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How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities?

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https://hal.archives-ouvertes.fr/hal-01287839
Contributor : Benjamin Favier Connect in order to contact the contributor
Submitted on : Tuesday, October 12, 2021 - 11:38:16 AM
Last modification on : Wednesday, October 27, 2021 - 3:43:21 PM

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Benjamin Favier, Laurène Jouve, William Edmunds, Lara Silvers, Michael Proctor. How can large-scale twisted magnetic structures naturally emerge from buoyancy instabilities?. Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2012, ⟨10.1111/j.1365-2966.2012.21920.x⟩. ⟨hal-01287839⟩

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