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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.