Computer Science
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...1e..47k&link_type=abstract
Cosmic Particle Acceleration, 26th meeting of the IAU, Joint Discussion 1, 16-17 August, 2006, Prague, Czech Republic, JD01, #47
Computer Science
Scientific paper
A role of particle beams is studied in the origin and evolution of small-scale chromospheric events appeared before the main phase onset at 13:37 UT of the July 25, 2004 flare. The main goal of our investigation was to detect possible locations of energy release and to trace the processes of energy transport by high-energy particles to the chromosphere. Based on the plasma and beam parameters deduced from hard X-ray flux and UV data, 1D hydrodynamic responses of the atmosphere is calculated and used for a full non-LTE simulation of hydrogen H-alpha line emission taking into account thermal and non-thermal processes. Theoretical line profiles are compared with the observed dynamics of H-alpha intensity. A comparison is carried out of the high energy particle parameters deduced from chromospheric emission, hard X-ray flux and UV data that allows us to find a possible scenario of the event evolution.
Chornogo S. N.
Kashapova Larisa K.
Kotrč Pavel
Zharkova Valentin
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