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

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..335b&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 335-3

Physics

Particle Emission, Solar Wind, Photosphere, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A three-dimensional cellular automata (CA) 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 Alfvén 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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