Shukhobodskaia, D. ; Talpeanu, D.-C. ; Rodriguez, L. ; D’Huys, E. ; Mierla, M. ; Dorsch, B. D. ; West, M. ; Berghmans, D. ; Zhukov, A. ; Verbeeck, C.

Poster presented at European Space Weather Week 2024, Coimbra, Portugal on 2024-11-08

Abstract: This study deals with prominence eruptions captured by the Extreme Ultraviolet Imager/Full Sun Imager (EUI/FSI) on board Solar Orbiter. We analyse a selection of 230 eruptions from the detailed catalogue, focusing on events where prominences reach projected heights beyond 2 solar radii. The large field of view (up to fourteen solar radii) allows FSI to observe solar eruptions from the solar disc up to heights never before observed in EUV passbands. This makes the instrument uniquely suited for tracing the early phases of eruptions through the middle corona. The large set of investigated events offers a wide perspective on the inherent variability within these phenomena. This ongoing statistical analysis aims at uncovering the various properties of these eruptions, such as speed and deflection, morphological features, 3D characteristics, and their interaction with neighbouring magnetic field structures. We present here the status of this statistical study with an overview of the observed prominence eruptions and their properties.