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Statistical study of influence of ULF waves and their compressibility on the solar wind velocity in the Earth’s foreshock

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    SYSNO ASEP0503861
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleStatistical study of influence of ULF waves and their compressibility on the solar wind velocity in the Earth’s foreshock
    Author(s) Urbář, Jaroslav (UFA-U) RID, ORCID
    Němeček, Z. (CZ)
    Šafránková, J. (CZ)
    Přech, L. (CZ)
    Number of authors4
    Source TitleGeophysical Research Abstracts, EGU General Assembly 2018, Vol. 21. - Göttingen : European Geosciences Union, 2019
    EGU2019-5385
    Number of pages1 s.
    Publication formOnline - E
    ActionEGU General Assembly 2019
    Event date07.04.2019 - 12.04.2019
    VEvent locationVienna
    CountryAT - Austria
    Event typeWRD
    Languageeng - English
    CountryDE - Germany
    Keywordssolar wind ; foreshock ; ultra low frequency (ULF) waves ; THEMIS mission
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    Institutional supportUFA-U - RVO:68378289
    AnnotationThe parameters of solar wind (SW) ion populations are modified upstream the Earth’s bow shock, in the ion foreshock region, which is typically observed ahead of the quasi-parallel bow shock. The interaction of the incoming SW with the ions reflected at the bow shock generate ULF waves, among them fast magnetosonic waves with an in-phase relationship between the ion flux and magnetic field fluctuations. Using cautiously selected SW proton population from the THEMIS ion 3D distributions, we present statistical maps of a modification of the SW proton velocity due to foreshock processes. We evaluated both electric and magnetic field fluctuation levels associated with ULF waves and their compressibility. A special attention is devoted to evaluation of a contribution of alpha particles to the proton moments using intervals of the solar wind unaffected by the foreshock processes.
    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 Publishing2020
Number of the records: 1  

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