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October 14, 2026
At HSE University–St Petersburg, Experts Discuss How AI Changes Tourist Routes and Cultural Heritage
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HSE Experts Take Part in 23rd Annual Meeting of Valdai Discussion Club
The 23rd Annual Meeting of the Valdai Discussion Club was held from September 28 to October 1, 2026 under the theme ‘Responsibility for the Future: Limits of the Possible, or Limitless Possibilities?’ The forum brought together 120 experts from 40 countries, including representatives of China, the United States, India, Brazil, the United Kingdom, Germany, Egypt, Iran, and Japan.

 

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

Lobachevskii Journal of Mathematics. 2025. Vol. 46. No. 9. P. 4526–4533.
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–Helmholtz instability. This study investigates the role of charge exchange collisions between protons and hydrogen (H) atoms in reduction of the Kelvin–Helmholtz growth rate at the heliopause. Using a two-dimensional gasdynamic model with the inclusion of H atoms, we perform numerical simulations of the plasma flow near the heliopause flanks. We conduct a parametric study by varying the Knudsen number. Our results indicate that charge exchange collisions play a crucial role in suppressing the Kelvin–Helmholtz instability. As the Knudsen number decreases, the flow transitions from an unstable regime to a smoother state.

Research target: Physics
Language: English
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Keywords: mathematical modelingresonant charge exchangeрезонансная перезарядкаheliosphereinterstellar mediumгелиосферамежзвездная средаastrosphere-interstellar medium interactionsМатематическое моделированиеKelvin-Helmholtz instabilityНеустойчивость Кельвина-Гельмгольца
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