Christensen, U. R.: Magnetic fields a window into the deep interiors of planets. Workshop on Structure and Dynamics of the interior of rocky planets. Structure and Dynamics of Earth-like Planets, Paris, France (2014)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Gläser, P.; Stark, A.; Steinbrügge, G.; Oberst, J.: Simultaneous retrieval of the lunar solid body tide and topography from laser altimetry. AGU Fall Meeting , online (2020)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Gläser, P.; Stark, A.; Steinbrügge, G.; Oberst, J.: Simultaneous retrieval of the lunar solid body tide and topography from laser altimetry. EGU General Assembly , online (2020)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Stark, A.; Steinbrügge, G.; Ruscio, A. D.; Cappuccio, P.; Iess, L.; Hussmann, H.; Oberst, J.: Prospects for the Measurement of Mercury's Solid Body Tides with the BepiColombo Laser Altimeter. 51st Lunar and Planetary Science Conference, online (2020)
Christensen, U. R.: Deodynamo Models with a Stable Layer and Meterogeneous CMB Heat Flow. 16th Symposium of SEDI (Study of the Earth's Deep Interior), Edmonton, Canada (2018)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Oberst, J.: Retrieval of h2 from laser altimetry. Workshop in Geology and Geophysics of the Solar System, Petnica, Serbia (2018)
Thor, R. N.; Kallenbach, R.; Christensen, U. R.; Oberst, J.: Retrieving the planetary h2 tidal Love number from laser altimetry data. 1st IUGG Symposium on Planetary Science, DLR Adlershof, Berlin, Germany (2017)
Thor, R. N.; Kallenbach, R.; Christensen, U. R.; Oberst, J.: Retrieving the planetary h2 tidal Love number from laser altimetry data. Rocks \& Stars II, Göttingen, Germany (2017)
Bossmann, A. B.; Wicht, J.; Gastine, T.; Christensen, U. R.: Magnetic field morphology of the ice giants linked to their internal structure. 5th Meeting of the DFG-SPP Planetary Magnetism, Nördlingen, Germany (2015)
Christensen, U. R.: Planetary Magnetic Fields and Dynamos. In: Oxford Research Encyclopedia: Planetary Science (Ed. Oxford University Press). Oxford Univ. Press, Oxford (2019)
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).