Schühle, U.: Design and Space Qualification of a Telescope Mirror for Solar Orbiter SPICE. Seminar Rutherford Appleton Laboratories, Chilton, UK (2014)
Aznar Cuadrado, R.; Berghmans, D.; Teriaca, L.; Gissot, S.; Schühle, U.; Auchere, F.; Harra, L.; Long, D.; Rochus, P. L.; Heerlein, K.et al.; Kraaikamp, E.; Smith, P.; Stegen, K.; Verbeeck, C.: Very high-resolution observations of the solar atmosphere in H I Lyman alpha and Fe IX-X at 17.4 nm as seen by EUI aboard Solar Orbiter. AGU Fall Meeting, Online (2020)
Buchlin, E.; Teriaca, L.; Giunta, A. S.; Grundy, T.; Andretta, V.; Auchere, F.; Peter, H.; Berghmans, D.; Carlsson, M.; Fludra, A.et al.; Harra, L.; Hassler, D.; Long, D.; Rochus, P. L.; Schühle, U.; Aznar Cuadrado, R.; Caldwell, M.; Caminade, S.; DeForest, C.; Fredvik, T.; Gissot, S.; Heerlein, K.; Janvier, M.; Kraaikamp, E.; Kucera, T. A.; Müller, D.; Parenti, S.; Schmutz, W. K.; Sidher, S.; Smith, P.; Stegen, K.; Thompson, W. T.; Verbeeck, C.; Williams, D.; Young, P. R.: First results from the EUI and SPICE observations of Alpha Leo near Solar Orbiter first perihelion. AGU Fall Meeting, Online (2020)
Frassetto, F.; Deppo, V. D.; Zuppella, P.; Romoli, M.; Fineschi, S.; Antonucci, E.; Nicolini, G.; Naletto, G.; Nicolosi, P.; Spadaro, D.et al.; Andretta, V.; Castronuovo, M.; Casti, M.; Capobianco, G.; Massone, G.; Susino, R.; Landini, F.; Pancrazzi, M.; Teriaca, L.; Schühle, U.; Heerlein, K.; Uslenghi, M.: Optical performance of the Metis coronagraph on the Solar Orbiter ESA mission. International Conference on Space Optics - ICSO 2018 , Chania, Greece (2018)
Ramanath, S.; Schühle, U.: Efficiency of Bakeout Methods for Space Materials. International Symposium on Materials in the Space Environment (ISMSE) and the 12th International Conference on Protection of Materials from Space Environment (ICPMSE), Biarritz, France (2018)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
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.