An investigation into both small and large amplitude dust acoustic solitary waves in dusty
plasmas with cold negative dust grains and kappa-distributed ions and/or electrons is …

Pre-Cassini models of Saturn's E ring [Horányi, M., Burns, J., Hamilton, D., 1992. Icarus 97,
248–259; Juhász, A., Horányi, M., 2002. J. Geophys. Res. 107, 1–10] failed to reproduce its …

Saturn's rich magnetospheric environment is unique in the solar system, with a large number
of active magnetospheric processes and phenomena. Observations of this environment from …

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 …

The flyby measurements of the Cassini spacecraft at Saturn's moon Rhea reveal a tenuous
oxygen (O2)–carbon dioxide (CO2) atmosphere. The atmosphere appears to be sustained …

Cassini observations confirm that Saturn's rings are predominantly water ice. The particles in
Saturn's rings cover a range of sizes, from dust to small moons. Occultation results show the …

We review recent progress concerning the composition and size distribution of the particles
in Saturn's main ring system, and describe how these properties vary from place to place …

Saturn is orbited by a half dozen ice rich middle-sized moons (MSMs) of diverse geology
and composition. These comprise∼ 4.4% of Saturn's satellite mass; the rest is Titan, more …

Using Cassini images, we examine the faint material along the orbits of Methone, Anthe and
Pallene, three small moons that reside between the orbits of Mimas and Enceladus. A …

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) …