Interplanetary propagation of relativistic solar protons
Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lumme, M. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1986 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1986 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 107(1986), 1 vom: März, Seite 183-194 |
|---|---|
| Übergeordnetes Werk: |
volume:107 ; year:1986 ; number:1 ; month:03 ; pages:183-194 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00155352 |
|---|
| Katalog-ID: |
OLC2033560570 |
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| 520 | |a Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. | ||
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| 700 | 1 | |a Torsti, J. J. |4 aut | |
| 700 | 1 | |a Vainikka, E. |4 aut | |
| 700 | 1 | |a Peltonen, J. |4 aut | |
| 700 | 1 | |a Valtonen, E. |4 aut | |
| 700 | 1 | |a Arvela, H. |4 aut | |
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10.1007/BF00155352 doi (DE-627)OLC2033560570 (DE-He213)BF00155352-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Lumme, M. verfasserin aut Interplanetary propagation of relativistic solar protons 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. Free Path Pitch Angle Particle Trajectory Angle Distribution Particle Flux Nieminen, M. aut Torsti, J. J. aut Vainikka, E. aut Peltonen, J. aut Valtonen, E. aut Arvela, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 107(1986), 1 vom: März, Seite 183-194 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:107 year:1986 number:1 month:03 pages:183-194 https://doi.org/10.1007/BF00155352 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 107 1986 1 03 183-194 |
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10.1007/BF00155352 doi (DE-627)OLC2033560570 (DE-He213)BF00155352-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Lumme, M. verfasserin aut Interplanetary propagation of relativistic solar protons 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. Free Path Pitch Angle Particle Trajectory Angle Distribution Particle Flux Nieminen, M. aut Torsti, J. J. aut Vainikka, E. aut Peltonen, J. aut Valtonen, E. aut Arvela, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 107(1986), 1 vom: März, Seite 183-194 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:107 year:1986 number:1 month:03 pages:183-194 https://doi.org/10.1007/BF00155352 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 107 1986 1 03 183-194 |
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10.1007/BF00155352 doi (DE-627)OLC2033560570 (DE-He213)BF00155352-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Lumme, M. verfasserin aut Interplanetary propagation of relativistic solar protons 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. Free Path Pitch Angle Particle Trajectory Angle Distribution Particle Flux Nieminen, M. aut Torsti, J. J. aut Vainikka, E. aut Peltonen, J. aut Valtonen, E. aut Arvela, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 107(1986), 1 vom: März, Seite 183-194 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:107 year:1986 number:1 month:03 pages:183-194 https://doi.org/10.1007/BF00155352 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 107 1986 1 03 183-194 |
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10.1007/BF00155352 doi (DE-627)OLC2033560570 (DE-He213)BF00155352-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Lumme, M. verfasserin aut Interplanetary propagation of relativistic solar protons 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. Free Path Pitch Angle Particle Trajectory Angle Distribution Particle Flux Nieminen, M. aut Torsti, J. J. aut Vainikka, E. aut Peltonen, J. aut Valtonen, E. aut Arvela, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 107(1986), 1 vom: März, Seite 183-194 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:107 year:1986 number:1 month:03 pages:183-194 https://doi.org/10.1007/BF00155352 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 107 1986 1 03 183-194 |
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10.1007/BF00155352 doi (DE-627)OLC2033560570 (DE-He213)BF00155352-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Lumme, M. verfasserin aut Interplanetary propagation of relativistic solar protons 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. Free Path Pitch Angle Particle Trajectory Angle Distribution Particle Flux Nieminen, M. aut Torsti, J. J. aut Vainikka, E. aut Peltonen, J. aut Valtonen, E. aut Arvela, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 107(1986), 1 vom: März, Seite 183-194 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:107 year:1986 number:1 month:03 pages:183-194 https://doi.org/10.1007/BF00155352 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 107 1986 1 03 183-194 |
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Interplanetary propagation of relativistic solar protons |
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Interplanetary propagation of relativistic solar protons |
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Lumme, M. |
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Solar physics |
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Lumme, M. Nieminen, M. Torsti, J. J. Vainikka, E. Peltonen, J. Valtonen, E. Arvela, H. |
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interplanetary propagation of relativistic solar protons |
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Interplanetary propagation of relativistic solar protons |
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Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. © D. Reidel Publishing Company 1986 |
| abstractGer |
Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. © D. Reidel Publishing Company 1986 |
| abstract_unstemmed |
Abstract Particle fluxes and pitch angle distributions of relativistic solar protons at Earth's orbit have been determined by Monte Carlo calculations. The analysis covers two hours after the release of the particles from the Sun and total of 8 × $ 10^{6} $ particle trajectories were simulated. The pitch angle scattering was assumed to be isotropic and the scattering mean free path was varied from 0.1 to 4 AU. The intensity-time profiles after a delta-like injection from the Sun show that the interplanetary propagation is clearly non-diffusive at scattering mean-free paths above 0.5 AU. All pitch angle distributions have a steady minimum at 90 °, and they become similar about 20 min after the arrival of first particles. As an application, the solar injection profile and the interplanetary scattering mean-free path of particles that gave rise to the GLE on 7 May, 1978 were determined. In contrast to the values of 3–5 AU published by other authors, the average scattering mean-free path was found to be about 1 AU. © D. Reidel Publishing Company 1986 |
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Interplanetary propagation of relativistic solar protons |
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