9–13 Sept 2024
Turin, Italy
Europe/Rome timezone

Analysis of solar eruptive events captured by Solar Orbiter during the "Eruption Watch" coordination campaigns.

Not scheduled
1h
Turin, Italy

Turin, Italy

Centro Congressi Unione Industriali Torino Via Vela, 17 - 10128 Torino
Poster Multi-scale energy release, flares and coronal mass ejections Coffee break and poster session 2

Description

Solar Orbiter's observations, during Remote Science Windows, a period of ~30 days happening twice per year, are organized into Solar Orbiter Observing Plans (SOOPs). Each SOOP consists of a coordinated set of operations involving multiple instruments to address mission objectives. The Eruption Watch SOOP is a high-resolution plan designed to capture eruptive events, engaging all remote sensing and in-situ instruments.
This presentation focuses on analyzing eruptive events observed during two specific Eruption Watch campaigns in April and October 2023. We have selected events captured by the PHI, EUI, Metis, and SolOHI instruments to study their physical and dynamic properties from the photosphere to the extended corona.
Finally, using observations starting from 2022, we conducted a statistical analysis of the observed erupting events.

Primary author

Clementina Sasso (Istituto Nazionale di Astrofisica (INAF))

Co-authors

Angelos Vourlidas (Johns Hopkins University - Applied Physics Laboratory) David Berghmans (Royal Observatory of Belgium) David Orozco Suarez (Instituto de Astrofísica de Andalucía (IAA-CSIC)) Federico Landini (Istituto Nazionale di Astrofisica (INAF)) Frédéric Auchère (Institut d'Astrophysique Spatiale) Gherardo Valori (MPS) Giuliana Russano (Istituto Nazionale di Astrofisica (INAF)) Hanna Strecker (Instituto de Astrofísica de Andalucía (IAA-CSIC)) Johann Hirzberger (Max-Planck-Institute für Sonnensystemforschung) Luciano Rodriguez (Royal Observatory of Belgium) Phillip Hess (U.S. Naval Research Laboratory (NRL), Washington D.C., USA)

Presentation materials

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