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Properties of Type III and Type IIIb Bursts in the Frequency Band of 8 - 80 MHz During PSP Perihelion at the Beginning of April 2019
Melnik, V.~N.; Brazhenko, A.~I.; Konovalenko, A.~A.; Frantsuzenko, A.~V.; Yerin, S.~M.; Dorovskyy, V.~V.; Bubnov, I.~M.;
Published by: \solphys Published on: 01/2021
YEAR: 2021   DOI: 10.1007/s11207-020-01754-5
Type III bursts; Type IIIb bursts; Frequency drift rates; Durations; Brightness temperatures; Astrophysics - Solar and Stellar Astrophysics
Radio Signature of a Distant behind-the-limb CME on 2017 September 6
We discuss properties of a Type IV burst, which was observed on 2017 September 6, as a result of the powerful flare X 9.3. At decameter wavelengths this burst was observed by the radio telescopes STEREO A, URAN-2, and the Nancay Decameter Array at frequencies 5-35 MHz. This moving Type IV burst was associated with a coronal mass ejection (CME) propagating in the southwest direction with a speed of 1570 km s(-1). The maximum radio flux of this burst was about 300 s.f.u. and the polarization was more than 40\%. In the frequenc ...
Melnik, V.; Rucker, H.; Brazhenko, I.; Panchenko, M.; Konovalenko, A.; , Frantsuzenko; Dorovskyy, V.; , Shevchuk;
Published by: ASTROPHYSICAL JOURNAL Published on: 12/2020
YEAR: 2020   DOI: 10.3847/1538-4357/abbfb3