Observations of microwave bursts with different types of fine structure using data with high spatial and spectral resolution

摘要

The observations of the bursts with fine structures are one of the best remote sensing probe of the primary energy release sites in solar flares The Siberian Solar Radiotelescope (SSRT) gives us the unique possibility of direct measurements of their positions with temporal resolution up to 14 ms and spatial resolution of a few arcsec. National Astronomical Observatories of China (NAOC) spectropolarimeters (5,2-7,7 GHz) provide us with the simultaneous spectral data around the SSRT receiving frequency (5,7 GHz) An analysis is made of the sub-second pulses observations: short wide range pulses, U-type microwave bursts, the bursts with zebra pattern.