Dynamics of the Earth’s Particle Radiation Environment
Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Vainio, Rami [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2009 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2009 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 147(2009), 3-4 vom: 11. März, Seite 187-231 |
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| Übergeordnetes Werk: |
volume:147 ; year:2009 ; number:3-4 ; day:11 ; month:03 ; pages:187-231 |
| Links: |
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| DOI / URN: |
10.1007/s11214-009-9496-7 |
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| Katalog-ID: |
OLC203369576X |
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| 520 | |a Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. | ||
| 650 | 4 | |a Radiation environment | |
| 650 | 4 | |a Solar energetic particles | |
| 650 | 4 | |a Radiation belts | |
| 650 | 4 | |a Cosmic rays | |
| 650 | 4 | |a Radiation effects | |
| 700 | 1 | |a Desorgher, Laurent |4 aut | |
| 700 | 1 | |a Heynderickx, Daniel |4 aut | |
| 700 | 1 | |a Storini, Marisa |4 aut | |
| 700 | 1 | |a Flückiger, Erwin |4 aut | |
| 700 | 1 | |a Horne, Richard B. |4 aut | |
| 700 | 1 | |a Kovaltsov, Gennady A. |4 aut | |
| 700 | 1 | |a Kudela, Karel |4 aut | |
| 700 | 1 | |a Laurenza, Monica |4 aut | |
| 700 | 1 | |a McKenna-Lawlor, Susan |4 aut | |
| 700 | 1 | |a Rothkaehl, Hanna |4 aut | |
| 700 | 1 | |a Usoskin, Ilya G. |4 aut | |
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10.1007/s11214-009-9496-7 doi (DE-627)OLC203369576X (DE-He213)s11214-009-9496-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vainio, Rami verfasserin aut Dynamics of the Earth’s Particle Radiation Environment 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. Radiation environment Solar energetic particles Radiation belts Cosmic rays Radiation effects Desorgher, Laurent aut Heynderickx, Daniel aut Storini, Marisa aut Flückiger, Erwin aut Horne, Richard B. aut Kovaltsov, Gennady A. aut Kudela, Karel aut Laurenza, Monica aut McKenna-Lawlor, Susan aut Rothkaehl, Hanna aut Usoskin, Ilya G. aut Enthalten in Space science reviews Springer Netherlands, 1962 147(2009), 3-4 vom: 11. März, Seite 187-231 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 https://doi.org/10.1007/s11214-009-9496-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 147 2009 3-4 11 03 187-231 |
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10.1007/s11214-009-9496-7 doi (DE-627)OLC203369576X (DE-He213)s11214-009-9496-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vainio, Rami verfasserin aut Dynamics of the Earth’s Particle Radiation Environment 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. Radiation environment Solar energetic particles Radiation belts Cosmic rays Radiation effects Desorgher, Laurent aut Heynderickx, Daniel aut Storini, Marisa aut Flückiger, Erwin aut Horne, Richard B. aut Kovaltsov, Gennady A. aut Kudela, Karel aut Laurenza, Monica aut McKenna-Lawlor, Susan aut Rothkaehl, Hanna aut Usoskin, Ilya G. aut Enthalten in Space science reviews Springer Netherlands, 1962 147(2009), 3-4 vom: 11. März, Seite 187-231 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 https://doi.org/10.1007/s11214-009-9496-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 147 2009 3-4 11 03 187-231 |
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10.1007/s11214-009-9496-7 doi (DE-627)OLC203369576X (DE-He213)s11214-009-9496-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vainio, Rami verfasserin aut Dynamics of the Earth’s Particle Radiation Environment 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. Radiation environment Solar energetic particles Radiation belts Cosmic rays Radiation effects Desorgher, Laurent aut Heynderickx, Daniel aut Storini, Marisa aut Flückiger, Erwin aut Horne, Richard B. aut Kovaltsov, Gennady A. aut Kudela, Karel aut Laurenza, Monica aut McKenna-Lawlor, Susan aut Rothkaehl, Hanna aut Usoskin, Ilya G. aut Enthalten in Space science reviews Springer Netherlands, 1962 147(2009), 3-4 vom: 11. März, Seite 187-231 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 https://doi.org/10.1007/s11214-009-9496-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 147 2009 3-4 11 03 187-231 |
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10.1007/s11214-009-9496-7 doi (DE-627)OLC203369576X (DE-He213)s11214-009-9496-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vainio, Rami verfasserin aut Dynamics of the Earth’s Particle Radiation Environment 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. Radiation environment Solar energetic particles Radiation belts Cosmic rays Radiation effects Desorgher, Laurent aut Heynderickx, Daniel aut Storini, Marisa aut Flückiger, Erwin aut Horne, Richard B. aut Kovaltsov, Gennady A. aut Kudela, Karel aut Laurenza, Monica aut McKenna-Lawlor, Susan aut Rothkaehl, Hanna aut Usoskin, Ilya G. aut Enthalten in Space science reviews Springer Netherlands, 1962 147(2009), 3-4 vom: 11. März, Seite 187-231 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 https://doi.org/10.1007/s11214-009-9496-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 147 2009 3-4 11 03 187-231 |
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10.1007/s11214-009-9496-7 doi (DE-627)OLC203369576X (DE-He213)s11214-009-9496-7-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Vainio, Rami verfasserin aut Dynamics of the Earth’s Particle Radiation Environment 2009 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2009 Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. Radiation environment Solar energetic particles Radiation belts Cosmic rays Radiation effects Desorgher, Laurent aut Heynderickx, Daniel aut Storini, Marisa aut Flückiger, Erwin aut Horne, Richard B. aut Kovaltsov, Gennady A. aut Kudela, Karel aut Laurenza, Monica aut McKenna-Lawlor, Susan aut Rothkaehl, Hanna aut Usoskin, Ilya G. aut Enthalten in Space science reviews Springer Netherlands, 1962 147(2009), 3-4 vom: 11. März, Seite 187-231 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 https://doi.org/10.1007/s11214-009-9496-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 147 2009 3-4 11 03 187-231 |
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Enthalten in Space science reviews 147(2009), 3-4 vom: 11. März, Seite 187-231 volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 |
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Enthalten in Space science reviews 147(2009), 3-4 vom: 11. März, Seite 187-231 volume:147 year:2009 number:3-4 day:11 month:03 pages:187-231 |
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Vainio, Rami @@aut@@ Desorgher, Laurent @@aut@@ Heynderickx, Daniel @@aut@@ Storini, Marisa @@aut@@ Flückiger, Erwin @@aut@@ Horne, Richard B. @@aut@@ Kovaltsov, Gennady A. @@aut@@ Kudela, Karel @@aut@@ Laurenza, Monica @@aut@@ McKenna-Lawlor, Susan @@aut@@ Rothkaehl, Hanna @@aut@@ Usoskin, Ilya G. @@aut@@ |
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Vainio, Rami Desorgher, Laurent Heynderickx, Daniel Storini, Marisa Flückiger, Erwin Horne, Richard B. Kovaltsov, Gennady A. Kudela, Karel Laurenza, Monica McKenna-Lawlor, Susan Rothkaehl, Hanna Usoskin, Ilya G. |
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Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. © Springer Science+Business Media B.V. 2009 |
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Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. © Springer Science+Business Media B.V. 2009 |
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Abstract The physical processes affecting the dynamics of the Earth’s particle radiation environment are reviewed along with scientific and engineering models developed for its description. The emphasis is on models that are either operational engineering models or models presently under development for this purpose. Three components of the radiation environment, i.e., galactic cosmic rays (GCRs), solar energetic particles (SEPs) and trapped radiation, are considered separately. In the case of SEP models, we make a distinction between statistical flux/fluence models and those aimed at forecasting events. Models of the effects of particle radiation on the atmosphere are also reviewed. Further, we summarize the main features of the models and discuss the main outstanding issues concerning the models and their possible use in operational space weather forecasting. We emphasize the need for continuing the development of physics-based models of the Earth’s particle radiation environment, and their validation with observational data, until the models are ready to be used for nowcasting and/or forecasting the dynamics of the environment. © Springer Science+Business Media B.V. 2009 |
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