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)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.