Thompson, W.; Schühle, U.; Young, P.: Calibrating Optical Distortions In The Solar Orbiter Spice Spectrograph. 238th Meeting of the American Astronomical Society, Solar Physics Division, Online (2021)
Horbury, T. S.; Auchere, F.; Antonucci, E.; Berghmans, D.; Bruno, R.; Carlsson, M.; del Toro Iniesta, J. C.; Fludra, A.; Harra, L.; Hassler, D.et al.; Heinzel, P.; Howard, R. A.; Krucker, S.; Livi, S. A.; Long, D.; Louarn, P.; Maksimovic, M.; Mueller, D.; Owen, C. J.; Peter, H.; Rochus, P. L.; Rodriguez-Pacheco, J.; Romoli, M.; Schühle, U.; Solanki, S. K.; Teriaca, L.; Wimmer-Schweingruber, R. F.; Zouganelis, Y.; Laker, R.: Solar Orbiter: connecting remote sensing and in situ measurements. AGU Fall Meeting, Online (2020)
Peter, H.; Aznar Cuadrado, R.; Schühle, U.; Teriaca, L.; Auchere, F.; Carlsson, M.; Fludra, A.; Hassler, D.; Buchlin, E.; Caminade, S.et al.; Caldwell, M.; DeForest, C.; Fredvik, T.; Harra, L. K.; Janvier, M.; Kucera, T. A.; Giunta, A. S.; Grundy, T.; Müller, D.; Parenti, S.; Schmutz, W. K.; Sidher, S.; Thompson, W. T.; Williams, D.; Young, P. R.: Dynamics and thermal structure in the quiet Sun seen by SPICE. AGU Fall Meeting, Online (2020)
Fiedler, T.; Teriaca, L.; Perske, M.; Pauer, H.; Naujok, P.; Schühle, U.; Feigl, T.: Broad Band EUV/VUV Multilayer Coatings from 16.9 to 130 nm for a Solar Spectrograph Space Mission. Physics of X-Ray and Neutron Multilayer Structures, Palaiseau, France (2018)
Gabrielli, A.; Castronuovo, M. M.; Cesare, S.; Morea, D.; Montabone, M.; Teriacam, L.; Schühle, U.; Barthol, P.; Solanki, S.: METIS Coronagraph A System Engineering Approach. 66th International Astronautical Congress, Jerusalem, Israel (2015)
Halain, J.-P.; Rochus, P.; Renotte, E.; Hermans, A.; Jacques, L.; Auchère, F.; Berghmans, D.; Harra, L.; Schühle, U.; Schmutz, W.et al.; Zhukov, A.; Cuadrado, R. A.; Delmotte, F.; Dumesnil, C.; Gyo, M.; Kennedy, T.; Smith, P.; Tandy, J.; Mercier, R.; Verbeeck, C.: The Extreme UV Imager telescope on-board the Solar Orbiter mission Overview of phase C and D. Solar Physics and Space Instrumentation VI, San Diego, USA (2015)
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".
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.