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The apparent source size of type III radio bursts: Preliminary results by the STEREO/WAVES instruments

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    SYSNO ASEP0357561
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThe apparent source size of type III radio bursts: Preliminary results by the STEREO/WAVES instruments
    Author(s) Krupař, Vratislav (UFA-U) RID, ORCID
    Maksimovic, M. (FR)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Cecconi, B. (FR)
    Nguyen, Q. N. (FR)
    Hoang, S. (FR)
    Goetz, K. (US)
    Source TitleAIP Conference Proceedings Series - ISSN 0094-243X
    Roč. 1216, č. 1 (2010), s. 284-287
    Number of pages4 s.
    ActionInternational Solar Wind Conference /12./
    Event date21.06.2009-26.06.2009
    VEvent locationSaint-Milo
    CountryFR - France
    Event typeWRD
    Languageeng - English
    CountryUS - United States
    KeywordsWAVES Instrument ; Solar Radio Emissions ; Singular Value Decomposition technique
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsGAP205/10/2279 GA ČR - Czech Science Foundation (CSF)
    IAA301120601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    ME09107 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000281438100067
    DOI10.1063/1.3395856
    AnnotationaThe S/WAVES instrument onboard the STEREO spacecraft measures electromagnetic waves in the solar wind. This unique project allows us to investigate properties of type III and type II radio bursts related to solar flares and propagation of coronal mass ejections (CMEs) in the interplanetary medium, respectively. We have focused on the High Frequency Receiver (HFR; a part of the STEREO/WAVES instrument) which covers the frequency range 125 kHz similar to 16.025 MHz. We present first results of a goniopolarimetric inversion for an extended source using the Singular Value Decomposition technique (SVD). We show a joint observation (including the WIND spacecraft) of the single type III radio burst connected with the X flare as a preliminary example of estimation of the apparent source size and its position.
    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 Publishing2011
Number of the records: 1  

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