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On the Physics of Kinetic-Alfven Turbulence

Observations reveal nearly power-law spectra of magnetic and density plasma fluctuations at subproton scales in the solar wind, which indicates the presence of a turbulent cascade. We discuss the three-field and two-field models for micro-scale plasma fluctuations, and then present the results of numerical simulations of a two-field model of kinetic-Alfven turbulence, which models plasma motion at sub-proton scales.

preprint2013arXivOpen access
Stanislav BoldyrevJean Carlos Perez
physics.space-phphysics.plasm-phastro-ph.GAastro-ph.SR
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Stanislav BoldyrevJean Carlos Perez

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