Study of High-Reynolds Number Isotropic Turbulence by Direct Numerical Simulation

By Takashi Ishihara, T. Gotoh, Yukio Kaneda. 2009

681 citations recorded by the source corpus.

Subfields: Atmospheric Science, Computational Mechanics, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/ebb972f522f8f6bef0f0a2f33eed8d739f8dd7e4

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In Atmospheric Science

1. Lance R. Collins
2. Luca Biferale
3. Jerry Westerweel
4. A. Alexakis
5. Peter J. Ireland
6. A. Bragg
7. J. Hunt

In Computational Mechanics

1. A. Bragg
2. Peter J. Ireland
3. Jerry Westerweel
4. J. Hunt
5. A. Alexakis
6. Lance R. Collins
7. F. Rincon
8. Carlos C. N. da Silva

In Global and Planetary Change

1. A. Alexakis
2. F. Rincon
3. Lance R. Collins
4. Luca Biferale
5. Michel Rieutord
6. Jerry Westerweel
7. Peter J. Ireland
8. A. Bragg

Citations in the corpus

• The effect of Reynolds number on inertial particle dynamics in isotropic turbulence. Part 2. Simulations with gravitational effects (2015, methodology): “urposes of the following discussion, we dene the dissipation range as the region over which the uid velocity variances follow r2- scaling, which is seen to be 0 6 r=. 10 in gure12, in agreement withIshihara et al. (2009). At small separations, the relative velocity variances parallel to the separati”
• Interfacial Layers Between Regions of Different Turbulence Intensity (2014, background): “These thin ribbonlike features are characterized by large velocity gradients and contain microscale vortex structures (Worth & Nickels 2011, Ishihara et al. 2009).”
• The effect of Reynolds number on inertial particle dynamics in isotropic turbulence. Part 1. Simulations without gravitational effects (2015, background): “It is a common practice to report the power-law exponents of higher-order velocity structure functions for fluid particles (e.g. see Kerr, Meneguzzi & Gotoh 2001; Gotoh et al. 2002; Shen & Warhaft 2002; Ishihara et al. 2009).”
• Cascades and transitions in turbulent flows (2018, background): “For completeness it is important to remark that empirical observations show that at small and moderate Re, longitudinal and transverse velocity increments scale slightly differently [129, 135], with a slow tendency toward a recovery of similar scaling properties by increasing the Reynolds number [12”
• The Sun’s Supergranulation (2010, background): “homogeneous turbulence (Vincent and Meneguzzi 1991; Ishihara et al. 2009), but also face a few problems when it comes to the simulation of compressible flows: for instance, they cannot capture shocks easily.”