The role of Stewartson and Ekman layers in turbulent rotating Rayleigh-B\'enard convection
Rudie P.J. Kunnen, Richard J.A.M. Stevens, Jim Overkamp, Chao Sun,, GertJan F. van Heijst, Herman J.H. Clercx

TL;DR
This study investigates how Stewartson and Ekman boundary layers influence turbulent rotating Rayleigh-Bénard convection across different rotation regimes, revealing distinct temperature profile behaviors and boundary layer dynamics through experiments and simulations.
Contribution
It provides new insights into the boundary layer mechanisms and temperature profiles in rotating RB convection, highlighting the roles of Stewartson and Ekman layers across flow regimes.
Findings
Azimuthal temperature profiles change with rotation regimes.
Vertical temperature gradients have different origins in each regime.
Boundary layer dynamics drive secondary flows affecting temperature transport.
Abstract
When the classical Rayleigh-B\'enard (RB) system is rotated about its vertical axis roughly three regimes can be identified. In regime I (weak rotation) the large scale circulation (LSC) is the dominant feature of the flow. In regime II (moderate rotation) the LSC is replaced by vertically aligned vortices. Regime III (strong rotation) is characterized by suppression of the vertical velocity fluctuations. Using results from experiments and direct numerical simulations of RB convection for a cell with a diameter-to-height aspect ratio equal to one at () and we identified the characteristics of the azimuthal temperature profiles at the sidewall in the different regimes. In regime I the azimuthal wall temperature profile shows a cosine shape and a vertical temperature gradient due to plumes that travel with the LSC close to the…
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