Langevin, Y.; Merouane, S.; Hilchenbach, M.; Vincendon, M.; Hornung, K.; Engrand, C.; Schulz, R.; Kissel, J.; Ryno, J.: Optical properties of cometary particles collected by COSIMA: Assessing the differences between microscopic and macroscopic scales. Planetary and Space Science 182, 104815 (2020)
Paquette, J.; Engrand, C.; Hilchenbach, M.; Fray, N.; Stenzel, O. J.; Silen, J.; Rynö, J.; Kissel, J.; the COSIMA Team: The oxygen isotopic composition (18O/16O) in the dust of comet 67P/Churyumov-Gerasimenko measured by COSIMA on-board Rosetta. Monthly Notices of the Royal Astronomical Society 477 (3), pp. 3836 - 3844 (2018)
Paquette, J.; Engrand, C.; Stenzel, O. J.; Hilchenbach, M.; Kissel, J.; the COSIMA Team: Errata: Searching for calcium‐aluminum‐rich inclusions in cometary particles with Rosetta/COSIMA. Meteoritics and Planetary Science 53 (3), pp. 549 - 550 (2018)
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Paquette, J.; Hornung, K.; Stenzel, O. J.; Rynö, J.; Silen, J.; Kissel, J.; Hilchenbach, M.; The COSIMA Team: The 34S/32S Isotopic Ratio Measured in the Dust of Comet 67P/Churyumov-Gerasimenko by Rosetta/COSIMA. Mon. Not. Roy. Astron. Soc. 469, pp. S230 - S237 (2017)
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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, ...