361 citations · 1.9k across the 35 of their papers we have counts for
35 papers
Magnetic flux cancellation in the solar atmosphere through 3D realistic numerical modeling
F. Moreno-Insertis, V. H. Hansteen, D. Nóbrega-Siverio
We present a radiation-magnetohydrodynamics (RMHD) simulation of a magnetic cancellation event. The model is calculated with the Bifrost code and spans from the uppermost convectio…
Spectropolarimetric synthesis of forbidden lines in MHD models of coronal bright points
Ernest Alsina Ballester, Daniel Nóbrega-Siverio, Fernando Moreno-Insertis +1
The inference of the magnetic field vector from spectropolarimetric observations is crucial for understanding the physical processes governing the solar corona. We investigate whic…
Merging plasmoids and nanojet-like ejections in a coronal current sheet
Samrat Sen, F. Moreno-Insertis
Forced magnetic reconnection is triggered by external perturbations, which are ubiquitous in the solar corona. This process plays a crucial role in the energy release during solar…
Study of the excitation of large amplitude oscillations in a prominence by nearby flares
Manuel Luna, Reetika Joshi, Brigitte Schmieder +3
Large amplitude oscillations commonly occur in solar prominences, triggered by energetic phenomena such as jets and flares. On March 14-15, 2015, a filament partially erupted in tw…
High-resolution observations of recurrent jets from an arch filament system
Reetika Joshi, Luc Rouppe van der Voort, Brigitte Schmieder +4
Solar jets are collimated plasma ejections along magnetic field lines observed in hot (EUV jets) and cool (chromospheric surges) temperature diagnostics. Their trigger mechanisms a…
Deciphering the solar coronal heating: Energizing small-scale loops through surface convection
D. Nóbrega-Siverio, F. Moreno-Insertis, K Galsgaard +4
The solar atmosphere is filled with clusters of hot small-scale loops commonly known as Coronal Bright Points (CBPs). These ubiquitous structures stand out in the Sun by their stro…