Source position and duration of a solar type III radio burst observed by LOFAR
Published Date: 1/21/2020
Source: phys.org
Type III solar radio bursts are generated by non-thermal electron beams propagating through the solar corona and interplanetary space. In dynamic spectra, the flux of solar type III radio bursts have a time profile of rising and decay phases at a given frequency, which has been actively studied since the 1970s.