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)
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)
Stenzel, O. J.; Hilchenbach, M.: Towards machine learning assisted error identification in orbital laser altimetry for tides derivation. Europlanet Science Congress 2021, Online (2021)
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)
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".