An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …

A dynamical approach, rather than the usual statistical approach, is taken to explore the
physical mechanisms underlying the nonlinear transfer of energy, the damping of the …

The past decade has seen a flurry of research activity focused on discerning the physics of
kinetic scale turbulence in high-speed astrophysical plasma flows. By 'kinetic'we mean …

Turbulence is ubiquitous in the solar wind. Turbulence causes kinetic and magnetic energy
to cascade to small scales where they are eventually dissipated, adding heat to the plasma …

We review some aspects of solar wind turbulence with an emphasis on the ability of the
turbulence to account for the observed heating of the solar wind. Particular attention is paid …

Crossing the Earth's bow shock is known to crucially affect solar wind plasma including
changes in turbulent cascade. The present review summarizes results of more than 15 years …

This paper analyzes solar wind power spectra of bulk and thermal speed fluctuations that
are computed with a time resolution of 32 ms in the frequency range of 0.001–2 Hz. The …

Statistical characteristics of plasma fluctuations in the solar wind (SW), the Earth's
magnetosphere and fusion devices are reviewed. The turbulence in all these media has a …

The Earth's magnetosphere is permanently influenced by the solar wind. When supersonic
and superalfvenic plasma flow interacts with the magnetosphere, the magnetosheath region …

Interplanetary (IP) shocks as typical large-scale disturbances arising from processes such as
stream–stream interactions or Interplanetary Coronal Mass Ejection (ICME) launching play a …