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Energy spectra of finite temperature superfluid helium-4 turbulence

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Figure

FIG. 1. Left: Initial energy spectrum Ekn(k) of the homogeneous isotropic turbulence in the normal-fluid
FIG. 2. Left: Superimposed normal-fluid energy spectra at times tleft). In order to match the low wavenumber energy levels, I multiplied later time spectra by the factors 1.7, 5, and 180
FIG. 3. Isosurfaces of intense normal-fluid vorticity (red tubes) and superfluid vortices (green lines) at tt = 0.0113 s (left) and = 0.0262 s (right)
FIG. 4. Superfluid energy spectra at tshows a clear-cut = 0.0262 s (bottom curve) and t = 0.0619 s (top curve)

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