112 citations · 1.2k across the 62 of their papers we have counts for
5 papers · 1 filter
Non-LTE inversions of a confined X2.2 flare: I. Vector magnetic field in the photosphere and chromosphere
G. J. M. Vissers, S. Danilovic, J. de la Cruz Rodriguez +7
Obtaining the magnetic field vector accurately in the solar atmosphere is essential for studying changes in field topology during flares and to reliably model space weather. We tac…
Electron acceleration and radio emission following the early interaction of two coronal mass ejections
D. E. Morosan, E. Palmerio, J. E. Räsänen +6
Context. Coronal mass ejections (CMEs) are large eruptions of magnetised plasma from the Sun that are often accompanied by solar radio bursts produced by accelerated electrons. Aim…
Using radio triangulation to understand the origin of two subsequent type II radio bursts
Immanuel Christopher Jebaraj, Jasmina Magdalenic, Tatiana Podladchikova +7
Context: Eruptive events such as coronal mass ejections (CMEs) and flares accelerate particles and generate shock waves which can arrive at Earth and can disturb the magnetosphere.…
Three-dimensional reconstruction of multiple particle acceleration regions during a coronal mass ejection
D. E. Morosan, E. Palmerio, J. Pomoell +3
Context. Some of the most prominent sources for particle acceleration in our Solar System are large eruptions of magnetised plasma from the Sun called coronal mass ejections (CMEs)…
The effect of drifts on the decay phase of SEP events
Nicolas Wijsen, Angels Aran, Blai Sanahuja +2
We study the effect of the magnetic gradient and curvature drifts on the pitch-angle dependent transport of solar energetic particles (SEPs), focusing on 3 - 36 MeV protons. By con…