Search Results - "Charikov, Yu. E"
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Simulation of a Looptop Hard X-ray Source in Turbulent Plasma of Solar Flares
Published in Technical physics (01-09-2021)“…The kinetics of electron beams accelerated in the collisional plasma of solar (stellar) flares is considered. The stationary ion-acoustic turbulent mode…”
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The Influence of the Hydrodynamic Response of the Flare Plasma on the Kinetics of an Accelerated Electron Beam and Hard X-rays
Published in Geomagnetism and Aeronomy (01-12-2020)“…The transfer of accelerated electrons in the plasma of flaring loops is accompanied by a hydrodynamic response of the heated plasma. The dynamics of the…”
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Subsecond X-ray Spikes in Solar Flares: Kinematics of Acceleration and Transport of Accelerated Electrons
Published in Geomagnetism and Aeronomy (01-12-2020)“…Hard X-rays time structure of solar flares can be caused by the timing of electrons acceleration, the kinematics of their propagation in the flaring plasma,…”
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Simulation of Accelerated Electron Beam Transport with a Fine Time Structure in Flare Loop Plasma
Published in Geomagnetism and Aeronomy (01-12-2019)“…This work discusses the results of the analysis of the pulsed time structure of X-ray radiation for the SOL1996-07-09T09:09:01, GOES X2.6-class flare recorded…”
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5
Dynamics of Fast Electrons in an Inhomogeneous Plasma with Plasma Beam Instability
Published in Geomagnetism and Aeronomy (01-12-2019)“…The results of numerical simulation of the one-dimensional propagation of fast electrons in a plasma with Langmuir turbulence are presented. The resonant…”
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6
Hard X-ray generation in the turbulent plasma of solar flares
Published in Geomagnetism and Aeronomy (01-12-2016)“…The influence of scattering of accelerated electrons in the turbulent plasma on the transformation of their distribution function is studied. The turbulence is…”
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Accelerated Electron Propagation Model for the Flare Arcade of the September 23, 2014, Event from RHESSI, SDO, and Nobeyama Radioheliograph Observations
Published in Geomagnetism and Aeronomy (01-12-2019)“…A multi-wavelength study and simulation is conducted for the solar flare SOL2014-09-23T23:11. GOES-class M2.5. Radio (Nobeyama Radioheliograph) and X-ray…”
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Influence of magnetic turbulence on the propagation of accelerated electrons and hard X-ray brightness distribution in solar flares
Published in Geomagnetism and Aeronomy (01-12-2015)“…The influence of magnetic turbulence on the hard X-ray brightness distribution in magnetic loops during solar flares was studied. An analysis was perfomed…”
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9
Time Evolution of the Energy Spectra of Accelerated Electrons and Hard X-Rays from Local Sources of Solar Flares
Published in Geomagnetism and Aeronomy (01-12-2018)“…Modern observations of solar flares in hard X-rays are carried out with a high spatial resolution of ~2–4 arcsec with the RHESSI satellite. In this way one can…”
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Quasi-Periodic Hard X-Ray Pulsations in Solar Flares Based on RHESSI and Konus-Wind Data
Published in Geomagnetism and Aeronomy (01-12-2019)“…The results of the study of quasi-periodic hard X-ray pulsations in solar flares with respect to the spatial localization of emission sources based on data…”
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11
Compton Scattering of the Hard X-Ray Flux of Solar Flares with Various Angular Anisotropies of Hard X-Ray Sources
Published in Geomagnetism and Aeronomy (01-12-2018)“…The contribution of photons reflected from the solar photosphere to the intensity and the change in the slope of the energy spectrum of solar flare hard X-rays…”
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12
Directivity and polarization dynamics of hard X-ray and gamma-ray emission of a flare loop
Published in Geomagnetism and Aeronomy (01-12-2015)“…The peculiarities of the directivity and polarization dynamics of hard X-rays and gamma-rays from different regions of a flare loop were studied based on…”
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13
Konus-Wind and Helicon-Coronas-F observations of solar flares
Published in Geomagnetism and Aeronomy (01-12-2014)“…Results of solar flare observations obtained in the Konus- Wind experiment from November, 1994 to December, 2013 and in the Helicon Coronas-F experiment during…”
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14
Localization of electron acceleration in solar flares based on the spectrum analysis of hard X-ray time delays
Published in Geomagnetism and Aeronomy (01-12-2015)“…Data on hard X-rays of solar flares recorded by the BATSE spectrometer are analyzed. Time delays were determined and their spectra were constructed for X-ray…”
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15
Intensity and polarization of the hard X-ray radiation of solar flares at the top and footpoints of a magnetic loop
Published in Geomagnetism and Aeronomy (01-12-2012)“…The spatial distributions of the intensity and polarization of hard X-rays (HXR) were modeled based on a numerical solution of the nonstationary kinetic…”
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16
Time structure of the X-ray emission of thermal solar flares
Published in Geomagnetism and Aeronomy (01-12-2013)“…Based on observations of electromagnetic radiation, a concept of thermal solar flares has been proposed. The absence of hard X-ray emission implies no…”
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Spatial brightness distribution of hard X-Ray emission along flare loops
Published in Geomagnetism and Aeronomy (01-12-2013)“…The work is devoted to the simulation of recently discovered hard X-ray and gamma radiation sources localized near the top of solar flare loops. The…”
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18
Hard X rays of relativistic electrons accelerated in solar flares
Published in Geomagnetism and Aeronomy (01-12-2012)“…The direction and polarization degree of hard X rays (HXRs) in solar flares are studied. The continuous injection of relativistic electrons, which is…”
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Superfine time structure and polarization of hard X-ray emission during solar flares: Simulation of isolated pulses
Published in Geomagnetism and Aeronomy (01-04-2012)“…A superfine time structure has been detected recently via hard X-ray satellite observations during solar flares. Some pulses are hundreds of milliseconds in…”
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On the reconstruction of the energy distribution of electrons accelerated in solar flares
Published in Technical physics (01-12-2012)“…A technique for reconstructing energy spectra of electrons accelerated in solar flares is suggested that is based on the rigorous solution of the inverse…”
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