Počet záznamů: 1  

Non-stationarity of the quasi-perpendicular bow shock: comparison between Cluster observations and simulations

  1. 1.
    SYSNO ASEP0360928
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevNon-stationarity of the quasi-perpendicular bow shock: comparison between Cluster observations and simulations
    Tvůrce(i) Comisel, H. (RO)
    Scholer, M. (DE)
    Souček, Jan (UFA-U) RID, ORCID
    Matsukiyo, S. (JP)
    Zdroj.dok.Annales Geophysicae. - : Copernicus - ISSN 0992-7689
    Roč. 29, č. 2 (2011), s. 263-274
    Poč.str.12 s.
    Jazyk dok.eng - angličtina
    Země vyd.DE - Německo
    Klíč. slovabow shock ; Cluster ; plasma waves ; shock waves
    Vědní obor RIVBL - Fyzika plazmatu a výboje v plynech
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000287800700005
    DOI10.5194/angeo-29-263-2011
    AnotaceWe performed full particle electromagnetic simulations of a quasi-perpendicular shock with parameters corresponding to the Earth's bow shock observed by Cluster on 24 January 2001. In run 1, modified two-stream instability (MTSI) is excited by the reflected solar wind ions. The waves due to the MTSI are on the whistler mode branch and have downstream directed phase velocities in the shock frame. The Poynting flux far upstream in the foot is also directed downstream. However, in the density and magnetic field compression region of the overshoot the waves are refracted and the Poynting flux in the shock frame points upstream. The MTSI is suppressed in the low mass ratio run 2, where significant reformation (“breathing”) is observed. It is suggested that the high frequency upstream waves are due to the MTSI and are not related to a nonlinear phase standing whistler. Different profiles observed by different Cluster spacecraft are due to the non-stationary behavior on a larger time scale.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2012
    Elektronická adresahttp://www.ann-geophys.net/29/263/2011/angeo-29-263-2011.pdf
Počet záznamů: 1  

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