Three Eruptions Observed by Remote Sensing Instruments Onboard Solar Orbiter
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Published:2023-03
Issue:3
Volume:298
Page:
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ISSN:0038-0938
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Container-title:Solar Physics
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language:en
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Short-container-title:Sol Phys
Author:
Mierla Marilena,Cremades Hebe,Andretta Vincenzo,Chifu Iulia,Zhukov Andrei N.,Susino Roberto,Auchère Frédéric,Vourlidas Angelos,Talpeanu Dana-Camelia,Rodriguez Luciano,Janssens Jan,Nicula Bogdan,Aznar Cuadrado Regina,Berghmans David,Bemporad Alessandro,D’Huys Elke,Dolla Laurent,Gissot Samuel,Jerse Giovanna,Kraaikamp Emil,Long David M.,Mampaey Benjamin,Möstl Christian,Pagano Paolo,Parenti Susanna,West Matthew J.,Podladchikova Olena,Romoli Marco,Sasso Clementina,Stegen Koen,Teriaca Luca,Thompson William,Verbeeck Cis,Davies Emma
Abstract
AbstractOn February 21 and March 21 – 22, 2021, the Extreme Ultraviolet Imager (EUI) onboard Solar Orbiter observed three prominence eruptions. The eruptions were associated with coronal mass ejections (CMEs) observed by Metis, Solar Orbiter’s coronagraph. All three eruptions were also observed by instruments onboard the Solar–TErrestrial RElations Observatory (Ahead; STEREO-A), the Solar Dynamics Observatory (SDO), and the Solar and Heliospheric Observatory (SOHO). Here we present an analysis of these eruptions. We investigate their morphology, direction of propagation, and 3D properties. We demonstrate the success of applying two 3D reconstruction methods to three CMEs and their corresponding prominences observed from three perspectives and different distances from the Sun. This allows us to analyze the evolution of the events, from the erupting prominences low in the corona to the corresponding CMEs high in the corona. We also study the changes in the global magnetic field before and after the eruptions and the magnetic field configuration at the site of the eruptions using magnetic field extrapolation methods. This work highlights the importance of multi-perspective observations in studying the morphology of the erupting prominences, their source regions, and associated CMEs. The upcoming Solar Orbiter observations from higher latitudes will help to constrain this kind of study better.
Funder
Max Planck Institute for Solar System Research
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
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