9 citations · 47 across the 11 of their papers we have counts for
15 papers
Observations of shock propagation through turbulent plasma in the solar corona
Eoin P. Carley, Baptiste Cecconi, Hamish A. Reid +14
Eruptive activity in the solar corona can often lead to the propagation of shock waves. In the radio domain the primary signature of such shocks are type II radio bursts, observed…
Solar Type U Burst Associated with a High Coronal Loop
V. V. Dorovskyy, V. N. Melnik, A. A. Konovalenko +2
An inverted U burst with equally developed ascending and descending branches observed by Giant Ukrainian Radio Telescope (GURT) on 18 April 2017 in meter wavelengths band is discus…
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
V. N. Melnik, A. I. Brazhenko, A. A. Konovalenko +4
Properties of type III and type IIIb bursts in the frequency band of 8-80 MHz observed by the radio telescopes Ukrainian Radio Interferometer of NASU-2 (URAN-2) (Poltava) and Giant…
Radio signature of a distant behind-the-limb CME on 2017 September 6
V. N. Melnik, H. O. Rucker, A. I. Brazhenko +5
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 r…
First observation of the solar Type III burst decay and its interpretation
Valentin N. Melnik, Alexandr A. Konovalenko, Sergey M. Yerin +6
A decay of Type III burst into two Type III bursts was registered during solar observations by GURT and URAN-2 radio telescopes on April 18, 2017. Such phenomenon was observed for…
Comparative analysis of solar radio bursts before and during CME propagation
G. Dididze, B. M. Shergelashvili, V. N. Melnik +5
As is well known, CME propagation often results in the fragmentation of the solar atmosphere on smaller regions of density (magnetic field) enhancement (depletion). It is expected…