activity
20142020
most citedDynamics of flare processes and variety of the fine structure of solar radio emission over a wide frequency range of 30 - 7000 MHz

7 citations · 16 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020★ 4 cited

Termination shock as a source of unusual solar radio bursts

Valery Fomichev, Gennady Chernov

Using centimeter wave and decimeter wave solar radio spectral observations of the flares of November 18, 2003 and September 12, 2004, we have discussed two type II like bursts at t…

astro-ph.SR2018★ 3 cited

On the Possibility of Generating Harmonics of the Electron Plasma Frequency in the Solar Atmosphere due to Explosive Instability in a System of Interpenetrating Electron and Ion Flows

V. V. Fomichev, S. M. Fainshtein, G. P. Chernov

An alternative mechanism is proposed for the generation of harmonics of the electron plasma frequency due to the development of explosive instability in a system of interpenetratin…

astro-ph.SR2018

A Model of Zebra Patterns in Solar Radio Emission

G. P. Chernov, V. V. Fomichev, R. A. Sych

We analyze complex zebra patterns and fiber bursts during type-IV solar radio bursts on August 1, 2010. It was shown that all of the main details of sporadic zebra patterns can be…

astro-ph.SR2017★ 1 cited

Development of Solar Flares and Features of the Fine Structure of Solar Radio Emission

G. P. Chernov, V. V. Fomichev, Y. Yan +3

The reason for the occurrence of different elements of the fine structure of solar radio bursts in the decimeter and centimeter wavelength ranges has been determined based on all a…

astro-ph.SR2017

Comparison of alternative zebra-structure models in solar radio emission

G. P. Chernov, V. V. Fomichev, R. A. Sych

Discussion about the nature of zebra-structure (ZS) in the type IV radio bursts continues, despite the ten proposed models. First of all, this is due to the wide variety of stripes…

astro-ph.SR2015★ 1 cited

Flare processes evolution and polarization changes of fine structures of solar radio emission in the April 11, 2013 event

Gennady Chernov, Robert Sych, Baolin Tan +5

The measurement of positions and sizes of radio sources in the observations of solar radio spectral fine structures in an M6.5 flare on April 11, 2013 were observed simultaneously…

astro-ph.SR2014★ 7 cited

Dynamics of flare processes and variety of the fine structure of solar radio emission over a wide frequency range of 30 - 7000 MHz

Gennady Chernov, Valery Fomichev, Baolin Tan +3

Radiobursts exibiting fine structure observed over two years during the rising phase of Cycle 24 by the SBRS are analyzed. In five events zebra structure, various fiber bursts and…