The electron–cyclotron maser is a process that generates coherent radiation from plasma. In
the last two decades, it has gained increasing attention as a dominant mechanism of …

Jupiter is the source of the strongest planetary radio emissions in the solar system.
Variations in these emissions are symptomatic of the dynamics of Jupiter's magnetosphere …

We report on FAST observations of large amplitude (up to 500 mV m− 1) envelope solitary
waves at the edges of the AKR source region. These edges are characterized by the …

The FAST satellite mission investigates plasma processes occurring in the low altitude
auroral acceleration region, where magnetic field‐aligned currents couple global …

We present a detailed description of the auroral kilometric radiation (AKR) source region
based on observations from the Fast Auroral SnapshoT (FAST) satellite and discuss how …

The Fast Auroral SnapshoT (FAST) satellite has made observations in the Auroral Kilometric
Radiation (AKR) source region with unprecedented frequency and time resolution. We …

Abundant evidence for the occurrence of modulated envelope plasma wave packets is
provided by recent satellite missions. These excitations are characterized by a slowly …

The ionospheric response to auroral precipitation at the giant planets is reviewed, using
models and observations. The emission processes for aurorae at radio, infrared, visible …

Using the Quantum hydrodynamic (QHD) model Korteweg-de Vries (KdV) type solitary
excitations of electron-acoustic waves (EAWs) have been examined in a two-electron …

The Fast Auroral Snapshot (FAST) explorer satellite was designed to investigate the
microscale structure of the auroral acceleration region that was unresolved by previous …