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Martian surface microtexture from orbital CRISM multi-angular observations: A new perspective for the characterization of the geological processes
DOI: 10.1016/j.pss.2016.05.005 Bibcode: 2016P&SS..128...30F

Schmidt, F.; Douté, S.; Fernando, J.

The surface of Mars has a high morphological and mineralogical diversity due to the intricacy of external, internal processes, and exchanges with the atmosphere, the hydrosphere and the cryosphere. In particular, liquid water played an important role in surface evolution. However, the origin, duration and intensity of those wet events have been hi…

2016 Planetary and Space Science
MEx 18
The daily processing of asteroid observations by Gaia
DOI: 10.1016/j.pss.2015.11.009 Bibcode: 2016P&SS..123...87T

Muinonen, Karri; Fedorets, Grigori; Pentikäinen, Hanna +15 more

The Gaia mission started its regular observing program in the summer of 2014, and since then it is regularly obtaining observations of asteroids. This paper draws the outline of the data processing for Solar System objects, and in particular on the daily ;short-term; processing, from the on-board data acquisition to the ground-based processing. We…

2016 Planetary and Space Science
Gaia 18
Separation of dynamic and isostatic components of the Venusian gravity and topography and determination of the crustal thickness of Venus
DOI: 10.1016/j.pss.2016.06.001 Bibcode: 2016P&SS..129...24Y

Yang, An; Huang, Jinshui; Wei, Daiyun

Assuming that the long-wavelength geoid and topography of Venus are supported by both mantle convection and Airy isostasy, we propose a method to separate the dynamic and isostatic components of the Venusian gravity and topography with the aid of the dynamic admittance from numerical models of mantle convection and the isostatic admittance from an…

2016 Planetary and Space Science
VenusExpress 17
A comprehensive analysis of ion cyclotron waves in the equatorial magnetosphere of Saturn
DOI: 10.1016/j.pss.2016.06.003 Bibcode: 2016P&SS..129...47M

Simon, Sven; Kabanovic, Slawa; Meeks, Zachary

We present a comprehensive analysis of ion cyclotron waves in the equatorial magnetosphere of Saturn, considering all magnetic field data collected during the Cassini era (totaling to over 4 years of data from the equatorial plane). This dataset includes eight targeted flybys of Enceladus, three targeted flybys of Dione, and three targeted flybys …

2016 Planetary and Space Science
Cassini 16
Systematic processing of Mars Express HRSC panchromatic and colour image mosaics: Image equalisation using an external brightness reference
DOI: 10.1016/j.pss.2015.12.002 Bibcode: 2016P&SS..121...18M

Jaumann, R.; van Gasselt, S.; Dumke, A. +8 more

After more than ten years in orbit at Mars, the coverage from the High Resolution Stereo Camera (HRSC) on the European Space Agency's Mars Express is sufficient to begin constructing mosaic products on a global scale. We describe our systematic processing procedure and, in particular, the technique used to bring images affected by atmospheric dust…

2016 Planetary and Space Science
MEx 15
Polarimetry observations of comets: Status, questions, future pathways
DOI: 10.1016/j.pss.2015.11.016 Bibcode: 2016P&SS..123...41H

Hines, Dean C.; Levasseur-Regourd, Anny-Chantal

Polarimetric observations of comets have provided crucial insight into the composition and evolution of cometary dust particles. Herein, we present a brief overview of the polarization properties observed in comets, and some possible interpretations. We also discuss recent imaging polarimetry observations of C/2012 S1 (ISON) and 67P/Churyumov-Gera…

2016 Planetary and Space Science
Rosetta eHST 15
The morphology of the topside ionosphere of Mars under different solar wind conditions: Results of a multi-instrument observing campaign by Mars Express in 2010
DOI: 10.1016/j.pss.2015.10.013 Bibcode: 2016P&SS..120...24W

Fränz, M.; Pätzold, M.; Wild, J. A. +17 more

Since the internally-generated magnetic field of Mars is weak, strong coupling is expected between the solar wind, planetary magnetosphere, and planetary ionosphere. However, few previous observational studies of this coupling incorporated data that extended from the solar wind to deep into the ionosphere. Here we use solar wind, magnetosphere, an…

2016 Planetary and Space Science
MEx VenusExpress 14
A novel method for surface exploration: Super-resolution restoration of Mars repeat-pass orbital imagery
DOI: 10.1016/j.pss.2015.11.010 Bibcode: 2016P&SS..121..103T

Tao, Y.; Muller, J. -P.

Higher resolution imaging data of planetary surfaces is considered desirable by the international community of planetary scientists interested in improving understanding of surface formation processes. However, given various physical constraints from the imaging instruments through to limited bandwidth of transmission one needs to trade-off spatia…

2016 Planetary and Space Science
MEx 13
The color ratio-intensity relation in the Jovian aurora: Hubble observations of auroral components
DOI: 10.1016/j.pss.2016.06.004 Bibcode: 2016P&SS..131...14G

Bonfond, B.; Gérard, J. -C.; Grodent, D. +1 more

Spectral observations made with the long slit of the Space Telescope Imaging Spectrograph (STIS) on board Hubble have been used to construct spectral maps of the FUV Jovian aurora. They reveal that the amount of absorption by overlying methane shows significant spatial variations. In this report, we examine the relationship between the auroral bri…

2016 Planetary and Space Science
eHST 13
InSight coordinates determination from direct-to-Earth radio-tracking and Mars topography model
DOI: 10.1016/j.pss.2015.11.003 Bibcode: 2016P&SS..121....1L

Le Maistre, Sébastien

The InSight mission is planned to land on the surface of Mars in September 2016. Close to the equator in Elysium Planitia, in the vicinity of the Curiosity location, the exact landing site coordinates cannot be provided by the navigation team. The direct-to-Earth (DTE) Doppler measurements are rarely included in the early lander localization proce…

2016 Planetary and Space Science
MEx 13