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Nonstationarity of a two-dimensional perpendicular shock: Competing mechanisms

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    SYSNO ASEP0323282
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleNonstationarity of a two-dimensional perpendicular shock: Competing mechanisms
    TitleNestacionarita dvoudimenzionálních kolmých rázových vln: Soupeříci mechanismy
    Author(s) Lembège, B. (FR)
    Savoini, P. (FR)
    Hellinger, Petr (UFA-U) RID, ORCID
    Trávníček, Pavel M. (UFA-U) RID, ORCID
    Number of authors4
    Source TitleJournal of Geophysical Research - ISSN 0148-0227
    Roč. 114, A03217 (2009), A03217/1-A03217/21
    Number of pages21 s.
    Publication formweb - web
    Languageeng - English
    CountryUS - United States
    KeywordsCollisionless shocks ; self-reformation ; nonlinear waves
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsIAA300420702 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    IAA300420602 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000264687100002
    DOI10.1029/2008JA013618
    AnnotationTwo-dimensional PIC simulations are used for analyzing in detail different nonstationary behaviors of a perpendicular supercritical shock. A recent study by Hellinger et al. (2007) has shown that the front of a supercritical shock can be dominated by the emission of large-amplitude whistler waves. These waves inhibit the self-reformation driven by the reflected ions; then, the shock front appears almost quasi-stationary. The present study stresses new complementary results. For a fixed βi value, the whistler waves emission persists for high MA above a critical Mach number. The quasi-stationarity is only apparent and disappears when considering the full 3-D field profiles. For lower MA, the self-reformation is retrieved and becomes dominant as the amplitude of the whistler waves becomes negligible. There exists a transition regime in MA within which both processes compete each other.
    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 Publishing2009
Number of the records: 1  

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