collaborators

5 papers

physics.space-ph2026

Real-time prediction of two geomagnetic storms using Solar Orbiter as a far upstream solar wind monitor

Emma E. Davies, Eva Weiler, Christian Möstl +8

We present the first real-time predictions of coronal mass ejection (CME) magnetic structure and resulting geomagnetic impact at Earth for two events using far-upstream observation…

astro-ph.SR2026

Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure

Hannah T. Rüdisser, Emma E. Davies, Ute V. Amerstorfer +6

We present an automated pipeline for operational short-term forecasting of coronal mass ejection (CME) magnetic field structure at L1, coupling arrival time prediction, in situ det…

astro-ph.SR2026

On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au

Christian Möstl, Emma E. Davies, Eva Weiler +8

A central question for understanding interplanetary coronal mass ejection (ICME) physics and improving space weather forecasting is how ICMEs evolve in interplanetary space. We hav…

physics.space-ph2026

ARCANE -- Early Detection of Interplanetary Coronal Mass Ejections

H. T. Rüdisser, G. Nguyen, J. Le Louëdec +2

Interplanetary coronal mass ejections (ICMEs) are major drivers of space weather disturbances, posing risks to both technological infrastructure and human activities. Automatic det…

astro-ph.SR2025

Intermittency in Interplanetary Coronal Mass Ejections Observed by Parker Solar Probe and Solar Orbiter

Julia Ruohotie, Simon Good, Christian Möstl +1

Intermittency has been studied extensively in the fast and slow solar winds but to a far lesser extent in interplanetary coronal mass ejections (ICMEs). While ICMEs are often chara…