Energetic electrons along the high-latitude magnetopause

A case study is presented to determine the source of the energetic electron layer frequently observed along the high-latitude magnetopause. Measurements by the Cluster spacecraft show bursts of field-aligned electrons occurring during time periods with high potential for dayside reconnection. The...

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Main Authors: B. M. Walsh, S. E. Haaland, P. W. Daly, E. A. Kronberg, T. A. Fritz
Format: Article
Language:English
Published: Copernicus Publications 2012-06-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/30/1003/2012/angeo-30-1003-2012.pdf
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spelling doaj-c000e3325a39440bb8347d368f3e2a5f2020-11-24T22:10:09ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762012-06-01301003101310.5194/angeo-30-1003-2012Energetic electrons along the high-latitude magnetopauseB. M. Walsh0B. M. Walsh1S. E. Haaland2S. E. Haaland3P. W. Daly4E. A. Kronberg5T. A. Fritz6Center for Space Physics, Boston University, Boston, MA, USANASA, Goddard Space Flight Center, Greenbelt, MD, USAMax Planck Institute for Solar System Research, Lindau, GermanyDepartment of Physics and Technology, University of Bergen, Bergen, NorwayMax Planck Institute for Solar System Research, Lindau, GermanyMax Planck Institute for Solar System Research, Lindau, GermanyCenter for Space Physics, Boston University, Boston, MA, USAA case study is presented to determine the source of the energetic electron layer frequently observed along the high-latitude magnetopause. Measurements by the Cluster spacecraft show bursts of field-aligned electrons occurring during time periods with high potential for dayside reconnection. These properties are compared with the expected signatures from several sources including escape from the exterior cusp, acceleration in a reconnection region, and release from the dayside trapping region through reconnection. The observed properties are most consistent with the electrons being released from the magnetosphere due to reconnection. In this model the electrons would flow along the newly reconnected IMF draped along the magnetopause and propagate along the high-latitude magnetopause. These observations demonstrate an active source for populating the energetic particle layer frequently observed along and just outside the high-latitude magnetopause.https://www.ann-geophys.net/30/1003/2012/angeo-30-1003-2012.pdf
collection DOAJ
language English
format Article
sources DOAJ
author B. M. Walsh
B. M. Walsh
S. E. Haaland
S. E. Haaland
P. W. Daly
E. A. Kronberg
T. A. Fritz
spellingShingle B. M. Walsh
B. M. Walsh
S. E. Haaland
S. E. Haaland
P. W. Daly
E. A. Kronberg
T. A. Fritz
Energetic electrons along the high-latitude magnetopause
Annales Geophysicae
author_facet B. M. Walsh
B. M. Walsh
S. E. Haaland
S. E. Haaland
P. W. Daly
E. A. Kronberg
T. A. Fritz
author_sort B. M. Walsh
title Energetic electrons along the high-latitude magnetopause
title_short Energetic electrons along the high-latitude magnetopause
title_full Energetic electrons along the high-latitude magnetopause
title_fullStr Energetic electrons along the high-latitude magnetopause
title_full_unstemmed Energetic electrons along the high-latitude magnetopause
title_sort energetic electrons along the high-latitude magnetopause
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2012-06-01
description A case study is presented to determine the source of the energetic electron layer frequently observed along the high-latitude magnetopause. Measurements by the Cluster spacecraft show bursts of field-aligned electrons occurring during time periods with high potential for dayside reconnection. These properties are compared with the expected signatures from several sources including escape from the exterior cusp, acceleration in a reconnection region, and release from the dayside trapping region through reconnection. The observed properties are most consistent with the electrons being released from the magnetosphere due to reconnection. In this model the electrons would flow along the newly reconnected IMF draped along the magnetopause and propagate along the high-latitude magnetopause. These observations demonstrate an active source for populating the energetic particle layer frequently observed along and just outside the high-latitude magnetopause.
url https://www.ann-geophys.net/30/1003/2012/angeo-30-1003-2012.pdf
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AT pwdaly energeticelectronsalongthehighlatitudemagnetopause
AT eakronberg energeticelectronsalongthehighlatitudemagnetopause
AT tafritz energeticelectronsalongthehighlatitudemagnetopause
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