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Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind

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    0125041 - ASU-R 20020139 RIV US eng J - Journal Article
    Vandas, Marek - Odstrčil, Dušan - Watari, S.
    Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind.
    Journal of Geophysical Research. Roč. 107, A9 (2002), s. SSH2-1 - SSH2-11. ISSN 0148-0227
    R&D Projects: GA AV ČR KSK3012103; GA ČR GA205/99/1712; GA AV ČR IAA3003003; GA AV ČR IBS1003006
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : magnetic clouds * MHD simulations * interplanetary magnetic fields
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 2.245, year: 2002

    A magnetic cloud ejected from the Sun is simulated as a part of a toroid. Its evolution and propagation through interplanetary space are studing using three-dimensional magnetohydrodynamics self-consistent numerical simulations. The flux rope deforms as it moves from the Sun, and this deformation causes a hypothetical spacecraft to observe the flux rope two times at some location.
    Permanent Link: http://hdl.handle.net/11104/0023299

     
     

Number of the records: 1  

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