Faber, C.; Knapmeyer, M.; Roll, R.; Chares, B.; Schroeder, S.; Witte, L.; Seidensticker, K. J.; Fischer, H.-H.; Moehlmann, D.; Arnold, W.: A method for inverting the touchdown shock of the Philae lander on comet 67P/Churyumov-Gerasimenko. Planetary and Space Science 106, pp. 46 - 55 (2015)
Goesmann, F.; Raulin, F.; Bredehoeft, J. H.; Cabane, M.; Ehrenfreund, P.; MacDermott, A. J.; McKenna-Lawlor, S.; Meierhenrich, U. J.; Munoz Caro, G. M.; Szopa, C.et al.; Sternberg, R.; Roll, R.; Thiemann, W. H.-P.; Ulamec, S.: COSAC prepares for sampling and in situ analysis of cometary matter from comet 67P/Churyumov-Gerasimenko. Planetary and Space Science 103, pp. 318 - 330 (2014)
Goesmann, F.; McKenna-Lawlor, S.; Roll, R.; Bredehöft, J. H.; Meierhenrich, U.; Raulin, F.; Thiemann, W.; Caro, G. M. M.; Szopa, C.: Interpretation of COSAC mass spectrometer data acquired during Rosettas Lutetia fly-by 10 July 2010. Planetary and Space Science 66, pp. 187 - 191 (2012)
Meierhenrich, U. J.; Thiemann, W.; Goesmann, F.; Roll, R.; Rosenbauer, H.: Enantioselective amino acid analysis in cometary matter planned for the COSAC instrument onboard ROSETTA lander. International Journal of Astrobiology 1, p. 255 (2002)
Szopa, C.; Meierhenrich, U. J.; Coscia, D.; Janin, L.; Goesmann, F.; Sternberg, A.; Brun, J. F.; Israel, G.; Cabane, M.; Roll, R.et al.; Raulin, F.; Thiemann, W.; Vidal-Madjar, C.; Rosenbauer, H.: Gas chromatography for in situ analysis of a cometary nucleus - IV. Study of capillary column robustness for space application. J. Chromatogr. A 982 (2), pp. 303 - 312 (2002)
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, ...