Search Publications

The science process for selecting the landing site for the 2020 Mars rover
DOI: 10.1016/j.pss.2018.07.001 Bibcode: 2018P&SS..164..106G

Golombek, Matthew P.; Wilson, Sharon A.; Grant, John A. +3 more

The process of identifying the landing site for NASA's Mars 2020 rover began in 2013 by defining threshold mission science criteria related to seeking signs of ancient habitable conditions, searching for biosignatures of past microbial life, assembling a returnable cache of samples for possible future return to Earth, and collecting data for plann…

2018 Planetary and Space Science
MEx 59
MarsSI: Martian surface data processing information system
DOI: 10.1016/j.pss.2017.09.014 Bibcode: 2018P&SS..150..157Q

Poulet, F.; Quantin-Nataf, C.; Leyrat, C. +10 more

MarsSI (Acronym for Mars System of Information, https://emars.univ-lyon1.fr/MarsSI/, is a web Geographic Information System application which helps managing and processing martian orbital data. The MarsSI facility is part of the web portal called PSUP (Planetary SUrface Portal) developed by the Observatories of Paris Sud (OSUPS) and Lyon (OSUL) to…

2018 Planetary and Space Science
MEx 48
ESA's Planetary Science Archive: Preserve and present reliable scientific data sets
DOI: 10.1016/j.pss.2017.07.013 Bibcode: 2018P&SS..150..131B

De Marchi, G.; Besse, S.; Vallat, C. +15 more

The European Space Agency (ESA) Planetary Science Archive (PSA) is undergoing a significant refactoring of all its components to improve the services provided to the scientific community and the public. The PSA supports ESA's missions exploring the Solar System by archiving scientific peer-reviewed observations as well as engineering data sets. Th…

2018 Planetary and Space Science
ExoMars-16 MEx Rosetta SMART-1 VenusExpress 42
On the relationship between surface pressure, terrain elevation, and air temperature. Part I: The large diurnal surface pressure range at Gale Crater, Mars and its origin due to lateral hydrostatic adjustment
DOI: 10.1016/j.pss.2018.07.003 Bibcode: 2018P&SS..164..132R

Newman, Claire E.; Richardson, Mark I.

The daily variation of surface pressure observed by the Curiosity Rover Environmental Monitoring Station (REMS) is both significantly larger than observed at other landing sites on Mars and larger than simulated for the Curiosity site by global circulation models (GCM). Mesoscale numerical models are able to simulate the large REMS daily pressure …

2018 Planetary and Space Science
MEx 32
Estimate of the water flow duration in large Martian fluvial systems
DOI: 10.1016/j.pss.2018.06.001 Bibcode: 2018P&SS..163...83O

Di Achille, Gaetano; Mancarella, Francesca; Orofino, Vincenzo +1 more

The presence of ancient fluvial systems on Mars, known as valley networks, is considered one of the most compelling evidence that liquid water was once stable on the planet's surface.

To understand the formation mechanisms of these valleys and to acquire information on the ancient climatic conditions of the planet, we determined the formation…

2018 Planetary and Space Science
MEx 26
The LatHyS database for planetary plasma environment investigations: Overview and a case study of data/model comparisons
DOI: 10.1016/j.pss.2017.02.015 Bibcode: 2018P&SS..150...13M

André, N.; Fedorov, A.; Budnik, E. +19 more

We present the Latmos Hybrid Simulation (LatHyS) database, which is dedicated to the investigations of planetary plasma environment. Simulation results of several planetary objects (Mars, Mercury, Ganymede) are available in an online catalogue. The full description of the simulations and their results is compliant with a data model developped in t…

2018 Planetary and Space Science
MEx 25
Massive stereo-based DTM production for Mars on cloud computers
DOI: 10.1016/j.pss.2018.02.012 Bibcode: 2018P&SS..154...30T

Tao, Y.; Muller, J. -P.; Sidiropoulos, P. +5 more

Digital Terrain Model (DTM) creation is essential to improving our understanding of the formation processes of the Martian surface. Although there have been previous demonstrations of open-source or commercial planetary 3D reconstruction software, planetary scientists are still struggling with creating good quality DTMs that meet their science nee…

2018 Planetary and Space Science
MEx 24
The Multi-Temporal Database of Planetary Image Data (MUTED): A web-based tool for studying dynamic Mars
DOI: 10.1016/j.pss.2018.04.015 Bibcode: 2018P&SS..159...56H

Jaumann, R.; Hiesinger, H.; Bernhardt, H. +4 more

Multi-temporal spacecraft observations are key to detect and understand surface changes and time-critical processes on Mars. Since the 1970s, the number of orbital observations of Mars has increased to over one million images. The observations have revealed that the surface of Mars is changing due to exogenic processes, including eolian activity, …

2018 Planetary and Space Science
MEx 17
Automatic Coregistration and orthorectification (ACRO) and subsequent mosaicing of NASA high-resolution imagery over the Mars MC11 quadrangle, using HRSC as a baseline
DOI: 10.1016/j.pss.2017.10.012 Bibcode: 2018P&SS..151...33S

Muller, Jan-Peter; Sidiropoulos, Panagiotis; Watson, Gillian +2 more

This work presents the coregistered, orthorectified and mosaiced high-resolution products of the MC11 quadrangle of Mars, which have been processed using novel, fully automatic, techniques. We discuss the development of a pipeline that achieves fully automatic and parameter independent geometric alignment of high-resolution planetary images, start…

2018 Planetary and Space Science
MEx 10
PSUP: A Planetary SUrface Portal
DOI: 10.1016/j.pss.2017.01.016 Bibcode: 2018P&SS..150....2P

Gondet, B.; Poulet, F.; Quantin-Nataf, C. +9 more

The large size and complexity of planetary data acquired by spacecraft during the last two decades create a demand within the planetary community for access to the archives of raw and high level data and for the tools necessary to analyze these data. Among the different targets of the Solar System, Mars is unique as the combined datasets from the …

2018 Planetary and Space Science
MEx 9