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] Hydrodynamic model for generation of global poloidal flow of the Sun. Kosm. nauka tehnol. 2011 ;17(1):29-35.
Hydrodynamic model of torsional oscillations of the Sun. Kosm. nauka tehnol. 2012 ;18(1):74–81.
The influence of compressibility and non-isothermality of the atmosphere on the propagation of acoustic-gravity waves. Kosm. nauka tehnol. 2010 ;16(1):09-19.
Influence of high-frequency vibration on crystallization surface in cylindrical Bridgeman's ampule. Kosm. nauka tehnol. 2014 ;20(1):14-22.
Influence of the upper atmosphere inhomogeneity on acoustic gravity wave propagation. Kosm. nauka tehnol. 2012 ;18(4):30–36.
Instability of Kelvin-Helmholtz and magnetohydrodynamic modes on the boundary of geomagnetic tail. Space Science and Technology. 2019 ;25(2):43-59.
Interaction of high-energy particles with magnetohydrodynamic modes in the Earth's magnetosphere. Kosm. nauka tehnol. 2002 ;8(5-6):091-095.
Investigation of perturbations and collective motions of plasma in the inner magnetosphere of the Earth. Kosm. nauka tehnol. 2008 ;14(5):095-106.
Ionospheric response to acoustic influence according to the data of DEMETER and Chibis-M microsatellites. Space Sci. & Technol. 2018 ;24(6):41-56.
Nonlinear dynamical-information magnetosphere models for space weather forecasting. Kosm. nauka tehnol. 2008 ;14(1):77-84.