Mall, U.: Der neue Mond - was wir in den letzten 10 Jahren Neues über den alten Mond gelernt haben. Bundesweite Lehrer-Fortbildung zur Astronomie, Heidelberg,Germany (2015)
Bučík, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R.: Long-lasting 3He-rich solar energetic particle sources. STEREO SEP meeting, Laurel, Maryland, USA (2014)
Bickel, V. T.; Manconi, A.; Loew, S.; Mall, U.: Entering Schrödinger’s Pyroclastic Vent and PSR: A Trafficability Analysis for the next Generation of Lunar Exploration Rovers. EGU General Assembly 2019, Vienna, Austria (2019)
Mall, U.; Kloskowski, D.; Schmidt, H.; Bickel, V. T.; Basilevsky, A.; Bugiolacchi, R.: On the variability of lunar soil properties – bearing capacity. EGU General Assembly 2019, Vienna, Austria (2019)
Bickel, V. T.; Lanaras, C.; Manconi, A.; Loew, S.; Mall, U.: Automated Detection and Mapping of lunar Rockfalls using a CNN. 1st Swiss “Workshop on Machine Learning for Environmental and Geosciences” (MLEG2019), Dübendorf, Switzerland (2019)
Bickel, V. T.; Lanaras, C.; Manconi, A.; Loew, S.; Mall, U.: Automated detection of lunar rockfalls using a Convolutional Neural Network. AGU Fall Meeting, Washington, D.C., USA (2018)
Bickel, V. T.; Manconi, A.; Loew, S.; Mall, U.: Automatic Detection of Rockfalls with Deep Neural Networks: Lessons learned on the Moon and Mars. ESA Living Planet Symposium, Milan, Italy (2018)
Mall, U.; Schmidt , H.; Kloskowski, D.; Bickel, V. T.; Bugiolacchi, R.: Lunar Rock Boulders as a Tool in comparative Planetology to investigate Rock Weathering. 7th European Lunar Symposium , Manchester, U.K. (2018)
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 dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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).