Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons
The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive inst...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Métrailler, Lionel [verfasserIn] Bélanger, Guillaume [verfasserIn] Kretschmar, Peter [verfasserIn] Kuulkers, Erik [verfasserIn] Martínez, Ricardo Pérez [verfasserIn] Ness, Jan-Uwe [verfasserIn] Rodriguez, Pedro [verfasserIn] Casale, Mauro [verfasserIn] Fauste, Jorge [verfasserIn] Finn, Timothy [verfasserIn] Sanchez, Celia [verfasserIn] Godard, Thomas [verfasserIn] Southworth, Richard [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2019 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Advances in space research - Amsterdam [u.a.] : Elsevier Science, 1981, 64, Seite 1701-1711 |
|---|---|
| Übergeordnetes Werk: |
volume:64 ; pages:1701-1711 |
| DOI / URN: |
10.1016/j.asr.2019.07.036 |
|---|
| Katalog-ID: |
ELV002927780 |
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| 245 | 1 | 0 | |a Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons |
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| 520 | |a The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. | ||
| 650 | 4 | |a Van Allen Belts | |
| 650 | 4 | |a Radiation belt modelling | |
| 650 | 4 | |a Trapped particles | |
| 650 | 4 | |a Radiation environment | |
| 650 | 4 | |a Space environment | |
| 650 | 4 | |a Space weather | |
| 700 | 1 | |a Bélanger, Guillaume |e verfasserin |4 aut | |
| 700 | 1 | |a Kretschmar, Peter |e verfasserin |4 aut | |
| 700 | 1 | |a Kuulkers, Erik |e verfasserin |4 aut | |
| 700 | 1 | |a Martínez, Ricardo Pérez |e verfasserin |4 aut | |
| 700 | 1 | |a Ness, Jan-Uwe |e verfasserin |4 aut | |
| 700 | 1 | |a Rodriguez, Pedro |e verfasserin |4 aut | |
| 700 | 1 | |a Casale, Mauro |e verfasserin |4 aut | |
| 700 | 1 | |a Fauste, Jorge |e verfasserin |4 aut | |
| 700 | 1 | |a Finn, Timothy |e verfasserin |4 aut | |
| 700 | 1 | |a Sanchez, Celia |e verfasserin |4 aut | |
| 700 | 1 | |a Godard, Thomas |e verfasserin |4 aut | |
| 700 | 1 | |a Southworth, Richard |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Advances in space research |d Amsterdam [u.a.] : Elsevier Science, 1981 |g 64, Seite 1701-1711 |h Online-Ressource |w (DE-627)320626113 |w (DE-600)2023311-5 |w (DE-576)255629427 |x 0273-1177 |7 nnns |
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10.1016/j.asr.2019.07.036 doi (DE-627)ELV002927780 (ELSEVIER)S0273-1177(19)30542-3 DE-627 ger DE-627 rda eng 520 620 DE-600 39.00 bkl 50.93 bkl Métrailler, Lionel verfasserin aut Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather Bélanger, Guillaume verfasserin aut Kretschmar, Peter verfasserin aut Kuulkers, Erik verfasserin aut Martínez, Ricardo Pérez verfasserin aut Ness, Jan-Uwe verfasserin aut Rodriguez, Pedro verfasserin aut Casale, Mauro verfasserin aut Fauste, Jorge verfasserin aut Finn, Timothy verfasserin aut Sanchez, Celia verfasserin aut Godard, Thomas verfasserin aut Southworth, Richard verfasserin aut Enthalten in Advances in space research Amsterdam [u.a.] : Elsevier Science, 1981 64, Seite 1701-1711 Online-Ressource (DE-627)320626113 (DE-600)2023311-5 (DE-576)255629427 0273-1177 nnns volume:64 pages:1701-1711 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.00 Astronomie: Allgemeines 50.93 Weltraumforschung AR 64 1701-1711 |
| spelling |
10.1016/j.asr.2019.07.036 doi (DE-627)ELV002927780 (ELSEVIER)S0273-1177(19)30542-3 DE-627 ger DE-627 rda eng 520 620 DE-600 39.00 bkl 50.93 bkl Métrailler, Lionel verfasserin aut Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather Bélanger, Guillaume verfasserin aut Kretschmar, Peter verfasserin aut Kuulkers, Erik verfasserin aut Martínez, Ricardo Pérez verfasserin aut Ness, Jan-Uwe verfasserin aut Rodriguez, Pedro verfasserin aut Casale, Mauro verfasserin aut Fauste, Jorge verfasserin aut Finn, Timothy verfasserin aut Sanchez, Celia verfasserin aut Godard, Thomas verfasserin aut Southworth, Richard verfasserin aut Enthalten in Advances in space research Amsterdam [u.a.] : Elsevier Science, 1981 64, Seite 1701-1711 Online-Ressource (DE-627)320626113 (DE-600)2023311-5 (DE-576)255629427 0273-1177 nnns volume:64 pages:1701-1711 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.00 Astronomie: Allgemeines 50.93 Weltraumforschung AR 64 1701-1711 |
| allfields_unstemmed |
10.1016/j.asr.2019.07.036 doi (DE-627)ELV002927780 (ELSEVIER)S0273-1177(19)30542-3 DE-627 ger DE-627 rda eng 520 620 DE-600 39.00 bkl 50.93 bkl Métrailler, Lionel verfasserin aut Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather Bélanger, Guillaume verfasserin aut Kretschmar, Peter verfasserin aut Kuulkers, Erik verfasserin aut Martínez, Ricardo Pérez verfasserin aut Ness, Jan-Uwe verfasserin aut Rodriguez, Pedro verfasserin aut Casale, Mauro verfasserin aut Fauste, Jorge verfasserin aut Finn, Timothy verfasserin aut Sanchez, Celia verfasserin aut Godard, Thomas verfasserin aut Southworth, Richard verfasserin aut Enthalten in Advances in space research Amsterdam [u.a.] : Elsevier Science, 1981 64, Seite 1701-1711 Online-Ressource (DE-627)320626113 (DE-600)2023311-5 (DE-576)255629427 0273-1177 nnns volume:64 pages:1701-1711 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.00 Astronomie: Allgemeines 50.93 Weltraumforschung AR 64 1701-1711 |
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10.1016/j.asr.2019.07.036 doi (DE-627)ELV002927780 (ELSEVIER)S0273-1177(19)30542-3 DE-627 ger DE-627 rda eng 520 620 DE-600 39.00 bkl 50.93 bkl Métrailler, Lionel verfasserin aut Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather Bélanger, Guillaume verfasserin aut Kretschmar, Peter verfasserin aut Kuulkers, Erik verfasserin aut Martínez, Ricardo Pérez verfasserin aut Ness, Jan-Uwe verfasserin aut Rodriguez, Pedro verfasserin aut Casale, Mauro verfasserin aut Fauste, Jorge verfasserin aut Finn, Timothy verfasserin aut Sanchez, Celia verfasserin aut Godard, Thomas verfasserin aut Southworth, Richard verfasserin aut Enthalten in Advances in space research Amsterdam [u.a.] : Elsevier Science, 1981 64, Seite 1701-1711 Online-Ressource (DE-627)320626113 (DE-600)2023311-5 (DE-576)255629427 0273-1177 nnns volume:64 pages:1701-1711 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.00 Astronomie: Allgemeines 50.93 Weltraumforschung AR 64 1701-1711 |
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10.1016/j.asr.2019.07.036 doi (DE-627)ELV002927780 (ELSEVIER)S0273-1177(19)30542-3 DE-627 ger DE-627 rda eng 520 620 DE-600 39.00 bkl 50.93 bkl Métrailler, Lionel verfasserin aut Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather Bélanger, Guillaume verfasserin aut Kretschmar, Peter verfasserin aut Kuulkers, Erik verfasserin aut Martínez, Ricardo Pérez verfasserin aut Ness, Jan-Uwe verfasserin aut Rodriguez, Pedro verfasserin aut Casale, Mauro verfasserin aut Fauste, Jorge verfasserin aut Finn, Timothy verfasserin aut Sanchez, Celia verfasserin aut Godard, Thomas verfasserin aut Southworth, Richard verfasserin aut Enthalten in Advances in space research Amsterdam [u.a.] : Elsevier Science, 1981 64, Seite 1701-1711 Online-Ressource (DE-627)320626113 (DE-600)2023311-5 (DE-576)255629427 0273-1177 nnns volume:64 pages:1701-1711 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.00 Astronomie: Allgemeines 50.93 Weltraumforschung AR 64 1701-1711 |
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Métrailler, Lionel ddc 520 bkl 39.00 bkl 50.93 misc Van Allen Belts misc Radiation belt modelling misc Trapped particles misc Radiation environment misc Space environment misc Space weather Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons |
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520 620 DE-600 39.00 bkl 50.93 bkl Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons Van Allen Belts Radiation belt modelling Trapped particles Radiation environment Space environment Space weather |
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Métrailler, Lionel Bélanger, Guillaume Kretschmar, Peter Kuulkers, Erik Martínez, Ricardo Pérez Ness, Jan-Uwe Rodriguez, Pedro Casale, Mauro Fauste, Jorge Finn, Timothy Sanchez, Celia Godard, Thomas Southworth, Richard |
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data-driven modelling of the van allen belts: the 5drbm model for trapped electrons |
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Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons |
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The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. |
| abstractGer |
The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. |
| abstract_unstemmed |
The magnetosphere sustained by the rotation of the Earth’s liquid iron core traps charged particles, mostly electrons and protons, into structures referred to as the Van Allen Belts. These radiation belts, in which the density of charged energetic particles can be very destructive for sensitive instrumentation, have to be crossed on every orbit of satellites traveling in elliptical orbits around the Earth, as is the case for ESA’s INTEGRAL and XMM-Newton missions. This paper presents the first working version of the 5DRBM-e model, a global, data-driven model of the radiation belts for trapped electrons. The model is based on in situ measurements of electrons by the radiation monitors on board the INTEGRAL and XMM-Newton satellites along their long elliptical orbits for respectively 16 and 19 years of operations. This model, in its present form, features the integral flux for trapped electrons within energies ranging from 0.7 to 1.75 MeV. Cross-validation of the 5DRBM-e with the well-known AE8min/max and AE9mean models for a low eccentricity GPS orbit shows excellent agreement, and demonstrates that the new model can be used to provide reliable predictions along widely different orbits around Earth for the purpose of designing, planning, and operating satellites with more accurate instrument safety margins. Future work will include extending the model based on electrons of different energies and proton radiation measurement data. |
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Data-driven modelling of the Van Allen Belts: The 5DRBM model for trapped electrons |
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