Interactions between magnetohydrodynamic shear instabilities and convective flows in the solar interior
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/400/1/337/18696034/mnras0400-0337.pdf
Reference43 articles.
1. Three-dimensional simulations of shear instabilities in magnetized flows
2. Formation of buoyant magnetic structures by a localized velocity shear
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4. Spatially intermittent fields in photospheric magnetoconvection
5. The nonlinear breakup of a magnetic layer: instability to interchange modes
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1. Shear-driven magnetic buoyancy in the solar tachocline: the mean electromotive force due to rotation;Monthly Notices of the Royal Astronomical Society;2023-01-14
2. The effect of time-dependent γ-pumping on buoyant magnetic structures;Geophysical & Astrophysical Fluid Dynamics;2018-10-26
3. Evolution and characteristics of forced shear flows in polytropic atmospheres: large and small Péclet number regimes;Monthly Notices of the Royal Astronomical Society;2018-10-05
4. Evolution of forced shear flows in polytropic atmospheres: a comparison of forcing methods and energetics;Monthly Notices of the Royal Astronomical Society;2016-08-03
5. Shear instabilities in a fully compressible polytropic atmosphere;Astronomy & Astrophysics;2015-05
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