Number of the records: 1  

Interplanetary Magnetic Field B-y Controls the Magnetopause Location

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    SYSNO ASEP0573095
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleInterplanetary Magnetic Field B-y Controls the Magnetopause Location
    Author(s) Nafchi, M. A. (CZ)
    Němec, F. (CZ)
    Pi, G. (CZ)
    Němeček, Z. (CZ)
    Šafránková, J. (CZ)
    Grygorov, K. (CZ)
    Šimůnek, Jiří (UFA-U) RID, ORCID
    Number of authors7
    Article numbere2023JA031303
    Source TitleJournal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 128, č. 5 (2023)
    Number of pages8 s.
    Languageeng - English
    CountryUS - United States
    Keywordsmagnetopause ; empirical model ; interplanetary magnetic field ; imf
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    Method of publishingOpen access
    Institutional supportUFA-U - RVO:68378289
    UT WOS001000426400001
    EID SCOPUS85160418602
    DOI10.1029/2023JA031303
    AnnotationWe present a statistical study of interplanetary magnetic field (IMF) effects on the magnetopause location based on nearly 15,000 magnetopause crossings identified in the THEMIS A-E, Magion 4, Geotail, and Interball-1 satellite data. In order to exclude the dominant controlling role of the solar wind dynamic pressure, differences between observed and empirical model magnetopause distances are analyzed. We find that the magnetopause distance is significantly controlled by the IMF clock angle, not considered in the used empirical models. Furthermore, during very low Alfven Mach numbers (M-A < 4), IMF B-y component can induce a considerable dawn-dusk asymmetry of the magnetopause shape. The magnetopause distance is found to be larger in the direction of the IMF vector, that is, not only the magnitude but also the orientation of the IMF B-y component is eventually important. The obtained results are qualitatively consistent with a magnetohydrodynamic model run at the Community Coordinated Modeling Center.
    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 Publishing2024
    Electronic addresshttps://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023JA031303
Number of the records: 1  

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