Effect of Charge accumulation on Magnetic Rayleigh-Taylor Instability
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/s41598-019-47550-5.pdf
Reference24 articles.
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2. Isobe, H. et al. Filamentary structure on the Sun from the magnetic Rayleigh–Taylor instability. Nature 434(7032), 478 (2005).
3. Sultan, P. J. Linear theory and modeling of the Rayleigh‐Taylor instability leading to the occurrence of equatorial spread F. Journal of Geophysical Research: Space Physics 101, 26875–26891 (1996).
4. Robinson, K. et al. Morphology of rising hydrodynamic and magnetohydrodynamic bubbles from numerical simulations. The Astrophysical Journal 601(2), 621 (2004).
5. Atzeni, S., Meyer-Ter-Vehn, J. & Meyer-ter-Vehn, J. The Physics of Inertial Fusion: BeamPlasma Interaction, Hydrodynamics, Hot Dense Matter. Vol. 125 (Oxford University Press on Demand, 2004).
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