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Alpha Transmitter Signals Observed by the Van Allen Probes: Ducted Versus Nonducted Propagation

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    SYSNO ASEP0558677
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleAlpha Transmitter Signals Observed by the Van Allen Probes: Ducted Versus Nonducted Propagation
    Author(s) Němec, F. (CZ)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Hospodarsky, G. B. (US)
    Kurth, W. S. (US)
    Number of authors4
    Article numbere2022GL098328
    Source TitleGeophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 49, č. 12 (2022)
    Number of pages10 s.
    Languageeng - English
    CountryUS - United States
    Keywordsvlf ; emissions ; model ; Alpha transmitters ; ducted ; nonducted ; wave analysis
    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 WOS000813623100001
    EID SCOPUS85133000898
    DOI10.1029/2022GL098328
    AnnotationThe interaction of very low frequency transmitter signals with radiation belt electrons depends ultimately on their wave normal angles. In the equatorial interaction region, these can be either low (ducted propagation) or comparatively large (nonducted propagation). Experimentally distinguishing the two modes is complicated, as multicomponent spacecraft data typically do not extend to high enough frequencies with a sufficient frequency resolution. One exception that we exploit are 11.9 kHz signals from Alpha transmitters detectable by the Van Allen Probes spacecraft. We use multicomponent burst mode measurements to distinguish between the ducted and nonducted modes of propagation and to evaluate their relative importance. While the ducted waves are detected less often, they tend to have larger Poynting fluxes. The total power propagating in the two modes is thus comparable. Magnetic local time and in-situ density fluctuations are main parameters controlling the relative fraction of ducted waves.
    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 Publishing2023
    Electronic addresshttps://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2022GL098328
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