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Extremely Distant Magnetopause Locations Caused by Magnetosheath Jets

  1. 1.
    SYSNO ASEP0580522
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleExtremely Distant Magnetopause Locations Caused by Magnetosheath Jets
    Author(s) Němeček, Z. (CZ)
    Šafránková, J. (CZ)
    Grygorov, K. (CZ)
    Mokrý, A. (CZ)
    Pi, G. (CZ)
    Nafchi, M. A. (CZ)
    Němec, F. (CZ)
    Xirogiannopoulou, N. (CZ)
    Šimůnek, Jiří (UFA-U) RID, ORCID
    Number of authors9
    Article numbere2023GL106131
    Source TitleGeophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 50, č. 24 (2023)
    Number of pages9 s.
    Languageeng - English
    CountryUS - United States
    Keywordsinterplanetary magnetic field ; magnetopause ; magnetosheath jets ; solar wind
    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 WOS001127489700001
    EID SCOPUS85180371776
    DOI10.1029/2023GL106131
    AnnotationMagnetopause position is controlled mainly by the solar wind dynamic pressure and north-south interplanetary magnetic field component and these quantities are included in different empirical magnetopause models. We have collected about 50,000 of dayside magnetopause crossings observed by THEMIS in course of 2007–2019 and compared the observed magnetopause position with model prediction. The difference between observed and predicted magnetopause radial distance, Robs − Rmod is used for quantifying the model-observation agreement. Its median values are well predicted for cases up to Robs ≈ 12 RE for all models but higher positive deviations are found for larger magnetopause distances, mainly under a nearly radial field and low dynamic pressure. The analysis reveals their connection with transient magnetopause displacements caused by strong sunward flows in the magnetosheath. We discuss the possible origin of the observed magnetosheath flow switching in terms of the interaction of magnetosheath jets with the magnetopause.
    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/10.1029/2023GL106131
Number of the records: 1  

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