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3-D MHD simulations of CMES by coupled coronal and heliospheric models

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    0125067 - ASU-R 20020165 RIV NL eng C - Conference Paper (international conference)
    Odstrčil, Dušan - Linker, J. A. - Lionello, R. - Mikic, Z. - Riley, P. - Pizzo, J. - Luhmann, J. G.
    3-D MHD simulations of CMES by coupled coronal and heliospheric models.
    Solar variabiliy: from core to outer frontiers. Vol. 1. Noordwijk: ESA Publication Division, 2002 - (Wilson, A.), s. 95-98
    [European Solar Physics Meeting /10./. Praha (CZ), 09.09.2002-14.09.2002]
    R&D Projects: GA AV ČR IAA3003003
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : coronal mass ejection * magnetic flux * rope
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    Merging of coronal and heliospheric magnetohydrodynamic (MHD) models in demonstrated for a 3-D idealized case involving a magnetic flux rope, shock, streamer belt, and current sheet. The disruption of a sheared coronal arcade launches a coronal mass ejection, vhich evolves during its propagation through interplanetary space.
    Permanent Link: http://hdl.handle.net/11104/0023325
     

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