The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves
The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers whic...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Drake, J. F [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Rechteinformationen: |
Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Geophysical research letters - Washington, DC : Union, 1974, 42(2015), 8, Seite 2563-2570 |
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| Übergeordnetes Werk: |
volume:42 ; year:2015 ; number:8 ; pages:2563-2570 |
| Links: |
|---|
| DOI / URN: |
10.1002/2015GL063528 |
|---|
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| 520 | |a The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front | ||
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| 650 | 4 | |a parallel electric fields | |
| 650 | 4 | |a precipitating electrons | |
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10.1002/2015GL063528 doi PQ20160617 (DE-627)OLC1964148049 (DE-599)GBVOLC1964148049 (PRQ)c2492-d85e7538fd42b518ce233af6c5a0d42db29480c56aacb4c3733e667e0f868760 (KEY)0026932820150000042000802563developmentofaburstyprecipitationfrontwithintensel DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Drake, J. F verfasserin aut The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. particle acceleration Earth's outer radiation belts parallel electric fields precipitating electrons Electric fields Agapitov, O. V oth Mozer, F. S oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 42(2015), 8, Seite 2563-2570 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:42 year:2015 number:8 pages:2563-2570 http://dx.doi.org/10.1002/2015GL063528 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 42 2015 8 2563-2570 |
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10.1002/2015GL063528 doi PQ20160617 (DE-627)OLC1964148049 (DE-599)GBVOLC1964148049 (PRQ)c2492-d85e7538fd42b518ce233af6c5a0d42db29480c56aacb4c3733e667e0f868760 (KEY)0026932820150000042000802563developmentofaburstyprecipitationfrontwithintensel DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Drake, J. F verfasserin aut The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. particle acceleration Earth's outer radiation belts parallel electric fields precipitating electrons Electric fields Agapitov, O. V oth Mozer, F. S oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 42(2015), 8, Seite 2563-2570 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:42 year:2015 number:8 pages:2563-2570 http://dx.doi.org/10.1002/2015GL063528 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 42 2015 8 2563-2570 |
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10.1002/2015GL063528 doi PQ20160617 (DE-627)OLC1964148049 (DE-599)GBVOLC1964148049 (PRQ)c2492-d85e7538fd42b518ce233af6c5a0d42db29480c56aacb4c3733e667e0f868760 (KEY)0026932820150000042000802563developmentofaburstyprecipitationfrontwithintensel DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Drake, J. F verfasserin aut The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. particle acceleration Earth's outer radiation belts parallel electric fields precipitating electrons Electric fields Agapitov, O. V oth Mozer, F. S oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 42(2015), 8, Seite 2563-2570 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:42 year:2015 number:8 pages:2563-2570 http://dx.doi.org/10.1002/2015GL063528 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 42 2015 8 2563-2570 |
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10.1002/2015GL063528 doi PQ20160617 (DE-627)OLC1964148049 (DE-599)GBVOLC1964148049 (PRQ)c2492-d85e7538fd42b518ce233af6c5a0d42db29480c56aacb4c3733e667e0f868760 (KEY)0026932820150000042000802563developmentofaburstyprecipitationfrontwithintensel DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Drake, J. F verfasserin aut The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. particle acceleration Earth's outer radiation belts parallel electric fields precipitating electrons Electric fields Agapitov, O. V oth Mozer, F. S oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 42(2015), 8, Seite 2563-2570 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:42 year:2015 number:8 pages:2563-2570 http://dx.doi.org/10.1002/2015GL063528 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 42 2015 8 2563-2570 |
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10.1002/2015GL063528 doi PQ20160617 (DE-627)OLC1964148049 (DE-599)GBVOLC1964148049 (PRQ)c2492-d85e7538fd42b518ce233af6c5a0d42db29480c56aacb4c3733e667e0f868760 (KEY)0026932820150000042000802563developmentofaburstyprecipitationfrontwithintensel DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Drake, J. F verfasserin aut The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front Nutzungsrecht: © 2015. American Geophysical Union. All Rights Reserved. particle acceleration Earth's outer radiation belts parallel electric fields precipitating electrons Electric fields Agapitov, O. V oth Mozer, F. S oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 42(2015), 8, Seite 2563-2570 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:42 year:2015 number:8 pages:2563-2570 http://dx.doi.org/10.1002/2015GL063528 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 42 2015 8 2563-2570 |
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The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves |
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| title_full |
The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves |
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Drake, J. F |
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Geophysical research letters |
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Drake, J. F |
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Drake, J. F |
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10.1002/2015GL063528 |
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550 |
| title_sort |
development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves |
| title_auth |
The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves |
| abstract |
The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front |
| abstractGer |
The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front |
| abstract_unstemmed |
The dynamics and structure of whistler turbulence relevant to electron acceleration in the Earth's outer radiation belt are explored with simulations and comparisons with observations. An initial state with an electron temperature anisotropy in a spatially localized domain drives whistlers which scatter electrons. An outward propagating front of whistlers and hot electrons nonlinearly evolves to form regions of intense parallel electric field with structure similar to observations. The precipitating hot electrons propagate away from the source region in intense bunches rather than as a smooth flux. Electron beams are generated by anisotropy‐driven whistler waves Electron beams drive localized parallel electric fields with structure similar to VAP observations Parallel electric fields trap electrons to form a bursty precipitation front |
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| title_short |
The development of a bursty precipitation front with intense localized parallel electric fields driven by whistler waves |
| url |
http://dx.doi.org/10.1002/2015GL063528 http://onlinelibrary.wiley.com/doi/10.1002/2015GL063528/abstract http://search.proquest.com/docview/1681021737 |
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Agapitov, O. V Mozer, F. S |
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