The Sprint-A satellite with the EUV spectrometer (Extreme Ultraviolet Spectroscope for
Exospheric Dynamics: EXCEED) was launched in September 2013 by the Epsilon rocket …

The dynamics of the giant planet magnetodiscs are strongly influenced by planetary rotation.
Yet the solar wind must ultimately remove plasma from these rapidly rotating magnetodiscs …

New global maps of the five inner midsize icy saturnian satellites, Mimas, Enceladus, Tethys,
Dione, and Rhea, have been constructed in three colors (UV, Green and near-IR) at …

To address factors dictating similarities and differences between solar system radiation
belts, we present comparisons between relativistic electron radiation belt spectra of all five …

Mars lacks a global magnetic field, and instead possesses small-scale crustal magnetic
fields, making its magnetic environment fundamentally different from intrinsic …

We report sample results on Saturn magnetospheric energetic ion spectral shapes using
measurements obtained from the Magnetospheric Imaging Instrument (MIMI) suite onboard …

Jupiter hosts the most hazardous radiation belts of our solar system that, besides electrons
and protons, trap an undetermined mix of heavy ions. The details of this mix are critical to …

Observations of the radial locations of satellite absorption microsignatures in energetic
particle data at Saturn have suggested the existence of an average convection pattern, fixed …

In this chapter, we review selected fundamental plasma processes that control the extensive
space environment, or magnetosphere, of Saturn (see Chapter 9, for the global context) …

The lack of an upstream solar wind monitor poses a major challenge to any study that
investigates the influence of the solar wind on the configuration and the dynamics of Saturn's …