2007
DOI: 10.1007/978-3-540-72604-3_68
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Direct Numerical Simulation of Turbulent Taylor-Couette Flow with High Reynolds Number

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Cited by 7 publications
(6 citation statements)
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“…also for independently rotating cylinders and in the strongly turbulent regime, well beyond the onset of chaos. Many new experimental setups have been built to examine various aspects of strongly turbulent TC flow with co-and counter-rotating cylinders (Ji et al 2006;Ravelet, Delfos & Westerweel 2010;Borrero-Echeverry, Schatz & Tagg 2010;van Gils et al 2011avan Gils et al ,b, 2012van Hout & Katz 2011;Paoletti & Lathrop 2011;Schartman et al 2012;Huisman et al 2012;Merbold, Brauckmann & Egbers 2013;Huisman et al , 2014 and correspondingly numerical simulations have been pushed to very high Reynolds numbers (He, Tanahashi & Miyauchi 2007;Bilson & Bremhorst 2007;Dong 2007Dong , 2008 -Mónico et al 2013-Mónico et al , 2014aChouippe et al 2014). Figure 3 shows the currently explored parameter space in different representations.…”
Section: Introductionmentioning
confidence: 99%
“…also for independently rotating cylinders and in the strongly turbulent regime, well beyond the onset of chaos. Many new experimental setups have been built to examine various aspects of strongly turbulent TC flow with co-and counter-rotating cylinders (Ji et al 2006;Ravelet, Delfos & Westerweel 2010;Borrero-Echeverry, Schatz & Tagg 2010;van Gils et al 2011avan Gils et al ,b, 2012van Hout & Katz 2011;Paoletti & Lathrop 2011;Schartman et al 2012;Huisman et al 2012;Merbold, Brauckmann & Egbers 2013;Huisman et al , 2014 and correspondingly numerical simulations have been pushed to very high Reynolds numbers (He, Tanahashi & Miyauchi 2007;Bilson & Bremhorst 2007;Dong 2007Dong , 2008 -Mónico et al 2013-Mónico et al , 2014aChouippe et al 2014). Figure 3 shows the currently explored parameter space in different representations.…”
Section: Introductionmentioning
confidence: 99%
“…Three-dimensional solutions of INSE theoretically require a number of grid point scaling like Re 9/4 . The actual memory limit of the largest supercomputers bounds the largest Reynolds number that can be simulated to Re ≈ 10 4 [19,20]. The second limit comes from the time it takes to simulate a certain amount of evolution time.…”
Section: Introductionmentioning
confidence: 99%
“…The state-of-the-art of high Reynolds number Taylor-Couette turbulence is treated by Grossmann, Lohse, and Sun [4], which is the regime we focus on in the present work. Since the research of Wendt [5] in 1933 and the Austin-Maryland experiments [6][7][8] in the nineties, only in the past decade more researchers have started to explore the strongly turbulent regime with independently rotating cylinders, both experimentally [9][10][11][12][13][14][15][16][17][18] and numerically [19][20][21][22][23][24][25].…”
Section: Introductionmentioning
confidence: 99%