Plasmaspheric density structures have been studied since the discovery of the
plasmasphere in the late 1950s. But the advent of the Cluster and Image missions in 2000 …

Aurora is the result of the interaction between precipitating energetic electrons and protons
with the upper atmosphere. Viewed from space, it generally occurs in continuous and diffuse …

Whistler‐mode waves are electromagnetic waves pervasively observed in the Earth's and
other planetary magnetospheres. They are considered to be mainly responsible for …

As an inner magnetospheric phenomenon the plasmapause region is of interest for a
number of reasons, one being the occurrence there of geophysically important interactions …

Using the sounding measurements from the radio plasma imager on IMAGE and a plasma
density inversion algorithm, we derive the plasma density profiles along the magnetic field in …

It is well known that strong electron heating by a powerful HF‐facility can lead to the
formation of electron and ion density perturbations that stretch along the magnetic field line …

We report on satellite observations of plasma density enhancements (ducts) in the topside
ionosphere during four HAARP/BRIOCHE campaigns during 2009–2010. Artificial ducts …

Magnetosonic waves inside and outside the plasmasphere differ statistically in occurrence
rate, frequency, and intensity. How the density interface separates magnetosonic waves …

The electron density profiles derived from the EFW and WHISPER instruments on board the
four Cluster spacecraft reveal density structures inside the plasmasphere and at its outer …

Context. Rotational modulation has been observed in different magnetospheric phenomena
at Saturn, including radio emissions, which reflect the fundamental plasma processes in key …