Transport of magnetic bright points on the Sun. Analysis of subdiffusion scenarios

Details Transport of magnetic bright points on the Sun. Analysis of subdiffusion scenarios Transport of magnetic bright points on the Sun. Analysis of subdiffusion scenarios

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.323..351s&link_type=abstract

Astrophysics and Space Science, Vol. 323, p. 351-355

Astronomy and Astrophysics

Astrophysics

Diffusion, Sun: Magnetic Fields, Sun: Photosphere, Sun: Transport Processes

Scientific paper

In this paper we compare two types of subdiffusion applied to random motion of magnetic bright points at the solar photosphere. One is due to the inverse-time α-stable Lévy process as a subordinator, another is subordinated by the α-stable process. The recommendation to identify each type of subdiffusion in the solar experiment is suggested. The difference of these scenarios lies in distinct contrast to the description with the corresponding subdiffusive fractional Fokker-Planck approach, thus providing experimentalists an test to differentiate between the two subdiffusion scenarios.

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