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Very Low Frequency Whistler Mode Wave Events Observed Simultaneously by the Kannuslehto Station and Van Allen Probes

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    SYSNO ASEP0573096
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleVery Low Frequency Whistler Mode Wave Events Observed Simultaneously by the Kannuslehto Station and Van Allen Probes
    Author(s) Bezděková, B. (CZ)
    Němec, F. (CZ)
    Manninen, J. (FI)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Hospodarsky, G. B. (US)
    Kurth, W. S. (US)
    Number of authors6
    Article numbere2022JA031078
    Source TitleJournal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 128, č. 1 (2023)
    Number of pages12 s.
    Languageeng - English
    CountryUS - United States
    KeywordsVLF emissions ; ULF waves ; chorus
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    Method of publishingLimited access
    Institutional supportUFA-U - RVO:68378289
    UT WOS000998856700001
    EID SCOPUS85146977876
    DOI https://doi.org/10.1029/2022JA031078
    AnnotationEvents characterized by substantial intensity enhancements in the frequency range between about 1.5 and 4 kHz in the measurements of the ground-based Kannuslehto station, Finland are analyzed. Altogether, as many as 465 events are identified in the Kannuslehto data measured during the campaigns between December 2012 and October 2019. It is shown that the events usually last for several hours and they occur preferentially on the dawn side during geomagnetically active periods. Simultaneous measurements performed by the Van Allen Probes spacecraft are used to reveal the L-shells and magnetic local times where a corresponding intensity increase occurs in space. A backward ray tracing analysis is further employed to investigate the wave propagation between the tentative source region and the ground. Wave normal angles of waves eventually detectable at Kannuslehto are determined and compared with those obtained from a detailed wave analysis. Either a wave ducting, propagation in the Earth-ionosphere waveguide, or their combination seem to be needed for the waves to reach Kannuslehto.
    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 Publishing2024
    Electronic addresshttps://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022JA031078
Number of the records: 1  

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