Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections
Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and para...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Getmanov, V. G. [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 1282-1287 |
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| Übergeordnetes Werk: |
volume:81 ; year:2018 ; number:9 ; month:12 ; pages:1282-1287 |
| Links: |
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| DOI / URN: |
10.1134/S1063778818090107 |
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OLC2049930631 |
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| 520 | |a Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. | ||
| 650 | 4 | |a muon hodoscope | |
| 650 | 4 | |a coronal mass ejections | |
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| 650 | 4 | |a observations | |
| 650 | 4 | |a Forbush decrease | |
| 700 | 1 | |a Gvishiani, A. D. |4 aut | |
| 700 | 1 | |a Sidorov, R. V. |4 aut | |
| 700 | 1 | |a Soloviev, A. A. |4 aut | |
| 700 | 1 | |a Bogoutdinov, Sh. R. |4 aut | |
| 700 | 1 | |a Yashin, I. I. |4 aut | |
| 700 | 1 | |a Dmitrieva, A. N. |4 aut | |
| 700 | 1 | |a Kovylyaeva, A. A. |4 aut | |
| 700 | 1 | |a Astapov, I. I. |4 aut | |
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10.1134/S1063778818090107 doi (DE-627)OLC2049930631 (DE-He213)S1063778818090107-p DE-627 ger DE-627 rakwb eng 530 VZ Getmanov, V. G. verfasserin aut Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. muon hodoscope coronal mass ejections modeling observations Forbush decrease Gvishiani, A. D. aut Sidorov, R. V. aut Soloviev, A. A. aut Bogoutdinov, Sh. R. aut Yashin, I. I. aut Dmitrieva, A. N. aut Kovylyaeva, A. A. aut Astapov, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1282-1287 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1282-1287 https://doi.org/10.1134/S1063778818090107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1282-1287 |
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10.1134/S1063778818090107 doi (DE-627)OLC2049930631 (DE-He213)S1063778818090107-p DE-627 ger DE-627 rakwb eng 530 VZ Getmanov, V. G. verfasserin aut Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. muon hodoscope coronal mass ejections modeling observations Forbush decrease Gvishiani, A. D. aut Sidorov, R. V. aut Soloviev, A. A. aut Bogoutdinov, Sh. R. aut Yashin, I. I. aut Dmitrieva, A. N. aut Kovylyaeva, A. A. aut Astapov, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1282-1287 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1282-1287 https://doi.org/10.1134/S1063778818090107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1282-1287 |
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10.1134/S1063778818090107 doi (DE-627)OLC2049930631 (DE-He213)S1063778818090107-p DE-627 ger DE-627 rakwb eng 530 VZ Getmanov, V. G. verfasserin aut Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. muon hodoscope coronal mass ejections modeling observations Forbush decrease Gvishiani, A. D. aut Sidorov, R. V. aut Soloviev, A. A. aut Bogoutdinov, Sh. R. aut Yashin, I. I. aut Dmitrieva, A. N. aut Kovylyaeva, A. A. aut Astapov, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1282-1287 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1282-1287 https://doi.org/10.1134/S1063778818090107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1282-1287 |
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10.1134/S1063778818090107 doi (DE-627)OLC2049930631 (DE-He213)S1063778818090107-p DE-627 ger DE-627 rakwb eng 530 VZ Getmanov, V. G. verfasserin aut Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. muon hodoscope coronal mass ejections modeling observations Forbush decrease Gvishiani, A. D. aut Sidorov, R. V. aut Soloviev, A. A. aut Bogoutdinov, Sh. R. aut Yashin, I. I. aut Dmitrieva, A. N. aut Kovylyaeva, A. A. aut Astapov, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1282-1287 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1282-1287 https://doi.org/10.1134/S1063778818090107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1282-1287 |
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10.1134/S1063778818090107 doi (DE-627)OLC2049930631 (DE-He213)S1063778818090107-p DE-627 ger DE-627 rakwb eng 530 VZ Getmanov, V. G. verfasserin aut Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections 2018 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2018 Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. muon hodoscope coronal mass ejections modeling observations Forbush decrease Gvishiani, A. D. aut Sidorov, R. V. aut Soloviev, A. A. aut Bogoutdinov, Sh. R. aut Yashin, I. I. aut Dmitrieva, A. N. aut Kovylyaeva, A. A. aut Astapov, I. I. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 81(2018), 9 vom: Dez., Seite 1282-1287 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:81 year:2018 number:9 month:12 pages:1282-1287 https://doi.org/10.1134/S1063778818090107 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 81 2018 9 12 1282-1287 |
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mathematical model of observations from a muon hodoscope taking into account the kinematics and geometry of solar coronal mass ejections |
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Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections |
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Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. © Pleiades Publishing, Ltd. 2018 |
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Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. © Pleiades Publishing, Ltd. 2018 |
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Abstract A mathematical model for observations from a muon hodoscope which takes into account the kinematic and geometric parameters of solar coronal mass ejections (CMEs) is proposed. Equations for the calculation of mutual motions of the elements of the Sun–CME–Earth–muon hodoscope system and parameters of solar CMEs for the plane case are formulated. A model for a sequence of observations from the muon hodoscope with possible Forbush decreases is developed. The application of the developed mathematical observation model to problems of estimating CME parameters is presented. © Pleiades Publishing, Ltd. 2018 |
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Mathematical Model of Observations from a Muon Hodoscope Taking into Account the Kinematics and Geometry of Solar Coronal Mass Ejections |
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Gvishiani, A. D. Sidorov, R. V. Soloviev, A. A. Bogoutdinov, Sh. R. Yashin, I. I. Dmitrieva, A. N. Kovylyaeva, A. A. Astapov, I. I. |
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Gvishiani, A. D. Sidorov, R. V. Soloviev, A. A. Bogoutdinov, Sh. R. Yashin, I. I. Dmitrieva, A. N. Kovylyaeva, A. A. Astapov, I. I. |
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