Glassmeier, K.-H.; Boehnhardt, H.; Koschny, D.; Kuehrt, E.; Richter, I.: The Rosetta Mission: Flying Towards the Origin of the Solar System. In: Rosetta-ESA's Mission to the Origin of the Solar System, pp. 1 - 20 (Eds. Schulz, R.; Alexander, C.; Boehnhardt, H.; Glassmeier, K.-H.). Springer Press, Heidelberg (2009)
Barucci, M. A.; Boehnhardt, H.; Cruikshank, D. P.; Morbidelli, A.: The Solar System Beyond Neptune: Overview and Perspectives. In: The Solar System Beyond Neptune (Eds. Barucci, M. A.; Boehnhardt, H.; Cruikshank, D. P.; Morbidelli, A.). The University of Arizona Press, Tucson, USA (2008)
Doressoundiram, A.; Boehnhardt, H.; Tegler, S. C.; Trujillo, C.: Color Properties and Trends of the Transneptunian Objects. In: The Solar System Beyond Neptune (Eds. Barucci, M. A.; Boehnhardt, H.; Cruikshank, D. P.; Morbidelli, A.). The University of Arizona Press, Tucson, USA (2008)
Boehnhardt, H.; Ageorges, N.; Bagnulo, S.; Barrera, L.; Bonev, T.; Hainaut, O.; Jehin, E.; Käufl, H. U.; Kerber, F.; Locurto, G.et al.; Manfroid, J.; Marco, O.; Pantin, E.; Pompei, E.; Rauer, H.; Saviane, I.; Selman, F.; Sterken, C.; Tozzi, G. P.; Weiler, M.: The Dusty View of DI from ESO Chile. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 147 - 154 (Eds. Kaeufl, H. U.; Sterken, C.). Springer Press, Berlin Heidelberg (2009)
Käufl, H. U.; Saviane, I.; Ivanov, V.; Bonev, T.; Boehnhardt, H.: Serendipitous Occultation of U0975-07195164 by 9P/Tempel 1 Witnessed from LaSilla. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 185 - 187 (Eds. Kaeufl, H. U.; Sterken, C.). Springer Press, Berlin Heidelberg (2009)
Agarwal, J.; Mueller, M.; Boehnhardt, H.; Gruen, E.: Imaging the Dust Trail and Neckline of 67P/Churyumov-Gerasimenko. In: Workshop on Dust in Planetary Systems, 26-30 Sept. 2005, Kauai, Hawaii (Ed. Wilson, A.). (2007)
Masoumzadeh, N.; Böhnhardt, H.; Vilenius, E.; Lara, L. M.: Photometry and radiometric modeling of Transneptunian objects in support of the Herschel key program 'TNOs are Cool'. EPSC-DPS Joint Meeting, Geneva, Switzerland (2019)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".