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On the cross-helicity dependence of the energy spectrum in magnetohydrodynamic turbulence
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10.1063/1.3533671
/content/aip/journal/pop/18/1/10.1063/1.3533671
http://aip.metastore.ingenta.com/content/aip/journal/pop/18/1/10.1063/1.3533671
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Figures

Image of FIG. 1.
FIG. 1.

The energy cascade rate as a function of the normalized cross-helicity for, from bottom to top, the generalized Boldyrev theory with (bottom curve, blue), Eq. (79); the theory of Lithwick et al. (second curve from the bottom, green), Eq. (75); the generalized Boldyrev theory with (third curve from the bottom, orange), Eq. (81); and the generalized GS theory with (top curve, red), Eq. (80).

Image of FIG. 2.
FIG. 2.

Data from the simulations of Beresnyak and Lazarian (Ref. 47), the two points on the left-hand side, and from the simulations of Perez and Boldyrev (Ref. 46), the point furthest to the right. The rectangular boxes around the Perez and Boldyrev data indicate uncertainties of ±10% and ±20% for reference. The black line is the relation and the gray (red) line is the relation .

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/content/aip/journal/pop/18/1/10.1063/1.3533671
2011-01-21
2014-04-24
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: On the cross-helicity dependence of the energy spectrum in magnetohydrodynamic turbulence
http://aip.metastore.ingenta.com/content/aip/journal/pop/18/1/10.1063/1.3533671
10.1063/1.3533671
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