The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

The plasma particle velocity distributions observed in the solar wind generally show
enhanced (non-Maxwellian) suprathermal tails, decreasing as a power law of the velocity …

Spacecraft measurements of charged particles in the solar wind show that their velocity
distributions deviate from thermal Maxwellian model, having energetic components with …

Voyager 1 has been moving through the very local interstellar medium (VLISM) from the time
that it crossed the heliopause on 2012/DOY 238 to 2020/DOY 292. Three notable objects in …

Quasi‐thermal noise spectroscopy is an efficient tool for measuring in situ macroscopic
plasma properties in space, using a passive wave receiver at the ports of an electric …

Recently, a very weak, nearly continuous plasma wave emission line has been discovered
in the nearby interstellar medium at the electron plasma frequency. The new observations …

Kinetic theory of weakly turbulent nonlinear processes in plasma helped form the foundation
of modern plasma physics. This book provides a systematic overview of the kinetic theory of …

We present Jovian electron densities measured by the Juno Waves instrument at high‐
latitudes (with magnetic latitudes of on magnetic field lines threading the Io torus and plasma …

The smallest characteristic scales, at which electron dynamics determines the plasma
behaviour, are the next frontier in space and astrophysical plasma research. The analysis of …

New data for the calculation of ionization and recombination rates have been published in
the past few years, most of which are included in the CHIANTI database. We used these …