Advanced spectral and statistical data analysis techniques have greatly contributed to
shaping our understanding of microphysical processes in plasmas. We review some of the …

Electron scale solar wind (SW) turbulence has attracted great interest in recent years.
Considerable evidence exists that the turbulence is not fully dissipated near the proton …

The anisotropic nature of solar wind magnetic turbulence fluctuations is investigated scale
by scale using high cadence in situ magnetic field measurements from the Cluster and ACE …

The nature of solar wind (SW) turbulence below the proton gyroscale is a topic that is being
investigated extensively nowadays, both theoretically and observationally. Although recent …

We present a first statistical study of subproton-and electron-scale turbulence in the
terrestrial magnetosheath using waveform data measured by the Cluster/STAFF search coil …

This paper describes the design and performance of the search coil magnetometers (SCM),
which are part of the Plasma Wave Investigation (PWI) instrument onboard the …

ABSTRACT A phenomenological turbulence model for kinetic Alfvén waves in a magnetized
collisionless plasma that is able to reproduce the non-universal power-law spectra observed …

In single-spacecraft observations the Taylor frozen-in-flow hypothesis is usually used to infer
wavenumber spectra of turbulence from the frequency ones. While this hypothesis can be …

The cascade of kinetic Alfvén waves (KAWs) at sub-ion scales in the solar wind is simulated
numerically using a fluid approach that retains ion and electron Landau damping, together …

Turbulence at MagnetoHydroDynamics (MHD) scales in the solar wind has been studied for
more than three decades, using data analysis, theoretical and numerical modeling …