Computer Science
Scientific paper
Jan 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..215i&link_type=abstract
Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO a
Computer Science
6
Sun, Transition Region
Scientific paper
The transition region appears to be a complicated mix of highly dynamic, rapidly cooling loop-like structures in a background of steady loops and funnels with gravitationally stratified chromosphere-corona transition zones. This review concentrates on the time varying emission. The heating and plasma acceleration appears to be strongly dependent on the photospheric field. Parallels are discussed with active region dynamics and in particular the influence of the underlying field on event character. Explosive events are mostly found above complex field configurations, whereas brightenings not associated with flows occur at closed-bipole sites. Simulations of reconnection, rotation and shock generation are briefly described in the context of the transition region flows.
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