Podrobnosti záznamu

    Geomagnetic response to solar and interplanetary disturbances
    Bochníček, Josef
    Cerrato, Y.
    Cid, C.
    Danov, D.
    Demetrescu, C.
    Dobrica, V.
    Gonzalez, W. D.
    Hejda, Pavel
    Maris, G.
    Nenovski, P.
    Saiz, E.
    Stauning, P.
    Teodosiev, D.
    Valach, F.
Typ dokumentu
    článek v odborném periodiku
Zdrojový dokument - seriál
    Journal of Space Weather and Space Climate
    Roč. 3, July
    Projekt: OC09070, GA MŠk3cav_un_auth*0252836
    Rozsah: 20 s. : E
Předmětová kategorie
    interplanetary medium
    ionosphere (general)
    ring current
    solar activity
Klíčové slovo
Abstrakt (anglicky)
   The space weather discipline involves different physical scenarios, which are characterised by very different physical conditions, ranging from the Sun to the terrestrial magnetosphere and ionosphere. Thanks to the great modelling effort made during the last years, a few Sun-to-ionosphere/thermosphere physics-based numerical codes have been developed. However, the success of the prediction is still far from achieving the desirable results and much more progress is needed. Some aspects involved in this progress concern both the technical progress (developing and validating tools to forecast, selecting the optimal parameters as inputs for the tools, improving accuracy in prediction with short lead time, etc.) and the scientific development, i.e., deeper understanding of the energy transfer process from the solar wind to the coupled magnetosphere-ionosphere-thermosphere system.
    AV ČR Brno, Geofyzikální ústav
Kód přispěvatele
    AV ČR, GFÚ
Zdrojový formát
Datum importu
    23. 10. 2014