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Semiempirical modeling of large-scale flow on the Sun

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    0124814 - ASU-R 20010067 RIV NL eng J - Journal Article
    Ambrož, Pavel
    Semiempirical modeling of large-scale flow on the Sun.
    Solar Physics. Roč. 199, č. 2 (2001), s. 251-266. ISSN 0038-0938. E-ISSN 1573-093X
    R&D Projects: GA AV ČR IAA3003806; GA AV ČR KSK1003601
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : sun * magnetic field * horizontal flow
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 2.103, year: 2001

    Image of the 2-D large-scale flow on the sphere is derived from the trajectories of the independent fee testing particles driven by the derived velocity field. The horizontal flow displays a velocity gradient and an eddy structure. The sllow- and long-lived temporal evolution of the low structures is descibed.

    Permanent Link: http://hdl.handle.net/11104/0023073

     
     

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