Search Publications

Transient surface liquid in Titan's polar regions from Cassini
DOI: 10.1016/j.icarus.2010.08.017 Bibcode: 2011Icar..211..655H

Lorenz, R. D.; Wye, L. C.; Zebker, H. A. +12 more

Cassini RADAR images of Titan's south polar region acquired during southern summer contain lake features which disappear between observations. These features show a tenfold increases in backscatter cross-section between images acquired one year apart, which is inconsistent with common scattering models without invoking temporal variability. The mo…

2011 Icarus
Cassini 119
The haze and methane distributions on Neptune from HST-STIS spectroscopy
DOI: 10.1016/j.icarus.2010.08.013 Bibcode: 2011Icar..211..780K

Karkoschka, Erich; Tomasko, Martin G.

We analyzed a data cube of Neptune acquired with the Hubble STIS spectrograph on August 3, 2003. The data covered the full afternoon hemisphere at 0.1 arcsec spatial resolution between 300 and 1000 nm wavelength at 1 nm resolution. Navigation was accurate to 0.004 arcsec and 0.05 nm. We constrained the vertical aerosol structure with radiative tra…

2011 Icarus
eHST 118
Redefinition of the crater-density and absolute-age boundaries for the chronostratigraphic system of Mars
DOI: 10.1016/j.icarus.2011.07.024 Bibcode: 2011Icar..215..603W

Werner, S. C.; Tanaka, K. L.

For the boundaries of each chronostratigraphic epoch on Mars, we present systematically derived crater-size frequencies based on crater counts of geologic referent surfaces and three proposed "standard" crater size-frequency production distributions as defined by (a) a simple -2 power law, (b) Neukum and Ivanov, (c) Hartmann. In turn, these crater…

2011 Icarus
MEx 115
Heavy ion escape from Mars, influence from solar wind conditions and crustal magnetic fields
DOI: 10.1016/j.icarus.2011.08.003 Bibcode: 2011Icar..215..475N

Barabash, Stas; Lundin, Rickard; Nilsson, Hans +5 more

We have used more than 4 years of Mars Express ion data to estimate the escape of heavy ions ( O+,O2+ and CO2+) from Mars. To take the limited field of view of the instrument into account, the data has been binned into spatial bins and angular bins to create average distribution functions for different positions in the near Mars space. …

2011 Icarus
MEx 114
Plasma, plumes and rings: Saturn system dynamics as recorded in global color patterns on its midsize icy satellites
DOI: 10.1016/j.icarus.2010.08.016 Bibcode: 2011Icar..211..740S

Johnson, Robert E.; Hamilton, Douglas P.; McKinnon, William B. +4 more

New global maps of the five inner midsize icy saturnian satellites, Mimas, Enceladus, Tethys, Dione, and Rhea, have been constructed in three colors (UV, Green and near-IR) at resolutions of 1 km/pixel. The maps reveal prominent global patterns common to several of these satellites but also three major color features unique to specific satellites …

2011 Icarus
Cassini 111
Energy deposition and primary chemical products in Titan’s upper atmosphere
DOI: 10.1016/j.icarus.2011.03.001 Bibcode: 2011Icar..213..233L

Lewis, G. R.; Coates, A. J.; Galand, M. +4 more

Cassini results indicate that solar photons dominate energy deposition in Titan's upper atmosphere. These dissociate and ionize nitrogen and methane and drive the subsequent complex organic chemistry. The improved constraints on the atmospheric composition from Cassini measurements demand greater precision in the photochemical modeling. Therefore,…

2011 Icarus
Cassini 108
The mesosphere and lower thermosphere of Titan revealed by Cassini/UVIS stellar occultations
DOI: 10.1016/j.icarus.2011.09.022 Bibcode: 2011Icar..216..507K

Sandel, B. R.; West, R. A.; Yelle, R. V. +5 more

Stellar occultations observed by the Cassini/UVIS instrument provide unique data that probe the mesosphere and lower thermosphere of Titan at altitudes between 400 and 1400 km. This region is a site of complex photochemistry that forms hydrocarbon and nitrile species, and plays a crucial role in the formation of the organic hazes observed in the s…

2011 Icarus
Cassini IUE 97
Organic sedimentary deposits in Titan's dry lakebeds: Probable evaporite
DOI: 10.1016/j.icarus.2011.08.022 Bibcode: 2011Icar..216..136B

Nicholson, Philip D.; Sotin, Christophe; Barnes, Jason W. +14 more

We report the discovery of organic sedimentary deposits at the bottom of dry lakebeds near Titan's north pole in observations from the Cassini Visual and Infrared Mapping Spectrometer (VIMS). We show evidence that the deposits are evaporitic, making Titan just the third known planetary body with evaporitic processes after Earth and Mars, and is th…

2011 Icarus
Cassini 96
Methane on Uranus: The case for a compact CH 4 cloud layer at low latitudes and a severe CH 4 depletion at high-latitudes based on re-analysis of Voyager occultation measurements and STIS spectroscopy
DOI: 10.1016/j.icarus.2011.06.024 Bibcode: 2011Icar..215..292S

Sromovsky, L. A.; Fry, P. M.; Kim, J. H.

Lindal et al. (Lindal, G.F., Lyons, J.R., Sweetnam, D.N., Eshleman, V.R., Hinson, D.P. [1987]. J. Geophys. Res. 92 (11), 14987-15001) presented a range of temperature and methane profiles for Uranus that were consistent with 1986 Voyager radio occultation measurements of refractivity versus altitude. A localized refractivity slope variation near 1…

2011 Icarus
eHST 92
Saturn's zonal wind profile in 2004-2009 from Cassini ISS images and its long-term variability
DOI: 10.1016/j.icarus.2011.07.005 Bibcode: 2011Icar..215...62G

Hueso, R.; Sánchez-Lavega, A.; García-Melendo, E. +1 more

Five years of Cassini Imaging Science Subsystem images, from 2004 to 2009, are analyzed in this work to retrieve global zonal wind profiles of Saturn's northern and southern hemispheres in the methane absorbing bands at 890 and 727 nm and in their respective adjacent continuum wavelengths of 939 and 752 nm. A complete view of Saturn's global circu…

2011 Icarus
Cassini eHST 89