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The roles of charge exchange and dissociation in spreading Saturn's neutral clouds
DOI: 10.1029/2011JE003996 Bibcode: 2012JGRE..117.5007F

Delamere, P. A.; Bagenal, F.; Fleshman, B. L. +1 more

Neutrals sourced directly from Enceladus's plumes are initially confined to a dense neutral torus in Enceladus's orbit around Saturn. This neutral torus is redistributed by charge exchange, impact/photodissociation, and neutral-neutral collisions to produce Saturn's neutral clouds. Here we consider the former processes in greater detail than in pr…

2012 Journal of Geophysical Research (Planets)
Cassini 39
The CH4 structure in Titan's upper atmosphere revisited
DOI: 10.1029/2012JE004222 Bibcode: 2012JGRE..11711006C

Strobel, D. F.; Galand, M.; Yelle, R. V. +4 more

In this study, we reanalyze the CH4 structure in Titan's upper atmosphere combining the Cassini Ion Neutral Mass Spectrometer (INMS) data from 32 flybys and incorporating several updates in the data reduction algorithms. We argue that based on our current knowledge of eddy mixing and neutral temperature, strong CH4 escape mus…

2012 Journal of Geophysical Research (Planets)
Cassini 37
Analysis of disk-resolved OMEGA and CRISM spectral observations of Phobos and Deimos
DOI: 10.1029/2012JE004137 Bibcode: 2012JGRE..117.0J15F

Bibring, J. -P.; Arvidson, R. E.; Gondet, B. +8 more

Disk-resolved observations of Phobos acquired by OMEGA at a range of lighting and viewing geometries were fit with the Hapke photometric function to solve for the single particle phase function and single scattering albedos from 0.4 to 2.5 µm. Single scattering albedos were recovered from CRISM observations of Phobos using the OMEGA derived …

2012 Journal of Geophysical Research (Planets)
MEx 37
Titan's ionospheric composition and structure: Photochemical modeling of Cassini INMS data
DOI: 10.1029/2011JE003883 Bibcode: 2012JGRE..117.1003W

Wahlund, J. -E.; Magee, B. A.; Mandt, K. E. +4 more

Titan's upper atmosphere produces an ionosphere at high altitudes from photoionization and electron impact that exhibits complex chemical processes in which hydrocarbons and nitrogen-containing molecules are produced through ion-molecule reactions. The structure and composition of Titan's ionosphere has been extensively investigated by the Ion and…

2012 Journal of Geophysical Research (Planets)
Cassini 33
Estimating erosional exhumation on Titan from drainage network morphology
DOI: 10.1029/2012JE004085 Bibcode: 2012JGRE..117.8006B

Black, Benjamin A.; Perron, J. Taylor; Burr, Devon M. +1 more

Drainage networks on Titan, Earth, and Mars provide the only known examples of non-volcanic fluvial activity in our solar system. The drainage networks on Titan are apparently the result of a methane-ethane cycle similar to Earth's water cycle. The scarcity of impact craters and the uneven distribution of fluvial dissection on Titan suggest that t…

2012 Journal of Geophysical Research (Planets)
Cassini 32
Compositional investigation of the proposed chloride-bearing materials on Mars using near-infrared orbital data from OMEGA/MEx
DOI: 10.1029/2012JE004108 Bibcode: 2012JGRE..117.0J13R

Bibring, Jean-Pierre; Gondet, Brigitte; Poulet, François +7 more

Several hundred occurrences of chloride-bearing salt deposits have been proposed in terrains within the southern highlands of Mars on the basis of Thermal Emission Imaging System and Thermal Emission Spectrometer infrared observations. The spectral identification of chloride salts by remote sensing is challenging because they are transparent over …

2012 Journal of Geophysical Research (Planets)
MEx 31
First detection of O2 1.27 µm nightglow emission at Mars with OMEGA/MEX and comparison with general circulation model predictions
DOI: 10.1029/2011JE003890 Bibcode: 2012JGRE..117.0J04B

Gondet, B.; Montmessin, F.; Bertaux, J. L. +2 more

We report the first detection in the atmosphere of Mars of the nightside O2(a1Δg) emission at 1.27 µm from limb observations of the OMEGA imaging spectrometer on board Mars Express (MEX). The emission, detected in three cases out of 40 observations, is due to recombination in a downwelling air parcel of O ato…

2012 Journal of Geophysical Research (Planets)
MEx 31
Density variations within the south polar layered deposits of Mars
DOI: 10.1029/2011JE003937 Bibcode: 2012JGRE..117.4006L

Zuber, Maria T.; Plaut, Jeffrey J.; Phillips, Roger J. +3 more

The south polar layered deposits (SPLD) constitute the largest known reservoir of water on Mars. Previous studies solved for the best fit uniform density of the deposits using a forward approach. Here we invert for the lateral density variations in the layered deposit using gravity data from radio tracking of Mars Reconnaissance Orbiter, topograph…

2012 Journal of Geophysical Research (Planets)
MEx 28
Density and lithospheric thickness of the Tharsis Province from MEX MaRS and MRO gravity data
DOI: 10.1029/2011JE003976 Bibcode: 2012JGRE..117.4002B

Pätzold, M.; Rosenblatt, P.; Le Maistre, S. +2 more

Radio science tracking of Mars Express (MaRS experiment) and Mars Reconnaissance Orbiter produced high resolution Martian gravity data. Applying localized spectral analysis on the new gravity data sets, we study the surface density and lithospheric elastic thickness in the Tharsis province. The gravity signal is predicted with geophysical models e…

2012 Journal of Geophysical Research (Planets)
MEx 27
Emitted power of Jupiter based on Cassini CIRS and VIMS observations
DOI: 10.1029/2012JE004191 Bibcode: 2012JGRE..11711002L

West, Robert A.; Baines, Kevin H.; Nixon, Conor A. +11 more

The emitted power of Jupiter and its meridional distribution are determined from observations by the Composite Infrared Spectrometer and Visual and Infrared Mapping Spectrometer onboard Cassini during its flyby en route to Saturn in late 2000 and early 2001. Jupiter's global-average emitted power and effective temperature are measured to be 14.10 …

2012 Journal of Geophysical Research (Planets)
Cassini 24