Search Publications

Dayside thermal structure of Venus' upper atmosphere characterized by a global model
DOI: 10.1029/2012JE004079 Bibcode: 2012JGRE..117.8002B

Brecht, A. S.; Bougher, S. W.

Observations of Venus' dayside thermal structure are being conducted through ground based observatories. These temperature measurements, along with those from several instruments onboard the current Venus Express mission, are augmenting the previous thermal structure data from past missions (e.g., Veneras', Pioneer Venus Orbiter, Pioneer Venus Pro…

2012 Journal of Geophysical Research (Planets)
VenusExpress 20
Iron mineralogy of the surface of Mars from the 1 µm band spectral properties
DOI: 10.1029/2012JE004091 Bibcode: 2012JGRE..117.0J17C

Bibring, J. -P.; Poulet, F.; Bellucci, G. +3 more

We study the 1 µm absorption from OMEGA/MEX spectra to map Martian iron mineralogy at a global scale. This band is covered on the left by the VNIR (visible and near infrared) OMEGA channel and on the right by the SWIR (short wavelengths infrared) one. We first perform a systematic spatial coregistration of the two channels after an improveme…

2012 Journal of Geophysical Research (Planets)
MEx 20
Upper ionosphere of Mars is not axially symmetrical
DOI: 10.5047/eps.2011.05.022 Bibcode: 2012EP&S...64..113D

Gurnett, D. A.; Barabash, S.; Lundin, R. +6 more

The measurements carried out by the ASPERA-3 and MARSIS experiments on board the Mars Express (MEX) spacecraft show that the upper Martian ionosphere (h ≥ 400 km) is strongly azimuthally asymmetrical. There are several factors, e.g., the crustal magnetization on Mars and the orientation of the interplanetary magnetic field (IMF) which c…

2012 Earth, Planets and Space
MEx 20
HST/STIS spectroscopy of the magnetic Of?p star HD 108: the low state at ultraviolet wavelengths
DOI: 10.1111/j.1365-2966.2012.20820.x Bibcode: 2012MNRAS.422.2314M

Bouret, J. -C.; Howarth, I. D.; Hillier, D. J. +6 more

We present the first ultraviolet spectrum of the peculiar, magnetic Of?p star HD 108 obtained in its spectroscopic low state. The new data, obtained with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope, reveal significant changes compared to IUE spectra obtained in the high state: N Vλ1240, Si IVλ1400 and C IVλ1550 pr…

2012 Monthly Notices of the Royal Astronomical Society
IUE eHST 20
Asymmetric magnetosphere deformation driven by hot flow anomaly(ies)
DOI: 10.1029/2012GL052636 Bibcode: 2012GeoRL..3915107S

Němeček, Z.; Šafránková, J.; Přech, L. +2 more

We present a case study of a large deformation of the magnetopause on November 26, 2008. The investigation is based on observations of five THEMIS spacecraft located at the dawn flank in the magnetosphere and magnetosheath, on Cluster measurements at the dusk magnetosheath, and is supported by ACE solar wind monitoring. The main revelation of our …

2012 Geophysical Research Letters
Cluster 20
Refinements in the data analysis of VIRTIS-M-IR Venus nightside spectra
DOI: 10.1016/j.asr.2012.03.029 Bibcode: 2012AdSpR..50..228K

Drossart, Pierre; Piccioni, Giuseppe; Haus, Rainer +2 more

The successful long-duration radiation measurements performed by the VIRTIS instrument aboard ESA's Venus Express spacecraft have provided an excellent collection of atmospheric and surface data that stand out due to their high temporal and spatial coverage of the planet and due to a high diversity of measurement and environmental conditions. A de…

2012 Advances in Space Research
VenusExpress 20
Sublimation-driven erosion on Hyperion: Topographic analysis and landform simulation model tests
DOI: 10.1016/j.icarus.2012.05.013 Bibcode: 2012Icar..220..268H

Schenk, Paul M.; White, Oliver L.; Moore, Jeffrey M. +2 more

The unique appearance of Hyperion can be explained in part by the loss to space of ballistic ejecta during impact events, as was proposed by Thomas et al. (Thomas, P.C. et al. [2007a]. Icarus 190, 573-584). We conclude that such loss is a partial explanation, accounting for the lack of appreciable intercrater plains on a saturation-cratered surfac…

2012 Icarus
Cassini 20
GALEX-selected Lyman Break Galaxies at z ~ 2: Comparison with Other Populations
DOI: 10.1088/0004-637X/745/1/96 Bibcode: 2012ApJ...745...96H

Nesvadba, N.; Haberzettl, L.; Lehnert, M. D. +2 more

We present results of a search for bright Lyman break galaxies (LBGs) at 1.5 <= z <= 2.5 in the GOODS-S field using an NUV-dropout technique in combination with color selection. We derived a sample of 73 LBG candidates. We compare our selection efficiencies to BM/BX and BzK methods (techniques solely based on ground-based data sets), and fin…

2012 The Astrophysical Journal
eHST 20
Possible optical counterpart of PSR J1357-6429
DOI: 10.1051/0004-6361/201118591 Bibcode: 2012A&A...540A..28D

Mennickent, R. E.; Zharikov, S.; Kirichenko, A. +4 more

Context. PSR J1357-6429 is a Vela-like radio pulsar that has been recently detected in X-rays and γ-rays. It powers a compact tail-like X-ray pulsar wind nebula and X-ray-radio plerion associated with an extended TeV source HESS J1356-645.
Aims: We present our deep optical observations with the Very Large Telescope to search for an optical co…

2012 Astronomy and Astrophysics
XMM-Newton 20
CO and H2 Absorption in the AA Tauri Circumstellar Disk
DOI: 10.1088/0004-637X/744/1/22 Bibcode: 2012ApJ...744...22F

Herczeg, Gregory J.; Brown, Alexander; France, Kevin +7 more

The direct study of molecular gas in inner protoplanetary disks is complicated by uncertainties in the spatial distribution of the gas, the time variability of the source, and the comparison of observations across a wide range of wavelengths. Some of these challenges can be mitigated with far-ultraviolet spectroscopy. Using new observations obtain…

2012 The Astrophysical Journal
eHST 20