Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt

Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using...
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Autor*in:	Guan, ChunYi [verfasserIn] Shang, XiongJun [verfasserIn] Xie, YanQiong [verfasserIn] Yang, Chang [verfasserIn] Zhang, Sai [verfasserIn] Liu, Si [verfasserIn] Xiao, FuLiang [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Schlagwörter:	EMIC waves instability nightside radiation belt Van Allen Probes coordinated observations

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 1997, 63(2020), 11 vom: 13. Juli, Seite 2369-2374
Übergeordnetes Werk:	volume:63 ; year:2020 ; number:11 ; day:13 ; month:07 ; pages:2369-2374

Links:	Volltext

DOI / URN:	10.1007/s11431-019-1545-6

Katalog-ID:	SPR041917030

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520			\|a Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions.
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allfields	10.1007/s11431-019-1545-6 doi (DE-627)SPR041917030 (SPR)s11431-019-1545-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Guan, ChunYi verfasserin aut Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions. EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213 Shang, XiongJun verfasserin aut Xie, YanQiong verfasserin aut Yang, Chang verfasserin aut Zhang, Sai verfasserin aut Liu, Si verfasserin aut Xiao, FuLiang verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 63(2020), 11 vom: 13. Juli, Seite 2369-2374 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374 https://dx.doi.org/10.1007/s11431-019-1545-6 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 63 2020 11 13 07 2369-2374
spelling	10.1007/s11431-019-1545-6 doi (DE-627)SPR041917030 (SPR)s11431-019-1545-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Guan, ChunYi verfasserin aut Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions. EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213 Shang, XiongJun verfasserin aut Xie, YanQiong verfasserin aut Yang, Chang verfasserin aut Zhang, Sai verfasserin aut Liu, Si verfasserin aut Xiao, FuLiang verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 63(2020), 11 vom: 13. Juli, Seite 2369-2374 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374 https://dx.doi.org/10.1007/s11431-019-1545-6 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 63 2020 11 13 07 2369-2374
allfields_unstemmed	10.1007/s11431-019-1545-6 doi (DE-627)SPR041917030 (SPR)s11431-019-1545-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Guan, ChunYi verfasserin aut Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions. EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213 Shang, XiongJun verfasserin aut Xie, YanQiong verfasserin aut Yang, Chang verfasserin aut Zhang, Sai verfasserin aut Liu, Si verfasserin aut Xiao, FuLiang verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 63(2020), 11 vom: 13. Juli, Seite 2369-2374 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374 https://dx.doi.org/10.1007/s11431-019-1545-6 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 63 2020 11 13 07 2369-2374
allfieldsGer	10.1007/s11431-019-1545-6 doi (DE-627)SPR041917030 (SPR)s11431-019-1545-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Guan, ChunYi verfasserin aut Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions. EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213 Shang, XiongJun verfasserin aut Xie, YanQiong verfasserin aut Yang, Chang verfasserin aut Zhang, Sai verfasserin aut Liu, Si verfasserin aut Xiao, FuLiang verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 63(2020), 11 vom: 13. Juli, Seite 2369-2374 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374 https://dx.doi.org/10.1007/s11431-019-1545-6 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 63 2020 11 13 07 2369-2374
allfieldsSound	10.1007/s11431-019-1545-6 doi (DE-627)SPR041917030 (SPR)s11431-019-1545-6-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Guan, ChunYi verfasserin aut Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions. EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213 Shang, XiongJun verfasserin aut Xie, YanQiong verfasserin aut Yang, Chang verfasserin aut Zhang, Sai verfasserin aut Liu, Si verfasserin aut Xiao, FuLiang verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 63(2020), 11 vom: 13. Juli, Seite 2369-2374 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374 https://dx.doi.org/10.1007/s11431-019-1545-6 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 63 2020 11 13 07 2369-2374
language	English
source	Enthalten in Science in China 63(2020), 11 vom: 13. Juli, Seite 2369-2374 volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374
sourceStr	Enthalten in Science in China 63(2020), 11 vom: 13. Juli, Seite 2369-2374 volume:63 year:2020 number:11 day:13 month:07 pages:2369-2374
format_phy_str_mv	Article
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topic_facet	EMIC waves instability nightside radiation belt Van Allen Probes coordinated observations
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container_title	Science in China
authorswithroles_txt_mv	Guan, ChunYi @@aut@@ Shang, XiongJun @@aut@@ Xie, YanQiong @@aut@@ Yang, Chang @@aut@@ Zhang, Sai @@aut@@ Liu, Si @@aut@@ Xiao, FuLiang @@aut@@
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author	Guan, ChunYi
spellingShingle	Guan, ChunYi ddc 600 bkl 50.00 misc EMIC waves instability misc nightside radiation belt misc Van Allen Probes misc coordinated observations Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt
authorStr	Guan, ChunYi
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topic_title	600 ASE 50.00 bkl Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt EMIC waves instability (dpeaa)DE-He213 nightside radiation belt (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 coordinated observations (dpeaa)DE-He213
topic	ddc 600 bkl 50.00 misc EMIC waves instability misc nightside radiation belt misc Van Allen Probes misc coordinated observations
topic_unstemmed	ddc 600 bkl 50.00 misc EMIC waves instability misc nightside radiation belt misc Van Allen Probes misc coordinated observations
topic_browse	ddc 600 bkl 50.00 misc EMIC waves instability misc nightside radiation belt misc Van Allen Probes misc coordinated observations
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title	Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt
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title_full	Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt
author_sort	Guan, ChunYi
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author_browse	Guan, ChunYi Shang, XiongJun Xie, YanQiong Yang, Chang Zhang, Sai Liu, Si Xiao, FuLiang
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title_sort	generation of simultaneous $ h^{+} $ and $ he^{+} $ band emic waves in the nightside radiation belt
title_auth	Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt
abstract	Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions.
abstractGer	Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions.
abstract_unstemmed	Abstract Previous studies have shown that EMIC waves occur preferentially in the afternoon sector of the magnetosphere. Here we report obliquely propagating $ H^{+} $ and $ He^{+} $ band EMIC waves detected by Van Allen Probe B in the region of MLT=22.7–23.5 during the June 20, 2013 substorm. Using the correlated energetic proton data, we present continuous calculations on EMIC wave growth rates along the inward orbit in the region L=5.5−4.2. The modeled growth rate shows remarkable agreement with the observed double band EMIC waves in both temporal and spatial evolutions. The current results demonstrate that $ H^{+} $ and $ He^{+} $ band EMIC waves can be simultaneously excited in the midnight sector under appropriate conditions.
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title_short	Generation of simultaneous $ H^{+} $ and $ He^{+} $ band EMIC waves in the nightside radiation belt
url	https://dx.doi.org/10.1007/s11431-019-1545-6
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author2	Shang, XiongJun Xie, YanQiong Yang, Chang Zhang, Sai Liu, Si Xiao, FuLiang
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up_date	2024-07-04T00:08:12.099Z
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