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Large-Eddy Simulations of Magnetohydrodynamic Turbulence in Heliophysics and Astrophysics

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Figure

Fig. 1 The “Terra Incognita” and the realm of LES (from Wyngaard 2004, presented atthe turbulence is partially resolved, capturing the peak in the spectrum but not the viscousdissipation scalethe workshop by Peter Sullivan)
Fig. 2 Left: Normalized energy spectra ofconfiguration at the upper surface near the end of the simulation
Fig. 3 (Left) Volume rendering of magnitude of current densityproton gyroradii. Again, fine scale structure is evident, now at kinetic scales
Fig. 4 (are normalized by the electron inertial scalewavenumbers are normalized by the thermal ion gyroradiusmeasurements by the Cluster spacecraft, from Bale et al
+3

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