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 comprehensive examination of particle and wave data from multiple Thermal Emission
Imaging System (THEMIS) satellites has been made of an electron injection structure in the …

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 review of observations and theories of the dynamics of Jupiter's
magnetosphere from Pioneer to New Horizons. We suggest that Jupiter's solar wind–driven …

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 …

We examine traversals on 20 November 2001 of the equatorial magnetopause boundary
layer simultaneously at∼ 1500 magnetic local time (MLT) by the Geotail spacecraft and at∼ …

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

We report in situ observations from the Cluster and FAST spacecraft showing the deposition
of energy into the auroral ionosphere from broadband ULF waves in the cusp and low …

The solar wind is a supersonic magnetized plasma streaming far into the heliosphere.
Although cooling as it flows, it is rapidly heated upon encountering planetary obstacles. At …