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- W2891717849 abstract "Intermittent large-scale high-shear flows are found to occur frequently and spontaneously in direct numerical simulations of statistically stationary turbulent Boussinesq magnetohydrodynamic (MHD) convection. The energetic steady-state of the system is sustained by convective driving of the velocity field and small-scale dynamo action. The intermittent emergence of flow structures with strong velocity and magnetic shearing generates magnetic energy at an elevated rate over time-scales longer than the characteristic time of the large-scale convective motion. The resilience of magnetic energy amplification suggests that intermittent shear-bursts are a significant driver of dynamo action in turbulent magnetoconvection." @default.
- W2891717849 created "2018-09-27" @default.
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- W2891717849 date "2013-03-31" @default.
- W2891717849 modified "2023-09-26" @default.
- W2891717849 title "Fluctuation dynamo driven by shear-bursts in convectively-driven magnetohydrodynamic turbulence" @default.
- W2891717849 hasPublicationYear "2013" @default.
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