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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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Flow patterns in inclined-layer turbulent convection.
1School of Computer Science, China University of Geosciences, 430074, Wuhan, China, qw@cug.edu.cn.
The European Physical Journal. E, Soft Matter
|July 24, 2014
Summary
Turbulent convection in inclined layers becomes isotropic at high Rayleigh numbers and low inclination angles. Individual plumes remain isotropic regardless of inclination, while boundary layers shrink with increasing Rayleigh numbers.
Area of Science:
- Fluid dynamics
- Heat transfer
- Geophysics
Background:
- Turbulent convection is crucial in natural phenomena like atmospheric and oceanic circulation.
- Understanding flow patterns in inclined layers is essential for various engineering applications.
Purpose of the Study:
- To investigate the flow patterns of turbulent convection in inclined layers.
- To analyze the effects of inclination angle and Rayleigh number on flow dynamics.
- To determine the conditions for achieving an isotropic turbulent state.
Main Methods:
- Three-dimensional numerical simulations were performed.
- The study covered a range of Rayleigh numbers (9 × 10^4 to 2 × 10^7) and inclination angles (5° to 60°).
- The Prandtl number was fixed at σ = 0.7.
Main Results:
- Initial transient flow evolves into a quasi-periodic pattern before full turbulent convection.
- Flow becomes statistically steady and isotropic at high Rayleigh numbers (≃ 2 × 10^7) and low inclination angles (≤ 17°).
- Individual plumes exhibit isotropy independent of inclination at Rayleigh numbers above 5 × 10^6.
- Boundary layer regions shrink with increasing Rayleigh numbers, with a scaling exponent of approximately 2/7.
Conclusions:
- Inclination significantly affects large-scale flow but not individual plumes in turbulent convection.
- An isotropic turbulent state is achievable under specific conditions of high Rayleigh number and low inclination.
- The findings provide insights into heat and mass transport in inclined convective systems.
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