Water‐group gas continuously escapes from Jupiter's icy moons to form co‐orbiting
populations of particles or neutral toroidal clouds. These clouds provide insights into their …

The Alfvén wave mode transmits field‐aligned currents and large‐scale turbulence
throughout Jupiter's magnetosphere. Magnetometer data from the Juno spacecraft have …

Electron acceleration by dispersive scale Alfvén waves at Jupiter is investigated using a
Gyrofluid‐Kinetic‐Electron model. Specifically, the simulations consider the propagation of …

Discs of plasma around giant planets are natural laboratories that contain within
mechanisms of transferring and keeping energy into the plasma and magnetic field system …

Using a combination of Juno magnetometer and plasma data, we show evidence of Alfvénic
turbulence within the mid‐to‐high latitude magnetosphere with sufficient conditions to trigger …

Jupiter's plasma sheet has been understood to be primarily composed of Io‐genic sulfur and
oxygen, along with protons at lower mass density. These ions move radially away from …

The Juno mission flew through the plasma disk near the equator in Jupiter's magnetosphere
frequently. We identify 274 plasma disk crossings of Juno between 10 and 40 RJ from PJ5 to …

One of the grand challenge problems of the giant planet magnetospheres is the issue of
nonadiabatic plasma heating. Simple turbulent heating models consider the energy cascade …

Observations from various missions to Jupiter and Saturn showed that temperature of heavy-
ion plasma contained in expanding discs around planets is increasing with radial distance …

The magnetospheres of the outer planets exhibit turbulent phenomena in an environment
which is qualitatively different compared to the solar wind or the interstellar medium. The key …