One of the most important issues in space physics is to identify the dominant processes that
transfer energy from the solar wind to energetic particle populations in Earth's inner …

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 …

We present a comprehensive observational study of the magnetospheric response to an
interplanetary magnetic field (IMF) tangential discontinuity, which first struck the postnoon …

We present Time History of Events and Macroscale Interactions during Substorms (THEMIS)
observations of a “Spontaneous Hot Flow Anomaly”(SHFA) upstream from the prenoon bow …

Abstract Pc5 (2–7 mHz) ultralow frequency (ULF) waves play a significant role in resonating
with particles and transferring energy in the coupled magnetospheric and ionospheric …

Global signatures of the aurora caused by interplanetary shocks/pressure pulses have been
studied in recent years using ultraviolet imager data from polar orbiting spacecraft. The …

Magnetosheath high‐speed jets (HSJs) are dayside upstream transient disturbances with
enhanced flow velocity and dynamic pressure. They are associated with significant …

Dayside aurora is related to processes in the dayside magnetosphere and especially at the
dayside magnetopause. A number of dayside aurora phenomena are driven by …

The foreshock region involves localized and transient structures such as foreshock cavities
and hot flow anomalies due to solar wind‐bow shock interactions, and foreshock transients …

In recent years, it has become increasingly clear that space weather disturbances can be
triggered by transient upstream mesoscale structures (TUMS), independently of the …