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Akademický článek
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Autor:
Felipe, T., Manrique, S. J. González, Martínez-Gómez, D., Gómez-Míguez, M. M., Khomenko, E., Noda, C. Quintero, Socas-Navarro, H.
In sunspot umbrae, the core of some chromospheric lines exhibits periodic brightness enhancements known as umbral flashes. The consensus is that they are produced by the upward propagation of shock waves. This view has recently been challenged by the
Externí odkaz:
http://arxiv.org/abs/2411.16467
Simple active models of matter recapitulate complex biological phenomena. Their out-of-equilibrium nature, however, often makes these models beyond the reach of first-principle descriptions. This limitation is particularly perplexing when attempting
Externí odkaz:
http://arxiv.org/abs/2409.12037
Autor:
Khomenko, Elena, Martínez-Gómez, David
Publikováno v:
Chapter 6 in "Magnetohydrodynamic Processes in Solar Plasmas", ed. A.K. Srivastava, M. Goossens and I. Arregui, Elsevier (2024), pp. 203-271 https://www.sciencedirect.com/science/article/abs/pii/B9780323956642000116
This Chapter outlines the basic properties of waves in solar partially ionized plasmas. It provides a summary of the main sets of equations, from the single-fluid formalism, to the multi-fluid one, giving examples for purely hydrogen, and for hydroge
Externí odkaz:
http://arxiv.org/abs/2409.11528
Autor:
Malafeyev, O. A., Khomenko, I. E.
In economics, there are many ways to describe the interaction between a "seller" and a "buyer". The most common one, with which we interact almost every day, is selling for a fixed price. This option is perfect for selling a mass product, when we hav
Externí odkaz:
http://arxiv.org/abs/2407.06248
Autor:
Kondeti, V. S. Santosh K., Yatom, Shurik, Romadanov, Ivan, Raitses, Yevgeny, Dorf, Leonid, Khomenko, Andrei
A wide variety of feed gases are used to generate low-temperature plasmas for the microelectronics and the sustainability applications. These plasmas often have a complex combination of reactive and non-reactive species which may have spatial and tem
Externí odkaz:
http://arxiv.org/abs/2406.07747
Aims. Our aim is to test how different binning strategies previously studied in one-dimensional models perform in three-dimensional radiative hydrodynamic simulations of stellar atmospheres. Methods. Realistic box-in-a-star simulations of the near-su
Externí odkaz:
http://arxiv.org/abs/2406.02271
Solar partially ionized plasma is frequently modeled using single-fluid (1F) or two-fluid (2F) approaches. In the 1F case, charge-neutral interactions are often described through ambipolar diffusion, while the 2F model fully considers charge-neutral
Externí odkaz:
http://arxiv.org/abs/2402.13813