activity
20242026
most citedNew possible way to determine stellar wind terminal velocity from analysis of Lyman- absorption spectra

3 citations · 5 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026★ 3 cited

New possible way to determine stellar wind terminal velocity from analysis of Lyman- absorption spectra

Sergey D. Korolkov, Vladislav V. Izmodenov

Stellar winds interact with the partially ionized interstellar medium (ISM), forming astrospheres. A key feature of this interaction is the hydrogen wall - secondary interstellar a…

astro-ph.SR2025★ 2 cited

The Effect of Magnetic Field Dissipation in the Inner Heliosheath: Reconciling Global Heliosphere Model and Voyager Data

Sergey D. Korolkov, Igor I. Baliukin, Merav Opher

Global ideal magnetohydrodynamic models of the heliosphere typically predict a greatly exaggerated magnetic field pile-up in the inner heliosheath (IHS), the region between the ter…

astro-ph.SR2025

Mathematical Modeling of Kelvin-Helmholtz Instability at Tangential Discontinuities in Partially Ionized Plasma: Application to Heliopause Dynamics

A. V. Titova, S. D. Korolkov, V. V. Izmodenov

The stability of the heliopause, the tangential discontinuity separating the solar wind from the interstellar medium, is influenced by various processes, including the Kelvin-Helmh…

astro-ph.SR2024

Unstable gas flow in a flat channel under the influence of a transverse force field: self-oscillations of the jet

S. D. Korolkov, V. V. Izmodenov

A subsonic flow of an ideal gas through a flat channel in the presence of a mass force field is considered. The forces acting on the gas are reduced to the attraction to the channe…

astro-ph.SR2024

Effects of charge exchange on plasma flow in the heliosheath and astrosheathes

S. D. Korolkov, V. V. Izmodenov

Shock boundary layers are regions bounded by a shock wave on the one side and tangential discontinuity on the other side. These boundary layers are commonly observed in astrophysic…