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Basilevsky, A. T.; Keller, H. U.; Nathues, A.; Mall, U.; Hiesinger, H.; Rosiek, M.: Scientific objectives and selection of targets for the SMART-1 Infrared Spectrometer (SIR). Planetary and Space Science 52 (14), pp. 1261 - 1285 (2004)
Basilevsky, A. T.; Keller, H. U.; Nathues, A.; Mall, U.; Hiesinger, H.; Rosiekd, M.: Scientific objectives and selection of targets for the SMART-1 Infrared Spectrometer (SIR). Planetary and Space Science 52 (14), pp. 1261 - 1285 (2004)
Kaasalainen, M.; Pravec, P.; Krugly, Y. N.; Sarounova, L.; Torppa, J.; Virtanen, J.; Kaasalainen, S.; Erikson, A.; Nathues, A.; Durech, J.et al.; Wolf, M.; Lagerros, J. S. V.; Lindgren, M.; Lagerkvist, C. I.; Koff, R.; Davies, J.; Mann, R.; Kusnirak, P.; Gaftonyuk, N. M.; Shevchenko, V. G.; Chiorny, V. G.; Belskaya, I. N.: Photometry and models of eight near-Earth Asteroids. Icarus 167 (1), pp. 178 - 196 (2004)
Foing, B. H.; Racca, G. D.; Marini, A.; Heather, D. J.; Koschny, D.; Grande, M.; Huovelin, J.; Keller, H. U.; Nathues, A.; Josset, J. L.et al.; Malkki, A.; Schmidt, W.; Noci, G.; Birkl, R.; Iess, L.; Sodnik, Z.; McManamon, P.: SMART-1 mission to the moon: Technology and science goals. Advances in Space Research 31 (11), pp. 2323 - 2333 (2003)
Williams, D. A.; Nathues, A.; Nathues, A.; Scully, J. E. C.: Geomorphology of Ceres. In: Vesta and Ceres. Insights from the Dawn Mission for the Origin of the Solar System, p. 143 (2022)
Nathues, A.; Mall, U.; Keller, H. U.: Near infrared spectrometry with SIR on SMART-1. In: Proc. 4th International Conference on the Exploration and Utilisation of the Moon, ESTEC, Noordwijk, The Netherlands, 10-14 July 2000, pp. 101 - 103 (Eds. Foing, B. H.; Perry, M.). ESA Publ. Div., Noordwijk (2000)
Buczkowski, D. L.; Schenk, P. M.; Scully, J. E. C.; Otto, K.; von der Gathen, I.; Williams, D. A.; Mest, S. C.; Park, R.; Preusker, F.; Jaumann, R.et al.; Roatsch, T.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C. A.; Russell, C. T.: Linear Structures on Ceres: Morphology, Orientation, and Possible Formation Mechanisms. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Buczkowski, D.; Williams, D.; Scully, J.; Mest, S.; Crown, D.; Aileen Yingst, R.; Schenk, P.; Jaumann, R.; Roatsch, T.; Preusker, F.et al.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C.; Russell, C.: Geological Mapping of the Ac-H-9 Occator Quadrangle of Ceres from NASA Dawn Mission. European Geosciences Union General Assembly, Vienna, Austria (2016)
Buczkowski, D. L.; Williams, D. A.; Scully, J. E. C.; Mest, S. C.; Crown, D. A.; Yingst, R. A.; Schenk, P. M.; Jaumann, R.; Roatsch, T.; Preusker, F.et al.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C. A.; Russell, C. T.: Geologic Mapping of the Ac-H-9 Occator Quadrangle of Ceres from NASA's Dawn Mission. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Crown, D.; Yingst, A.; Mest, S.; Platz, T.; Sizemore, H.; Berman, D.; Williams, D.; Roatsch, T.; Preusker, F.; Nathues, A.et al.; Hoffman, M.; Schäfer, M.; Raymond, C.; Russell, C.: Geological Mapping of the Ac-H-14 Yalode Quadrangle of Ceres from NASA's Dawn Mission. European Geosciences Union General Assembly, Vienna, Austria (2016)
Crown, D. A.; Yingst, R. A.; Mest, S. C.; Platz, T.; Sizemore, H. G.; Berman, D. C.; Williams, D. A.; Roatsch, T.; Preusker, F.; Nathues, A.et al.; Hoffman, M.; Schäfer, M.; Raymond, C. A.; Russell, C. T.; the Dawn Science Team: Geologic Mapping of the Ac-H-14 Yalode Quadrangle of Ceres from NASA's Dawn Mission. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
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".