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Large-eddy simulation of magnetohydrodynamic turbulence in compressible fluid
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10.1063/1.2171705
/content/aip/journal/pop/13/3/10.1063/1.2171705
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/3/10.1063/1.2171705
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Time evolution of the kinetic energy. DNS results (diamond line); LES results without subgrid closures (solid line); Kolmogorov model (dotted line); Smagorinsky model (dashed line); and cross-helicity model (dashed-dotted line).

Image of FIG. 2.
FIG. 2.

Time evolution of the magnetic energy. Notations are the same as in the Fig. 1.

Image of FIG. 3.
FIG. 3.

Kinetic energy spectrum at . Notations are the same as in the Fig. 1.

Image of FIG. 4.
FIG. 4.

Magnetic energy spectrum at . Notations are the same as in the Fig. 1.

Image of FIG. 5.
FIG. 5.

Kinetic energy spectrum at . Notations are the same as in the Fig. 1.

Image of FIG. 6.
FIG. 6.

Magnetic energy spectrum at . Notations are the same as in the Fig. 1.

Image of FIG. 7.
FIG. 7.

Kinetic energy spectrum at . Notations are the same as in the Fig. 1.

Image of FIG. 8.
FIG. 8.

Magnetic energy spectrum at . Notations are the same as in the Fig. 1.

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/content/aip/journal/pop/13/3/10.1063/1.2171705
2006-03-10
2014-04-17
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Large-eddy simulation of magnetohydrodynamic turbulence in compressible fluid
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/3/10.1063/1.2171705
10.1063/1.2171705
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