Physics
Scientific paper
Jul 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..222..151m&link_type=abstract
Solar Physics, v. 222, Issue 1, p. 151-166 (2004).
Physics
14
Scientific paper
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.
Abranin Edward P.
Boudjada Mohammed Y.
Dorovskii V. V.
Konovalenko Aleksander
Lecacheux Alain
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