A study of the Relationship Between the Microwave and Meter-Wavelength Emissions from the Solar Flare on June 3, 2021

Abstract

We present a preliminary analysis of a flare event that took place on 3 June 2021 at 01:36 UT. It was observed in microwaves by the Siberian Radioheliograph (SRH) within 3-6 GHz and by the Broadband Microwave Spectropolarimeter (BBMS), and in the meter-wavelength range by the e-Callisto spectrometer network. We found several type III bursts and a type-J burst in the meterwavelength range. At the same time, only one burst was detected in the averaged time profiles of microwave emission. This one corresponds to the strongest type III radio burst. Using images from the SRH, we defined two sources and separately analysed their time profiles. This approach allowed us to find microwave bursts associated with radio bursts, which were indistinguishable in the averaged time profiles. The observed delays between the microwave and meter-wavelength emissions were compared with the results of a preliminary analysis of dynamic spectra in the meter-wavelength range.