Dorsch, Brenda Daniela ; Talpeanu, Dana Camelia ; Rodriguez, Luciano ; D'Huys, Elke ; Mierla, Marilena ; Shukhobodskaia, Daria ; West, Matt ; Berghmans, David ; Zhukov, Andrei ; Verbeek, Cis

Talk presented at CoCo-Con, Leuven, Belgium. on 2024-05-23

Abstract: In this study, we are analyzing prominence eruptions recorded by the Extreme Ultraviolet Imager/Full Sun Imager (EUI/FSI) telescope on board Solar Orbiter. We are using the comprehensive list of eruptions available at https://www.sidc.be/EUI/solar-eruptions. From these, we selected events based on the available data frames and on their observed projected heights exceeding 2 solar radii. The large field of view (up to 14 solar radii) and CMOS (Complementary Metal-Oxide-Semiconductor) sensors allow the FSI telescope 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 extremely large set of investigated events (230 eruptions) offers a wide perspective on the inherent variability within these phenomena. This ongoing statistical analysis aims at uncovering the various properties of these eruptions, including their kinematic attributes, such as speed and deflection, morphological features, 3D characteristics, and their interaction with the neighboring magnetic field structures. We present here the current progress of this statistical study with an overview of the observed prominence eruptions and their properties, as well as the associated features.

Keyword(s): Prominence ; EUI ; Solar Orbiter ; CoCo-Con