Cross-field Diffusion of Electrons and Implications for Coronal Structure

Details Cross-field Diffusion of Electrons and Implications for Coronal Structure Cross-field Diffusion of Electrons and Implications for Coronal Structure

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..370..274g&link_type=abstract

Solar and Stellar Physics Through Eclipses ASP Conference Series, Vol. 370, proceedings of the conference held 27-29 March, 2006

Physics

Scientific paper

The loop structures observed in the corona show a range of geometrical attributes (length, aspect ratio, etc.). We identify Rechester-Rosenbluth diffusion in tangled fields as the most rapid cross-scattering mechanism. We simulate the appearance of loops under the assumption of Rechester-Rosenbluth diffusion and compare the results with TRACE images to constrain the degree of tangling of coronal field lines.

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