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Transition to ultimate Rayleigh-Bénard turbulence revealed through extended self-similarity scaling analysis of the temperature structure functions

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Lohse,  Detlef
Max Planck Institute for Dynamics and Self-Organization, Max Planck Society;

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Citation

Krug, D., Zhu, X., Chung, D., Marusic, I., Verzicco, R., & Lohse, D. (2018). Transition to ultimate Rayleigh-Bénard turbulence revealed through extended self-similarity scaling analysis of the temperature structure functions. Journal of Fluid Mechanics, 851: R3. doi:10.1017/jfm.2018.561.


Cite as: https://hdl.handle.net/21.11116/0000-0001-E829-C
Abstract
In turbulent Rayleigh-Bénard (RB) convection, a transition to the so-called ultimate regime, in which the boundary layers (BL) are of turbulent type, has been postulated. Indeed, at very large Rayleigh number Ra approximate to 10(13)-10(14) a transition in the scaling of the global Nusselt number Nu (the dimensionless heat transfer) and the Reynolds number with Ra has been observed in experiments and very recently in direct numerical simulations (DNS) of two-dimensional (2D) RB convection. In this paper, we analyse the local scaling properties of the lateral temperature structure functions in the BLs of this simulation of 2D RB convection, employing extended self-similarity (ESS) (i.e., plotting the structure functions against each other, rather than only against the scale) in the spirit of the attached-eddy hypothesis, as we have recently introduced for velocity structure functions in wall turbulence (Krug et al., J. Fluid Mech., vol. 830, 2017, pp. 797-819). We find no ESS scaling at Ra below the transition and in the near-wall region. However, beyond the transition and for large enough wall distance z(+) > 100, we find clear ESS behaviour, as expected for a scalar in a turbulent boundary layer. In striking correspondence to the Nu scaling, the ESS scaling region is negligible at Ra = 10(11) and well developed at Ra = 10(14), thus providing strong evidence that the observed transition in the global Nusselt number at Ra approximate to 10(13) indeed is the transition from a laminar type BL to a turbulent type BL. Our results further show that the relative slopes for scalar structure functions in the ESS scaling regime are the same as for their velocity counterparts, extending their previously established universality. The findings are confirmed by comparing to scalar structure functions in three-dimensional turbulent channel flow.