Observation of a Magnetic Switchback in the Solar Corona
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Published:2022-09-01
Issue:2
Volume:936
Page:L25
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ISSN:2041-8205
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Container-title:The Astrophysical Journal Letters
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language:
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Short-container-title:ApJL
Author:
Telloni DanieleORCID, Zank Gary P.ORCID, Stangalini MarcoORCID, Downs CooperORCID, Liang HaomingORCID, Nakanotani MasaruORCID, Andretta VincenzoORCID, Antonucci EsterORCID, Sorriso-Valvo LucaORCID, Adhikari LaxmanORCID, Zhao LinglingORCID, Marino RaffaeleORCID, Susino RobertoORCID, Grimani CatiaORCID, Fabi MicheleORCID, D’Amicis RaffaellaORCID, Perrone DeniseORCID, Bruno RobertoORCID, Carbone FrancescoORCID, Mancuso SalvatoreORCID, Romoli MarcoORCID, Deppo Vania DaORCID, Fineschi SilvanoORCID, Heinzel PetrORCID, Moses John D.ORCID, Naletto GiampieroORCID, Nicolini GianalfredoORCID, Spadaro DanieleORCID, Teriaca LucaORCID, Frassati FedericaORCID, Jerse GiovannaORCID, Landini FedericoORCID, Pancrazzi MaurizioORCID, Russano GiulianaORCID, Sasso ClementinaORCID, Biondo RuggeroORCID, Burtovoi AleksandrORCID, Capuano Giuseppe E.ORCID, Casini ChiaraORCID, Casti MartaORCID, Chioetto PaoloORCID, Leo Yara DeORCID, Giarrusso MarinaORCID, Liberatore AlessandroORCID, Berghmans DavidORCID, Auchère FrédéricORCID, Cuadrado Regina AznarORCID, Chitta Lakshmi P.ORCID, Harra LouiseORCID, Kraaikamp EmilORCID, Long David M.ORCID, Mandal SudipORCID, Parenti SusannaORCID, Pelouze GabrielORCID, Peter HardiORCID, Rodriguez LucianoORCID, Schühle UdoORCID, Schwanitz ConradORCID, Smith Phil J.ORCID, Verbeeck CisORCID, Zhukov Andrei N.ORCID
Abstract
Abstract
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.
Funder
Agenzia Spaziale Italiana
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
36 articles.
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