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Generation of whistler mode emissions in the inner magnetosphere: An event study
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SYSNO ASEP 0356509 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Generation of whistler mode emissions in the inner magnetosphere: An event study Author(s) Schriver, D. (US)
Ashour-Abdalla, M. (US)
Coroniti, F.V. (US)
LeBoeuf, J. N. (US)
Decyk, V. (US)
Trávníček, Pavel M. (ASU-R) RID, ORCID
Santolík, Ondřej (UFA-U) RID, ORCID
Winningham, D. (US)
Pickett, J. (US)
Goldstein, M. L. (US)
Fazakerley, A. N. (GB)Source Title Journal of Geophysical Research - ISSN 0148-0227
Roč. 115, A9 (2010), A00F17/1-A00F17/13Number of pages 13 s. Language eng - English Country US - United States Keywords magnetospheric physics ; plasma waves and instabilities ; space plasma physics Subject RIV BL - Plasma and Gas Discharge Physics CEZ AV0Z10030501 - ASU-R (2005-2011) AV0Z30420517 - UFA-U, BC-A (2005-2011) UT WOS 000281146600002 DOI 10.1029/2009JA014932 Annotation On July 24, 2003, when the Cluster 4 satellite crossed the magnetic equator at about 4.5 RE radial distance on the dusk side (approx. 15 MLT), whistler wave emissions were observed below the local electron gyrofrequency (fce) in two bands, one band above one-half the gyrofrequency (0.5fce) and the other band below 0.5fce. A careful analysis of the wave emissions for this event has shown that Cluster 4 passed through the wave generation region. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
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