Le Corre, L.; Reddy, V.; Nathues, A.: Spectral Indices for Identifying Terrains on Vesta with Dawn Framing Camera Filters. Meteorit. Planet. Sci. 46, p. A135 - A135 (2011)
Le Corre, L.; Reddy, V.; Nathues, A.; Cloutis, E. A.: How to characterize terrains on 4 Vesta using Dawn Framing Camera color bands? Icarus 216 (2), pp. 376 - 386 (2011)
Reddy, V.; Nathues, A.; Gaffey, M. J.; Schaeff, S.: Mineralogical characterization of potential targets for the ASTEX mission scenario. Planetary and Space Science 59 (8), pp. 772 - 778 (2011)
Li, J.-Y.; Le Corre, L.; Reddy, V.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Ciarniello, M.; Mottola, S.; Schröder, S. E.; Raymond, C. A.et al.; Russell, C. T.: Spectrophotometric Modeling and Mapping of Ceres. European Geosciences Union General Assembly, Vienna, Austria (2016)
Li, J.-Y.; Le Corre, L.; Reddy, V.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Ciarniello, M.; Mottola, S.; Schröder, S. E.; Raymond, C. A.et al.; Russell, C. T.: Spectrophotometric Modeling and Mapping of Ceres. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Schmidt, B. E.; Hughson, K. G.; Chilton, H. T.; Scully, J. E. C.; Platz, T.; Nathues, A.; Sizemore, H.; Bland, M. T.; Byrne, S.; Marchi, S.et al.; O'Brien, D. P.; Schorghofer, N.; Hiesinger, H.; Jaumann, R.; Lawrence, J.; Buczkowski, D.; Castillo, J. C.; Schenk, P. M.; Sykes, M. V.; De Sanctis, M. C.; Mitri, G.; Formisano, M.; Li, J.-Y.; Reddy, V.; LeCorre, L.; Russell, C. T.; Raymond, C. A.; the Dawn Science and Operations Team: Ground Ice on Ceres? 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".