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Simultaneous observations of quasi-periodic ELF/VLF wave emissions and electron precipitation by DEMETER satellite: A case study

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    SYSNO ASEP0394777
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleSimultaneous observations of quasi-periodic ELF/VLF wave emissions and electron precipitation by DEMETER satellite: A case study
    Author(s) Hayosh, Mykhaylo (UFA-U) RID, ORCID
    Pasmanik, D. L. (RU)
    Demekhov, A. G. (RU)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Parrot, M. (FR)
    Titova, E. E. (RU)
    Source TitleJournal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 118, č. 7 (2013), s. 4523-4533
    Number of pages11 s.
    Languageeng - English
    CountryUS - United States
    Keywordsquasi-periodic ELF/VLF emissions in the magnetosphere ; wave-particle interactions ; demeter spacecraft measurements ; whistler-mode waves
    Subject RIVDG - Athmosphere Sciences, Meteorology
    R&D ProjectsGAP209/11/2280 GA ČR - Czech Science Foundation (CSF)
    LH12231 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportUFA-U - RVO:68378289
    UT WOS000325073600051
    DOI10.1002/jgra.50179
    AnnotationWe present results of case studies of quasi-periodic (QP) ELF/VLF hiss emissions detected onboard the DEMETER satellite. Three events with simultaneous periodic modulation in VLF wave intensity and energetic electron precipitation are found. In each event we observe exact coincidence of one or two busts of VLF wave intensity with energetic electron precipitation peaks. To our knowledge, such observations made onboard satellites have not been reported earlier. All events are observed at fairly quiet geomagnetic conditions (Kp <3). The dynamic spectrum of the VLF waves in these QP events was characterized by a regular frequency increase in each burst, and the repetition period was less than or about 20 s. These features allow us to suggest that the observed events belong to the QP2-class, i.e., events which are not associated with geomagnetic pulsations. We also analyze energetic electron data from NOAA-17 spacecraft which has helio-synchronous circular orbit similar to DEMETER spacecraft and measured in the same region of the magnetosphere within 30 min for the analyzed events. NOAA-17 data confirm that the QP emissions were detected by DEMETER in the region of isotropization of energetic electrons, which is typically associated with the development of the cyclotron instability. Modulation of electron flux with a period close to the QP emission period is observed in two events. Based on the observed correlation between bursts of wave intensity and energetic particle flux, we estimate the location and spatial extent of the source region for QP emissions.
    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 Publishing2014
Number of the records: 1  

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