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Observation of a Magnetic Switchback in the Solar Corona

MPG-Autoren
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Heinzel,  Petr
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Teriaca,  Luca
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Sasso,  Clementina
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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De Leo,  Yara
IMPRS for Solar System Science at the University of Göttingen, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Aznar Cuadrado,  Regina
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Mandal,  Sudip
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Peter,  Hardi
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Rodriguez,  Luciano
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Schühle,  Udo
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Zitation

Telloni, D., Zank, G. P., Stangalini, M., Downs, C., Liang, H., Nakanotani, M., et al. (2022). Observation of a Magnetic Switchback in the Solar Corona. The Astrophysical Journal, 936, L25. doi:10.3847/2041-8213/ac8104.


Zitierlink: https://hdl.handle.net/21.11116/0000-000C-9550-1
Zusammenfassung
Switchbacks are sudden, large radial deflections of the solar wind magnetic field, widely revealed in interplanetary space by the Parker Solar Probe. The switchbacks' formation mechanism and sources are still unresolved, although candidate mechanisms include Alfvénic turbulence, shear-driven Kelvin-Helmholtz instabilities, interchange reconnection, and geometrical effects related to the Parker spiral. This Letter presents observations from the Metis coronagraph on board a Solar Orbiter of a single large propagating S-shaped vortex, interpreted as the first evidence of a switchback in the solar corona. It originated above an active region with the related loop system bounded by open-field regions to the east and west. Observations, modeling, and theory provide strong arguments in favor of the interchange reconnection origin of switchbacks. Metis measurements suggest that the initiation of the switchback may also be an indicator of the origin of slow solar wind.