Protopapa, S.; Boehnhardt, H.; Herbst, T.; Cruikshank, D.; Grundy, W.; Merlin, F.; Olkin, C.: Surface characterization of Pluto and Charon by L and M band spectra. Astronomy and Astrophysics 490, pp. 365 - 375 (2008)
Tubiana, C.; Barrera, L.; Drahus, M.; Boehnhardt, H.: Comet 67P/Churyumov-Gerasimenko at a large heliocentric distance. Astronomy and Astrophysics 490, pp. 377 - 386 (2008)
Glassmeier, K.-H.; Boehnhardt, H.; Koschny, D.; Kuehrt, E.; Richter, I.: The Rosetta Mission: Flying Towards the Origin of the Solar System. Space Science Reviews 128, pp. 1 - 21 (2007)
Lara, L. M.; Boehnhardt, H.; Gredel, R.; Gutierrez, P. J.; Rodrigo, R.; Vidal-Nunez, M. J.: Behavior of Comet 9P/Tempel 1 around the Deep Impact event. Astronomy and Astrophysics 465, pp. 1061 - 1067 (2007)
Tubiana, C.; Duffard, R.; Barrera, L.; Boehnhardt, H.: Photometric and spectroscopic observations of (132524) 2002 JF56: fly-by target of the New Horizons mission. Astronomy and Astrophysics 463, pp. 1197 - 1199 (2007)
Agarwal, J.; Müller, M.; Boehnhardt, H.; Grün, E.: Modelling the large particle environment of comet 67P/Churyumov-Gerasimenko. Advances in Space Research 38, pp. 2049 - 2053 (2006)
Delsanti, A.; Peixinho, N.; Boehnhardt, H.; Barucci, A.; Merlin, F.; Doressoundiram, A.; Davies, J. K.: Near-infrared color properties of Kuiper Belt objects and Centaurs: Final results from the ESO Large Program. Astronomical Journal 131, pp. 1851 - 1863 (2006)
Doressoundiram, A.; Barucci, M. A.; Tozzi, G. P.; Poulet, F.; Boehnhardt, H.; de Bergh, C.; Peixinho, N.: Spectral characteristics and modeling of the Transneptunian object (55565) 2002 AW197 and the Centaurs (55576) 2002 GB10 and (83982) 2002 GO9: ESO Large Program on TNOs and Centaurs. Planetary and Space Science 53, pp. 1501 - 1509 (2005)
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, ...