Paquette, J. A.; Engrand, C.; Stenzel, O.; Hilchenbach, M.; Kissel, J.: Searching for calcium-aluminum-rich inclusions in cometary particles with Rosetta/COSIMA. Meteoritics and Planetary Science 51 (7), pp. 1340 - 1352 (2016)
Heidrich-Messner, V.; Berger, L.; Wimmer-Schweingruver, R. F.; Wurz, P.; Bochsler, P.; Ipavich, F. M.; Paquette, J. A.; Klecker, B.: FIP effect for minor heavy solar wind ions as seen with SOHO/CELIAS/MTOF. In: Proceedings of the 14th International Solar Wind Conference (Eds. Wang, L.; Bruno, R.; Moebius, E.; Zank, G.). American Institute of Physics, Melville, NY, USA (2016)
Paquette, J.; Engrand, C.; Fray, N.; Hilchenbach, M.; Cottin, H.: Measuring The 13C/12C Ratio in the Dust of Comet 67P Using COSIMA. EPSC-DPS Joint Meeting, Geneva, Switzerland (2019)
Paquette, J.; Hilchenbach, M.; Engrand, C.; Fray, N.: The 13C/12C Ratio in the Dust of Comet 67P/Churyumov-Gerasimenko. 16th Annual Asia Oceania Geosciences Society Meeting, Singapore (2019)
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)
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".