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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...