Magnetic Field Turbulence in the Solar Wind at Sub‐ion Scales: In Situ Observations and Numerical Simulations

Magnetic Field Turbulence in the Solar Wind at Sub‐ion Scales: In Situ Observations and Numerical Simulations

We investigate the transition of the solar wind turbulent cascade from MHD to sub‐ion range by means of a detailed comparison between in situ observations and hybrid numerical simulations. In particular, we focus on the properties of the magnetic field and its component anisotropy in Cluster measure...

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Bibliographic Details
Main Authors: L. Matteini, L. Franci, O. Alexandrova, C. Lacombe, S. Landi, P. Hellinger, E. Papini, A. Verdini
Format: Article
Language:English
Published: Frontiers Media S.A. 2020-12-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
solar wind
plasma turbulence
kinetic physics
numerical simulations
in situ observation
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2020.563075/full

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