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Witte, M.; Banaszkiewicz, M.; Rosenbauer, H.; McMullin, D.: Kinetic parameters of interstellar neutral helium: updated results from the ULYSSES/GAS-instrument. Advances in Space Research 34, pp. 61 - 65 (2004)
Szopa, C.; Sternberg, R.; Raulin, F.; Rosenbauer, H.: What can we expect from the in situ chemical investigation of a cometary nucleus by gas chromatography: First results from laboratory studies. Planetary and Space Science 51 (13), pp. 863 - 877 (2003)
Witte, M.; Banaszkiewicz, M.; Rosenbauer, H.; McMullin, D.: Improved determination of the ionization rates acting on the interstellar He-atoms observed by the ULYSSES/GAS instrument. Geophysical Research Abstracts 5, p. 31-1-2003 (2003)
Biele, J.; Ulamec, S.; Feuerbacher, B.; Rosenbauer, H.; Mugnuolo, R.; Moura, D.; Bibring, J. P.: Current status and scientific capabilities of the ROSETTA Lander payload. Advances in Space Research 29 (8), pp. 1199 - 1208 (2002)
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)
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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, ...