Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

The plasma sheet is populated in part by the solar wind plasma. Four solar entry
mechanisms are examined:(1) double cusp or double lobe reconnection,(2) Kelvin …

Large amplitude compressional type ULF waves can propagate from the magnetosheath to
the magnetopause where there are large gradients in density, pressure and magnetic field …

The magnetopause and boundary layer are typically characterized by large amplitude
transverse wave activity with frequencies below the ion cyclotron frequency. The signatures …

We present a study of magnetic field fluctuations in a slow solar wind stream, close to ion
scales, where an increase of the level of magnetic compressibility is observed. Here, the …

Research work in the area of the Global Electric Circuit (GEC) has rapidly expanded in
recent years mainly through observations of lightning from satellites and ground-based …

During periods of northward IMF, plasma sheet ions often have two components: hot
(magnetospheric origin) and cold (magnetosheath origin). The temperatures of the cold …

This paper reviews the state of knowledge concerning the source of magnetospheric plasma
at Earth. Source of plasma, its acceleration and transport throughout the system, its …

A three‐dimensional global‐scale hybrid simulation is carried out, for the first time, for
dynamics of the dayside bow shock‐magnetosphere system associated with the quasi …

Recent advances in heliospheric exploration spurred by NASA's Parker Solar Probe (PSP)
mission require a deeper understanding of the intricate dynamics of the solar corona and …