Krüger, H.; Strub, P.; Grün, E.: Ulysses spacecraft data revisited: Detection of cometary meteoroid streams by following in situ dust impacts. European Planetary Science Congress 2021, Online (2021)
Krüger, H.: Philae landing on comet 67P/Churyumov-Gerasimenko and the compressive strength and elastic modulus at the Agilkia landing site derived from SESAME/CASSE touchdown signals. Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan (2020)
Krüger, H.; Strub, P.; Srama, R.; Kobayashi, M.; Kimura, H.; Arai, T.; Altobelli, N.; Sterken, V.; Agarwal, J.; Sommer, M.et al.; Grün, E.: Dust Modelling for the Destiny+ Cruise Phase to (3200) Phaethon. ESA Topical Team Meeting for the Deep Space Gateway
, Canterbury, U.K. (2019)
Krüger, H.: Interstellar and Interplanetary Dust Modelling for the Destiny+ Mission to (3200) Phaethon. Chiba Institute of Technology, Narashino/Chiba, Japan (2019)
Krüger, H.: Galileo, Ulysses, Cassini In-Situ Dust Measurements. International Workshop ''Cosmic Lab" at Chiba Institute of Technology, Narashino/Chiba, Japan (2019)
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, ...