113 citations · 222 across the 9 of their papers we have counts for
10 papers
Influence of numerical domain design in simulations of solar coronal heating with the MAGEC code
Anamaría Navarro, E. Khomenko, T. Felipe +1
Numerical simulations are essential for studying the solar atmosphere, especially in the context of the coronal heating problem. Understanding how numerical factors and boundary co…
Magnetoacoustic Shocks and Spectropolarimetric Signals in He I 10830 Å
Hirdesh Kumar, Tobias Felipe, Christoph Kuckein +2
Umbral flashes are manifestations of magnetoacoustic shocks in the solar chromosphere. These phenomena are thought to influence the evolution of chromospheric umbral magnetic field…
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…
Multi-wavelength spectropolarimetric observations of AR13724 performed by GRIS
C. Quintero Noda, J. C. Trelles Arjona, T. del Pino Alemán +10
Multi-line spectropolarimetric observations allow for the simultaneous inference of the magnetic field at different layers of the solar atmosphere and provide insight into how thes…
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…
Observations of umbral flashes in the resonant sunspot chromosphere
T. Felipe, S. J. González Manrique, D. Martínez-Gómez +4
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 pro…
Mancha3D code: Multi-purpose Advanced Non-ideal MHD Code for High resolution simulations in Astrophysics
M. Modestov, E. Khomenko, N. Vitas +14
The Mancha3D code is a versatile tool for numerical simulations of magnetohydrodynamic processes in solar/stellar atmospheres. The code includes non-ideal physics derived from plas…
Two fluid dynamics in solar prominences
S. J. González Manrique, E. Khomenko, M. Collados +3
Solar prominences contain a significant amount of neutral species. The dynamics of the ionised and neutral fluids composing the prominence plasma can be slightly different if the c…
Magneto-acoustic waves in sunspots: first results from a new 3D nonlinear magnetohydrodynamic code
T. Felipe, E. Khomenko, M. Collados
Waves observed in the photosphere and chromosphere of sunspots show complex dynamics and spatial patterns. The interpretation of high-resolution sunspot wave observations requires…
Non-linear numerical simulations of magneto-acoustic wave propagation in small-scale flux tubes
E. Khomenko, M. Collados, T. Felipe
We present results of non-linear, 2D, numerical simulations of magneto-acoustic wave propagation in the photosphere and chromosphere of small-scale flux tubes with internal structu…