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The Atmospheres of Saturn and Titan in the Near-Infrared First Results of Cassini/vims
DOI: 10.1007/s11038-005-9058-2 Bibcode: 2005EM&P...96..119B

Sotin, C.; Brown, R. H.; Baines, K. H. +21 more

The wide spectral coverage and extensive spatial, temporal, and phase-angle mapping capabilities of the Visual Infrared Mapping Spectrometer (VIMS) onboard the Cassini-Huygens Orbiter are producing fundamental new insights into the nature of the atmospheres of Saturn and Titan. For both bodies, VIMS maps over time and solar phase angles provide in…

2005 Earth Moon and Planets
Cassini 62
Cassini CIRS Observations of a Roll-Off in Saturn Ring Spectra at Submillimeter Wavelengths
DOI: 10.1007/s11038-005-9060-8 Bibcode: 2005EM&P...96..149S

Edgington, S. G.; Spilker, L. J.; Pilorz, S. H. +4 more

The Cassini Composite Infrared Spectrometer (CIRS) spatially resolved Saturn's main rings in the far-infrared, measuring the spectrum from 20 to 400 wavenumbers (cm‑1) (tens of microns to submillimeter wavelengths). We find a spectral roll-off below 50 cm‑1 (200 µm) for each of the A, B and C rings. From these data we d…

2005 Earth Moon and Planets
Cassini 25
Dust Activity in Comet 67P/Churyumov–Gerasimenko from February 20 to April 20, 2003
DOI: 10.1007/s11038-006-9067-9 Bibcode: 2005EM&P...97..165L

Lara, L. M.; Gutiérrez, P. J.; Licandro, J. +1 more

Broadband imaging of Comet 67P/Churyumov–Gerasimenko has provided more data on the characterisation of the target of the ESA Rosetta Mission. The comet monitoring between rh=2.37 and rh=2.78 AU postperihelion shows a prominent dust coma which extends up to ≈ 25,000 km from the nucleus, and a long dust structure in approximate…

2005 Earth Moon and Planets
Rosetta 13
Titan's Ground Reflectance Retrieval from Cassini-Vims Data Taken during the July 2ND, 2004 Fly-By at 2 AM UT
DOI: 10.1007/s11038-005-9057-3 Bibcode: 2005EM&P...96..109A

D'Aversa, E.; Orosei, R.; Coradini, A. +5 more

An attempt to evaluate the preliminary values of the Titan's surface albedo at 2 µm from the first Cassini-VIMS observations of the moon is presented. The methodology is based on the application of radiative transfer calculations and a microphysical model of the Titan atmosphere based on fractal aerosol. As a first guess, the surface has bee…

2005 Earth Moon and Planets
Cassini 3