Abstract
We present the results of radio telescope UTR-2 observations of solar Type II radio bursts in the 10–30 MHz frequency range. These events possess a fine structure consisting of fast drift sub-bursts similar to Type III bursts. The frequency drift rate of the Type II bursts at decameter wavelengths is smaller than 0.1 MHz s−1. One of these bursts with herringbone structure has a wave-like backbone that almost does not drift. The features of the observed bursts are discussed.
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Mel'nik, V., Konovalenko, A., Rucker, H. et al. Observations of Solar Type II bursts at frequencies 10–30 MHz . Solar Physics 222, 151–166 (2004). https://doi.org/10.1023/B:SOLA.0000036854.66380.a4
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DOI: https://doi.org/10.1023/B:SOLA.0000036854.66380.a4