activity
20182026
most citedSTiC -- A multi-atom non-LTE PRD inversion code for full-Stokes solar observations

161 citations · 214 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026★ 1 cited

The magnetic sensitivity of the Ca II H and K lines

M. Kriginsky, J. Leenaarts, J. de la Cruz Rodriguez +2

The solar chromosphere is a transition layer between the cool, dense photosphere and the hot, rarefied corona. This boundary region plays a key role in regulating energy transport…

astro-ph.SR2025★ 1 cited

Active chromospheric fibril singularity: Coordinated observations from Solar Orbiter, SST, and IRIS

Reetika Joshi, Luc Rouppe van der Voort, Guillaume Aulanier +6

The fine structures of the solar chromosphere, driven by photospheric motions, play a crucial role in the dynamics of solar magnetic fields. Many have been already identified such…

astro-ph.SR2024★ 6 cited

Coronal kink oscillations and photospheric driving: combining SolO/EUI and SST/CRISP high-resolution observations

Nicolas Poirier, Sanja Danilovic, Petra Kohutova +4

The driving and excitation mechanisms of decay-less kink oscillations in coronal loops remain under debate. We aim to quantify and provide simple observational constraints on the p…

astro-ph.SR2019★ 6 cited

Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025)

Rolf Schlichenmaier, Luis R. Bellot Rubio, Manuel Collados Vera +31

The European Strategy Forum on Research Infrastructures (ESFRI) included the European Solar Telescope (EST) as an ESFRI Project in its 2016 Roadmap and confirmed this status in 202…

astro-ph.SR2019★ 39 cited

Solar image denoising with convolutional neural networks

C. J. Díaz Baso, J. de la Cruz Rodríguez, S. Danilovic

The topology and dynamics of the solar chromosphere are greatly affected by the presence of magnetic fields. The magnetic field can be inferred by analyzing polarimetric observatio…

astro-ph.SR2018★ 161 cited

STiC -- A multi-atom non-LTE PRD inversion code for full-Stokes solar observations

J. de la Cruz Rodríguez, J. Leenaarts, S. Danilovic +1

The inference of the underlying state of the plasma in the solar chromosphere remains extremely challenging because of the nonlocal character of the observed radiation and plasma c…