Number of the records: 1  

A new view on drivers of magnetopause locations

  1. 1.
    SYSNO ASEP0473477
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleA new view on drivers of magnetopause locations
    Author(s) Němeček, Z. (CZ)
    Šafránková, J. (CZ)
    Šimůnek, Jiří (UFA-U) RID, ORCID
    Shue, J.-H. (TW)
    Samsonov, A. A. (RU)
    Number of authors5
    Source Title4th Cluster and THEMIS workshop: Book of abstracts. - Paris : European Space Agency (ESA), 2017
    S. 22-23
    Number of pages2 s.
    Publication formOnline - E
    ActionCluster-THEMIS Workshop /4./.
    Event date07.11.2016 - 12.11.2016
    VEvent locationPalm Springs
    CountryUS - United States
    Event typeWRD
    Languageeng - English
    CountryFR - France
    Keywordssolar wind ; magnetopause ; THEMIS spacecraft
    Subject RIVBL - Plasma and Gas Discharge Physics
    Institutional supportUFA-U - RVO:68378289
    AnnotationThe solar wind dynamic pressure is the principal factor controlling the
    magnetopause location. Their mutual relation is usually considered in a power-law
    form and suggested indices vary from -1/4.8 to -1/6.6 in particular magnetopause
    models. The paper analyzes about ten thousands of THEMIS dayside magnetopause crossings observed in a broad range of upstream pressures (0.2-20 nPa) and
    discusses the relationship between the dynamic pressure and magnetopause standoff
    distance and flaring angle. We found that (1) the power-law form provides the
    best description of variations of the stand-off distance with upstream pressure for a
    full set of crossings as well as for subsets constrained by a sign of the interplanetary
    magnetic field (IMF) vertical component, IMF cone angle, and solar wind speed; (2)
    the most appropriate value of the power index resulting from the present study is
    -1/3.83 if only a dependence on the upstream solar wind pressure is considered;
    (3) the power index varies from -1/3.1 to -1/4.2 depending on the IMF direction and
    solar wind speed; and (4) the value of the power index increases to or above -1/6 if
    the orbital spacecraft limitations are not handled properly.
    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 Publishing2017
Number of the records: 1  

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