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 …

Kelvin–Helmholtz instability plays a particularly important role in plasma transport at
magnetospheric boundaries because it can control the development of a turbulent boundary …

We present simple models of the plasma disks surrounding Jupiter and Saturn based on
published measurements of plasma properties. We calculate radial profiles of the …

We investigate magnetic data showing the presence of field‐aligned magnetosphere‐
ionosphere coupling currents on 31 Cassini passes across Saturn's southern postmidnight …

Saturn's magnetospheric structure and the intensity of radio frequency emissions from its
immediate surroundings are modulated at close to the planet's rotation period. Analogous …

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 …

The giant‐planet magnetodiscs are shaped by the radial transport of plasma originating in
the inner magnetosphere. Magnetic flux transport is a key aspect of the stretched magnetic …

Magnetic reconnection is an important process that occurs at the magnetopause boundary
of Earth's magnetosphere because it leads to transport of solar wind energy into the system …

From 27 to 28 January 2009, the Cassini spacecraft remotely acquired combined
observations of Saturn's southern aurorae at radio, ultraviolet, and infrared wavelengths …

Although the exact rotation period of Saturn is unknown, Saturn's magnetosphere displays
an abundance of periodicities near~ 10.7 h. Such modulations appear in charged particles …