Magnetic Rayleigh–Taylor Instability in an Experiment Simulating a Solar Loop
Author:
Funder
NSF
The air force office
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ab6b2d/pdf
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1. QUIESCENT PROMINENCE DYNAMICS OBSERVED WITH THE HINODE SOLAR OPTICAL TELESCOPE. I. TURBULENT UPFLOW PLUMES
2. Growth rates of the ablative Rayleigh–Taylor instability in inertial confinement fusion
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