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Tubiana, C.; Böhnhardt, H.; Agarwal, J.; Drahus, M.; Barrera, L.; Ortiz, J. L.: 67P/Churyumov-Gerasimenko at large heliocentric distance. Astronomy and Astrophysics 527, A113 (2011)
Kelly, M. S.; Wooden, D. H.; Tubiana, C.; Boehnhardt, H.; Woodward, C. E.; Harker, D. E.: Spitzer Observations of Comet 67P/Churyumov-Gerasimenko at 5.5-4.3AU from the Sun. Astronomical Journal 137, pp. 4633 - 4642 (2009)
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)
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)
Tubiana, C.: The dust environment of 67P/Churyumov-Gerasimenko: a multi-instrument perspective. Rosetta Science workshop and SWT 49, Rhodos, Greece (2018)
Tubiana, C.: The Rosetta comet 67P/Churyumov-Gerasimenko through the eyes of OSIRIS: Major results and expectations for the exploration of a Main Belt Comet. International Symposium on Lunar & Planetary Science, Macau (2018)
Hofmann, M.; Güttler, C.; Vincent, J.-B.; Deshapriya, J. D. P.; Pajola, M.; Tubiana, C.; Feller, C.; Barucci, M. A.; Sierks, H.; The OSIRIS Team: Material strength on 67P/Churyumov-Gerasimenko and its influence on cliff stability. European Geosciences Union General Assembly, Vienna, Austria (2017)
Tubiana, C.: Characterization of the physical properties of the ROSETTA target comet 67P/Churyumov-Gerasimenko. Diploma, Technische Universität Braunschweig (2008)
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, ...