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Fluvial channels on Titan: Initial Cassini RADAR observations
DOI: 10.1016/j.pss.2008.02.009 Bibcode: 2008P&SS...56.1132L

Cassini RADAR Team; Kirk, Randolph L.; Lorenz, Ralph D. +13 more

Cassini radar images show a variety of fluvial channels on Titan's surface, often several hundreds of kilometers in length. Some (predominantly at low- and mid-latitude) are radar-bright and braided, resembling desert washes where fines have been removed by energetic surface liquid flow, presumably from methane rainstorms. Others (predominantly at…

2008 Planetary and Space Science
Cassini 127
Ion and neutral sources and sinks within Saturn's inner magnetosphere: Cassini results
DOI: 10.1016/j.pss.2007.06.006 Bibcode: 2008P&SS...56....3S

Thomsen, M. F.; Johnson, R. E.; Hartle, R. E. +16 more

Using ion-electron fluid parameters derived from Cassini Plasma Spectrometer (CAPS) observations within Saturn's inner magnetosphere as presented in Sittler et al. [2006a. Cassini observations of Saturn's inner plasmasphere: Saturn orbit insertion results. Planet. Space Sci., 54, 1197-1210], one can estimate the ion total flux tube content, N

2008 Planetary and Space Science
Cassini 114
Derivation of density and temperature from the Cassini Huygens CAPS electron spectrometer
DOI: 10.1016/j.pss.2007.12.017 Bibcode: 2008P&SS...56..901L

André, N.; Lewis, G. R.; Coates, A. J. +4 more

In this paper we present two methods to derive electron fluid parameters from the CAPS-ELS spectrometer on board the Cassini spacecraft currently in orbit around Saturn. In the first part of the paper we give a basic overview of the instrument and describe the challenges inherent in the derivation of density and temperature values using these tech…

2008 Planetary and Space Science
Cassini 87
Sputtering of ice grains and icy satellites in Saturn's inner magnetosphere
DOI: 10.1016/j.pss.2008.04.003 Bibcode: 2008P&SS...56.1238J

Johnson, R. E.; Sittler, E. C.; Smith, H. T. +3 more

Icy grains and satellites orbiting in Saturn's magnetosphere are immersed in a plasma that sputters their surfaces. This limits the lifetime of the E-ring grains and ejects neutrals that orbit Saturn until they are ionized and populate its magnetosphere. Here we re-evaluate the sputtering rate of ice in Saturn's inner magnetosphere using the recen…

2008 Planetary and Space Science
Cassini 45
Thermal observations of Saturn's main rings by Cassini CIRS: Phase, emission and solar elevation dependence
DOI: 10.1016/j.pss.2007.05.029 Bibcode: 2008P&SS...56..134A

Altobelli, Nicolas; Spilker, Linda J.; Leyrat, Cedric +1 more

Two and a half years after Saturn orbit insertion (SOI) the Cassini composite infrared spectrometer (CIRS) has acquired an extensive set of thermal measurements (including physical temperature and filling factor) of Saturn's main rings for a number of different viewing geometries, most of which are not available from Earth. Thermal mapping of both…

2008 Planetary and Space Science
Cassini 27
Infrared observations of Saturn's rings by Cassini CIRS : Phase angle and local time dependence
DOI: 10.1016/j.pss.2007.04.020 Bibcode: 2008P&SS...56..117L

Altobelli, Nicolas; Spilker, Linda J.; Ferrari, Cecile +2 more

Since the Saturn orbit insertion (SOI) of the Cassini spacecraft, in July 2004, the Cassini Composite Infrared Spectrometer (CIRS) has obtained a large number of thermal infrared spectra of Saturn's rings. Over the two and a half years of observations to date, ring temperatures were retrieved for a large range of unique geometries, inaccessible fr…

2008 Planetary and Space Science
Cassini 21
High-resolution Enceladus atlas derived from Cassini-ISS images
DOI: 10.1016/j.pss.2007.03.014 Bibcode: 2008P&SS...56..109R

Scholten, F.; Matz, K. -D.; Neukum, G. +8 more

The Cassini Imaging Science Subsystem (ISS) acquired 377 high-resolution images (<1 km/pixel) during three close flybys of Enceladus in 2005 [Porco, C.C., et al., 2006. Cassini observes the active south pole of Enceladus. Science 311, 1393-1401.]. We combined these images with lower resolution Cassini images and four others taken by Voyager cam…

2008 Planetary and Space Science
Cassini 20
High-resolution Dione atlas derived from Cassini-ISS images
DOI: 10.1016/j.pss.2008.06.008 Bibcode: 2008P&SS...56.1499R

Scholten, F.; Matz, K. -D.; Neukum, G. +7 more

The Cassini imaging science subsystem (ISS) acquired 449 high-resolution images (<800 m/pixel) during one close flyby of Dione in 2005 and three non-targeted flybys in 2004, 2006, and 2007. We combined these images with lower-resolution Cassini images and one other taken by Voyager cameras to produce a high-resolution semi-controlled mosaic of …

2008 Planetary and Space Science
Cassini 19
Optical properties of aerosols in Titan's atmosphere
DOI: 10.1016/j.pss.2007.11.013 Bibcode: 2008P&SS...56..660S

Keller, H. U.; Rodin, A. V.; Skorov, Yu. V.

In the frame of fractal modeling of tholin aggregates we made a systematic analysis of their optical properties. Ballistic particle-cluster aggregation (BPCA) and diffusion-limited aggregation (DLA) of spherical primary particles (monomers) identical in material composition were considered. Aggregates composed of identical particles (monodisperse …

2008 Planetary and Space Science
Cassini 16
Titan's surface from the Cassini RADAR radiometry data during SAR mode
DOI: 10.1016/j.pss.2007.03.015 Bibcode: 2008P&SS...56..100P

Lorenz, R. D.; Janssen, M. A.; Lunine, J. I. +8 more

We present initial results on the calibration and interpretation of the high-resolution radiometry data acquired during the Synthetic Aperture Radar (SAR) mode (SAR-radiometry) of the Cassini Radar Mapper during its first five flybys of Saturn's moon Titan. We construct maps of the brightness temperature at the 2-cm wavelength coincident with SAR …

2008 Planetary and Space Science
Cassini 12