Electron velocity distribution and lion roars in the magnetosheath

Whistler waves which are termed "lion roars" in the magnetosheath are studied using data obtained by the Spectrum Analyser (SA) of the Spatio-Temporal Analysis of Field Fluctuations (STAFF) experiment aboard Cluster. Kinetic theory is then employed to obtain the theoretical expression...

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Main Authors: W. Masood, S. J. Schwartz, M. Maksimovic, A. N. Fazakerley
Format: Article
Language:English
Published: Copernicus Publications 2006-07-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/24/1725/2006/angeo-24-1725-2006.pdf
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author W. Masood
W. Masood
W. Masood
S. J. Schwartz
M. Maksimovic
A. N. Fazakerley
author_facet W. Masood
W. Masood
W. Masood
S. J. Schwartz
M. Maksimovic
A. N. Fazakerley
author_sort W. Masood
collection DOAJ
description Whistler waves which are termed "lion roars" in the magnetosheath are studied using data obtained by the Spectrum Analyser (SA) of the Spatio-Temporal Analysis of Field Fluctuations (STAFF) experiment aboard Cluster. Kinetic theory is then employed to obtain the theoretical expression for the whistler wave with electron temperature anisotropy which is believed to trigger lion roars in the magnetosheath. This allows us to compare theory and data. This paper for the first time studies the details of the electron velocity distribution function as measured by the Plasma Electron And Current Experiment (PEACE) in order to investigate the underlying causes for the different types of lion roars found in the data. Our results show that while some instances of lion roars could be locally generated, the source of others must be more remote regions of the magnetosheath.
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spelling doaj.art-30d8b851479a4c5db83f8841331f42692022-12-22T03:45:22ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762006-07-01241725173510.5194/angeo-24-1725-2006Electron velocity distribution and lion roars in the magnetosheathW. Masood0W. Masood1W. Masood2S. J. Schwartz3M. Maksimovic4A. N. Fazakerley5Government College University (GCU), Lahore, PakistanPRD, PINSTECH, P.O.Nilore, Islamabad, PakistanAstronomy Unit, Queen Mary, University of London, UKThe Blackett Laboratory, Imperial College London, UKDESPA, Observatoire de Paris, FranceMullard Space Science Laboratory, University College London, UKWhistler waves which are termed "lion roars" in the magnetosheath are studied using data obtained by the Spectrum Analyser (SA) of the Spatio-Temporal Analysis of Field Fluctuations (STAFF) experiment aboard Cluster. Kinetic theory is then employed to obtain the theoretical expression for the whistler wave with electron temperature anisotropy which is believed to trigger lion roars in the magnetosheath. This allows us to compare theory and data. This paper for the first time studies the details of the electron velocity distribution function as measured by the Plasma Electron And Current Experiment (PEACE) in order to investigate the underlying causes for the different types of lion roars found in the data. Our results show that while some instances of lion roars could be locally generated, the source of others must be more remote regions of the magnetosheath.https://www.ann-geophys.net/24/1725/2006/angeo-24-1725-2006.pdf
spellingShingle W. Masood
W. Masood
W. Masood
S. J. Schwartz
M. Maksimovic
A. N. Fazakerley
Electron velocity distribution and lion roars in the magnetosheath
Annales Geophysicae
title Electron velocity distribution and lion roars in the magnetosheath
title_full Electron velocity distribution and lion roars in the magnetosheath
title_fullStr Electron velocity distribution and lion roars in the magnetosheath
title_full_unstemmed Electron velocity distribution and lion roars in the magnetosheath
title_short Electron velocity distribution and lion roars in the magnetosheath
title_sort electron velocity distribution and lion roars in the magnetosheath
url https://www.ann-geophys.net/24/1725/2006/angeo-24-1725-2006.pdf
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