86 citations · 507 across the 26 of their papers we have counts for
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LOFAR observations of fine spectral structure dynamics in type IIIb radio bursts
I. N. Sharykin, E. P. Kontar, A. A. Kuznetsov
Solar radio emission features a large number of fine structures demonstrating great variability in frequency and time. We present spatially resolved spectral radio observations of…
Flare Energy Release in the Magnetic Field Polarity Inversion Line During M1.2 Solar Flare of March 15, 2015. Paper I. Onset of Plasma Heating and Electrons Acceleration
I. N. Sharykin, I. V. Zimovets, I. I. Myshyakov +1
We present the study of SOL2015-03-15 M1.2 flare, revealing acceleration of electrons and plasma heating in the sheared twisted magnetic structure in the polarity inversion line (P…
Statistical Study of Chromospheric Evaporation in Impulsive Phase of Solar Flares
Viacheslav M Sadykov, Alexander G Kosovichev, Ivan N Sharykin +1
We present a statistical study of chromospheric evaporation in solar flares using simultaneous observations by the RHESSI X-ray telescope and the IRIS UV spectrograph. The results…
Onset of Photospheric Impacts and Helioseismic Waves in X9.3 Solar Flare of September 6, 2017
Ivan N. Sharykin, Alexander G. Kosovichev
The X9.3 flare of September 6, 2017, was the most powerful flare of Solar Cycle 24. It generated strong white-light emission and multiple helioseismic waves (sunquakes). By using d…
Flare Energy Release in the Lower Solar Atmosphere Near the Magnetic Field Polarity Inversion Line
I. N. Sharykin, V. M. Sadykov, A. G. Kosovichev +2
We study flare processes in the solar atmosphere using observational data for a M1-class flare of June 12, 2014, obtained by New Solar Telescope (NST/BBSO) and Helioseismic Magneti…
Probing Twisted Magnetic Field Using Microwave Observations in an M Class Solar Flare on 11 February, 2014
I. N. Sharykin, A. A. Kuznetsov, I. I. Myshyakov
This work demonstrates the possibility of magnetic field topology investigations using microwave polarimetric observations. We study a solar flare of GOES M1.7 class that occurred…