Search Publications

Bathymetry and composition of Titan's Ontario Lacus derived from Monte Carlo-based waveform inversion of Cassini RADAR altimetry data
DOI: 10.1016/j.icarus.2017.09.009 Bibcode: 2018Icar..300..203M

Lorenz, R. D.; Lunine, J. I.; Hayes, A. G. +8 more

Recently, the Cassini RADAR was used to sound hydrocarbon lakes and seas on Saturn's moon Titan. Since the initial discovery of echoes from the seabed of Ligeia Mare, the second largest liquid body on Titan, a dedicated radar processing chain has been developed to retrieve liquid depth and microwave absorptivity information from RADAR altimetry of…

2018 Icarus
Cassini 43
New polarimetric and spectroscopic evidence of anomalous enrichment in spinel-bearing calcium-aluminium-rich inclusions among L-type asteroids
DOI: 10.1016/j.icarus.2017.12.026 Bibcode: 2018Icar..304...31D

Surdej, J.; Tanga, P.; Carry, B. +14 more

Asteroids can be classified into several groups based on their spectral reflectance. Among these groups, the one belonging to the L-class in the taxonomic classification based on visible and near-infrared spectra exhibit several peculiar properties. First, their near-infrared spectrum is characterized by a strong absorption band interpreted as the…

2018 Icarus
AKARI 43
Europa's ice-related atmosphere: The sputter contribution
DOI: 10.1016/j.icarus.2018.03.022 Bibcode: 2018Icar..311..135V

Wurz, P.; Vorburger, A.

Europa, Jupiter's innermost icy satellite, is embedded well within Jupiter's magnetospheric plasma, an intense flux of ions and electrons that approximately co-rotate with Jupiter. The plasma can be thought of as consisting of two populations: The cold, thermal plasma containing charged particles with energies ranging from 1 eV to 1 keV, and the h…

2018 Icarus
eHST 40
Solar Energetic Particles (SEP) and Galactic Cosmic Rays (GCR) as tracers of solar wind conditions near Saturn: Event lists and applications
DOI: 10.1016/j.icarus.2017.08.040 Bibcode: 2018Icar..300...47R

Krupp, N.; Thomsen, M. F.; Jackman, C. M. +10 more

The lack of an upstream solar wind monitor poses a major challenge to any study that investigates the influence of the solar wind on the configuration and the dynamics of Saturn's magnetosphere. Here we show how Cassini MIMI/LEMMS observations of Solar Energetic Particle (SEP) and Galactic Cosmic Ray (GCR) transients, that are both linked to energ…

2018 Icarus
Cassini 32
Icy Saturnian satellites: Disk-integrated UV-IR characteristics and links to exogenic processes
DOI: 10.1016/j.icarus.2017.08.037 Bibcode: 2018Icar..300..103H

Hendrix, Amanda R.; Filacchione, Gianrico; Schenk, Paul +2 more

Combined Cassini observations obtained at similar observing geometries in the ultraviolet through infrared spectral range, along with additional ultraviolet (UV) data from Hubble Space Telescope where available, are used to study system-wide trends in spectral albedos of the inner icy Saturnian satellites (Mimas, Enceladus, Tethys, Dione, Rhea). W…

2018 Icarus
Cassini eHST 32
Characterization of dust activity on Mars from MY27 to MY32 by PFS-MEX observations
DOI: 10.1016/j.icarus.2017.10.045 Bibcode: 2018Icar..310...32W

Aoki, Shohei; Giuranna, Marco; Wolkenberg, Paulina +4 more

We present spatial and temporal distributions of dust on Mars from Ls = 331° in MY 26 until Ls = 80° in MY33 retrieved from the measurements taken by the Planetary Fourier Spectrometer (PFS) aboard Mars Express. In agreement with previous observations, large dust opacity is observed mostly in the southern hemisphere spring/summer and particularly …

2018 Icarus
MEx 32
A systematic search of sudden pressure drops on Gale crater during two Martian years derived from MSL/REMS data
DOI: 10.1016/j.icarus.2017.07.032 Bibcode: 2018Icar..299..308O

Hueso, Ricardo; Sánchez-Lavega, Agustín; Ordonez-Etxeberria, Iñaki

The Mars Science Laboratory (MSL) rover carries a suite of meteorological detectors that constitute the Rover Environmental Monitoring Station (REMS) instrument. REMS investigates the meteorological conditions at Gale crater by obtaining high-frequency data of pressure, air and ground temperature, relative humidity, UV flux at the surface and wind…

2018 Icarus
MEx 31
On deviations from free-radial outflow in the inner coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2018.03.010 Bibcode: 2018Icar..311....1G

Jorda, L.; Lamy, P. L.; Lara, L. M. +44 more

The Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) onboard the European Space Agency's Rosetta spacecraft acquired images of comet 67P/Churyumov-Gerasimenko (67P) and its surrounding dust coma starting from May 2014 until September 2016. In this paper we present methods and results from analysis of OSIRIS images regarding the …

2018 Icarus
Rosetta 30
Photochemistry, mixing and transport in Jupiter's stratosphere constrained by Cassini
DOI: 10.1016/j.icarus.2018.02.018 Bibcode: 2018Icar..307..106H

Sinclair, J. A.; Hue, V.; Cavalié, T. +2 more

In this work, we aim at constraining the diffusive and advective transport processes in Jupiter's stratosphere, using Cassini/CIRS observations published by Nixon et al. (2007,2010). The Cassini-Huygens flyby of Jupiter on December 2000 provided the highest spatially resolved IR observations of Jupiter so far, with the CIRS instrument. The IR spec…

2018 Icarus
ISO 30
Meter-scale thermal contraction crack polygons on the nucleus of comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2017.09.037 Bibcode: 2018Icar..301..173A

Jorda, L.; Lamy, P. L.; Lara, L. M. +48 more

We report on the detection and characterization of more than 6300 polygons on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, using images acquired by the OSIRIS camera onboard Rosetta between August 2014 and March 2015. They are found in consolidated terrains and grouped in localized networks. They are present at all latitudes (fro…

2018 Icarus
Rosetta 29