А. А. Чернышов

ORCID: 0000-0003-4692-9643
Publications
Citations
Views
---
Saved
---
About
Contact & Profiles
Research Areas
  • Ionosphere and magnetosphere dynamics
  • Solar and Space Plasma Dynamics
  • Earthquake Detection and Analysis
  • Fluid Dynamics and Turbulent Flows
  • Geomagnetism and Paleomagnetism Studies
  • Computational Fluid Dynamics and Aerodynamics
  • Complex Systems and Time Series Analysis
  • Astro and Planetary Science
  • Plasma Diagnostics and Applications
  • GNSS positioning and interference
  • Meteorological Phenomena and Simulations
  • Laser-induced spectroscopy and plasma
  • Geophysics and Gravity Measurements
  • Lightning and Electromagnetic Phenomena
  • Theoretical and Computational Physics
  • Gas Dynamics and Kinetic Theory
  • Astrophysics and Star Formation Studies
  • Statistical Mechanics and Entropy
  • Magnetic confinement fusion research
  • Solar Radiation and Photovoltaics
  • Atmospheric Ozone and Climate
  • Aerodynamics and Acoustics in Jet Flows
  • Heat Transfer Mechanisms
  • Advanced Research in Science and Engineering
  • Methane Hydrates and Related Phenomena

Space Research Institute
2016-2025

National Research University Higher School of Economics
2019-2024

Voronezh State University of Engineering Technologies
2023-2024

Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation
2020-2024

Bauman Moscow State Technical University
2024

National University Zaporizhzhia Polytechnic
2020

Baranov Central Institute of Aviation Motor Development
2018

Moscow Institute of Physics and Technology
2014-2017

Russian Academy of Sciences
2013-2015

A state-of-the-art review is given of research by computing physics methods on compressible magnetohydrodynamic turbulence in space plasmas. The presence magnetic fields and compressibility this case makes plasma much less amenable to direct numerical simulations than a neutral incompressible fluid. large eddy simulation method discussed, which was developed as an alternative modeling filters the initial equations uses subgrid-scale universal small-scale turbulence. detailed analysis made...

10.3367/ufne.0184.201405a.0457 article EN Physics-Uspekhi 2014-05-05

Abstract In this paper, the internal structuring of Polarization Jet (PJ)/Subauroral Ion Drift (SAID) is studied. It shown that PJ/SAID consists several Strata (PJS) electron density and temperature. A new type phenomena has been discovered called Stratified Subauroral (SSAID), which a containing small‐scale PJS. Internal structure SSAIDs measured during various geomagnetic events using data from NorSat‐1, DMSP F‐17 F‐18 satellites. High resolution measurements on Norsat‐1 satellite make it...

10.1029/2022ja031109 article EN cc-by-nc-nd Journal of Geophysical Research Space Physics 2023-02-16

We study the spatial structure of a polarization jet/Sub-Auroral Ion Drift (PJ/SAID) based on data from NorSat-1 and Swarm satellites during geomagnetic storm. Observations plasma parameters inside PJ/SAID are obtained with using system Langmuir probes nominal sampling rate up to 1 kHz, which allowed measurements such high temporal resolution for first time. A comparative analysis electron density spectra PJ according both is presented. Our results show that fluctuations increase at all...

10.1029/2021gl097107 article EN Geophysical Research Letters 2022-04-12

In the subauroral zone at boundary of auroral oval in evening and night hours during geomagnetic disturbances, a narrow (about 1°–2°) extended structure (several longitude) is formed. It known as polarization jet (PJ) or ion drift (SAID). The PJ/SAID fast westward one main signatures disturbance ionosphere altitudes F-layer, when AE index reaches more than 500 nT. Plasma speed can reach several kilometres per second, size plasma irregularities inside it scales from tens meters to hundred...

10.1038/s41598-025-86960-6 article EN cc-by-nc-nd Scientific Reports 2025-01-27

The ERG (Arase) satellite recently discovered a non-thermal hectometric continuum with narrowband frequency structure. mechanism behind the generation of this type emission in near-Earth plasma is still unknown. This study examines potential use electron cyclotron harmonics instability to explain line structure radio emissions for first time. By analyzing case continuum, proposed creation quasi-harmonic resulting quasi-parallel bands discussed. In other words, double resonance effect...

10.1063/5.0235182 article EN cc-by-nc Physics of Plasmas 2025-01-01

Abstract We report in situ measurements of plasma irregularities associated with a reverse flow event (RFE) the cusp F region ionosphere. The Investigation Cusp Irregularities 3 (ICI‐3) sounding rocket, while flying through RFE, encountered several regions density down to meter scales. address detail most intense small‐scale fluctuations both and AC electric field, which were observed on equatorward edge shear, coincided double‐humped jet fast flow. Due its long‐wavelength low‐frequency...

10.1002/2016ja022999 article EN Journal of Geophysical Research Space Physics 2016-10-01

Abstract The influence of an auroral substorm on the total electron content (TEC) jumps and cycle slips Global Positioning System (GPS) at high-latitudes is studied. For first time, optical data from all-sky imager, as well interplanetary magnetic field magnetometer are used to complete analysis occurrence monitor evolution. Two types considered: (i) instrumental including losses in measured phase GPS signal (ii) sharp TEC variations (TEC jumps) It demonstrated that determined signals mainly...

10.1038/s41598-020-63422-9 article EN cc-by Scientific Reports 2020-04-14

The large eddy simulation technique is developed for the study of decaying compressible magnetohydrodynamic turbulence. In present paper obtained results numerical computations are compared with direct three-dimensional turbulence under various similarity parameters, namely, magnetic Reynolds numbers, hydrodynamic and Mach numbers. comparison five subgrid-scale closures case made. between carried out regarding time evolution kinetic energy, cross helicity, molecular dissipations turbulent...

10.1063/1.2728936 article EN Physics of Fluids 2007-05-01

Fractal geometry is used to describe the spatial structure of ionospheric conductivity. Topological values fractal dimension and connectivity index, characterizing Pedersen Hall conductivities on nightside auroral zone, are analytically obtained. Restrictions imposed conductivity analyzed in terms percolation currents. It shown that observed scaling for fluctuations electric field glow region well within limitations by critical condition The multiple arc structures corresponds estimates...

10.1002/jgra.50321 article EN Journal of Geophysical Research Space Physics 2013-05-10

Inhomogeneities of plasma density and non-uniform electric fields are compared as possible sources a sort electrostatic ion cyclotron waves that can be identified with broadband extremely low frequency turbulence in the topside auroral ionosphere. Such excited by inhomogeneous energy-density-driven instability. To gain deeper insight generation these waves, computational modeling is performed various parameters. It demonstrated inhomogeneities give rise to this instability even absence...

10.1063/1.4916125 article EN Physics of Plasmas 2015-03-01

Abstract In this study, we employ a unique multi‐instrumental approach for comprehensive examination of Polarization Jet (PJ) (or, another name, Subauroral Ion Drift (SAID)). A diverse set data is used to assess the connection between appearance inhomogeneous structure PJ/SAID and its reflection in ground‐based observations during geomagnetic activity. Our combines satellite (Defense Meteorological Satellite Program, NorSat‐1, Swarm) (ionosondes, magnetometers, GPS/GLONASS receivers) data,...

10.1029/2024ja033222 article EN Journal of Geophysical Research Space Physics 2024-11-01

Abstract This work presents the first results of measurements artificial plasma disturbance characteristics using low‐orbit NorSat‐1 satellite, which are excited when ionospheric F2 layer is modified by powerful high‐frequency (HF) waves emitted SURA heating facility. carries multineedle Langmuir probe instrument, capable sampling electron density at a nominal rate up to 1 kHz. The uniqueness this experiment lies in fact that satellite passes very close center HF‐perturbed magnetic flux tube...

10.1029/2020gl088462 article EN Geophysical Research Letters 2020-06-10

In the present article, large eddy simulation (LES) technique for study of compressible magnetohydrodynamic turbulence is developed. The filtered equations magnetohydrodynamics fluid are obtained with use a mass-weighted filtering procedure (Favre filtering). Favre-filtered large-scale components include subgrid-scale terms describing subgrid phenomena. Different models closure suggested. this work numerical and an analysis received characteristics turbulent flow carried out. results...

10.1063/1.2171705 article EN Physics of Plasmas 2006-03-01

The excitation of electrostatic turbulence inside space-observed solitary structures is a central topic this exposition. Three representative observed in the topside auroral ionosphere as large-amplitude nonlinear signatures electric field and magnetic-field-aligned current on transverse scales ∼102–103 m are evaluated by theories wave generation inhomogeneous background configurations. A quantitative analysis shows that are, general, effective destabilizing energy-density-driven (IEDD)...

10.1063/1.4891668 article EN Physics of Plasmas 2014-08-01

10.1016/j.jastp.2017.06.013 article EN Journal of Atmospheric and Solar-Terrestrial Physics 2017-06-27

We present the large-eddy simulation method for studying forced compressible magnetohydrodynamic turbulence. The proposed is based on a solution of filtered basic equations magnetohydrodynamics by finite-difference methods and linear representation driving forces in momentum conservation equation magnetic induction equation. These supply production kinetic energies. emphasis placed upon important, not investigated, question about ability approach to reproduce Kolmogorov Iroshnikov–Kraichnan...

10.1063/1.3491835 article EN Physics of Plasmas 2010-10-01

Auroral kilometric radiation is used as a tool for the remote diagnostics of processes in Earth’s magnetosphere. Using satellite data and spectrum fluctuations auroral at various frequencies, fractal properties region magnetosphere depending on altitude source frequency generated are studied. The characteristics (Hurst exponent dimension) medium generation their dynamics determined from scaling law. It shown that Hurst increase with (or decrease signal frequency), whereas dimension decreases...

10.1134/s0021364022010076 article EN cc-by JETP Letters 2022-01-01

Many electrically and heat conducting fluid flows cannot be described within the framework of incompressible medium or by compressible magnetohydrodynamic equations on assumption polytropic (or adiabatic) process. Therefore, we consider a with use an energy equation. Application large eddy simulation approach to magnetohydrodynamics is considered. The system filtered total equation using mass-weighted filtering procedure has been obtained. It shown that novel subgrid-scale terms arise in...

10.1063/1.2969472 article EN Physics of Fluids 2008-08-01

We present the results of Auroral Kilometric Radiation (AKR) measurements near plasmapause on ERG (Arase) satellite. The apogee satellite's orbit is located ecliptic plane, at latitudes ±30°. According to generally accepted point view, AKR observation impossible in this region since it shielded by plasmasphere. Simultaneous and local plasma density made possible determine that near-equatorial regions occur channels — inhomogeneities elongated along magnetic field lines. from sources auroral...

10.12737/stp-101202403 article EN cc-by-nc-nd Solar-Terrestrial Physics 2024-03-26
Coming Soon ...