On Fast Chromospheric Responses to Microwave Subsecond Bursts

Physics

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Scientific paper

We present a multi-wavelength analysis of chromosphere responses produced during the subsecond bursts detected by Siberian Solar Radio Telescope (SSRT, 5.7 GHz) on April 26, 2003 at 08:05:30 UT. The data obtained by Nobeyama Radioheliograph (NoRH, 17 and 34 GHz), Ondrejov observatory and RHESSI were also used. A correlation of multi-wavelength observations (microwave emission, hard X-rays and the video-cadence chromospheric line spectra from the Ondrejov observatory obtained with 0.04 second resolution) was performed to study fluxes on various levels of solar atmosphere before, during and after the event. The temporal resolution was high enough to resolve responses to subsecond pulses in the individual correlated fluxes and their possible interrelations. The results and possible scenario are briefly discussed from point of view of the energy transport mechanisms.

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