Resolving the solar prominence/filament paradox using the magnetic Rayleigh–Taylor instability
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-022-01705-z.pdf
Reference77 articles.
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3. Adrover-González, A. & Terradas, J. 3D numerical simulations of oscillations in solar prominences. Astron. Astrophys. 633, A113 (2020).
4. Wyper, P. F. et al. A model for the coupled eruption of a pseudostreamer and helmet streamer. Astrophys. J. 909, 54 (2021).
5. Gibson, S. E. Solar prominences: theory and models. Fleshing out the magnetic skeleton. Liv. Rev. Sol. Phys. 15, 7 (2018).
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