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)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).