A Wide-Band High-Frequency Type-II Solar Radio Burst by Vasanth et al.
Type-II radio bursts are usually observed below 400 MHz with slowly-drifting narrow fundamental and/or harmonic bands. Events with starting frequencies higher than 400 MHz are rarely reported (e.g., Pohjolainen et al. 2008). Such high-frequency Type-IIs may stem from the CME interaction with surrounding dense structures in the corona, such as streamers, ray-like or loop structure, or from sources in the lower corona. Figure. 1. Dynamic spectrum of the high-frequency wide-band […]
