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Coherent whistler emissions in the magnetosphere - Cluster observations
Dubinin E.M., Maksimovic M., Cornilleau-Wehrlin N., Fontaine D., Travnicek P., Mangeney A., Alexandrova O., Sauer K., Fraenz M., Dandouras I. et al
Annales Geophysicae 25, 1 (2007) 303-315 - http://hal.archives-ouvertes.fr/hal-00330116
Article in peer-reviewed journal
Sciences of the Universe/Ocean, Atmosphere
Sciences of the Universe/Earth Sciences
Coherent whistler emissions in the magnetosphere – Cluster observations
E. M. Dubinin () 1, M. Maksimovic 2, N. Cornilleau-Wehrlin 3, D. Fontaine 3, P. Travnicek 4, A. Mangeney 2, O. Alexandrova 2, K. Sauer 1, M. Fraenz 1, I. Dandouras 5, E. Lucek 6, A. Fazakerley 7, A. Balogh 6, M. Andre 8
1:  Max-Planck-Institute für Sonnensystemforschung
Max-Planck-Institute für Sonnensystemforschung
Germany
2:  Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
http://lesia.obspm.fr/
CNRS : UMR8109 – INSU – Observatoire de Paris – Université Pierre et Marie Curie (UPMC) - Paris VI – Université Paris VII - Paris Diderot
5, place Jules Janssen 92190 MEUDON
France
3:  Centre d'étude des environnements terrestre et planétaires (CETP)
http://www.cetp.ipsl.fr/
CNRS : UMR8639 – INSU – Université de Versailles Saint-Quentin-en-Yvelines
10/12 avenue de l'Europe 78140 VELIZY
France
4:  Institute of Atmospheric Physics
Institute of Atmospheric Physics
Czech Republic
5:  Centre d'étude spatiale des rayonnements (CESR)
http://www.cesr.fr
CNRS : UMR5187 – Observatoire Midi-Pyrénées – INSU – Université Paul Sabatier [UPS] - Toulouse III
9 Av du colonel Roche - BP 4346 31028 TOULOUSE CEDEX 4
France
6:  Imperial College
Imperial College
United Kingdom
7:  Mullard Space Sci.Lab. Surey
Mullard Space Sci.Lab. Surey
United Kingdom
8:  Swedish Institute of Space Physics
Swedish Institute of Space Physics
Sweden
The STAFF-SC observations complemented by the data from other instruments on Cluster spacecraft were used to study the main properties of magnetospheric lion roars: sporadic bursts of whistler emissions at f~0.1–0.2fe where fe is the electron gyrofrequency. Magnetospheric lion roars are shown to be similar to the emissions in the magnetosheath while the conditions for their generation are much less favorable: the growth rate of the cyclotron temperature anisotropy instability is much smaller due to a smaller number of the resonant electrons. This implies a nonlinear mechanism of generation of the observed wave emissions. It is shown that the observed whistler turbulence, in reality, consists of many nearly monochromatic wave packets. It is suggested that these structures are nonlinear Gendrin's whistler solitary waves. Properties of these waves are widely discussed. Since the group velocity of Gendrin's waves is aligned with the magnetic field, these well guided wave packets can propagate through many magnetic "bottles" associated with mirror structures, without being trapped.
English

Annales Geophysicae (Ann. Geophys.)
Publisher European Geosciences Union (EGU)
ISSN 0992-7689 (eISSN : 1432-0576)
international
2007-02-01
25
1
303-315

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