The present paper comprises a review of kinetic instabilities that may be operative in the
solar wind, and how they influence the dynamics thereof. The review is limited to collective …

The terrestrial magnetosheath contains a rich variety of low-frequency (≲ proton
gyrofrequency) fluctuations. Kinetic and fluid-like processes at the bow shock, within the …

Correlations between plasma properties and magnetic fluctuations in the subsolar
magnetosheath downstream of a quasi‐perpendicular shock have been found and indicate …

This chapter focuses on the range of low frequency electromagnetic modes observed at and
upstream of collisionless shocks in the heliosphere. It discusses a specific class of whistler …

The term “magnetic hole” has been used to denote isolated intervals when the magnitude of
the interplanetary magnetic field drops to a few tenths, or less, of its ambient value for a time …

Dynamic spectral analysis covering frequencies 0.1 to 4.0 Hz has been applied to analyze
Active Magnetospheric Particle Tracer Explorers CCE magnetic field data during periods of …

Mirror modes are large amplitude nonpropagating compressive structures frequently
observed in the magnetosheath. They appear in the form of quasi‐sinusoidal oscillations in …

We utilize suprathermal ion and magnetic field measurements from the Mars Atmosphere
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …

Magnetosheath observations have shown an inverse correlation between the proton
temperature anisotropy and the parallel proton β. Computer simulations have produced …

We report the properties of a novel type of sub-proton scale magnetic hole found in two
dimensional particle-in-cell simulations of decaying turbulence with a guide field. The …