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Magnetic flux rope models and data-driven magnetohydrodynamic simulations of solar eruptions
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Mancha3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics
M. Modestov, E. Khomenko, N. Vitas, A. de Vicente, A. Navarro, P. A. González-Morales, M. Collados, T. Felipe, D. Martínez-Gómez, P. Hunana, M. Luna, M. Koll Pistarini, B. Popescu Braileanu, A. Perdomo García, V. Liakh, I. Santamaria and M. M. Gomez Miguez Solar Physics 299(2) (2024) https://doi.org/10.1007/s11207-024-02267-1
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Hydrodynamic simulations of cool stellar atmospheres with MANCHA
The influence of thermal pressure gradients and ionization (im)balance on the ambipolar diffusion and charge-neutral drifts
M. M. Gómez Míguez, D. Martínez Gómez, E. Khomenko and N. Vitas Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 382(2272) (2024) https://doi.org/10.1098/rsta.2023.0228
Gas-kinetic scheme for partially ionized plasma in hydrodynamic regime
Comparative clustering analysis of Ca II 854.2 nm spectral profiles from simulations and observations
Thore E. Moe, Tiago M. D. Pereira, Luc Rouppe van der Voort, Mats Carlsson, Viggo Hansteen, Flavio Calvo and Jorrit Leenaarts Astronomy & Astrophysics 682 A11 (2024) https://doi.org/10.1051/0004-6361/202347328
Opacity for realistic 3D MHD simulations of cool stellar atmospheres
A. Perdomo García, N. Vitas, E. Khomenko, M. Collados, C. Allende Prieto, I. Hubeny and Y. Osorio Astronomy & Astrophysics 675 A160 (2023) https://doi.org/10.1051/0004-6361/202346341
Chromospheric Heating from Local Magnetic Growth and Ambipolar Diffusion under Nonequilibrium Conditions
Juan Martínez-Sykora, Jaime de la Cruz Rodríguez, Milan Gošić, Alberto Sainz Dalda, Viggo H. Hansteen and Bart De Pontieu The Astrophysical Journal Letters 943(2) L14 (2023) https://doi.org/10.3847/2041-8213/acafe9
Numerical Simulations and Observations of Mg ii in the Solar Chromosphere
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Chromospheric Heating by Magnetohydrodynamic Waves and Instabilities
A. K. Srivastava, J. L. Ballester, P. S. Cally, et al. Journal of Geophysical Research: Space Physics 126(6) (2021) https://doi.org/10.1029/2020JA029097
Influence of ambipolar and Hall effects on vorticity in three-dimensional simulations of magneto-convection
E. Khomenko, M. Collados, N. Vitas and P. A. González-Morales Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 379(2190) (2021) https://doi.org/10.1098/rsta.2020.0176
Newly formed downflow lanes in exploding granules in the solar photosphere
Acoustic-gravity wave propagation characteristics in three-dimensional radiation hydrodynamic simulations of the solar atmosphere
B. Fleck, M. Carlsson, E. Khomenko, et al. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 379(2190) (2021) https://doi.org/10.1098/rsta.2020.0170
Spatial variation in the periods of ion and neutral waves in a solar magnetic arcade
Measurements of Photospheric and Chromospheric Magnetic Field Structures Associated with Chromospheric Heating over a Solar Plage Region
Tetsu Anan, Thomas A. Schad, Reizaburo Kitai, Gabriel I. Dima, Sarah A. Jaeggli, Lucas A. Tarr, Manuel Collados, Carlos Dominguez-Tagle and Lucia Kleint The Astrophysical Journal 921(1) 39 (2021) https://doi.org/10.3847/1538-4357/ac1b9c
Two-fluid Modeling of Acoustic Wave Propagation in Gravitationally Stratified Isothermal Media
Ion–neutral Interactions and Nonequilibrium Ionization in the Solar Chromosphere
Juan Martínez-Sykora, Jorrit Leenaarts, Bart De Pontieu, Daniel Nóbrega-Siverio, Viggo H. Hansteen, Mats Carlsson and Mikolaj Szydlarski The Astrophysical Journal 889(2) 95 (2020) https://doi.org/10.3847/1538-4357/ab643f
Wave heating of the solar atmosphere without shocks
On the Origin of the Magnetic Energy in the Quiet Solar Chromosphere
Juan Martínez-Sykora, Viggo H. Hansteen, Boris Gudiksen, Mats Carlsson, Bart De Pontieu and Milan Gošić The Astrophysical Journal 878(1) 40 (2019) https://doi.org/10.3847/1538-4357/ab1f0b
Magnetic fields and thermodynamic conditions in the pre-peak phase of M6.4 / 3N solar flare