Transport Of Solar Magnetic Elements In The Intergranular Lanes

Details Transport Of Solar Magnetic Elements In The Intergranular Lanes Transport Of Solar Magnetic Elements In The Intergranular Lanes

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..52s&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Physics

Scientific paper

The Sun is an excellent natural laboratory for studying the nonlinear plasma phenomena. Photospheric convective motions of magnetic flux elements cause much of the solar surface phenomena. Using the observed solar data to diffusion properties of photosphere bright points for times less than 20 minutes, we construct a transport model describing a subdiffusive motion of solar magnetic elements in the intergranular lanes. The anomalous diffusion arises from the probabilistic distribution of waiting times attracted to a stable law. This suggests an analytical explanation of this observations and a revision of the Leighton's model.

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