activity
20072021
most citedNumerical simulations of quiet Sun magnetic fields seeded by Biermann battery

44 citations · 67 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20215 cited

Newly formed downflow lanes in exploding granules in the solar photosphere

M. Ellwarth, C. E. Fischer, N. Vitas +2

Exploding granules have drawn renewed interest because of their interaction with the magnetic field. Especially the newly forming downflow lanes developing in their centre seem to…

astro-ph.SR2020

Joint action of Hall and ambipolar effects in 3D magneto-convection simulations of the quiet Sun. I. Dissipation and generation of waves

P. A. Gonzalez-Morales, E. Khomenko, N. Vitas +1

The partial ionization of the solar plasma causes several nonideal effects such as the ambipolar diffusion, the Hall effect, and the Biermann battery effect. Here we report on the…

astro-ph.SR2018

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…

astro-ph.SR201744 cited

Numerical simulations of quiet Sun magnetic fields seeded by Biermann battery

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

The magnetic fields of the quiet Sun cover at any time more than 90\% of its surface and their magnetic energy budget is crucial to explain the thermal structure of the solar atmos…

astro-ph.SR2016

How different are the Liège and Hamburg atlases of the solar spectrum?

H. -P. Doerr, N. Vitas, D. Fabbian

Context: The high-fidelity solar spectral atlas prepared by Delbouille and co-workers (Liège atlas), and the one by Neckel and co-workers (Hamburg atlas), are widely recognised as…

astro-ph200718 cited

On the solar abundance of indium

N. Vitas, I. Vince, M. Lugaro +3

The generally adopted value for the solar abundance of indium is over six times higher than the meteoritic value. We address this discrepancy through numerical synthesis of the 451…