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Eddy damped quasinormal Markovian simulations of superfluid turbulence in helium II
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10.1063/1.3527282
/content/aip/journal/pof2/22/12/10.1063/1.3527282
http://aip.metastore.ingenta.com/content/aip/journal/pof2/22/12/10.1063/1.3527282
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Energy spectra of normal fluid and superfluid components at high temperature and strong mutual friction coefficient. For each fluid, the initial (dash line) and steady states (solid line) are displayed.

Image of FIG. 2.
FIG. 2.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Case of a strong mutual friction coefficient in the high temperature regime.

Image of FIG. 3.
FIG. 3.

Energy spectra of normal fluid and superfluid (components at high temperature and weak mutual friction coefficients. For each fluid, the initial (dash line) and steady states (solid line) are presented.

Image of FIG. 4.
FIG. 4.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Case of a weak mutual friction coefficient in the high temperature regime.

Image of FIG. 5.
FIG. 5.

Energy spectra of normal fluid and superfluid components in helium II at high temperature.

Image of FIG. 6.
FIG. 6.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Case of helium II in the high temperature regime.

Image of FIG. 7.
FIG. 7.

Energy spectra of normal fluid and superfluid components at low temperature and strong mutual friction coefficient. For each fluid, the initial (dash line) and steady states (solid line) are displayed.

Image of FIG. 8.
FIG. 8.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Case of a strong mutual friction coefficient in the low temperature regime.

Image of FIG. 9.
FIG. 9.

Energy spectra of normal fluid and superfluid components at low temperature and weak mutual friction coefficient. For each fluid, the initial (dash line) and steady states (solid line) are represented.

Image of FIG. 10.
FIG. 10.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Inset (top plot): zoom in the power dissipation range. Case of a strong mutual friction coefficient in the low temperature regime.

Image of FIG. 11.
FIG. 11.

Compensated energy spectra of the superfluid component at low temperature and weak mutual friction coefficient. The bump at the end of the domain is the tendency to a -thermalization that is limited thanks to the viscosity

Image of FIG. 12.
FIG. 12.

Energy spectra of normal fluid and superfluid components in helium II at low temperature.

Image of FIG. 13.
FIG. 13.

Spectral variation of the nonlinear energy transfer (solid line), the viscous dissipation (dashed line), and the mutual friction flux (dot-dashed line) in the normal fluid (top) and the superfluid (bottom). Case of helium II in the low temperature regime.

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/content/aip/journal/pof2/22/12/10.1063/1.3527282
2010-12-14
2014-04-21
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Eddy damped quasinormal Markovian simulations of superfluid turbulence in helium II
http://aip.metastore.ingenta.com/content/aip/journal/pof2/22/12/10.1063/1.3527282
10.1063/1.3527282
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