Number of the records: 1  

Comparison of Observed and Modeled Magnetic Fields in the Earth's Magnetosheath

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    SYSNO ASEP0536925
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleComparison of Observed and Modeled Magnetic Fields in the Earth's Magnetosheath
    Author(s) Vandas, Marek (ASU-R) RID, ORCID
    Němeček, Z. (CZ)
    Šafránková, J. (CZ)
    Romashets, E. P. (US)
    Hájoš, Mychajlo (UFA-U) RID, ORCID
    Article numbere2019JA027705
    Source TitleJournal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 125, č. 3 (2020)
    Number of pages16 s.
    Publication formOnline - E
    Languageeng - English
    CountryUS - United States
    Keywordssolar-wind ; predictive model ; plasma-flow
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    Subject RIV - cooperationInstitute of Atmospheric Physics - Plasma and Gas Discharge Physics
    R&D ProjectsGA17-06065S GA ČR - Czech Science Foundation (CSF)
    Method of publishingLimited access
    Institutional supportASU-R - RVO:67985815 ; UFA-U - RVO:68378289
    UT WOS000535389600036
    EID SCOPUS85082311941
    DOI10.1029/2019JA027705
    AnnotationObservations of the magnetic field for two passages through the Earth's magnetosheath are used for comparison with two simple models of the magnetosheath field that describe it as a potential field. We apply the Kobel and Fluckiger (1994, https://doi.org/10.1029/94JA01778) model and the Romashets and Vandas (2019, https://doi.org/10.1029/2006JA012072) model complemented with the Jelinek et al. (2012, https://doi.org/10.1029/2011JA017252) empirical determination of the bow shock and magnetopause shapes and positions. The models yield a satisfactory match to observations when the positions and shapes of the bow shock and the magnetopause are controlled by the instantaneous solar wind upstream dynamic pressure and the instantaneous upstream interplanetary magnetic field vector is taken into account.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2021
    Electronic addresshttps://doi.org/10.1029/2019JA027705
Number of the records: 1  

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