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 …

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 …

Magnetosheath jets are localized high‐dynamic pressure pulses originating at Earth's bow
shock and propagating earthward through the magnetosheath. Jets can influence …

We report effects in the upper high-latitude atmosphere related to the interaction of fast
magnetosheath plasma streams, so-called jets, with the dayside magnetopause. The jets …

Magnetosheath jets are plasma entities that feature a significantly enhanced dynamic
pressure with respect to the ambient plasma. They occur more often downstream of the …

Auroral kilometric radiation (AKR) is generated at high latitudes and can propagate down to
low latitudes. Due to the lack of direct observations, the characteristics of AKR in the middle …

Poleward‐moving auroral arcs (PMAAs) with recurrence periods on the order of minutes
have been established as a distinct form of auroral activities. Their origin and characteristics …

Plasma entities, known as magnetosheath jets, with higher dynamic pressure than the
surrounding plasma, are often seen at Earth. They generate waves and contribute to energy …

Magnetospheric convection is a fundamental process in the coupling of the solar wind,
magnetosphere, and ionosphere. Recent studies have shown that dayside magnetopause …

Pulsating auroras are usually observed with ultralow-frequency (ULF) waves in the Pc 3–5
band (period 10–600 s). These auroras are thought to result from interactions between …