Schrinner, M.; Rädler, K.-H.; Schmitt, D.; Rheinhardt, M.; Christensen, U.: Mean-field view on magnetoconvection and dynamo models. In: Proceedings of the Joint 15th Riga and 6th pamir International Conference, pp. 85 - 88. (2005)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Stark, A.; Steinbrügge, G.; Di Ruscio, A.; Cappuccio, P.; Iess, L.; Hussmann, H.; Oberst, J.: Expected retrieval accuracy of the Love number h2 from the BepiColombo Laser Altimeter (BELA). 19th BepiColombo Science Working Team Meeting , Noordwijk, Netherlands (2019)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Gläser, P.; Stark, A.; Steinbrügge, G.; Oberst, J.: Combined retrieval of the lunar body tide and a global topographic grid from LOLA data. European Planetary Science Congress, Berlin, Germany (2018)
Thor, R.; Kallenbach, R.; Gläser, P.; Christensen, U. R.; Oberst, J.; Stark, A.; Steinbrügge, G.: Simultaneous retrieval of the h2 tidal Love number and the global shape of the Moon from laser altimetry. Asia Oceania Geosciences Society (AOGS) 15th Annual Meeting , Honolulu, Hawaii (2018)
Thor, R.; Kallenbach, R.; Christensen, U. R.; Oberst, J.: Algorithm for the retrieval of h2 from laser altimetry. BepiColombo SWT meeting, Braunschweig, Germany (2018)
Thor, R. N.; Kallenbach, R.; Christensen, U. R.; Oberst, J.; Stark, A.; Steinbrügge, G.: Improved algorithms for the retrieval of the h2 Love number of Mercury from laser altimetry data. European Geosciences Union General Assembly, Vienna, Austria (2017)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".