Geometrical Aspects of SOC Flare Models

Details Geometrical Aspects of SOC Flare Models Geometrical Aspects of SOC Flare Models

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp52b04m&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP52B-04

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7524 Magnetic Fields, 7549 Ultraviolet Emissions

Scientific paper

In this paper we address the geometrical properties of SOC Flare Models and possible connections to high spatial resolution observations of the solar coronal plasma. We discuss the study of geometrical projection effects and the fractal nature of avalanches in large two and three dimensional Cartesian lattice models and of (nano-)flares observed by the TRACE spacecraft. We examine the differences, and similarities, between the behavior of the lattice model and the observational data.

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