Paquette, J.; Fray, N.; Cottin, H.; Engrand, C.; Bardyn, A.; Stenzel, O. J.; Merouane, S.; Hilchenbach, M.; Alexander, C.M.O.; Langevin, Y.: The D/H ratio in cometary dust measured by Rosetta/COSIMA. 49th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2018)
Nuth, J. A.; Johnson, N. M.; Ferguson, F. T.; Hilchenbach, M.; Merouane, S.; Paquette, J. A.; Stenzel, O.; Cottin, H.; Fray, N.; Bardyn, A.et al.; Baklouti, D.; Le Roy, L.: Refractory Organics in Comet 67P/Churyumov-Gerasimenko: Additional Evidence for Large-Scale Mixing in the Primitive Solar Nebula? 48th Lunar and Planetary Science Conference, The Woodlands, Texas (2017)
Paquette, J. A.; Fray, N.; Cottin, H.; Bardyn, A.; Hilchenbach, M.: The 18O/16O Ratio in Cometary Dust and Other New Results from Cosima. 48th Lunar and Planetary Science Conference, The Woodlands, Texas (2017)
Bardyn, A.; Baklouti, D.; Briois, C.; Cottin, H.; Fray, N.; Engrand, C.; Fischer, H.; Hilchenbach, M.; Merouane, S.; Modica, P.et al.; Paquette, J.; Ryno, J.; Silén, J.; Stenzel, O.; Thirkell, L.: Cometary dust composition and its variation as seen by COSIMA over nearly two years of the Rosetta mission. Symposium Comets - A new vision after Rosetta and Philae, Toulouse, France (2016)
Fray, N.; Baklouti, D.; Bardyn, A.; Brois, C.; Cottin, H.; Engrand, C.; Fischer, H.; Hilchenbach, M.; Roy, L. L.; Modica, P.et al.; Paquette, J.; Ryno, J.; Stenzel, O.; Siljeström, S.; Thirkell, L.: Characterization of the refractory organic matter present in the dust particles of 67P/Churyumov-Gerasimenko. Symposium Comets - A new vision after Rosetta and Philae, Toulouse, France (2016)
Paquette, J.; Engrand, C.; Hilchenbach, M.; Fray, N.; Stenzel, O.: Oxygen Isotopes in Cometary Dust Measured in the Coma of Comate 67P/Churyumov-Gerasimenko with COSIMA Onboard Rosetta. AGU Fall Meeting, San Francisco, USA (2016)
Turbulence plays a very important role in many applications, ranging from geophysics and astrophysics to engineering. In our solar system, turbulence is often driving by thermal effect, rotation, and magnetic field. In this project you will use high-fidelity simulation tools, including direct numerical simulations, data assimilation, and machine learning, to study the physics of turbulence, focusing on convection and dynamos.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.