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of 1 191
pro vyhledávání: '"Lukin, V"'
Publikováno v:
Phil. Trans. R. Soc. A. 382:20230417 (2024)
This study explores non-linear development of the magnetized Rayleigh-Taylor instability (RTI) in a prominence-corona transition region. Using a two-fluid model of a partially ionized plasma, we compare RTI simulations for several different magnetic
Externí odkaz:
http://arxiv.org/abs/2401.03323
Publikováno v:
A&A 670, A31 (2023)
We report on results of high resolution two fluid non-linear simulations of the Rayleigh Taylor Instability (RTI) at the interface between a solar prominence and the corona. These follow results reported earlier by Popescu Braileanu et al. (2021a,b)
Externí odkaz:
http://arxiv.org/abs/2112.13043
Publikováno v:
A&A 650, A181 (2021)
In this work, we explore the dynamical impacts and observable signatures of two-fluid effects in the parameter regimes when ion-neutral collisions do not fully couple the neutral and charged fluids. The purpose of this study is to deepen our understa
Externí odkaz:
http://arxiv.org/abs/2101.12731
Publikováno v:
A&A 646, A93 (2021)
Solar prominences are formed by partially ionized plasma with inter-particle collision frequencies generally warranting magnetohydrodynamic treatment. In this work, we explore the dynamical impacts and observable signatures of two-fluid effects in th
Externí odkaz:
http://arxiv.org/abs/2007.15984
Akademický článek
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Publikováno v:
A&A 630, A79 (2019)
Waves and shocks traveling through the solar chromospheric plasma are influenced by its partial ionization and weak collisional coupling, and may become susceptible to multi-fluid effects, similar to interstellar shock waves. In this study, we consid
Externí odkaz:
http://arxiv.org/abs/1908.05262
Publikováno v:
A&A 627, A25 (2019)
Solar chromosphere consists of a partially ionized plasma, which makes modeling the solar chromosphere a particularly challenging numerical task. Here we numerically model chromospheric waves using a two-fluid approach with a newly developed numerica
Externí odkaz:
http://arxiv.org/abs/1905.03559
Autor:
Lukin, V. V., Malanchev, K. L., Shakura, N. I., Postnov, K. A., Chechetkin, V. M., Utrobin, V. P.
Publikováno v:
MNRAS, 2017, v. 467, pp. 2934-2942
We present the results of 3D-hydrodynamical simulations of accretion flow in the eclipsing dwarf nova V1239 Her in quiescence. The model includes the optical star filling its Roche lobe, a gas stream emanating from the inner Lagrangian point of the b
Externí odkaz:
http://arxiv.org/abs/1702.00587
Autor:
Lugovsky, A. Yu., Lukin, V. V.
Publikováno v:
Mathematical Models & Computer Simulations; Oct2024, Vol. 16 Issue 5, p676-686, 11p
