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Simulations, Data Analysis and Algorithms

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Figure 4 | Computational Astrophysics and Cosmology

Figure 4

From: Implicit large eddy simulations of anisotropic weakly compressible turbulence with application to core-collapse supernovae

Figure 4

Dissipation rate of the energy at the largest scales due to the turbulent cascade (not including direct dissipation by the numerical viscosity) as a function of resolution and for all of the schemes. The dissipation rate is normalized so as to be 1 in the limit of large Reynolds numbers/resolution. At 1283 points all of the schemes show an error of less than 10%, with the HLLC schemes already close to the 2% level.

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