Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

Abstract The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-
dimensional mass-resolved measurements of the full variety of plasma phenomena found in …

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 …

Updated chemical schemes and estimates of key rate coefficients are used in the present
investigation of the photochemistry of Titan atmosphere CH-and O-atom containing simple …

The Cassini‐Huygens probe gas chromatograph mass spectrometer (GCMS) determined
the composition of the Titan atmosphere from∼ 140 km altitude to the surface. After landing …

As Voyager 1 flew through the Saturn system it returned photographs revealing many new
and surprising characteristics of this complicated community of bodies. Saturn's atmosphere …

During the passage of Voyager 1 through the Saturn system, the infrared instrument
acquired spectral and radiometric data on Saturn, the rings, and Titan and other satellites …

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection
system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ …

Two coherently related radio signals transmitted from Voyager 1 at wavelengths of 13 cm (S-
band) and 3.6 cm (X-band) were used to probe the equatorial atmosphere of Titan. The …

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 …