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7 papers

astro-ph.SR2026

Understanding the Travel-time Asymmetry of Acoustic Waves in Sunspots With Time-distance Helioseismology

Haiyu Li, Tobías Felipe, Elena Khomenko +3

The paper studies how acoustic waves travel through a sunspot, measuring differences in travel times for waves moving into versus out of the spot and using both observations and si…

astro-ph.SR2026

Solar vortex detection methods in MHD simulations: impact of magnetic field and spatial resolution

M. Koll Pistarini, E. Khomenko, T. Felipe +1

The aim of this paper is to investigate the influence of different magnetic field configurations and spatial resolutions on vortex structures. We analyzed a set of six three-dimens…

astro-ph.SR2025

Modeling Solar Atmosphere Dynamics with MAGEC

Anamaría Navarro, E. Khomenko, N. Vitas +1

Modeling the solar atmosphere is challenging due to its layered structure and multi-scale dynamics. We aim to validate the new radiative MHD code MAGEC, which combines the MANCHA a…

astro-ph.SR2025

The effect of local magnetic fields in quiet regions of stellar atmospheres simulated with MANCHA

Andrea Perdomo García, Nikola Vitas, Elena Khomenko +1

Our aim is to characterize the effects of the local magnetic fields in quiet regions of stellar atmospheres. We compute magneto-hydrodynamic and purely hydrodynamic simulations of…

astro-ph.SR2025

Vortex Flows in the Solar Atmosphere: Detection and Heating Mechanisms in 3D MHD Numerical Simulations

M. Koll Pistarini, E. Khomenko, T. Felipe

Vortex flows are structures associated with the rotation of the plasma and/or the magnetic field that are present throughout the solar atmosphere. In recent years, their study has…

astro-ph.SR2025

Convergence study of ambipolar diffusion in realistic simulations of magneto-convection

E. Khomenko, N. Vitas, M. Collados +1

The aim of this paper is to improve our understanding of the heating mechanisms of the solar chromosphere via realistic three-dimensional (3D) modeling of solar magneto-convection,…