Number of the records: 1  

Shape of the dayside equatorial magnetopause

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    SYSNO ASEP0474176
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleShape of the dayside equatorial magnetopause
    Author(s) Šimůnek, Jiří (UFA-U) RID, ORCID
    Šafránková, J. (CZ)
    Němeček, Z. (CZ)
    Přech, L. (CZ)
    Source TitleGeophysical Research Abstracts. - Göttingen : European Geosciences Union, 2017 - ISSN 1607-7962
    EGU2017-13062
    Number of pages1 s.
    Publication formOnline - E
    ActionEGU General Assembly 2017
    Event date23.04.2017 - 28.04.2017
    VEvent locationVienna
    CountryAT - Austria
    Event typeWRD
    Languageeng - English
    CountryDE - Germany
    KeywordsTHEMIS spacecraft ; magnetopause ; solar wind
    Subject RIVBL - Plasma and Gas Discharge Physics
    Institutional supportUFA-U - RVO:68378289
    AnnotationA magnetopause location is generally believed to be determined by the solar wind
    dynamic pressure and by a sign and value of the interplanetary magnetic field (IMF)
    vertical (Bz) component. The contribution of other parameters is usually considered
    to be minor or negligible near the equatorial plane. A great majority of present
    magnetopause models describes the magnetopause shape with an ellipsoid or paraboloid
    of revolution. The axis of such surface usually reflects the Earth orbital motion
    around the Sun. Ten years of magnetopause observations near the equatorial plane by
    the THEMIS spacecraft allow to tests of this description and facilitates search for
    a better approximation of the magnetopause shape. We present a statistical study
    based on more than several thousand magnetopause crossings identified in the THEMIS
    data. The study accounts for a dependence of the magnetopause location on the
    upstream solar wind dynamic pressure and expects that all other effects can be
    averaged. The study suggests a very simple expression for the shape of the dayside
    magnetopause and examines the influence of IMF and solar wind parameters on this
    shape. The effects of magnetospheric current systems are also discussed.
    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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