Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt

Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below...
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Autor*in:	Wang, YongFu [verfasserIn] Zong, QiuGang [verfasserIn] Zhou, XuZhi [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2017

Schlagwörter:	inner radiation belt ion zebra stripes energetic ions energetic electrons

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 1997, 61(2017), 4 vom: 17. Aug., Seite 623-632
Übergeordnetes Werk:	volume:61 ; year:2017 ; number:4 ; day:17 ; month:08 ; pages:623-632

Links:	Volltext

DOI / URN:	10.1007/s11431-016-9087-x

Katalog-ID:	SPR019292961

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520			\|a Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current.
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allfields	10.1007/s11431-016-9087-x doi (DE-627)SPR019292961 (SPR)s11431-016-9087-x-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Wang, YongFu verfasserin aut Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current. inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Zhou, XuZhi verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 61(2017), 4 vom: 17. Aug., Seite 623-632 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:61 year:2017 number:4 day:17 month:08 pages:623-632 https://dx.doi.org/10.1007/s11431-016-9087-x 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 61 2017 4 17 08 623-632
spelling	10.1007/s11431-016-9087-x doi (DE-627)SPR019292961 (SPR)s11431-016-9087-x-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Wang, YongFu verfasserin aut Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current. inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Zhou, XuZhi verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 61(2017), 4 vom: 17. Aug., Seite 623-632 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:61 year:2017 number:4 day:17 month:08 pages:623-632 https://dx.doi.org/10.1007/s11431-016-9087-x 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 61 2017 4 17 08 623-632
allfields_unstemmed	10.1007/s11431-016-9087-x doi (DE-627)SPR019292961 (SPR)s11431-016-9087-x-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Wang, YongFu verfasserin aut Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current. inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Zhou, XuZhi verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 61(2017), 4 vom: 17. Aug., Seite 623-632 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:61 year:2017 number:4 day:17 month:08 pages:623-632 https://dx.doi.org/10.1007/s11431-016-9087-x 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 61 2017 4 17 08 623-632
allfieldsGer	10.1007/s11431-016-9087-x doi (DE-627)SPR019292961 (SPR)s11431-016-9087-x-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Wang, YongFu verfasserin aut Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current. inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Zhou, XuZhi verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 61(2017), 4 vom: 17. Aug., Seite 623-632 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:61 year:2017 number:4 day:17 month:08 pages:623-632 https://dx.doi.org/10.1007/s11431-016-9087-x 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 61 2017 4 17 08 623-632
allfieldsSound	10.1007/s11431-016-9087-x doi (DE-627)SPR019292961 (SPR)s11431-016-9087-x-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Wang, YongFu verfasserin aut Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current. inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Zhou, XuZhi verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 61(2017), 4 vom: 17. Aug., Seite 623-632 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:61 year:2017 number:4 day:17 month:08 pages:623-632 https://dx.doi.org/10.1007/s11431-016-9087-x 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 61 2017 4 17 08 623-632
language	English
source	Enthalten in Science in China 61(2017), 4 vom: 17. Aug., Seite 623-632 volume:61 year:2017 number:4 day:17 month:08 pages:623-632
sourceStr	Enthalten in Science in China 61(2017), 4 vom: 17. Aug., Seite 623-632 volume:61 year:2017 number:4 day:17 month:08 pages:623-632
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topic_facet	inner radiation belt ion zebra stripes energetic ions energetic electrons
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authorswithroles_txt_mv	Wang, YongFu @@aut@@ Zong, QiuGang @@aut@@ Zhou, XuZhi @@aut@@
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author	Wang, YongFu
spellingShingle	Wang, YongFu ddc 600 bkl 50.00 misc inner radiation belt misc ion zebra stripes misc energetic ions misc energetic electrons Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
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topic_title	600 ASE 50.00 bkl Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt inner radiation belt (dpeaa)DE-He213 ion zebra stripes (dpeaa)DE-He213 energetic ions (dpeaa)DE-He213 energetic electrons (dpeaa)DE-He213
topic	ddc 600 bkl 50.00 misc inner radiation belt misc ion zebra stripes misc energetic ions misc energetic electrons
topic_unstemmed	ddc 600 bkl 50.00 misc inner radiation belt misc ion zebra stripes misc energetic ions misc energetic electrons
topic_browse	ddc 600 bkl 50.00 misc inner radiation belt misc ion zebra stripes misc energetic ions misc energetic electrons
format_facet	Elektronische Aufsätze Aufsätze Elektronische Ressource
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title	Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
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title_full	Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
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author_browse	Wang, YongFu Zong, QiuGang Zhou, XuZhi
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title_sort	test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
title_auth	Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
abstract	Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current.
abstractGer	Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current.
abstract_unstemmed	Abstract During February 15–16, 2014, the energetic electron spectrogram for four successive inner radiation belt crossing show clearly the electron zebra structures and their time evolution which last for about 17 h. Unfortunately, the time of flight (TOF) in RBSPICE measurement is turned off below 3RE, and the ion measurement is contaminated by electrons. Thus in this study we studied the differences between the ion and electron zebra stripe structures and their time evolution using simple theory and test particle simulation, combining the electron measurement from RBSIPICE onboard Van Allen Probes. Theoretical analysis predicts that the ion zebra stripe structures should lie at a higher energy range than the corresponding electron zebra stripe structures due to that the directions of gradient B drift and corotation E×B drift are the same for electrons while opposite for ions. Test particle simulation with the dipole magnetic field and Volland-Stern electric field model have shown that the ion and electron zebra stripe structures could be produced by the convection electric field penetrating into the inner magnetosphere in this event, with their time evolution determined by total drift velocity that are different for ions and electrons. The predicted differences between the ion and electron zebra stripe structures are partially verified through observation. The ion zebra stripe structures could have potential influence to the ring current.
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title_short	Test particle simulation on the ion and electron zebra stripes and their time evolution in inner radiation belt
url	https://dx.doi.org/10.1007/s11431-016-9087-x
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doi_str	10.1007/s11431-016-9087-x
up_date	2024-07-04T00:59:31.131Z
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