Dawn–dusk asymmetries are ubiquitous features of the coupled solar-wind–magnetosphere–
ionosphere system. During the last decades, increasing availability of satellite and ground …

It has recently been proposed that ripples inherent to the bow shock during radial
interplanetary magnetic field (IMF) may produce local high speed flows in the …

On 12 August 2007 from 1436 to 1441 UT, when the five THEMIS probes (THA, THB, THC,
THD, and THE) were located near the subsolar magnetopause, a sunward flow was …

We report Time History of Events and Macroscale Interactions during Substorms (THEMIS)
and Geotail observations of prolonged magnetopause (MP) expansions during long‐lasting …

Magnetosheath jets are regions of high dynamic pressure, which can traverse from the bow
shock towards the magnetopause. Recent modelling efforts, limited to a single jet and a …

The magnetopause is a current sheet forming the boundary between the geomagnetic field
on one side and the shocked solar wind on the other side. This paper discusses properties …

We present the results of a statistical study of the distribution of mirror and Alfvén‐ion
cyclotron (AIC) waves in the magnetosheath together with plasma parameters important for …

Composed of shocked solar wind, the Earth's magnetosheath serves as a natural laboratory
to study the transition of turbulence from low Alfvén Mach number, MA, to high M A. The …

This paper analyzes the distribution of different pressure components (dynamic, thermal,
magnetic) in the magnetosheath along the Sun‐Earth line for northward and radial …

Abstract Design of the plasma spectrometer BMSW (Fast Monitor of the Solar Wind,
possessing high temporal resolution) is described in the paper, as well as its characteristics …