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 …

Kelvin–Helmholtz instability plays a particularly important role in plasma transport at
magnetospheric boundaries because it can control the development of a turbulent boundary …

A generalization of the traditional 12‐station auroral electrojet (AE) index to include more
than 100 magnetometer stations, SME, is an excellent predictor of global auroral power …

Recent numerical simulations suggest that as soon as the Kelvin‐Helmholtz instability (KHI)
has grown nonlinearly to form a highly rolled‐up vortex, plasma mixing is inevitably …

The solar wind‐magnetosphere system is nonlinear. The solar wind drivers of
geosynchronous electrons with energy range of 1.8–3.5 MeV are investigated using mutual …

Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

We have used THEMIS measurements to determine how the ion and electron temperatures
and their ratio (Ti/Te) change spatially in the magnetosheath and plasma sheet and to …

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 …

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

This review paper summarizes the research of Mercury's magnetosphere in the Post-
MESSENGER era and compares its dynamics to those in other planetary magnetospheres …