activity
20072024
most citedAn Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles

106 citations · 387 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2024

Giant post-flare loops in active regions with extremely strong coronal magnetic fields

Costas E. Alissandrakis, Gregory D. Fleishman, Viktor V. Fedenev +2

We report for the first time the detection of thermal free-free emission from post-flare loops at 34GHz in images from the Nobeyama Radioheliograph (NoRH). We studied 8 loops, 7 of…

astro-ph.SR2020★ 3 cited

Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares with Unusual Microwave Spectra

V. V. Grechnev, N. S. Meshalkina, A. M. Uralov +7

On 23 July 2016 after 05:00\,UTC, the first 48-antenna stage of the Siberian Radioheliograph detected two flares of M7.6 and M5.5 GOES importance that occurred within half an hour…

astro-ph.SR2019★ 15 cited

Rapid Variability in the SOL2011-08-04 Flare: Implications for Electron Acceleration

Alexander T. Altyntsev, Nataliia S. Meshalkina, Alexandra L. Lysenko +1

Particle acceleration in solar flares remains an outstanding problem in solar physics. It is yet unclear which of the acceleration mechanisms dominates and how exactly is the exces…

astro-ph.SR2018★ 30 cited

Multi-instrument view on solar eruptive events observed with the Siberian Radioheliograph: From detection of small jets up to development of a shock wave and CME

V. V. Grechnev, S. V. Lesovoi, A. A. Kochanov +7

The first 48-antenna stage of the Siberian Radioheliograph (SRH) started single-frequency test observations early in 2016, and since August 2016 it routinely observes the Sun at se…

astro-ph.SR2018★ 26 cited

Statistics of "Cold" Early Impulsive Solar Flares in X-ray and Microwave domains

Alexandra L. Lysenko, Alexander T. Altyntsev, Natalia S. Meshalkina +2

Solar flares often happen after a preflare / preheating phase, which is almost or entirely thermal. In contrast, there are the so-called early impulsive flares that do not show a (…

astro-ph.SR2017★ 10 cited

Flare SOL2012-07-06: on the origin of the circular polarization reversal between 17 GHz and 34 GHz

A. Altyntsev, N. Meshalkina, I. Myshyakov +2

The new generations of multiwavelength radioheliographs with high spatial resolution will employ microwave imaging spectropolarimetry to recover flare topology and plasma parameter…