This paper aims to assess the potential and requirements of photovoltaic arrays to provide
energy for more than 30 mission types to explore 14 celestial bodies in our solar system …

Cassini has identified a geologically active province at the south pole of Saturn's moon
Enceladus. In images acquired by the Imaging Science Subsystem (ISS), this region is …

The plumes discovered by the Cassini mission emanating from the south pole of Saturn׳ s
moon Enceladus and the unique chemistry found in them have fueled speculations that …

Periodic modulation of magnetospheric phenomena at Earth and Jupiter results principally
from the tilt of the dipole axis relative to the rotation axis. Saturn's nearly aligned dipole …

Since the arrival of the Cassini spacecraft at Saturn in July 2004, newly collected plasma
and magnetic field data have greatly expanded our knowledge on the interaction between …

Using ion–electron fluid parameters derived from Cassini Plasma Spectrometer (CAPS)
observations within Saturn's inner magnetosphere as presented in Sittler et al.[2006a …

Although there are substantial differences between the magnetospheres of Jupiter and
Saturn, it has been suggested that cryovolcanic activity at Enceladus,,,,,,,, could lead to …

ABSTRACT On 2005 November 27 (day 331), the Visual and Infrared Mapping
Spectrometer instrument onboard the Cassini spacecraft obtained high signal-to-noise …

By traversing the plume erupting from high southern latitudes on Saturn's moon Enceladus,
Cassini orbiter instruments can directly sample the material therein. Cassini Plasma …

Time variability of Enceladus' gas plume is deduced from a joint investigation of Cassini
spacecraft magnetic field data obtained during the first three flybys E0, E1 and E2 and …