The wind in confined thermal convection

A large-scale circulation velocity, often called the ‘wind’, has been observed in turbulent convection in the Rayleigh–Bénard apparatus, which is a closed box with a heated bottom wall. The wind survives even when the dynamical parameter, namely the Rayleigh number, is very large. Over a wide range of time scales greater than its characteristic turnover time, the wind velocity exhibits occasional and irregular reversals without a change in magnitude. We study this feature experimentally in an apparatus of aspect ratio unity, in which the highest attainable Rayleigh number is about 1016. A possible physical explanation is attempted.

[1]  Villermaux Memory-induced low frequency oscillations in closed convection boxes. , 1995, Physical review letters.

[2]  S. Zaleski,et al.  Scaling of hard thermal turbulence in Rayleigh-Bénard convection , 1989, Journal of Fluid Mechanics.

[3]  M. Manga,et al.  Interaction of rising and sinking mantle plumes , 2001 .

[4]  Sano,et al.  Turbulence in helium-gas free convection. , 1989, Physical review. A, General physics.

[5]  K. R. Sreenivasan,et al.  Turbulent convection at very high Rayleigh numbers , 1999, Nature.

[6]  Takeshita,et al.  Thermal turbulence in mercury. , 1996, Physical review letters.

[7]  L. Howard,et al.  Large-scale flow generation in turbulent convection. , 1981, Proceedings of the National Academy of Sciences of the United States of America.

[8]  R. A. Wentzell,et al.  Hydrodynamic and Hydromagnetic Stability. By S. CHANDRASEKHAR. Clarendon Press: Oxford University Press, 1961. 652 pp. £5. 5s. , 1962, Journal of Fluid Mechanics.

[9]  Paul H. Roberts,et al.  The role of the Earth's mantle in controlling the frequency of geomagnetic reversals , 1999, Nature.

[10]  V. Steinberg,et al.  High Rayleigh Number Turbulent Convection in a Gas near the Gas-Liquid Critical Point , 1999, chao-dyn/9903021.

[11]  L. Howard Convection at high Rayleigh number , 1966 .

[12]  Qiu,et al.  Large-scale coherent rotation and oscillation in turbulent thermal convection , 2000, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics.

[13]  S. Cioni,et al.  Strongly turbulent Rayleigh–Bénard convection in mercury: comparison with results at moderate Prandtl number , 1997, Journal of Fluid Mechanics.

[14]  Leo P. Kadanoff,et al.  Turbulent heat flow: Structures and scaling , 2001 .