File:Creating a solar switchback article.jpg

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Summary

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English: Close to the Sun, and especially above active regions, there are open and closed magnetic field lines. The closed lines are loops of magnetism that arch up into the solar atmosphere before curving round and disappearing back into the Sun.
Date
Source https://www.esa.int/Science_Exploration/Space_Science/Solar_Orbiter/Solar_Orbiter_solves_magnetic_switchback_mystery
Author ESA

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Captions

Close to the Sun, and especially above active regions, there are open and closed magnetic field lines. The closed lines are loops of magnetism that arch up into the solar atmosphere before curving round and disappearing back into the Sun.

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9 October 2020

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current14:30, 19 September 2022Thumbnail for version as of 14:30, 19 September 2022960 × 233 (51 KB)SkiPaddlerUploaded a work by ESA from https://www.esa.int/Science_Exploration/Space_Science/Solar_Orbiter/Solar_Orbiter_solves_magnetic_switchback_mystery with UploadWizard
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