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Analysis of fine ELF wave structures observed poleward from the ionospheric trough by the low-altitude satellite DEMETER

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    SYSNO ASEP0429238
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleAnalysis of fine ELF wave structures observed poleward from the ionospheric trough by the low-altitude satellite DEMETER
    Author(s) Parrot, M. (FR)
    Nĕmec, F. (CZ)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Source TitleJournal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 119, č. 3 (2014), s. 2052-2060
    Number of pages9 s.
    Publication formPrint - P
    Languageeng - English
    CountryUS - United States
    Keywordstrough ; EMIC ; substorm
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsGAP205/10/2279 GA ČR - Czech Science Foundation (CSF)
    LH12231 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportUFA-U - RVO:68378289
    UT WOS000336218300051
    EID SCOPUS84899057718
    DOI10.1002/2013JA019557
    AnnotationDEMETER was a three-axis stabilized Earth-pointing spacecraft launched on 29 June 2004 into a low-altitude (710 km) polar and circular orbit that was subsequently lowered to 650 km until the end of the mission in December 2010. DEMETER measured electromagnetic waves all around the Earth except at magnetic invariant latitudes >65°. The frequency range for the electric field was from DC up to 3.5 MHz and for the magnetic field from a few hertz up to 20 kHz. Electromagnetic ion cyclotron (EMIC) waves have been previously observed by DEMETER close to the ionospheric trough during high magnetic activity, and this paper describes another type of EMIC waves. These waves are also observed close to the trough, but they extend poleward, with the trough acting as a boundary. They are observed exclusively during the night and preferentially during geomagnetic substorms. The analysis of wave propagation shows that they propagate nearly along the ambient magnetic field and that they come from larger radial distances.
    WorkplaceInstitute of Atmospheric Physics
    ContactKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Year of Publishing2015
Number of the records: 1  

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