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Co-existence of whistler waves with kinetic Alfven wave turbulence for the high-beta solar wind plasma
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10.1063/1.4757638
/content/aip/journal/pop/19/10/10.1063/1.4757638
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/10/10.1063/1.4757638
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Image of FIG. 1.
FIG. 1.

The initial Maxwellian distribution evolves through QL diffusion with KAW to a distribution that has a plateau at velocities . For velocities , the distribution remains Maxwellian, since the minimum phase velocity of KAW is VA ; this feature is not shown in the figure.7 Thus, the Landau damping of KAW (8a) is diminished by a factor of 10 or more. The Landau damping of whistlers (17a) is also diminished by the same factor.

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/content/aip/journal/pop/19/10/10.1063/1.4757638
2012-10-11
2014-04-21
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Co-existence of whistler waves with kinetic Alfven wave turbulence for the high-beta solar wind plasma
http://aip.metastore.ingenta.com/content/aip/journal/pop/19/10/10.1063/1.4757638
10.1063/1.4757638
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