We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, regarding the scaling of heat transfer with the Rayleigh number for rotating systems at a fixed rate of rotation. The Prandtl number, Pr=6.4, is kept constant. We perform simulations, using a spectral element method, for Rayleigh numbers Ra from 106 to 109, and Rossby numbers Ro from 0.09 to ∞. We find that the Nusselt number Nu scales approximately with a power 2/7 of Ra at sufficiently high Ra for all Ro. The value of Ra beyond which this Nusselt scaling is well established increases with decreasing Ro. Depending on the rotation rate, the Nusselt number can increase up to 18% with respect to the non-rotating case.</p
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determi...
Numerical data for the heat transfer as a function of the Prandtl (Pr) and Rossby (Ro) numbers in tu...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh–Bénard convection, reg...
\u3cp\u3eWe report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convec...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The heat transfer and flow structure in rotating Rayleigh-Bénard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determi...
Numerical data for the heat transfer as a function of the Prandtl (Pr) and Rossby (Ro) numbers in tu...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convection, reg...
We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh–Bénard convection, reg...
\u3cp\u3eWe report results from Direct Numerical Simulation (DNS) of rotating Rayleigh-Bénard convec...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The Rayleigh-Bénard (RB) system is relevant to astro- and geophysical phenomena, including convectio...
The heat transfer and flow structure in rotating Rayleigh-Bénard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
The heat transfer and flow structure in rotating Rayleigh-Benard convection are strongly influenced ...
For given aspect ratio and given geometry, the nature of Rayleigh Benard convection (RBC) is determi...
Numerical data for the heat transfer as a function of the Prandtl (Pr) and Rossby (Ro) numbers in tu...