activity
20242026
collaborators

5 papers

astro-ph.SR2026

Performance of radio-based detection to operational monitoring M5+ class solar flares

Julia van Ravenswaaij, Ines Wilms, Ivan Ricardo +1

Early detection of major solar flares is critical for defense operations due to their potential to disturb radar and radio systems. Typically, soft X-ray flux is used to monitor an…

astro-ph.SR2025

Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT

Haopeng Wang, Stefaan Poedts, Andrea Lani +6

Compared to quasi-steady-state corona models that are constrained by a time-invariant magnetogram over a CR period, time-evolving corona models driven by time-varying photospheric…

physics.space-ph2024

Constraining the inner boundaries of COCONUT through plasma \b{eta} and Alfvén speed

Michaela Brchnelova, Boris Gudiksen, Mats Carlsson +2

Space weather modelling has been gaining importance due to our increasing dependency on technology sensitive to space weather effects, such as satellite services, air traffic and p…

astro-ph.SR2024

CME propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA

L. Linan, T. Baratashvili, A. Lani +4

This paper aims to present the time-dependent coupling between the coronal model COolfluid COroNal UnsTructured (COCONUT) and the heliospheric forecasting tool EUHFORIA. We perform…

astro-ph.SR2024

Cross-Field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope

Edin Husidic, Nicolas Wijsen, Luis Linan +3

Solar energetic particles (SEPs) associated with solar flares and coronal mass ejections (CMEs) are key agents of space weather phenomena, posing severe threats to spacecraft and a…