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Similarities between characteristics of convective turbulence in confined and extended domains

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arxiv 2208.09713 v1 pith:OSCLKBQL submitted 2022-08-20 physics.flu-dyn astro-ph.SR

Similarities between characteristics of convective turbulence in confined and extended domains

classification physics.flu-dyn astro-ph.SR
keywords convectionaspectcellfluctuationsincreasingnumberratioslender
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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To understand turbulent convection at very high Rayleigh numbers typical of natural phenomena, computational studies in slender cells are an option if the needed resources have to be optimized within available limits. However, the accompanying horizontal confinement affects some properties of the flow. Here, we explore the characteristics of turbulent fluctuations in the velocity and temperature fields in a cylindrical convection cell of aspect ratio 0.1 by varying the Prandtl number $Pr$ between 0.1 and 200 at a fixed Rayleigh number $Ra = 3 \times 10^{10}$, and find that the fluctuations weaken with increasing $Pr$, quantitatively as in aspect ratio 25. The probability density function (PDF) of temperature fluctuations in the bulk region of the slender cell remains mostly Gaussian, but increasing departures occur as $Pr$ increases beyond unity. We assess the intermittency of the velocity field by computing the PDFs of velocity derivatives and of the kinetic energy dissipation rate, and find increasing intermittency as $Pr$ decreases. In the bulk region of convection, a common result applicable to the slender cell, large aspect ratio cells, as well as in 2D convection, is that the turbulent Prandtl number decreases as $Pr^{-1/3}$.

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