Coherent structures at ion scales in fast solar wind: {\it Cluster} observations

Abstract

We investigate the nature of magnetic turbulent fluctuations, around ion characteristic scales, in a fast solar wind stream, by using {\it Cluster} data. Contrarily to slow solar wind, where both Alfvénic ($\delta b_{\perp }\gg \delta b_{\parallel }$) and compressive ($\delta b_{\parallel }\gg \delta b_{\perp }$) coherent structures are observed \cite[]{per16}, the turbulent cascade of fast solar wind is dominated by Alfvénic structures, namely Alfvén vortices, with small and/or finite compressive part, with the presence also of several current sheets aligned with the local magnetic field. Several examples of vortex chains are also recognized. Although an increase of magnetic compressibility around ion scales is observed also for fast solar wind, no strongly compressive structures are found, meaning that the nature of the slow and fast winds is intrinsically different. Multi-spacecraft analysis applied to this interval of fast wind indicate that the coherent structures are almost convected by the flow and aligned with the local magnetic field, i.e. their normal is perpendicular to {\bf B}, that is consistent with a two dimensional turbulence picture. Understanding intermittency and the related generation of coherent structures could provide a key insight into the nonlinear energy transfer and dissipation processes in magnetized and collisionless plasmas.

References in corpus (4)

• Small Scale Energy Cascade of the Solar Wind Turbulence
• Solar wind turbulent spectrum at plasma kinetic scales
• Spectral Slope Variation at Proton Scales from Fast to Slow Solar Wind
• Anisotropies of the magnetic field fluctuations at kinetic scales in the solar wind : Cluster observations

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• Space-filter techniques for quasi-neutral hybrid-kinetic models
• Intermittency and Ion Temperature-Anisotropy Instabilities: Simulation and Magnetosheath Observation
• Three-dimensional local anisotropy of velocity fluctuations in the solar wind
• Nature of electrostatic fluctuations in the terrestrial magnetosheath