Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions
Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collecte...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Zhou, XiaoPing [verfasserIn] Xiao, FuLiang [verfasserIn] He, YiHua [verfasserIn] Yang, Chang [verfasserIn] Zhou, QingHua [verfasserIn] Zhang, ZeLong [verfasserIn] Gao, ZhongLei [verfasserIn] Ding, YuanHui [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2013 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Science in China - Heidelberg : Springer, 1997, 56(2013), 12 vom: 10. Okt., Seite 2006-2014 |
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| Übergeordnetes Werk: |
volume:56 ; year:2013 ; number:12 ; day:10 ; month:10 ; pages:2006-2014 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11430-013-4688-0 |
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| Katalog-ID: |
SPR019238606 |
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| 520 | |a Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. | ||
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| 650 | 4 | |a chorus waves |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a wave-particle interaction |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a geomagnetic condition |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Xiao, FuLiang |e verfasserin |4 aut | |
| 700 | 1 | |a He, YiHua |e verfasserin |4 aut | |
| 700 | 1 | |a Yang, Chang |e verfasserin |4 aut | |
| 700 | 1 | |a Zhou, QingHua |e verfasserin |4 aut | |
| 700 | 1 | |a Zhang, ZeLong |e verfasserin |4 aut | |
| 700 | 1 | |a Gao, ZhongLei |e verfasserin |4 aut | |
| 700 | 1 | |a Ding, YuanHui |e verfasserin |4 aut | |
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10.1007/s11430-013-4688-0 doi (DE-627)SPR019238606 (SPR)s11430-013-4688-0-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Zhou, XiaoPing verfasserin aut Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. energetic electron flux (dpeaa)DE-He213 chorus waves (dpeaa)DE-He213 wave-particle interaction (dpeaa)DE-He213 geomagnetic condition (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut He, YiHua verfasserin aut Yang, Chang verfasserin aut Zhou, QingHua verfasserin aut Zhang, ZeLong verfasserin aut Gao, ZhongLei verfasserin aut Ding, YuanHui verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 56(2013), 12 vom: 10. Okt., Seite 2006-2014 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:56 year:2013 number:12 day:10 month:10 pages:2006-2014 https://dx.doi.org/10.1007/s11430-013-4688-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 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_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 56 2013 12 10 10 2006-2014 |
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10.1007/s11430-013-4688-0 doi (DE-627)SPR019238606 (SPR)s11430-013-4688-0-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Zhou, XiaoPing verfasserin aut Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. energetic electron flux (dpeaa)DE-He213 chorus waves (dpeaa)DE-He213 wave-particle interaction (dpeaa)DE-He213 geomagnetic condition (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut He, YiHua verfasserin aut Yang, Chang verfasserin aut Zhou, QingHua verfasserin aut Zhang, ZeLong verfasserin aut Gao, ZhongLei verfasserin aut Ding, YuanHui verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 56(2013), 12 vom: 10. Okt., Seite 2006-2014 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:56 year:2013 number:12 day:10 month:10 pages:2006-2014 https://dx.doi.org/10.1007/s11430-013-4688-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 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_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 56 2013 12 10 10 2006-2014 |
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10.1007/s11430-013-4688-0 doi (DE-627)SPR019238606 (SPR)s11430-013-4688-0-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Zhou, XiaoPing verfasserin aut Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. energetic electron flux (dpeaa)DE-He213 chorus waves (dpeaa)DE-He213 wave-particle interaction (dpeaa)DE-He213 geomagnetic condition (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut He, YiHua verfasserin aut Yang, Chang verfasserin aut Zhou, QingHua verfasserin aut Zhang, ZeLong verfasserin aut Gao, ZhongLei verfasserin aut Ding, YuanHui verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 56(2013), 12 vom: 10. Okt., Seite 2006-2014 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:56 year:2013 number:12 day:10 month:10 pages:2006-2014 https://dx.doi.org/10.1007/s11430-013-4688-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 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_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 56 2013 12 10 10 2006-2014 |
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10.1007/s11430-013-4688-0 doi (DE-627)SPR019238606 (SPR)s11430-013-4688-0-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Zhou, XiaoPing verfasserin aut Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. energetic electron flux (dpeaa)DE-He213 chorus waves (dpeaa)DE-He213 wave-particle interaction (dpeaa)DE-He213 geomagnetic condition (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut He, YiHua verfasserin aut Yang, Chang verfasserin aut Zhou, QingHua verfasserin aut Zhang, ZeLong verfasserin aut Gao, ZhongLei verfasserin aut Ding, YuanHui verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 56(2013), 12 vom: 10. Okt., Seite 2006-2014 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:56 year:2013 number:12 day:10 month:10 pages:2006-2014 https://dx.doi.org/10.1007/s11430-013-4688-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 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_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 56 2013 12 10 10 2006-2014 |
| allfieldsSound |
10.1007/s11430-013-4688-0 doi (DE-627)SPR019238606 (SPR)s11430-013-4688-0-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Zhou, XiaoPing verfasserin aut Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions 2013 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. energetic electron flux (dpeaa)DE-He213 chorus waves (dpeaa)DE-He213 wave-particle interaction (dpeaa)DE-He213 geomagnetic condition (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut He, YiHua verfasserin aut Yang, Chang verfasserin aut Zhou, QingHua verfasserin aut Zhang, ZeLong verfasserin aut Gao, ZhongLei verfasserin aut Ding, YuanHui verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 56(2013), 12 vom: 10. Okt., Seite 2006-2014 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:56 year:2013 number:12 day:10 month:10 pages:2006-2014 https://dx.doi.org/10.1007/s11430-013-4688-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 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_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 56 2013 12 10 10 2006-2014 |
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Zhou, XiaoPing @@aut@@ Xiao, FuLiang @@aut@@ He, YiHua @@aut@@ Yang, Chang @@aut@@ Zhou, QingHua @@aut@@ Zhang, ZeLong @@aut@@ Gao, ZhongLei @@aut@@ Ding, YuanHui @@aut@@ |
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Zhou, XiaoPing |
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responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions |
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Responses of geostationary orbit energetic electron fluxes to chorus waves under different geomagnetic conditions |
| abstract |
Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. |
| abstractGer |
Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. |
| abstract_unstemmed |
Abstract We investigate the flux evolution of geostationary orbit energetic electrons during a strong storm on 24 August 2005 (event A, the storm index Dst<-200 nT, the average substorm index AE=436 nT) and a weak storm on 28 October 2006 (event B, Dst>-50 nT, average AE=320 nT). Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. Our results provide new observational support for chorus-driven acceleration of radiation belt energetic electrons. |
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Data collected by LANL and GOES-12 satellites show that energetic electron fluxes increase by a factor of 10 during the recovery phase compared to the prestorm level for both events A and B. As the substorm continued, the Cluster C4 satellite observed strong whistler-mode chorus waves (with spectral density approaching $ 10^{−5} $ $ nT^{2} $/Hz). The wave amplitude correlates with the substorm AE index, but is less correlated with the storm Dst index. Using a Gaussian distribution fitting method, we solve the Fokker-Planck diffusion equation governing the wave-particle interaction. Numerical results demonstrate that chorus waves efficiently accelerate ∼1 MeV energetic electrons, particularly at high pitch angles. The calculated acceleration time scale and amplitude are comparable to observations. 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