Turbulent thermal superstructures in RayleighBénard convection
Abstract
We report the observation of superstructures, i.e., very largescale and long living coherent structures in highly turbulent RayleighBénard convection up to Rayleigh Ra=10^{9} . We perform direct numerical simulations in horizontally periodic domains with aspect ratios up to Γ =128 . In the considered Ra number regime the thermal superstructures have a horizontal extend of six to seven times the height of the domain and their size is independent of Ra. Many laboratory experiments and numerical simulations have focused on small aspect ratio cells in order to achieve the highest possible Ra. However, here we show that for very high Ra integral quantities such as the Nusselt number and volume averaged Reynolds number only converge to the large aspect ratio limit around Γ ≈4 , while horizontally averaged statistics such as standard deviation and kurtosis converge around Γ ≈8 , the integral scale converges around Γ ≈32 , and the peak position of the temperature variance and turbulent kinetic energy spectra only converge around Γ ≈64 .
 Publication:

Physical Review Fluids
 Pub Date:
 April 2018
 DOI:
 10.1103/PhysRevFluids.3.041501
 arXiv:
 arXiv:1804.02310
 Bibcode:
 2018PhRvF...3d1501S
 Keywords:

 Physics  Fluid Dynamics
 EPrint:
 7 pages, 4 figures