Nonkeplerian dust dynamics at Saturn

Cassini Cosmic Dust Analyser: Composition of Dust at Saturn

We discuss issues involved with interpreting time-offlight mass spectra (TOFMS) obtained by the Chemical Analyser subsystem of the Cassini Cosmic Dust Analyser (CDA). We use an in-house ion dynamics code specifically written for CDA which helps us to understand and constrain the initial impact plasma ion kinetic energy and angular distributions. We also present some typical results obtained fro...

Does Enceladus govern magnetospheric dynamics at Saturn?

Instruments on the Cassini spacecraft reveal that a heat source within Saturn's moon Enceladus powers a great plume of water ice particles and dust grains, a geyser that jets outward from the south polar regions and most likely serves as the dominant source of Saturn's E ring. The interaction of flowing magnetospheric plasma with the plume modifies the particle and field environment of Enceladu...

Increasing Productivity at Saturn

T o remain competitive, manufacturing enterprises must increase throughput and simultaneously reduce costs. This requires daily and long-term examination and analysis of a plant’s functions and operations. Using this data, an enterprise can identify production flow bottlenecks and analyze capacity and other factors, which in turn helps identify improvement opportunities. While such information ...

Observation of similar radio signatures at Saturn and Jupiter: Implications for the magnetospheric dynamics

Propagation of Dust Acoustic Solitary Waves in Saturn F-ring’s Region

Effect of hot and cold dust charge on the propagation of dust-acoustic waves (DAWs) in unmagnetized plasma having electrons, singly charged ions, hot and cold dust grains have been investigated. The reductive perturbation method is employed to reduce the basic set of fluid equations to the Korteweg-de Vries (KdV) equation. The effect of cold (hot) dusty plasma density nc (nh) and the charge num...