Search Publications

Stereo topographic mapping concept for the upcoming Luna-Resurs-1 orbiter mission
DOI: 10.1016/j.pss.2017.09.013 Bibcode: 2018P&SS..162..216P

Oberst, J.; Polyansky, I.; Zhukov, B. +4 more

We report on the Lunar Stereo Topographic Camera (LSTC), currently being developed for the upcoming Luna-Resurs-1 Orbiter mission, which will perform observations from an orbit with the altitude to be optimized in the range from 50 to 100 km. The LSTC is composed of two identical optical heads and a common data processing unit. Each optical head h…

2018 Planetary and Space Science
MEx 2
Mapping and dating based evolution studies of the Niger Vallis outflow channel, Mars
DOI: 10.1016/j.pss.2017.12.012 Bibcode: 2018P&SS..153...54K

Kostama, V. -P.; Kukkonen, S.

Niger Vallis is one of the four large outflow channel systems in the eastern Hellas rim region of Mars. Niger, as well as the other nearby valles, is assumed to have been carved by water and later covered by ice-rich deposits. Thus, it plays a significant role both in the fluvial and glacial evolution of the region. This work presents the photogeo…

2018 Planetary and Space Science
MEx 1
Retrieving cloud, dust and ozone abundances in the Martian atmosphere using SPICAM/UV nadir spectra
DOI: 10.1016/j.pss.2017.04.011 Bibcode: 2017P&SS..142....9W

Vandaele, A. C.; Montmessin, F.; Willame, Y. +4 more

We present the retrieval algorithm developed to analyse nadir spectra from SPICAM/UV aboard Mars-Express. The purpose is to retrieve simultaneously several parameters of the Martian atmosphere and surface: the dust optical depth, the ozone total column, the cloud opacity and the surface albedo. The retrieval code couples the use of an existing com…

2017 Planetary and Space Science
ExoMars-16 MEx 43
Idunn Mons on Venus: Location and extent of recently active lava flows
DOI: 10.1016/j.pss.2016.12.002 Bibcode: 2017P&SS..136...25D

Helbert, Jörn; D'Incecco, Piero; D'Amore, Mario +1 more

From 2006 until 2014 the ESA Venus Express probe observed the atmosphere and surface of the Earth's twin planet. The Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) has provided data that indicate the occurrence of recent volcanic activity on Venus. We selected the eastern flank of Idunn Mons - Imdr Regio's single large volcano - as the…

2017 Planetary and Space Science
VenusExpress 38
Sensitivity and fragmentation calibration of the time-of-flight mass spectrometer RTOF on board ESA's Rosetta mission
DOI: 10.1016/j.pss.2016.11.011 Bibcode: 2017P&SS..135...64G

Mall, Urs; Fiethe, Björn; Wurz, Peter +8 more

The European Space Agency's Rosetta spacecraft, with the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) onboard, has been following and observing comet 67P/Churyumov-Gerasimenko since summer 2014. Prior to this period, and due to a technical failure also during this period, optimization and calibration campaigns have been condu…

2017 Planetary and Space Science
Rosetta 26
New constraints on Ganymede's hydrogen corona: Analysis of Lyman-α emissions observed by HST/STIS between 1998 and 2014
DOI: 10.1016/j.pss.2017.10.006 Bibcode: 2017P&SS..148...35A

Alday, Juan; Saur, Joachim; Roth, Lorenz +4 more

Far-ultraviolet observations of Ganymede's atmospheric emissions were obtained with the Space Telescope Imaging Spectrograph (STIS) onboard of the Hubble Space Telescope (HST) on several occasions between 1998 and 2014. We analyze the Lyman-α emission from four HST campaigns in order to constrain the abundance and variation of atomic hydrogen in G…

2017 Planetary and Space Science
eHST 21
Ultra low frequency waves at Venus: Observations by the Venus Express spacecraft
DOI: 10.1016/j.pss.2017.08.011 Bibcode: 2017P&SS..146...55F

Fränz, M.; Zhang, T. L.; Dubinin, E. +2 more

The generation of waves with low frequencies (below 100 mHz) has been observed in the environment of most bodies in the solar system and well studied at Earth. These waves can be generated either upstream of the body in the solar wind by ionization of planetary exospheres or ions reflected from a bow shock or in the magnetosheath closer to the mag…

2017 Planetary and Space Science
VenusExpress 20
Bidirectional reflectance and VIS-NIR spectroscopy of cometary analogues under simulated space conditions
DOI: 10.1016/j.pss.2017.07.009 Bibcode: 2017P&SS..145...14J

Thomas, Nicolas; Fornasier, Sonia; Pommerol, Antoine +7 more

This work is intended to be the second publication in a series of papers reporting on the spectro-photometric properties of cometary analogues measured in the laboratory. Herein, we provide in-situ hyperspectral imaging data in the 0.40-2.35 µm range from three sublimation experiments under simulated space conditions in thermal vacuum from s…

2017 Planetary and Space Science
Rosetta 16
Measurement of dust optical depth using the solar irradiance sensor (SIS) onboard the ExoMars 2016 EDM
DOI: 10.1016/j.pss.2017.01.015 Bibcode: 2017P&SS..138...33T

Rannou, P.; Toledo, D.; Gómez, L. +5 more

The solar irradiance sensor (SIS) was included in the DREAMS package onboard the ExoMars 2016 Entry Descent and Landing Demonstrator Module, and has been selected in the METEO meteorological station onboard the ExoMars 2020 Lander. This instrument is designed to measure at different time intervals the scattered flux or the sum of direct flux and s…

2017 Planetary and Space Science
ExoMars-16 16
Bidirectional reflectance of laboratory cometary analogues to interpret the spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.pss.2017.09.009 Bibcode: 2017P&SS..148....1J

Thomas, Nicolas; Fornasier, Sonia; Pommerol, Antoine +5 more

In this work we provide measurements of the bidirectional reflectance in the VIS-NIR spectral range for a selection of laboratory samples to deduce parameters such as their visible spectrum, phase curve, hemispheric albedo and phase reddening. The aim is to simulate the reflectance of the comet nucleus in order to aid the interpretation of data fr…

2017 Planetary and Space Science
Rosetta 16