25 citations · 133 across the 19 of their papers we have counts for
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Solar bursts as can be observed from the lunar farside with a single antenna at very low frequencies
A. A. Stanislavsky, A. A. Konovalenko, S. N. Yerin +10
Earth-based observations are complicated by the opacity of Earth's ionosphere at very low frequencies and strong man-made radio frequency interference. This explains long standing…
Revisiting the frequency drift rates of decameter type III solar bursts observed in July-August 2002
A. A. Stanislavsky, A. A. Konovalenko, E. P. Abranin +4
Estimating for the frequency drift rates of type III solar bursts is crucial for characterizing their source development in solar corona. According to Melnik et al. (Solar Phys. 26…
Interferometric Observations of the Quiet Sun at 20 and 25 MHz in May 2014
V. N. Melnik, V. A. Shepelev, S. Poedts +3
Results of solar observations at 20 and 25 MHz by the UTR-2 (\textit{Ukrainian T-shaped Radio telescope of the second modification}) radio telescope in the interferometric session…
Decameter Type IV Burst Associated with a behind-the-limb CME Observed on 7 November 2013
V. N. Melnik, A. I. Brazhenko, A. A. Konovalenko +5
We report on the results of observations of a type IV burst by URAN-2 (Ukrainian Radio interferometer of Academy Scienses) in the frequency range 22 - 33 MHz, which is associated w…
Solar Type IV bursts at frequencies 10-30 MHz
V. N. Melnik, H. O. Rucker, A. A. Konovalenko +5
The results of the first observations of Type IV bursts at frequencies 10-30 MHz are presented. These observations were carried out at radio telescopes UTR-2 (Kharkov, Ukraine) and…
Properties of Decameter IIIb-III Pairs
V. N. Melnik, A. I. Brazhenko, A. V. Frantsuzenko +2
A large number of Type IIIb-III pairs, in which the first component is a Type IIIb burst and the second one is a Type III burst, are often recorded during decameter Type III burst…