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On the Multifractality of Plasma Turbulence in the Solar Wind by Sebastián Echeverría; Pablo S. Moya; Denisse Pastén is a Physics and Astronomy article available to read on EtoBox.

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## Abstract In this work we have analyzed turbulent plasma in the kinetic scale by the characterization of magnetic fluctuations time series. Considering numerical Particle-In-Cell (PIC) simulations we apply a method known as MultiFractal Detrended Fluctuation Analysis (MFDFA) to study the fluctuations of solar-wind-like plasmas in thermodynamic equilibrium (represented by Maxwellian velocity distribution functions), and out of equilibrium plasma represented by Tsallis velocity distribution functions, characterized by the __kappa__ (κ) parameter, to stablish relations between the fractality of magnetic fluctuation and the kappa parameter.

Who reads On the Multifractality of Plasma Turbulence in the Solar Wind?

Author

Sebastián Echeverría; Pablo S. Moya; Denisse Pastén

Publisher

Cambridge University Press; Cambridge University Press (CUP) (ISSN 1743-9213)

Published

2019

Language

EN

Field

Physics and Astronomy (Physical Sciences)