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Mars Express measurements of surface albedo changes over 2004-2010
DOI: 10.1016/j.icarus.2014.10.029 Bibcode: 2015Icar..251..145V

Altieri, F.; Vincendon, M.; Audouard, J. +1 more

The pervasive Mars dust is continually transported between the surface and the atmosphere. When on the surface, dust increases the albedo of darker underlying rocks and regolith, which modifies climate energy balance and must be quantified. Remote observation of surface albedo absolute value and albedo change is however complicated by dust itself …

2015 Icarus
MEx 29
Deep alteration between Hellas and Isidis Basins
DOI: 10.1016/j.icarus.2015.06.037 Bibcode: 2015Icar..260..141B

Quantin-Nataf, C.; Bultel, B.; Andréani, M. +2 more

Recent investigations of alteration of martian crustal outcrops suggest putative crustal hydrothermal systems, which are favorable environments for the emergence of life. In this study, we perform an analysis of the CRISM targeted observations covering crustal outcrops in the region between the Hellas and Isidis basins with the goal of investigati…

2015 Icarus
MEx 29
Integrating CRISM and TES hyperspectral data to characterize a halloysite-bearing deposit in Kashira crater, Mars
DOI: 10.1016/j.icarus.2014.11.034 Bibcode: 2015Icar..250..165G

Mustard, John F.; Goudge, Timothy A.; Head, James W. +2 more

We present morphologic observations and spectral modeling results of a large, kaolin-group mineral-bearing deposit within Kashira crater in the southern highlands of Mars. We employ both non-linear unmixing of Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) visible to near-infrared (VNIR) reflectance data and linear unmixing of Therma…

2015 Icarus
MEx 28
Seasonal variation of the HDO/H2O ratio in the atmosphere of Mars at the middle of northern spring and beginning of northern summer
DOI: 10.1016/j.icarus.2015.06.021 Bibcode: 2015Icar..260....7A

Aoki, Shohei; Kasaba, Yasumasa; Sagawa, Hideo +4 more

We present the seasonal variation of the HDO/H2O ratio caused by sublimation-condensation processes in a global view of the martian water cycle. The HDO/H2O ratio was retrieved from ground-based observations using high-dispersion echelle spectroscopy of the Infrared Camera and Spectrograph (IRCS) of the Subaru telescope. Coor…

2015 Icarus
MEx 28
Mars thermospheric scale height: CO Cameron and CO2+ dayglow observations from Mars Express
DOI: 10.1016/j.icarus.2014.09.051 Bibcode: 2015Icar..245..295S

Montmessin, F.; Bertaux, J. -L.; Gérard, J. -C. +3 more

The CO Cameron (170-270 nm) and CO2+ ultraviolet doublet (298 and 299 nm) emissions have been observed on the Mars dayside with Mars Express Spectroscopy for Investigation of Characteristics of the Atmosphere of Mars (SPICAM) instrument in the limb viewing mode. These ultraviolet emissions ultimately arise from the excitation…

2015 Icarus
MEx 27
Constraints on the depths of origin of peak rings on the Moon from Moon Mineralogy Mapper data
DOI: 10.1016/j.icarus.2015.06.013 Bibcode: 2015Icar..258..164B

Head, James W.; Baker, David M. H.

Important to understanding the process of basin formation on planetary bodies are constraints on the mineralogy and depths of origin of interior ring structures. We summarize previous analyses of the mineralogy of basin materials on the Moon and use hyperspectral image-cubes from the Chandrayaan-1's Moon Mineralogy Mapper (M3) to determ…

2015 Icarus
Chandrayaan-1 27
Variations in peak electron densities in the ionosphere of Mars over a full solar cycle
DOI: 10.1016/j.icarus.2014.08.008 Bibcode: 2015Icar..251....5W

Gurnett, D. A.; Morgan, D. D.; Withers, Paul

Peak electron densities in the ionosphere of Mars are strongly influenced by the intensity of ionizing solar flux and hence by the solar cycle. Datasets used in previous studies of this relationship have incompletely sampled the range of solar irradiances encountered over a full solar cycle. Here, thousands of Mars Global Surveyor radio occultatio…

2015 Icarus
MEx 26
Carbon monoxide and temperature in the upper atmosphere of Venus from VIRTIS/Venus Express non-LTE limb measurements
DOI: 10.1016/j.icarus.2014.10.047 Bibcode: 2015Icar..248..478G

López-Valverde, M. A.; Gilli, G.; Drossart, P. +4 more

The upper mesosphere and the lower thermosphere of Venus (from 90 to 150 km altitude) seems to play a transition region in photochemistry, dynamics and radiation, but is still very poorly constrained observationally. Since 2006 VIRTIS on board Venus Express has been obtaining limb observations of CO fluorescent infrared emissions in a systematic m…

2015 Icarus
VenusExpress 25
Volcanism-induced, local wet-based glacial conditions recorded in the Late Amazonian Arsia Mons tropical mountain glacier deposits
DOI: 10.1016/j.icarus.2014.11.016 Bibcode: 2015Icar..250...18S

Head, James W.; Marchant, David R.; Scanlon, Kathleen E.

The tropical mountain glacial fan-shaped deposit (FSD) to the northwest of the Arsia Mons volcano on Mars contains numerous glacial and volcanic landforms. While most of the glacial landforms are interpreted to have formed by cold-based glacial processes, several glacial landforms near glaciovolcanic edifices are more consistent with localized wet…

2015 Icarus
MEx 24
Seasonal changes in Saturn's stratosphere inferred from Cassini/CIRS limb observations
DOI: 10.1016/j.icarus.2015.05.025 Bibcode: 2015Icar..258..224S

Flasar, F. M.; Spiga, A.; Fouchet, T. +4 more

We present temperature and hydrocarbons abundances (C2H6, C2H2, C3H8) retrieved from Cassini/CIRS limb spectra, acquired during northern spring in 2010 (LS = 12 °) and 2012 (LS = 31 °). We compare them to the previous limb measurements performed by Guerlet et a…

2015 Icarus
Cassini 22