Unusual Solar Radio Burst Observed at Decameter Wavelengths
Rucker, H. O.; Panchenko, M.; Konovalenko, A. A.; Melnik, V. N.; Dorovskyy, V. V.; Brazhenko, A. I.; Frantsuzenko, A. V.; Stanislavskyy, A. A.
Ukraine, Austria
Abstract
An unusual solar burst was observed simultaneously by two decameter radio telescopes UTR-2 (Kharkov, Ukraine) and URAN-2 (Poltava, Ukraine) on 3 June 2011 in the frequency range of 16 - 28 MHz. The observed radio burst had some unusual properties, which are not typical for the other types of solar radio bursts. Its frequency drift rate was positive (about 500 kHz s−1) at frequencies higher than 22 MHz and negative (100 kHz s−1) at lower frequencies. The full duration of this event varied from 50 s up to 80 s, depending on the frequency. The maximum radio flux of the unusual burst reached ≈103 s.f.u. and its polarization did not exceed 10 %. This burst had a fine frequency-time structure of unusual appearance. It consisted of stripes with the frequency bandwidth 300 - 400 kHz. We consider that several accompanied radio and optical events observed by SOHO and STEREO spacecraft were possibly associated with the reported radio burst. A model that may interpret the observed unusual solar radio burst is proposed.