Semiempirical Modeling of Large-Scale Flow on the Sun

Details Semiempirical Modeling of Large-Scale Flow on the Sun Semiempirical Modeling of Large-Scale Flow on the Sun

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..199..251a&link_type=abstract

Solar Physics, v. 199, Issue 2, p. 251-266 (2001).

Physics

7

Scientific paper

A horizontal velocity field is used to describe the large-scale transport of magnetic flux over the whole solar photosphere. The image of the 2-D large-scale flow on the sphere is derived from the trajectories of the independent free testing particles driven by the derived velocity field. The horizontal flow displays a velocity gradient and an eddy structure. The horizontal divergence of the vector field is used to describe the cellular-like patterns and limits of the discrete large-scale flow structures. The slow- and long-lived temporal evolution of the flow structures is described.

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