Resolving the solar prominence/filament paradox using the magnetic Rayleigh–Taylor instability - Nature.com

A full 3D high-resolution magnetohydrodynamic model of solar filaments and prominences highlights the crucial role of the magnetic Rayleigh–Taylor instability in their formation and evolution, as well as explaining their different appearance and contrasting b…

Vial, J.-C. & Engvold, O. Solar Prominences (Springer, 2015).

Zhou, Y. H., Chen, P. F., Hong, J. & Fang, C. Simulations of solar filament fine structures and their counterstream… [+13734 chars]

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