Počet záznamů: 1  

Van Allen Probes and Arase measurements of whistler mode waves in the Earth’s radiation belts

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    NázevVan Allen Probes and Arase measurements of whistler mode waves in the Earth’s radiation belts
    Tvůrce(i) Santolík, Ondřej (UFA-U) RID, ORCID
    Hospodarsky, G. B. (US)
    Kasahara, Y. (JP)
    Kurth, W. S. (US)
    Miyoshi, Y. (JP)
    Kletzing, C. A. (US)
    Celkový počet autorů6
    Zdroj.dok.URSI AP-RASC 2019 Proceedings. - Gent : URSI, 2019
    Poč.str.1 s.
    Forma vydáníOnline - E
    AkceURSI Asia Pacific Radio Science Conference (AT-RASC)
    Datum konání09.03.2019 - 15.03.2019
    Místo konáníNew Delhi
    ZeměIN - Indie
    Typ akceWRD
    Jazyk dok.eng - angličtina
    Země vyd.BE - Belgie
    Klíč. slovawhistler mode waves ; radiation belts ; Van Allen Probes ; hiss ; chorus
    Vědní obor RIVBL - Fyzika plazmatu a výboje v plynech
    Obor OECDFluids and plasma physics (including surface physics)
    Institucionální podporaUFA-U - RVO:68378289
    AnotaceNatural emissions of whistler-mode electromagnetic waves, especially chorus and hiss, can influence the
    dynamics of the Van Allen radiation belts via quasilinear or nonlinear wave particle interactions. They can play
    a role in complex processes of the energy transfer between different electron populations. Average intensities of
    chorus and hiss emissions have been found to increase with increasing levels of geomagnetic activity but their
    random variations in individual spacecraft measurements are usually stronger than these large-scale temporal
    effects. To separate temporal and spatial variations of wave characteristics, measurements at different points in
    space are necessary.
    We use two-point measurements of the Waves instruments of the Electric and Magnetic Field Instrument Suite
    and Integrated Science (EMFISIS) to investigate whistler-mode emissions in the Earth’s radiation belts.
    Identical instruments are carried onboard two Van Allen Probes. We systematically analyze their large data sets
    which have been collected since 2012 over a range of separation vectors of the two spacecraft. We investigate
    similar variations of the whistler-mode wave power occurring at the same time at different places.
    The Waves survey data give good orbital coverage in L, latitude, and magnetic local time (MLT) for whistlermode plasmaspheric hiss and chorus. The results show that average and/or median wave power exhibits a flat
    peak at MLT ≈ 8-17h and L ≈ 2-4 and that these characteristic values generally increase with geomagnetic
    activity while observed random variations are still comparable to the effects of systematic trends.
    We also use measurements of the onboard two Van Allen Probes to analyze these waves during conjunctions of
    one of the Van Allen Probes spacecraft with the Arase spacecraft at close separations.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2020
Počet záznamů: 1  

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