activity
20052026
most citedDynamics of the Solar Magnetic Network: Two-dimensional MHD Simulations

85 citations · 500 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.SR2026

Wave excitation by a collapsing granule: insights from IFU observations and high-resolution RMHD simulations

J. Buttler, G. Vigeesh, I. Milić +5

Context. Granular collapse is an ubiquitous process of granular evolution on the solar surface, but it is hard to analyze in sufficient spatial, temporal, and spectral detail. Aims…

astro-ph.SR2022★ 26 cited

An innovative and automated method for vortex identification. I. Description of the SWIRL algorithm

José Roberto Canivete Cuissa, Oskar Steiner

Context. A universally accepted definition of what a vortex is has not yet been reached. Therefore, we lack an unambiguous and rigorous method for the identification of vortices in…

astro-ph.SR2022★ 12 cited

Methodology for estimating the magnetic Prandtl number and application to solar surface small-scale dynamo simulations

Fabio Riva, Oskar Steiner

Context. A crucial step in the numerical investigation of small-scale dynamos in the solar atmosphere consists of an accurate determination of the magnetic Prandtl number, Prm, ste…

math.NA2021

A novel fourth-order WENO interpolation technique. A possible new tool designed for radiative transfer

Gioele Janett, Oskar Steiner, Ernest Alsina Ballester +2

Context. Several numerical problems require the interpolation of discrete data that present various types of discontinuities. The radiative transfer is a typical example of such a…

astro-ph.SR2021★ 46 cited

The Alfvénic nature of chromospheric swirls

Andrea Francesco Battaglia, José Roberto Canivete Cuissa, Flavio Calvo +2

We investigate the evolution and origin of small-scale chromospheric swirls by analyzing numerical simulations of the quiet solar atmosphere, using the radiative magnetohydrodynami…

astro-ph.SR2020★ 6 cited

On the effect of oscillatory phenomena on Stokes inversion results

P. H. Keys, O. Steiner, G. Vigeesh

Stokes inversion codes are crucial in returning properties of the solar atmosphere, such as temperature and magnetic field strength. However, the success of such algorithms to retu…