August saw many EuroVenusians attending the COSPAR (Committee on Space Research) Scientific Assembly in Moscow. This is an important forum for international discussion of space science and exploration.
The following list (which may not be complete!) shows presentations authored or coauthored by EuroVenus consortium members on the subjects of Venus science and exploration:
• A dynamic atmosphere revealed by the Venus Express mission
• A new view of Earth's sister: Insights following nine years of Venus Express observations
• Analysis of Venus Express optical extinction due to aerosols in the upper haze of Venus
• Analysis of Venus Express optical extinction due to aerosols in the upper haze of Venus
• CO density distribution in the lower thermosphere of Venus as a tracer of the thermospheric dynamics
• Composition of the Venus mesosphere: a synthesis of SOIR/VEX observations
• Compositional variability of the Venusian atmosphere above the clouds: sulphur dioxide and carbon monoxide
• Contribution of SPICAV/Venus Express experiment to the VIRA model update
• Contribution of the SOIR/VEX instrument to the VIRA update model
• Future Exploration of Venus: Opportunities and Challenges
• International Collaboration for Venus Exploration
• IR spectrometers for Venus and Mars measurements
• Life after Venus Express: Science goals for a European Venus radar orbiter
• Long-term Variation in Temperature and Dynamics in Venus Upper Atmosphere from ground-based Infrared Heterodyne Spectroscopy
• Minor gaseous constituents and aerosols of the Venus mesosphere measured by SPICAV/SOIR on board Venus Express
• Overview of SPICAV occultation results for the UV channel
• Particles size distribution in the upper haze of Venus from SPICAV IR data
• Progress towards a Venus reference cloud model
• Puzzles of SO2 on Venus
• Radio sounding of the solar corona with Mars Express, Venus Express and Rosetta
• Scientific Balloons for Venus Exploration
• SPICAV/SOIR on board Venus express: an overview of two years of observations.
• Stellar Occultations by Venus as Probes of Wind Speeds in the Transition Region between Retrograde and Sub-Solar-to-Anti-Solar Winds
• Sulfur dioxide observations above Venus’ clouds by means of solar occultation in the infrared
• Sulfur Dioxide variability in the Venus Atmosphere
• Temperature Structure at Venus as Observed by Venus Express (SPICAV)
• The SOIR Terminator Model: a model of the mesosphere and lower thermosphere of Venus based on observations from SOIR/VEX
• The Structure of the Venus Ionosphere
• The structure of the Venus neutral atmosphere from the Radio Science Experiment VeRa on Venus Express
• The Venus Neutral Atmosphere from the Radio Science Experiment VeRa on Venus Express
• Thermal structure of Venus night-side upper atmosphere from SPICAV/SOIR Venus Express occultations
• Thermal zonal winds in the Venus mesosphere from the Venus Express temperature soundings
• Towards a Self Consistent Model of the Thermal Structure of the Venus Atmosphere
• Venus Express atmospheric observations
• Venus' nightside upper atmospheric density measurements by SPICAV UV on Venus Express
• Venus Terminator Temperature Structure: Venus Express SOIR and VTGCM Comparisons
• Venusian upper haze properties from UV to IR wavelengths: results from SPICAV/SOIR on Venus Express
• Water abundance and hydrogen isotopic ratio in the upper atmosphere of Venus from SOIR measurements on board Venus Express
• Water vapor distribution in the Venusian mesosphere from SPICAV/SOIR observations

It can be seen that we've been busy!
Many of the abstracts of the above presentations can be downloaded from the COSPAR assembly website at www.cospar-assembly.org