Sporadic solar radio emission at decameter wavelengths

Details Sporadic solar radio emission at decameter wavelengths Sporadic solar radio emission at decameter wavelengths

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnts...5...61m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, v. 5, p. 61-66

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Scientific paper

Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) last years. Particular attention is devoted to such components of sporadic radio emission as Type III bursts, Type II bursts, ``drift pair'' bursts. New properties of these bursts, which distinguished for decameter band, are noted. They are as follows: - fine structure of Type III bursts unobserved before at other frequencies; - first discovered fine structure of Type II bursts in the form of small duration sub bursts with positive and negative frequency drift; - wavelike movement of Type II burst backbone with herringbone structure;

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