Boehnhardt, H.; The Philae Mission Team: Philae Lander Mission and Science Overview. Cometary science after Rosetta - The Royal Astronomical Society Discussion Meeting, London, U.K. (2016)
Boehnhardt, H.; Böhringer, H.; Genzel, R.; Kirtsin, T.; Völk, H.: Astronomy and astrophysics in the MPG from the 1980s to the present - Round Table. Opening New Windows on the Cosmos: Astrophysics and astronomy in the History of the Max Planck Society, Berlin, Germany (2016)
Böhnhardt, H.: Was Sie schon immer über Kometen wissen wollten, sich aber nie zu fragen trauten. Vagabunden im Weltraum - Rothenfelser Sternstunden, Burg Rothenfels, Germany (2016)
Böhnhardt, H.: Kuiper-Belt - Der asteroidengürtel am Rande des Planetensystems. Vagabunden im Weltraum - Rothenfelser Sternstunden, Burg Rothenfels, Germany (2016)
Böhnhardt, H.: Philae Achievements:Landing on a Comet - The Science View. Philae - From Dreams to Achievements - an International Conference, Budapest, Hungary (2016)
Böhnhardt, H.: Rosetta, die Weltraummission der ESA - Zweiter Teil. ahrestreffen der Internationalen Amateursternwarte e.V., Bad Soden - Salmünster, Germany (2016)
Böhnhardt, H.: Planetary science with Rosetta at comet 67P/Churyumov-Gerasimenko. Physikalisches Kolloquium der Friedrich-Alexander Universität, Erlangen, Germany (2016)
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, ...