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Thermal observations of Saturn's main rings by Cassini CIRS: Phase, emission and solar elevation dependence
DOI: 10.1016/j.pss.2007.05.029 Bibcode: 2008P&SS...56..134A

Altobelli, Nicolas; Spilker, Linda J.; Leyrat, Cedric +1 more

Two and a half years after Saturn orbit insertion (SOI) the Cassini composite infrared spectrometer (CIRS) has acquired an extensive set of thermal measurements (including physical temperature and filling factor) of Saturn's main rings for a number of different viewing geometries, most of which are not available from Earth. Thermal mapping of both…

2008 Planetary and Space Science
Cassini 27
Venus Doppler winds at cloud tops observed with ESPaDOnS at CFHT
DOI: 10.1016/j.pss.2008.07.005 Bibcode: 2008P&SS...56.1320W

Lellouch, Emmanuel; Widemann, Thomas; Donati, Jean-François

We present new wind measurements in Venus' lower mesosphere from visible spectroscopy during the 2007 worldwide coordinated ground campaign in support of ESA's Venus Express mission. These observations consisted of high-resolution spectra of Fraunhofer lines in the entire visible range (0.37-1.05 µm) to measure the winds near 68 km using the…

2008 Planetary and Space Science
VenusExpress 27
Suprathermal electron fluxes on the nightside of Mars: ASPERA-3 observations
DOI: 10.1016/j.pss.2007.12.010 Bibcode: 2008P&SS...56..846D

Barabash, S.; Lundin, R.; Woch, J. +4 more

Recently aurora-type UV emissions were discovered on the nightside of Mars [Bertaux, J.-L., Leblanc, F., Witasse, O., et al., 2005. Discovery of an aurora on Mars. Nature 439, doi:10.1038/nature03603]. It was suggested that these emissions are produced by suprathermal electrons with energies of tens of eV, rather than by the electrons with spectra…

2008 Planetary and Space Science
MEx 27
Hemispheric distributions of HCl above and below the Venus’ clouds by ground-based 1.7 µm spectroscopy
DOI: 10.1016/j.pss.2008.05.009 Bibcode: 2008P&SS...56.1424I

Imamura, T.; Kasaba, Y.; Sagawa, H. +8 more

The abundance of hydrogen chloride (HCl) in the Venus atmosphere was measured by ground-based IR spectroscopy. The dayside measurements were performed in May 2007 with a resolution of 40,000, and the nightside measurements in October 1999 with a resolution of 1000. The hemispheric distributions of the HCl mixing ratio measured above the Venus' clo…

2008 Planetary and Space Science
VenusExpress 26
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission
DOI: 10.1016/j.pss.2007.09.011 Bibcode: 2008P&SS...56..796K

Coates, A. J.; Kallio, E.; Fedorov, A. +49 more

Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed and compared with predictions of a global model. It is shown that in the orbit studied, the plasma and magnetic field observations obtained near the North Pole under solar minimum conditions were qualitatively and, in many cases also, quantitatively…

2008 Planetary and Space Science
VenusExpress 26
New laboratory measurements of CH 4 in Titan's conditions and a reanalysis of the DISR near-surface spectra at the Huygens landing site
DOI: 10.1016/j.pss.2007.10.008 Bibcode: 2008P&SS...56..613J

Lellouch, E.; Bézard, B.; Coustenis, A. +5 more

Laboratory spectra of methane-nitrogen mixtures have been recorded in the near-infrared range (1.0-1.65 µm) in conditions similar to Titan's near surface, to facilitate the interpretation of the DISR/DLIS (DISR - Descent Imager/Spectral Radiometer) spectra taken during the last phase of the descent of the Huygens Probe, when the surface was …

2008 Planetary and Space Science
Huygens 24
Observable effects of convection and gravity waves on the Venus condensational cloud
DOI: 10.1016/j.pss.2008.02.010 Bibcode: 2008P&SS...56.1112M

Toon, Owen B.; McGouldrick, Kevin

We present results of a simple two-dimensional model investigating the observable effects that convective motions and gravity waves can have on the condensational Venus cloud. Gravity waves have been observed in the Venus atmosphere in the form of temperature scintillations in the Magellan and Pioneer Venus occultation data. Multiple in situ probe…

2008 Planetary and Space Science
VenusExpress 23
Asymmetry of plasma fluxes at Mars. ASPERA-3 observations and hybrid simulations
DOI: 10.1016/j.pss.2007.12.006 Bibcode: 2008P&SS...56..832D

Barabash, S.; Lundin, R.; Winningham, J. D. +6 more

The asymmetry of fluxes of solar wind and planetary ions is studied by using the ASPERA-3 observations onboard the Mars Express spacecraft in February 2004 to March 2006. Due to the small scale of the Martian magnetosphere and its induced origin, the flow pattern near Mars is sensitive to the directions of the interplanetary magnetic and electric …

2008 Planetary and Space Science
MEx 21
Infrared observations of Saturn's rings by Cassini CIRS : Phase angle and local time dependence
DOI: 10.1016/j.pss.2007.04.020 Bibcode: 2008P&SS...56..117L

Altobelli, Nicolas; Spilker, Linda J.; Ferrari, Cecile +2 more

Since the Saturn orbit insertion (SOI) of the Cassini spacecraft, in July 2004, the Cassini Composite Infrared Spectrometer (CIRS) has obtained a large number of thermal infrared spectra of Saturn's rings. Over the two and a half years of observations to date, ring temperatures were retrieved for a large range of unique geometries, inaccessible fr…

2008 Planetary and Space Science
Cassini 21
Titan's aerosols: Comparison between our model and DISR findings
DOI: 10.1016/j.pss.2007.11.014 Bibcode: 2008P&SS...56..708B

Bar-Nun, A.; Dimitrov, V.; Tomasko, M.

Our model [Dimitrov, V., Bar-Nun, A., 1999. A model of energy dependent agglomeration of hydrocarbon aerosol particles and implication to Titan's aerosol. J. Aerosol. Sci. 30(1), 35-49] describes the experimentally found polymerization of C 2H 2 and HCN to form aerosol embryos, their growth and adherence to form various aeros…

2008 Planetary and Space Science
Huygens 21