- Magnetosheath plasma expansion: Hybrid simulations
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Magnetosheath plasma expansion: Hybrid simulations

  1. 1.
    SYSNO ASEP0088736
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleMagnetosheath plasma expansion: Hybrid simulations
    TitleExpanze plazmatu v magnetoobálce: hybridní simulace
    Author(s) Trávníček, Pavel (UFA-U) RID, ORCID
    Hellinger, Petr (UFA-U) RID, ORCID
    Taylor, M. G. G. T. (NL)
    Escoubet, C. P. (NL)
    Dandouras, I. (FR)
    Lucek, E. (GB)
    Source TitleGeophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 34, č. 15 (2007), L15104/1-L15104/5
    Number of pages5 s.
    Languageeng - English
    CountryUS - United States
    Keywordsnumerical simulations ; marginal stability ; mirror instability ; proton cyclotron instability ; hybrid simulations
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsGA205/05/1011 GA ČR - Czech Science Foundation (CSF)
    IAA300420602 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    DOI https://doi.org/10.1029/2007GL029728
    AnnotationWe investigate the effect of a slow expansion on a magnetosheath plasma and magnetosheath low-frequency turbulence using a two-dimensional hybrid expanding box simulation. We start our simulation with a high beta plasma almost stable with respect to the mirror and proton cyclotron instabilities. The expansion leads to a continuous decrease of proton beta and drives the increase of the proton temperature anisotropy. Both mirror and proton cyclotron waves appear. The system establishes a marginally stable state with respect to both mirror and proton cyclotron instabilities. During the first phase of the simulation the mirror waves dominate over the proton cyclotron waves, latter, in the low beta region the proton cyclotron waves become dominant. Our results also support the observational possibility of mirror mode waves in plasmas with a negative growth rate (The phenomenon of bistability). We also include an initial comparison with observations made by the Cluster spacecraft.
    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 Publishing2008
Number of the records: 1  

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