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Accelerated electrons in the LLBL as observed by Interball on February 15, 1996
We analyze electron observations in the low latitude boundary layer (LLBL) with the Interball Tail satellite under a southward–duskward magnetosheath magnetic field. It is well known that the LLBL is characterized by bi-directional electron velocity distributions, which leads to an enhancement of th...
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Published in: | Planetary and space science 2005, Vol.53 (1), p.149-156 |
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Main Authors: | , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | We analyze electron observations in the low latitude boundary layer (LLBL) with the Interball Tail satellite under a southward–duskward magnetosheath magnetic field. It is well known that the LLBL is characterized by bi-directional electron velocity distributions, which leads to an enhancement of the electron temperature. It is also well known that the electron temperature within the LLBL increases with a decrease of the LLBL number density. We found that the parallel electron velocity distribution changes self-consistently with varying number density. Namely, the shape of the parallel velocity distribution does not change in a log–log scale indicating that electron parallel velocities increase proportionately as the number density decreases. This suggests a possible role for the Fermi acceleration mechanism. We also discuss the LLBL topology that is provided by electron velocity distributions. |
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ISSN: | 0032-0633 1873-5088 |
DOI: | 10.1016/j.pss.2004.09.039 |