44 citations · 44 across the 1 of their papers we have counts for
10 papers
Long characteristics vs. short characteristics in 3D radiative transfer simulations of polarized radiation
A. de Vicente, T. del Pino Alemán, J. Trujillo Bueno
We compare maps of scattering polarization signals obtained from three-dimensional (3D) radiation transfer calculations in a magneto-convection model of the solar atmosphere using…
Two-fluid simulations of Rayleigh-Taylor instability in a magnetized solar prominence thread. I. Effects of prominence magnetization and mass loading
B. Popescu Braileanu, V. S. Lukin, E. Khomenko +1
Solar prominences are formed by partially ionized plasma with inter-particle collision frequencies generally warranting magnetohydrodynamic treatment. In this work, we explore the…
Two-fluid simulations of waves in the solar chromosphere II. Propagation and damping of fast magneto-acoustic waves and shocks
B. Popescu Braileanu, V. S. Lukin, E. Khomenko +1
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…
Two-fluid simulations of waves in the solar chromosphere I: numerical code verification
B. Popescu Braileanu, V. S. Lukin, E. Khomenko +1
Solar chromosphere consists of a partially ionized plasma, which makes modeling the solar chromosphere a particularly challenging numerical task. Here we numerically model chromosp…
Three-dimensional simulations of solar magneto-convection including effects of partial ionization
E. Khomenko, N. Vitas, M. Collados +1
Over the last decades, realistic 3D radiative-MHD simulations have become the dominant theoretical tool for understanding the complex interactions between the plasma and the magnet…
MHDSTS: a new explicit numerical scheme for simulations of partially ionised solar plasma
P. A. González-Morales, E. Khomenko, T. P. Downes +1
The interaction of plasma with magnetic field in the partially ionised solar atmosphere is frequently modelled via a single-fluid approximation, which is valid for the case of a st…