A Solar Cellular Automata Model Issued From Reduced MHD

Details A Solar Cellular Automata Model Issued From Reduced MHD A Solar Cellular Automata Model Issued From Reduced MHD

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..129b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

A three-dimensional cellular automata model inspired by the reduced magnetohydrodynamic equations is presented to describe impulsive events generated along a coronal magnetic loop. It consists of a set of planes, distributed along the loop, between which the information propagates through Alfven waves. Statistical properties in terms of power laws are obtained in agreement with SoHO observations of X-ray bright points of the quiet Sun. Physical meaning and limits of the model are discussed.

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