Spatial fragmentation of solar flare plasma and beams

Details Spatial fragmentation of solar flare plasma and beams Spatial fragmentation of solar flare plasma and beams

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...68...93b&link_type=abstract

Space Science Reviews, Volume 68, Issue 1-4, pp. 93-96

Computer Science

1

Flares, Solar, Beams, Fragmentation

Scientific paper

The observational and theoretical arguments for spatial fragmentation of the bulk of the thermal and non-thermal components of solar flare plasma are summarised. Observational aspects considered include XUV filling factors, EUV centre to limb variations, andH α impact polarisation. Theoretical points addressed are the high flare inductance and beam/return current closure at the acceleration site. A high degree of beam/plasma filamentation implies strong transverse temperature gradients so that cross-field conduction must be included in energy transport modelling. Preliminary results are described for a simple two-component model.

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