activity
20052026
most citedRadiative MHD simulation of sunspot structure

353 citations · 3.2k across the 63 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.IM2022

Towards data-driven modeling and real-time prediction of solar flares and coronal mass ejections

M. Rempel, Y. Fan, M. Dikpati +7

Modeling of transient events in the solar atmosphere requires the confluence of 3 critical elements: (1) model sophistication, (2) data availability, and (3) data assimilation. Thi…

astro-ph.SR2022★ 12 cited

Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere

M. Skan, S. Danilovic, J. Leenaarts +2

Recent observations revealed loop-like structures at very small scales visible in observables that sample transition region (TR) and coronal temperatures. Their formation remains u…

astro-ph.SR2022★ 6 cited

Rapid Blue- and Red-shifted Excursions in H line profiles synthesized from realistic 3D MHD simulations

S. Danilovic, J. P. Bjørgen, J. Leenaarts +1

Rapid blue- and red-shifted events (RBEs/RREs) may have an important role in mass-loading and heating the solar corona, but their nature and origin are still debatable. We aim to m…

astro-ph.SR2022★ 8 cited

Effects of spectral resolution on simple magnetic field diagnostics of the Mg II h & k lines

Rebecca Centeno, Matthias Rempel, Roberto Casini +1

We study the effects of finite spectral resolution on the magnetic field values retrieved through the weak field approximation (WFA) from the cores of the Mg II h & k lines. The re…

astro-ph.SR2022★ 55 cited

Chromospheric Extension of the MURaM Code

D. Przybylski, R. Cameron, S. K. Solanki +5

Detailed numerical models of chromosphere and corona are required to understand the heating of the solar atmosphere. An accurate treatment of the solar chromosphere is complicated…

astro-ph.SR2022★ 22 cited

Heating of the solar chromosphere through current dissipation

J. M. da Silva Santos, S. Danilovic, J. Leenaarts +5

The solar chromosphere is heated to temperatures higher than predicted by radiative equilibrium. This excess heating is greater in active regions where the magnetic field is strong…