Signatures of High Energy Particle Beams in the Chromospheric Events Before the 25 July 2004 Flare Onset

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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.

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