Chifu, I.; Wiegelmann, T.; Inhester, B.: Coronal magnetic field modeling using stereoscopic constraints. 15th European Solar Physics Meeting, Budapest, Hungary (2017)
Wiegelmann, T.: 3D-Coronal magnetic fields. Theoretical and observational approaches to the solar magnetic field: Achievements and remaining problems - conference in honor of Prof. Takashi Sakurai's career -, Tokyo, Japan (2016)
Wiegelmann, T.: The Magnetic Field of the Sun. AG 2016, Splinter meeting: The Role and Interaction of Stellar Magnetic Fields: From the Stellar Surface to the Interstellar Medium, Bochum, Germany (2016)
Wiegelmann, T.: Coronal modelling for Solar Orbiter. 16th Solar Orbiter SWT Meeting Numerical modeling support for Solar Orbiter (special MADAWG session), Göttingen, Germany (2015)
Wiegelmann, T.: Solar magnetic activity and space weather. Workshop and Research visit on: The synergy of magnetic reconnection and waves in evolution of the solar corona, Weihai, China (2015)
Wiegelmann, T.: Solar coronal magnetic fields: Source region for space weather activity. 4. Nationaler Weltraumwetterworkshop, Neustrelitz, Germany (2015)
Wiegelmann, T.; The Sunrise Team: Selfconsistent magnetostatic modelling of the solar atmosphere from Sunrise/IMAX measurements. AG Annual Meeting 2014, Bamberg, Germany (2014)
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).