Number of the records: 1  

Radio triangulation of the radio signatures of a CME-CME interaction

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    SYSNO ASEP0453201
    Document TypeA - Abstract
    R&D Document TypeThe record was not marked in the RIV
    R&D Document TypeNení vybrán druh dokumentu
    TitleRadio triangulation of the radio signatures of a CME-CME interaction
    Author(s) Magdalenic, J. (BE)
    Temmer, M. (AT)
    Krupař, Vratislav (UFA-U) RID, ORCID
    Marqué, C. (BE)
    Veronig, A. (AT)
    Vrsnak, B. (HR)
    Number of authors6
    Source Title12th European Space Weather Week. - Ostende : STCE, 2015
    Number of pages1 s.
    Publication formOnline - E
    ActionEuropean Space Weather Week /12./
    Event date23.11.2015-27.11.2015
    VEvent locationOstende
    CountryBE - Belgium
    Event typeWRD
    Languageeng - English
    CountryBE - Belgium
    Keywordscoronal mass ejection (CME) ; radio emission
    Subject RIVBL - Plasma and Gas Discharge Physics
    Institutional supportUFA-U - RVO:68378289
    AnnotationWe present a study of the radio emission associated with the complex interaction of two coronal mass ejections (CMEs), successively launched from the same active region (NOAA AR 11158), on February 14 and February 15, 2011. The continuum-like emission patch has a particular morphology and might be considered either as a continuation of the decametric type II radio emission associated with the second CME, either as a continuation of the type III radio bursts associated with a flare from NOAA AR 11158. This ambiguity complicates the question on the possible origin of the continuum-like emission. In this work, we make us of a radio triangulation technique presented by Magdalenic et al., (2014) to obtain the 3D source positions of the continuum-like emission. Comparing the location of this radio emission, with the positions of the structures of the interacting CMEs, brings important information on the possible origin of the continuum-like emission.The first results indicate that the continuum-like radio emission might be a consequence of the interaction between the shock driven by the second CME and the streamer-like, post-eruption current sheet formed behind the first CME, as suggested by Temmer et al., (2014).
    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 Publishing2016
Number of the records: 1  

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