoutdinov, Sh. R. aut Borog, V. V. aut Veselovsky, I. S. aut Getmanov, V. G. aut Gvishiani, A. D. aut Dmitrieva, A. N. aut Mishutina, Yu. N. aut Osetrova, N. V. aut Petrukhin, A. A. aut Sidorov, R. V. aut Solov’ev, A. A. aut Shutenko, V. V. aut Yashin, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1370-1373 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1370-1373 https://doi.org/10.1134/S106377881809003X lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1370-1373 |
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10.1134/S106377881809003X doi (DE-627)OLC204993050X (DE-He213)S106377881809003X-p DE-627 ger DE-627 rakwb eng 530 VZ Astapov, I. I. verfasserin aut Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. hodoscope muon detector muon flux coronal mass ejections the Sun Barbashina, N. S. aut Bogoutdinov, Sh. R. aut Borog, V. V. aut Veselovsky, I. S. aut Getmanov, V. G. aut Gvishiani, A. D. aut Dmitrieva, A. N. aut Mishutina, Yu. N. aut Osetrova, N. V. aut Petrukhin, A. A. aut Sidorov, R. V. aut Solov’ev, A. A. aut Shutenko, V. V. aut Yashin, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1370-1373 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1370-1373 https://doi.org/10.1134/S106377881809003X lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1370-1373 |
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10.1134/S106377881809003X doi (DE-627)OLC204993050X (DE-He213)S106377881809003X-p DE-627 ger DE-627 rakwb eng 530 VZ Astapov, I. I. verfasserin aut Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. hodoscope muon detector muon flux coronal mass ejections the Sun Barbashina, N. S. aut Bogoutdinov, Sh. R. aut Borog, V. V. aut Veselovsky, I. S. aut Getmanov, V. G. aut Gvishiani, A. D. aut Dmitrieva, A. N. aut Mishutina, Yu. N. aut Osetrova, N. V. aut Petrukhin, A. A. aut Sidorov, R. V. aut Solov’ev, A. A. aut Shutenko, V. V. aut Yashin, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1370-1373 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1370-1373 https://doi.org/10.1134/S106377881809003X lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1370-1373 |
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10.1134/S106377881809003X doi (DE-627)OLC204993050X (DE-He213)S106377881809003X-p DE-627 ger DE-627 rakwb eng 530 VZ Astapov, I. I. verfasserin aut Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. hodoscope muon detector muon flux coronal mass ejections the Sun Barbashina, N. S. aut Bogoutdinov, Sh. R. aut Borog, V. V. aut Veselovsky, I. S. aut Getmanov, V. G. aut Gvishiani, A. D. aut Dmitrieva, A. N. aut Mishutina, Yu. N. aut Osetrova, N. V. aut Petrukhin, A. A. aut Sidorov, R. V. aut Solov’ev, A. A. aut Shutenko, V. V. aut Yashin, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1370-1373 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1370-1373 https://doi.org/10.1134/S106377881809003X lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1370-1373 |
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Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 |
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| title_full |
Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 |
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Astapov, I. I. |
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Physics of atomic nuclei |
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Physics of atomic nuclei |
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eng |
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500 - Science |
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2018 |
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1370 |
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Astapov, I. I. Barbashina, N. S. Bogoutdinov, Sh. R. Borog, V. V. Veselovsky, I. S. Getmanov, V. G. Gvishiani, A. D. Dmitrieva, A. N. Mishutina, Yu. N. Osetrova, N. V. Petrukhin, A. A. Sidorov, R. V. Solov’ev, A. A. Shutenko, V. V. Yashin, I. I. |
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81 |
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530 VZ |
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Aufsätze |
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Astapov, I. I. |
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10.1134/S106377881809003X |
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530 |
| title_sort |
studying the anisotropy of the muon flux during nongeoeffective coronal mass ejections of 2016 |
| title_auth |
Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 |
| abstract |
Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. © Pleiades Publishing, Ltd. 2018 |
| abstractGer |
Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. © Pleiades Publishing, Ltd. 2018 |
| abstract_unstemmed |
Abstract Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented. © Pleiades Publishing, Ltd. 2018 |
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9 |
| title_short |
Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016 |
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https://doi.org/10.1134/S106377881809003X |
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Barbashina, N. S. Bogoutdinov, Sh. R. Borog, V. V. Veselovsky, I. S. Getmanov, V. G. Gvishiani, A. D. Dmitrieva, A. N. Mishutina, Yu. N. Osetrova, N. V. Petrukhin, A. A. Sidorov, R. V. Solov’ev, A. A. Shutenko, V. V. Yashin, I. I. |
| author2Str |
Barbashina, N. S. Bogoutdinov, Sh. R. Borog, V. V. Veselovsky, I. S. Getmanov, V. G. Gvishiani, A. D. Dmitrieva, A. N. Mishutina, Yu. N. Osetrova, N. V. Petrukhin, A. A. Sidorov, R. V. Solov’ev, A. A. Shutenko, V. V. Yashin, I. I. |
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2024-07-04T00:32:23.168Z |
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