Search Publications

Bimodal distribution of sulfuric acid aerosols in the upper haze of Venus
DOI: 10.1016/j.icarus.2013.10.013 Bibcode: 2014Icar..231...83G

Crisp, David; Zhang, Xi; Gao, Peter +2 more

Observations by the SPICAV/SOIR instruments aboard Venus Express have revealed that the upper haze (UH) of Venus, between 70 and 90 km, is variable on the order of days and that it is populated by two particle modes. We use a one-dimensional microphysics and vertical transport model based on the Community Aerosol and Radiation Model for Atmosphere…

2014 Icarus
VenusExpress 61
Methane depletion in both polar regions of Uranus inferred from HST/STIS and Keck/NIRC2 observations
DOI: 10.1016/j.icarus.2014.05.016 Bibcode: 2014Icar..238..137S

Sromovsky, L. A.; Fry, P. M.; Karkoschka, E. +3 more

From Space Telescope Imaging Spectrograph (STIS) observations of Uranus in 2012, when good views of its north polar regions were available, we found that the methane volume mixing ratio declined from about 4% at low latitudes to about 2% at 60-80°N. This depletion in the north polar region of Uranus in 2012 is similar in magnitude and depth to tha…

2014 Icarus
eHST 60
Plasma environment of a weak comet - Predictions for Comet 67P/Churyumov-Gerasimenko from multifluid-MHD and Hybrid models
DOI: 10.1016/j.icarus.2014.07.021 Bibcode: 2014Icar..242...38R

Altwegg, K.; Glassmeier, K. -H.; Richter, I. +8 more

The interaction of a comet with the solar wind undergoes various stages as the comet's activity varies along its orbit. For a comet like 67P/Churyumov-Gerasimenko, the target comet of ESA's Rosetta mission, the various features include the formation of a Mach cone, the bow shock, and close to perihelion even a diamagnetic cavity. There are differe…

2014 Icarus
Rosetta 59
Mineral abundances at the final four curiosity study sites and implications for their formation
DOI: 10.1016/j.icarus.2013.11.023 Bibcode: 2014Icar..231...65P

Poulet, F.; Bishop, J. L.; Carter, J. +2 more

A component of the landing site selection process for the Mars Science Laboratory (MSL) involved the presence of phyllosilicates as the main astrobiological targets. Gale crater was selected as the MSL landing site from among 4 down selected study sites (Gale, Eberswalde and Holden craters, Mawrth Vallis) that addressed the primary scientific goal…

2014 Icarus
MEx 58
Evidence for very recent melt-water and debris flow activity in gullies in a young mid-latitude crater on Mars
DOI: 10.1016/j.icarus.2014.03.005 Bibcode: 2014Icar..235...37J

Hiesinger, H.; Hauber, E.; Johnsson, A. +2 more

Terrestrial debris flows and their deposits are mainly studied and monitored because of their hazardous nature. On Mars they may serve as geomorphologic indicators of transient liquid water. We compared the morphology of debris flow-like deposits within a young (∼0.2 Ma) mid-latitude crater on Mars with debris flow fans on Svalbard as possible ter…

2014 Icarus
MEx 57
Atmospheric thermal structure and cloud features in the southern hemisphere of Venus as retrieved from VIRTIS/VEX radiation measurements
DOI: 10.1016/j.icarus.2014.01.020 Bibcode: 2014Icar..232..232H

Kappel, D.; Arnold, G.; Haus, R.

Thermal structure and cloud features in the atmosphere of Venus are investigated using spectroscopic nightside measurements recorded by the Visible and InfraRed Thermal Imaging Spectrometer (VIRTIS) aboard ESA’s Venus Express mission in the moderate resolution infrared mapping channel (M-IR, 1-5 µm). New methodical approaches and retrieval r…

2014 Icarus
VenusExpress 57
Mid-infrared spectroscopy of Uranus from the Spitzer infrared spectrometer: 2. Determination of the mean composition of the upper troposphere and stratosphere
DOI: 10.1016/j.icarus.2014.07.012 Bibcode: 2014Icar..243..471O

Fletcher, Leigh N.; Moses, Julianne I.; Line, Michael R. +7 more

Mid-infrared spectral observations Uranus acquired with the Infrared Spectrometer (IRS) on the Spitzer Space Telescope are used to determine the abundances of C2H2, C2H6, CH3C2H, C4H2, CO2, and tentatively CH3 on Uranus at the time of the …

2014 Icarus
ISO 55
Cassini observations reveal a regime of zonostrophic macroturbulence on Jupiter
DOI: 10.1016/j.icarus.2013.08.030 Bibcode: 2014Icar..229..295G

Read, Peter L.; Young, Roland M. B.; Armstrong, David +4 more

In December 2000, the Cassini fly-by near Jupiter delivered high-resolution images of Jupiter’s clouds over the entire planet in a band between 50°N and 50°S. Three daily-averaged two-dimensional velocity snapshots extracted from these images are used to perform spectral analysis of jovian atmospheric macroturbulence. A similar analysis is also pe…

2014 Icarus
Cassini 55
Neptune at summer solstice: Zonal mean temperatures from ground-based observations, 2003-2007
DOI: 10.1016/j.icarus.2013.11.035 Bibcode: 2014Icar..231..146F

de Pater, Imke; Fletcher, Leigh N.; Irwin, Patrick G. J. +3 more

Imaging and spectroscopy of Neptune's thermal infrared emission from Keck/LWS (2003), Gemini-N/MICHELLE (2005); VLT/VISIR (2006) and Gemini-S/TReCS (2007) is used to assess seasonal changes in Neptune's zonal mean temperatures between Voyager-2 observations (1989, heliocentric longitude Ls = 236 °) and southern summer solstice (2005, L<…

2014 Icarus
AKARI ISO 53
The dayside ionospheres of Mars and Venus: Comparing a one-dimensional photochemical model with MaRS (Mars Express) and VeRa (Venus Express) observations
DOI: 10.1016/j.icarus.2014.01.028 Bibcode: 2014Icar..233...66P

González-Galindo, F.; Tellmann, Silvia; Tyler, G. Leonard +8 more

The electron density distributions of the lower ionospheres of Mars and Venus are mainly dependent on the solar X-ray and EUV flux and the solar zenith angle. The influence of an increasing solar flux is clearly seen in the increase of the observed peak electron density and total electron content (TEC) of the main ionospheric layers. The model “Io…

2014 Icarus
MEx VenusExpress 52