Davidsson, B.; Stern, S. A.; Kofman, W.; Hilchenbach, M.; Rotundi, A.; Bentley, M.; Hofstadter, M.; Sierks, H.; Altwegg, K.; Nilsson, H.et al.; Burch, J. L.; Eriksson, A. I.; Glassmeier, K.-H.; Henri, P.; Carr, C. M.; Pätzold, M.; Capaccioni, F.; Boehnhardt, H.; Bibring, J.-P.; Fulle, M.; Fulchignoni, M.; Gruen, E.; Weissman, P. R.; Taylor, M.; Buratti, B. J.; Choukroun, M.; Altobelli, N.; Snodgrass, C.: The Rosetta mission: Clues on the origin of comet nuclei. DPS meeting #48, Pasadena, USA (2016)
Huybrighs, H.; Futaana, Y.; Barabash, S.; Wieser, M.; Wurz, P.; Krupp, N.; Glassmeier, K.-H.; Vermeersen, B.: Feasibility study of in-situ measurements of Europas neutral and plasma plumes with JUICE/PEP. European Geosciences Union General Assembly, Vienna, Austria (2016)
Huybrighs, H.; Futaana, Y.; Barabash, S.; Wieser, M.; Wurz, P.; Krupp, N.; Roussos, E.; Fränz, M.; Glassmeier, K.-H.; Vermeersen, B.: Feasibility study of the in-situ detectability of Europa's neutral and plasma plumes from a flyby mission. Europa-Enceladus Plumes Workshop, Pasadene, Caltech, USA (2016)
Auster, H.-U.; Heinisch, P.; Apathy, I.; Berghofer, G.; Fornacon, K.-H.; Hilchenbach, M.; Koenders, C.; Remizov, A.; Richter, I.; Glassmeier, K.-H.: ROMAP Magnetic Field Measurements in the Surface Boundary Layer of the Nucleus of 67P/Churyumov-Gerasimenko. European Geosciences Union General Assembly, Vienna, Austria (2015)
Huybrighs, H.; Roussos, E.; Krupp, N.; Fränz, M.; Futaana, Y.; Barabash, S.; Glassmeier, K.-H.: The search for Europa plume signatures in Galileo plasma particle data. Magnetospheres of the Outer planets conference (MOP), Uppsala, Sweden (2017)
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".