Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves

Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during t...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	He, ZhaoGuo [verfasserIn] Xiao, FuLiang [verfasserIn] Zong, QiuGang [verfasserIn] Wang, YongFu [verfasserIn] Chen, LiangXu [verfasserIn] Yue, Chao [verfasserIn] Zhang, Sai [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2011

Schlagwörter:	outer radiation belt energetic electron chorus

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 1997, 54(2011), 8 vom: 24. Juni, Seite 2209-2216
Übergeordnetes Werk:	volume:54 ; year:2011 ; number:8 ; day:24 ; month:06 ; pages:2209-2216

Links:	Volltext

DOI / URN:	10.1007/s11431-011-4445-6

Katalog-ID:	SPR019271735

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520			\|a Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms.
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allfields	10.1007/s11431-011-4445-6 doi (DE-627)SPR019271735 (SPR)s11431-011-4445-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl He, ZhaoGuo verfasserin aut Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms. outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Chen, LiangXu verfasserin aut Yue, Chao verfasserin aut Zhang, Sai verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 8 vom: 24. Juni, Seite 2209-2216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216 https://dx.doi.org/10.1007/s11431-011-4445-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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 50.00 ASE AR 54 2011 8 24 06 2209-2216
spelling	10.1007/s11431-011-4445-6 doi (DE-627)SPR019271735 (SPR)s11431-011-4445-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl He, ZhaoGuo verfasserin aut Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms. outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Chen, LiangXu verfasserin aut Yue, Chao verfasserin aut Zhang, Sai verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 8 vom: 24. Juni, Seite 2209-2216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216 https://dx.doi.org/10.1007/s11431-011-4445-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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 50.00 ASE AR 54 2011 8 24 06 2209-2216
allfields_unstemmed	10.1007/s11431-011-4445-6 doi (DE-627)SPR019271735 (SPR)s11431-011-4445-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl He, ZhaoGuo verfasserin aut Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms. outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Chen, LiangXu verfasserin aut Yue, Chao verfasserin aut Zhang, Sai verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 8 vom: 24. Juni, Seite 2209-2216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216 https://dx.doi.org/10.1007/s11431-011-4445-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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 50.00 ASE AR 54 2011 8 24 06 2209-2216
allfieldsGer	10.1007/s11431-011-4445-6 doi (DE-627)SPR019271735 (SPR)s11431-011-4445-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl He, ZhaoGuo verfasserin aut Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms. outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Chen, LiangXu verfasserin aut Yue, Chao verfasserin aut Zhang, Sai verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 8 vom: 24. Juni, Seite 2209-2216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216 https://dx.doi.org/10.1007/s11431-011-4445-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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 50.00 ASE AR 54 2011 8 24 06 2209-2216
allfieldsSound	10.1007/s11431-011-4445-6 doi (DE-627)SPR019271735 (SPR)s11431-011-4445-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl He, ZhaoGuo verfasserin aut Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms. outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213 Xiao, FuLiang verfasserin aut Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Chen, LiangXu verfasserin aut Yue, Chao verfasserin aut Zhang, Sai verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 54(2011), 8 vom: 24. Juni, Seite 2209-2216 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216 https://dx.doi.org/10.1007/s11431-011-4445-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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 50.00 ASE AR 54 2011 8 24 06 2209-2216
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source	Enthalten in Science in China 54(2011), 8 vom: 24. Juni, Seite 2209-2216 volume:54 year:2011 number:8 day:24 month:06 pages:2209-2216
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topic_facet	outer radiation belt energetic electron chorus
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author	He, ZhaoGuo
spellingShingle	He, ZhaoGuo ddc 600 bkl 50.00 misc outer radiation belt misc energetic electron misc chorus Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
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topic_title	600 ASE 50.00 bkl Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves outer radiation belt (dpeaa)DE-He213 energetic electron (dpeaa)DE-He213 chorus (dpeaa)DE-He213
topic	ddc 600 bkl 50.00 misc outer radiation belt misc energetic electron misc chorus
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title	Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
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title_full	Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
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author_browse	He, ZhaoGuo Xiao, FuLiang Zong, QiuGang Wang, YongFu Chen, LiangXu Yue, Chao Zhang, Sai
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title_sort	multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
title_auth	Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
abstract	Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms.
abstractGer	Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms.
abstract_unstemmed	Abstract The evolution of energetic outer zone electron fluxes during the strong magnetic storm on September 28, 2002 is investigated based on the observations of SAMPEX and GOES-10 satellites. The observations of both satellites showed that energetic electron fluxes increased significantly during the storm recovery phase, and reached the maximum on October 6. The 1.5–14 MeV and 2.5–14 MeV electron fluxes observed by SAMPEX peaked around L=3.5 with values of 6×$ 10^{2} $ $ cm^{−2} $ $ s^{−1} %$ sr^{−1} $ $ keV^{−1} $ and 5×$ 10^{3} $ $ cm^{−2} $ $ s^{−1} $ $ sr^{−1} $ $ keV^{−1} $, which were about 10 and 8 times the pre-storm values. At the geostationary orbit, the >0.6 MeV and >2 MeV electron fluxes observed by GOES-10 showed enhancement up to 50 and 30 times. The plasma parameters and whistler-mode chorus waves in the outer radiation belt are also analyzed based on the data from Cluster C3 satellite. Cluster C3 satellite went through the outer radiation belt twice from 1 October to 4 October, and observed whistler-mode chorus waves with high intensity ($ 10^{−5} $–$ 10^{−4} $ $ nT^{2} $ $ Hz^{−1} $). Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. The current observations and calculations provide new evidence for that the gyro-resonance with chorus waves contribute significantly to the buildup of energetic outer zone electron fluxes during storms.
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title_short	Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves
url	https://dx.doi.org/10.1007/s11431-011-4445-6
remote_bool	true
author2	Xiao, FuLiang Zong, QiuGang Wang, YongFu Chen, LiangXu Yue, Chao Zhang, Sai
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up_date	2024-07-04T00:54:42.416Z
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Numerical calculations indicated that the observed chorus waves were in gyro-resonance with the radiation belt electrons. 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Multi-satellite observations on the storm-time enhancements of energetic outer zone electron fluxes driven by chorus waves

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