Number of the records: 1  

Survey of intense whistler-mode emissions in Saturn’s magnetosheath

  1. 1.
    SYSNO ASEP0477554
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleSurvey of intense whistler-mode emissions in Saturn’s magnetosheath
    Author(s) Píša, David (UFA-U) RID, ORCID
    Sulaiman, A. H. (US)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Hospodarsky, G. B. (US)
    Kurth, W. S. (US)
    Gurnett, D. A. (US)
    Number of authors6
    Source TitleMOP 2017: Programme Book. - Uppsala : Swedish Institute for Space Physics, 2017
    S. 15
    Number of pages1 s.
    Publication formOnline - E
    ActionMagnetospheres of the Outer Planets
    Event date12.06.2017 - 16.06.2017
    VEvent locationUppsala
    CountrySE - Sweden
    Event typeWRD
    Languageeng - English
    CountrySE - Sweden
    Keywordswhistler mode waves ; Saturn ; magnetosphere
    Subject RIVBL - Plasma and Gas Discharge Physics
    Institutional supportUFA-U - RVO:68378289
    AnnotationIntense whistler-mode emissions known as ”lion-roars” have been already reported by
    many missions inside the terrestrial magnetosheath. Recently, we have reported the evidence
    of such emissions in Saturn’s magnetosheath. We present a survey of these intense emissions
    as detected by the Cassini spacecraft between years 2004 and 2010. We identified eight time
    intervals with almost 37 hours of the intense lion-roar-like emissions in the low-band (up to
    50 Hz) RPWS/WFR spectrogram. The emissions were observed across the day-side
    magnetosheath between magnetic local times from 0730 to 1600. The emissions were
    narrow-banded with a typical frequency up to 30 Hz, well below the local electron cyclotron
    frequency (100 – 1000 Hz). Using the minimum variance analysis method, we show that the
    waves are right hand circularly polarized and propagate at small wave normal angles (<40
    degrees) with respect to the ambient magnetic field. Finally, we discuss the statistical
    properties of the lion-roar-like emissions at Saturn and compare them to observations at
    Earth.
    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 Publishing2018
Number of the records: 1  

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