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Columbia Hills, Mars: Aeolian features seen from the ground and orbit
DOI: 10.1029/2007JE002971 Bibcode: 2008JGRE..113.6S06G

Greeley, Ronald; Whelley, Patrick L.; Neakrase, Lynn D. V. +15 more

Abundant wind-related features occur along Spirit's traverse into the Columbia Hills over the basaltic plains of Gusev Crater. Most of the windblown sands are probably derived from weathering of rocks within the crater, and possibly from deposits associated with Ma'adim Vallis. Windblown particles act as agents of abrasion, forming ventifacts, and…

2008 Journal of Geophysical Research (Planets)
MEx 34
Tropospheric carbon monoxide concentrations and variability on Venus from Venus Express/VIRTIS-M observations
DOI: 10.1029/2008JE003089 Bibcode: 2008JGRE..113.0B08T

Drossart, Pierre; Irwin, Patrick G. J.; Piccioni, Giuseppe +7 more

We present nightside observations of tropospheric carbon monoxide in the southern hemisphere near the 35 km height level, the first from Venus Express/Visible and Infrared Thermal Imaging Spectrometer (VIRTIS)-M-IR. VIRTIS-M data from 2.18 to 2.50 µm, with a spectral resolution of 10 nm, were used in the analysis. Spectra were binned, with w…

2008 Journal of Geophysical Research (Planets)
VenusExpress 34
Mineralogical composition, structure, morphology, and geological history of Aram Chaos crater fill on Mars derived from OMEGA Mars Express data
DOI: 10.1029/2008JE003131 Bibcode: 2008JGRE..11312006M

Le Mouélic, S.; Sotin, C.; Bibring, J. -P. +6 more

Aram Chaos is a crater 280 km in diameter centered at 2.5°N, 338.5°E. It is filled by chaotic terrains overlain by a dome-shaped, layered 900 m thick formation displaying spectral signatures of ferric oxides on Thermal Emission Spectrometer (TES) and Observatoire pour la Mineralogie, L'Eau, les Glaces et L'Activite (OMEGA) medium spatial resolutio…

2008 Journal of Geophysical Research (Planets)
MEx 33
Evidence for anomalous cloud particles at the poles of Venus
DOI: 10.1029/2008JE003108 Bibcode: 2008JGRE..113.0B13W

Carlson, R. W.; Irwin, P. G. J.; Drossart, P. +5 more

An analysis of near-infrared emissions on the nightside of Venus observed by the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) instrument on board Venus Express reveals anomalous cloud particles in the polar regions of Venus. These anomalous particles are found within the centers of polar vortices at both poles and are either larger o…

2008 Journal of Geophysical Research (Planets)
VenusExpress 31
Proton cyclotron waves in the solar wind at Venus
DOI: 10.1029/2008JE003148 Bibcode: 2008JGRE..113.0B06D

Zhang, T. L.; Volwerk, M.; Delva, M. +2 more

Magnetometer data from two Venus years of the Venus Express mission in orbit are investigated for the occurrence of ion cyclotron waves. Proton cyclotron waves were recently detected in the upstream region of Venus by the spacecraft, indicating pickup of planetary protons from Venus's exosphere by the solar wind and loss of hydrogen to interplanet…

2008 Journal of Geophysical Research (Planets)
VenusExpress 29
Limb observations of the ultraviolet nitric oxide nightglow with SPICAV on board Venus Express
DOI: 10.1029/2008JE003078 Bibcode: 2008JGRE..113.0B03G

Bertaux, J. -L.; Villard, E.; Gérard, J. -C. +3 more

Limb observations of the spectrum of nightglow emission in the δ (190-240 nm) and γ (225-270 nm) bands of nitric oxide have been made with the Spectroscopy for Investigation of Characteristics of the Atmosphere of Venus (SPICAV) ultraviolet spectrometer on board Venus Express. These emissions arise from radiative recombination between O(3

2008 Journal of Geophysical Research (Planets)
VenusExpress 27
Gray hematite distribution and formation in Ophir and Candor chasmata
DOI: 10.1029/2007JE002930 Bibcode: 2008JGRE..113.2016W

Weitz, Catherine M.; Lane, Melissa D.; Staid, Matthew +1 more

We have studied eight of the spatially largest locations in Ophir and Candor chasmata that have the highest abundances of coarse-grained gray hematite, as measured by the Mars Global Surveyor Thermal Emission Spectrometer (TES). All of the eight hematite locations correspond to relatively smooth dark units that overlie or are adjacent to light-ton…

2008 Journal of Geophysical Research (Planets)
MEx 27
Intermittent turbulence, noisy fluctuations, and wavy structures in the Venusian magnetosheath and wake
DOI: 10.1029/2008JE003159 Bibcode: 2008JGRE..113.0B21V

Zhang, T. L.; Baumjohann, W.; Volwerk, M. +3 more

Recent research has shown that distinct physical regions in the Venusian induced magnetosphere are recognizable from the variations of strength of the magnetic field and its wave/fluctuation activity. In this paper the statistical properties of magnetic fluctuations are investigated in the Venusian magnetosheath and wake regions. The main goal is …

2008 Journal of Geophysical Research (Planets)
VenusExpress 25
Dielectric properties of the Martian south polar layered deposits: MARSIS data inversion using Bayesian inference and genetic algorithm
DOI: 10.1029/2007JE002941 Bibcode: 2008JGRE..113.5004Z

Nielsen, Erling; Zhang, Zhenfei; Plaut, Jeffrey J. +3 more

Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) has offered abundant data, which have been used to estimate dielectric properties of the south polar layered deposits (SPLD) of Mars. This paper presents a new way to invert the data to estimate the dielectric properties of the SPLD. A total of 4364 measurements were analyzed. The…

2008 Journal of Geophysical Research (Planets)
MEx 25
Retrieval of air temperature profiles in the Venusian mesosphere from VIRTIS-M data: Description and validation of algorithms
DOI: 10.1029/2008JE003075 Bibcode: 2008JGRE..113.0B09G

Irwin, P. G. J.; Drossart, P.; Piccioni, G. +7 more

We present here methods developed for the retrieval of air temperature profiles in the Venusian mesosphere from the absolute radiances measured by the Visual and Infrared Thermal Imaging Spectrometer (VIRTIS) on board the Venus Express satellite. The infrared M channel of the instrument acquires multispectral images between 1000 and 5000 nm. In ni…

2008 Journal of Geophysical Research (Planets)
VenusExpress 23