The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures
We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ferradas, C.P. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021transfer abstract |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: List of Referees - 2014, Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:216 ; year:2021 ; pages:0 |
| Links: |
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| DOI / URN: |
10.1016/j.jastp.2020.105534 |
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ELV053495136 |
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| 245 | 1 | 4 | |a The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures |
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| 520 | |a We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. | ||
| 520 | |a We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. | ||
| 650 | 7 | |a Ion nose structure |2 Elsevier | |
| 650 | 7 | |a Convection electric field |2 Elsevier | |
| 650 | 7 | |a Ion injection |2 Elsevier | |
| 650 | 7 | |a Van allen probes |2 Elsevier | |
| 700 | 1 | |a Reeves, G.D. |4 oth | |
| 700 | 1 | |a Larsen, B.A. |4 oth | |
| 700 | 1 | |a Skoug, R.M. |4 oth | |
| 700 | 1 | |a Zhang, J.-C. |4 oth | |
| 700 | 1 | |a Funsten, H.O. |4 oth | |
| 700 | 1 | |a Spence, H.E. |4 oth | |
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10.1016/j.jastp.2020.105534 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001336.pica (DE-627)ELV053495136 (ELSEVIER)S1364-6826(20)30333-3 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Ferradas, C.P. verfasserin aut The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. Ion nose structure Elsevier Convection electric field Elsevier Ion injection Elsevier Van allen probes Elsevier Reeves, G.D. oth Larsen, B.A. oth Skoug, R.M. oth Zhang, J.-C. oth Funsten, H.O. oth Spence, H.E. oth Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:216 year:2021 pages:0 https://doi.org/10.1016/j.jastp.2020.105534 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 216 2021 0 |
| spelling |
10.1016/j.jastp.2020.105534 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001336.pica (DE-627)ELV053495136 (ELSEVIER)S1364-6826(20)30333-3 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Ferradas, C.P. verfasserin aut The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. Ion nose structure Elsevier Convection electric field Elsevier Ion injection Elsevier Van allen probes Elsevier Reeves, G.D. oth Larsen, B.A. oth Skoug, R.M. oth Zhang, J.-C. oth Funsten, H.O. oth Spence, H.E. oth Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:216 year:2021 pages:0 https://doi.org/10.1016/j.jastp.2020.105534 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 216 2021 0 |
| allfields_unstemmed |
10.1016/j.jastp.2020.105534 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001336.pica (DE-627)ELV053495136 (ELSEVIER)S1364-6826(20)30333-3 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Ferradas, C.P. verfasserin aut The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. Ion nose structure Elsevier Convection electric field Elsevier Ion injection Elsevier Van allen probes Elsevier Reeves, G.D. oth Larsen, B.A. oth Skoug, R.M. oth Zhang, J.-C. oth Funsten, H.O. oth Spence, H.E. oth Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:216 year:2021 pages:0 https://doi.org/10.1016/j.jastp.2020.105534 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 216 2021 0 |
| allfieldsGer |
10.1016/j.jastp.2020.105534 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001336.pica (DE-627)ELV053495136 (ELSEVIER)S1364-6826(20)30333-3 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Ferradas, C.P. verfasserin aut The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. Ion nose structure Elsevier Convection electric field Elsevier Ion injection Elsevier Van allen probes Elsevier Reeves, G.D. oth Larsen, B.A. oth Skoug, R.M. oth Zhang, J.-C. oth Funsten, H.O. oth Spence, H.E. oth Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:216 year:2021 pages:0 https://doi.org/10.1016/j.jastp.2020.105534 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 216 2021 0 |
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10.1016/j.jastp.2020.105534 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001336.pica (DE-627)ELV053495136 (ELSEVIER)S1364-6826(20)30333-3 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Ferradas, C.P. verfasserin aut The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures 2021transfer abstract nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. Ion nose structure Elsevier Convection electric field Elsevier Ion injection Elsevier Van allen probes Elsevier Reeves, G.D. oth Larsen, B.A. oth Skoug, R.M. oth Zhang, J.-C. oth Funsten, H.O. oth Spence, H.E. oth Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:216 year:2021 pages:0 https://doi.org/10.1016/j.jastp.2020.105534 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 216 2021 0 |
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effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures |
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The effects of the location and the timing of local convection electric field enhancements in the formation of ion multiple-nose structures |
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We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. |
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We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. |
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We investigate the formation of He+ and O+ multiple-nose structures observed by the Helium, Oxygen, Proton, and Electron instrument onboard Van Allen Probes A on December 2, 2012. Previous studies have suggested that multiple-nose structures can be formed by changes in the convection electric field. However, the specifics of how these changes can produce multiple-nose structures have been left unresolved. In this study, we simulate ions as they drift from the plasma sheet into the inner magnetosphere and find that the multiple-nose structures were created by the overlap of a nose structure and a spectral gap in the energy-time spectrograms of the measured ion fluxes. Ion drift path tracings show that the spectral gap was produced by an enhancement of the convection electric field several hours before. Furthermore, the simulations reveal new insight of how the timing and location of the local electric field enhancements play a key role in the formation of the observed multiple noses. |
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