Paquette, J.: The Oxygen Isotopic Ratio in Cometary Dust with Rostetta/COSIMA. 50th ESLAB Symposium: From Giotto to Rosetta, Leiden, Netherlands (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)
Heidrich-Meisner, V.; Bergner, L.; Wimmer-Schweingruber, R.; Wurz, P.; Bochsler, P.; Ipavich, F.; Gloeckler, G.; Klecker, B.; Paquette, J.: Minor Ion Species in the Solar Wind as Seen with SOHO/Celias/MTOF. American Geophysical Union Fall Meeting, San Francisco, USA (2014)
Paquette, J. A.: A Method of Identifying Additional Mass Peaks Using COSIMA Data. 77th Annual Meeting of the Meteoritical Society, Casablanca, Morocco (2014)
Paquette, J.; Engrand, C.; Fray, N.; Bardyn, A.; Alexander, C.; Hilchenbach, M.; Siljeström, S.; Cottin, H.; Baklouti, D.; Stenzel, O. J.et al.; Merouane, S.; Langevin, Y.; the COSIMA Team: The D/H ratio in the dust of comet 67P/Churyumov-Gerasimenko measured by Rosetta/COSIMA. AGU Fall Meeting, Washington, D.C., USA (2018)
Merouane, S.; Hilchenbach, M.; Langevin, Y.; Stenzel, O.; Fischer, H.; Hornung, K.; Silèn, J.; Altobelli, N.; Ligier, N.; Paquette, J.et al.; Rynö, J.; Schulz, R.; Kissel, J.: The flux and size distribution of dust particles ejected from 67P/C-G before and after perihelion measured by COSIMA/Rosetta. European Geosciences Union General Assembly, Vienna, Austria (2016)
Stenzel, O. J.; Paquette, J.; the Cosima Team: Boron and Oxygen in Cometary Particles. 79th Annual Meeting of the Meteoritical Society, Berlin, Germany (2016)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".