activity
20072023
most citedMagnetohydrodynamic waves in solar partially ionized plasmas: two-fluid approach

161 citations · 547 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2023

Spatial properties of the complex decameter type II burst observed on 31 May 2013

V. V. Dorovskyy, V. N. Melnik, A. A. Konovalenko +2

We present the results of observations of complex powerful type II burst associated with narrow Earth-directed CME, which was ejected at around 11 UT on 31 May 2013. The observatio…

astro-ph.SR2020★ 3 cited

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…

astro-ph.IM2018★ 8 cited

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…

astro-ph.SR2018★ 6 cited

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…

astro-ph.SR2018★ 8 cited

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…

astro-ph.SR2018★ 38 cited

LOFAR observations of the quiet solar corona

C. Vocks, G. Mann, F. Breitling +9

The quiet solar corona emits meter-wave thermal bremsstrahlung. Coronal radio emission can only propagate above that radius, , where the local plasma frequency eqals the obser…