Počet záznamů: 1  

Solar energetic particle flux enhancement as a predictor of geomagnetic activity in a neural network-based model

  1. 1.
    SYSNO ASEP0330299
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevSolar energetic particle flux enhancement as a predictor of geomagnetic activity in a neural network-based model
    Tvůrce(i) Valach, F. (SK)
    Revallo, M. (SK)
    Bochníček, Josef (GFU-E) ORCID, RID
    Hejda, Pavel (GFU-E) ORCID, RID
    Zdroj.dok.Space Weather-the International Journal of Research and Applications. - : Wiley
    Roč. 7, April (2009), S04004/1-S04004/7
    Poč.str.7 s.
    Jazyk dok.eng - angličtina
    Země vyd.US - Spojené státy americké
    Klíč. slovaneural networks ; coronal mass ejections ; energetic particles ; flares ; radio emissions ; magnetic storms
    Vědní obor RIVDE - Zemský magnetismus, geodézie, geografie
    CEPIAA300120608 GA AV ČR - Akademie věd
    1QS300120506 GA AV ČR - Akademie věd
    CEZAV0Z30120515 - GFU-E (2005-2011)
    UT WOS000265332500002
    DOI10.1029/2008SW000421
    AnotaceCoronal mass ejections (CMEs) are believed to be the principal cause of increased geomagnetic activity. They are regarded as being in context of a series of related solar energetic events, such as X-ray flares (XRAs) accompanied by solar radio bursts (RSPs) and also by solar energetic particle (SEP) flux. Two types of the RSP events are known to be geoeffective, namely, the RSP of type II, interpreted as the signature of shock initiation in the solar corona, and type IV, representing material moving upward in the corona. The SEP events causing geomagnetic response are known to be produced by CME-driven shocks. In this paper, we use the method of the artificial neural network in order to quantify the geomagnetic response of particular solar events. The data concerning XRAs and RSPs II and/or IV together with their heliographic positions are taken as the input for the neural network.
    PracovištěGeofyzikální ústav
    KontaktHana Krejzlíková, kniha@ig.cas.cz, Tel.: 267 103 028
    Rok sběru2010
Počet záznamů: 1  

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