Počet záznamů: 1

How do fits of simulated magnetic clouds correspond to their real shapes in 3D?

  1. 1.
    0348472 - ASU-R 2011 RIV DE eng J - Článek v odborném periodiku
    Vandas, Marek - Romashets, E. P. - Geranios, A.
    How do fits of simulated magnetic clouds correspond to their real shapes in 3D?.
    Annales Geophysicae. Roč. 28, č. 8 (2010), s. 1581-1588 ISSN 0992-7689.
    [STEREO-3/SOHO-22 Workshop: Three Eyes on the Sun, Multi-spacecraft studies of the corona and impacts on the heliosphere. Bournemouth, 27.04.2009-01.05.2009]
    Grant CEP: GA ČR GA205/09/0170; GA MŠk ME09032
    Grant ostatní: ESA(XE) ESA-PECS project No.98068
    Výzkumný záměr: CEZ:AV0Z10030501
    Klíčová slova: interplanetary magnetic fields * magnetic clouds * numerical simulations
    Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
    Impakt faktor: 1.620, rok: 2010

    MHD simulations of magnetic cloud propagation are used to check our fitting procedure. Simulated spacecraft measurements are fitted by models of magnetic clouds and resulting parameters are compared with real shapes of magnetic clouds which can be directly obtained from our simulations. The comparison shows that cloud parameters are determined quite reliably for spacecraft crossings near the cloud axis.
    Trvalý link: http://hdl.handle.net/11104/0189001