Variations of the relativistic electron flux after a magnetospheric compression event
Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this even...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Chen, Zhe [verfasserIn] Chen, HongFei [verfasserIn] Li, YiFan [verfasserIn] Xiang, HongWen [verfasserIn] Yu, XiangQian [verfasserIn] Shi, WeiHong [verfasserIn] Hao, ZhiHua [verfasserIn] Zou, Hong [verfasserIn] Zou, JiQing [verfasserIn] Zhong, WeiYing [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Science in China - Heidelberg : Springer, 1997, 60(2017), 4 vom: 14. März, Seite 638-647 |
|---|---|
| Übergeordnetes Werk: |
volume:60 ; year:2017 ; number:4 ; day:14 ; month:03 ; pages:638-647 |
| Links: |
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| DOI / URN: |
10.1007/s11431-016-9008-3 |
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SPR019290926 |
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| 520 | |a Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. | ||
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10.1007/s11431-016-9008-3 doi (DE-627)SPR019290926 (SPR)s11431-016-9008-3-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Chen, Zhe verfasserin aut Variations of the relativistic electron flux after a magnetospheric compression event 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. outer radiation belt (dpeaa)DE-He213 high-energy electrons (dpeaa)DE-He213 medium-energy electrons (dpeaa)DE-He213 space environment (dpeaa)DE-He213 Chen, HongFei verfasserin aut Li, YiFan verfasserin aut Xiang, HongWen verfasserin aut Yu, XiangQian verfasserin aut Shi, WeiHong verfasserin aut Hao, ZhiHua verfasserin aut Zou, Hong verfasserin aut Zou, JiQing verfasserin aut Zhong, WeiYing verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 4 vom: 14. März, Seite 638-647 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:60 year:2017 number:4 day:14 month:03 pages:638-647 https://dx.doi.org/10.1007/s11431-016-9008-3 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 60 2017 4 14 03 638-647 |
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10.1007/s11431-016-9008-3 doi (DE-627)SPR019290926 (SPR)s11431-016-9008-3-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Chen, Zhe verfasserin aut Variations of the relativistic electron flux after a magnetospheric compression event 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. outer radiation belt (dpeaa)DE-He213 high-energy electrons (dpeaa)DE-He213 medium-energy electrons (dpeaa)DE-He213 space environment (dpeaa)DE-He213 Chen, HongFei verfasserin aut Li, YiFan verfasserin aut Xiang, HongWen verfasserin aut Yu, XiangQian verfasserin aut Shi, WeiHong verfasserin aut Hao, ZhiHua verfasserin aut Zou, Hong verfasserin aut Zou, JiQing verfasserin aut Zhong, WeiYing verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 4 vom: 14. März, Seite 638-647 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:60 year:2017 number:4 day:14 month:03 pages:638-647 https://dx.doi.org/10.1007/s11431-016-9008-3 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 60 2017 4 14 03 638-647 |
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10.1007/s11431-016-9008-3 doi (DE-627)SPR019290926 (SPR)s11431-016-9008-3-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Chen, Zhe verfasserin aut Variations of the relativistic electron flux after a magnetospheric compression event 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. outer radiation belt (dpeaa)DE-He213 high-energy electrons (dpeaa)DE-He213 medium-energy electrons (dpeaa)DE-He213 space environment (dpeaa)DE-He213 Chen, HongFei verfasserin aut Li, YiFan verfasserin aut Xiang, HongWen verfasserin aut Yu, XiangQian verfasserin aut Shi, WeiHong verfasserin aut Hao, ZhiHua verfasserin aut Zou, Hong verfasserin aut Zou, JiQing verfasserin aut Zhong, WeiYing verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 4 vom: 14. März, Seite 638-647 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:60 year:2017 number:4 day:14 month:03 pages:638-647 https://dx.doi.org/10.1007/s11431-016-9008-3 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 60 2017 4 14 03 638-647 |
| allfieldsGer |
10.1007/s11431-016-9008-3 doi (DE-627)SPR019290926 (SPR)s11431-016-9008-3-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Chen, Zhe verfasserin aut Variations of the relativistic electron flux after a magnetospheric compression event 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. outer radiation belt (dpeaa)DE-He213 high-energy electrons (dpeaa)DE-He213 medium-energy electrons (dpeaa)DE-He213 space environment (dpeaa)DE-He213 Chen, HongFei verfasserin aut Li, YiFan verfasserin aut Xiang, HongWen verfasserin aut Yu, XiangQian verfasserin aut Shi, WeiHong verfasserin aut Hao, ZhiHua verfasserin aut Zou, Hong verfasserin aut Zou, JiQing verfasserin aut Zhong, WeiYing verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 4 vom: 14. März, Seite 638-647 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:60 year:2017 number:4 day:14 month:03 pages:638-647 https://dx.doi.org/10.1007/s11431-016-9008-3 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 60 2017 4 14 03 638-647 |
| allfieldsSound |
10.1007/s11431-016-9008-3 doi (DE-627)SPR019290926 (SPR)s11431-016-9008-3-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Chen, Zhe verfasserin aut Variations of the relativistic electron flux after a magnetospheric compression event 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. outer radiation belt (dpeaa)DE-He213 high-energy electrons (dpeaa)DE-He213 medium-energy electrons (dpeaa)DE-He213 space environment (dpeaa)DE-He213 Chen, HongFei verfasserin aut Li, YiFan verfasserin aut Xiang, HongWen verfasserin aut Yu, XiangQian verfasserin aut Shi, WeiHong verfasserin aut Hao, ZhiHua verfasserin aut Zou, Hong verfasserin aut Zou, JiQing verfasserin aut Zhong, WeiYing verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 4 vom: 14. März, Seite 638-647 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:60 year:2017 number:4 day:14 month:03 pages:638-647 https://dx.doi.org/10.1007/s11431-016-9008-3 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 60 2017 4 14 03 638-647 |
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The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. 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Chen, Zhe |
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Chen, Zhe ddc 600 bkl 50.00 misc outer radiation belt misc high-energy electrons misc medium-energy electrons misc space environment Variations of the relativistic electron flux after a magnetospheric compression event |
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variations of the relativistic electron flux after a magnetospheric compression event |
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Variations of the relativistic electron flux after a magnetospheric compression event |
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Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. |
| abstractGer |
Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. |
| abstract_unstemmed |
Abstract On January 21, 2015, a sharp increase of the solar wind dynamic pressure impacted the magnetosphere. The magnetopause moved inward to the region L< 8 without causing a geomagnetic storm. The flux of the relativistic electrons in the outer radiation belt decreased by half during this event based on the observations of the particle radiation monitor (PRM) of the fourth of the China-Brazil Earth Resource Satellites (CBERS-4). The flux remained low for approximately 11 d; it did not recover after a small magnetic storm on January 26 but after a small magnetic storm on February 2. The loss and recovery of the relativistic electrons during this event are investigated using the PRM data, medium- and high-energy electron observations of NOAA-15 and the Van Allen Probes, medium-energy electron observations of GOES-13, and wave observations of the Van Allen Probes. This study shows that the loss of energetic electrons in this event is related to magnetospheric compression. The chorus waves accelerate the medium-energy electrons, which causes the recovery of relativistic electrons. The Van Allen Probes detected strong chorus waves in the region L = 3–6 from January 21 to February 2. However, the flux of medium-energy electrons was low in the region. This implies that the long-lasting lack of recovery of the relativistic electrons after this event is due to the lack of the medium-energy “seed” electrons. The medium-energy electrons in the outer radiation belt may be a clue to predict the recovery of relativistic electrons. |
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