Krüger, H.: Rosetta - Rendezvous mit einem Kometen. Vortragsreihe "Raumfahrt aus Leidenschaft'' an der Universität Stuttgart, Institut für Raumfahrtsysteme, Stuttgart (2014)
Krüger, H.; The SESAME Team: Grain Properties at the Nucleus of Comet 67P/C-G. 37th Rosetta Science Working Team Meeting, Villafranca del Castillo, Spain (2014)
Krüger, H.; Altobelli, N.; Strub, P.; Sterken, V.; Srama, R.; Grün, E.: Interstellar Dust in the Solar System: Model versus In-Situ Spacecraft Data. European Geophysical Union General Assembly, Vienna, Austria (2019)
Boehnhardt, H.; Krueger, H.; Mall, U.: Assessing the Primordial Character of Comets and of 67P/Churyumov-Gerasimenko. 50th ESLAB Symposium 2016, Leiden, Netherlands (2016)
Jockers, K.; Boehnhardt, H.; Krueger, H.; Mall, U.: Assessing the Primordial Character of Comets and of 67P/Churyumov-Gerasimenko. COMETS 2016, 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".