Abstract The Juno Magnetic Field investigation (MAG) characterizes Jupiter's planetary
magnetic field and magnetosphere, providing the first globally distributed and proximate …

The Cassini radio and plasma wave investigation is designed to study radio emissions,
plasma waves, thermal plasma, and dust in the vicinity of Saturn. Three nearly orthogonal …

The spin of a single electron subject to a static magnetic field provides a natural two-level
system that is suitable for use as a quantum bit, the fundamental logical unit in a quantum …

The Jovian magnetosphere assumes a disc‐like geometrical configuration (“magnetodisc”)
owing to the persistent presence of a system of azimuthal currents circulating in a washer …

The dual technique magnetometer system onboard the Cassini orbiter is described. This
instrument consists of vector helium and fluxgate magnetometers with the capability to …

The Cassini Imaging Science Subsystem acquired about 26,000 images of the Jupiter
system as the spacecraft encountered the giant planet en route to Saturn. We report findings …

The present 15th volume of the ISSI Space Science Series is devoted to Auroral Plasma
Physics. The aurora is arguably the most intriguing phenomenon in space plasma physics …

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 …

This paper deals with acceleration processes in the magnetotail and the processes that
enhance particle precipitation from the tail into the ionosphere through electric fields in the …

We report data from the Cassini radio and plasma wave instrument during the approach and
first orbit at Saturn. During the approach, radio emissions from Saturn showed that the radio …