Cavalié, T.; Billebaud, F.; Dobrijevic, M.; Fouchet, T.; Lellouch, E.; Encrenaz, T.; Brillet, J.; Moriarty-Schieven, G. H.; Wouterloot, J. G. A.; Hartogh, P.: First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT. New constraints on its origin. Icarus 203, pp. 531 - 540 (2009)
Cavalié, T.; Moreno, R.; Lellouch, E.; Hartogh, P.; Jarchow, C.; Venot, O.; Hersant, F.; Selsis, F.; Orton, G.; Encrenaz, T.et al.; Fletcher, L.: First submillimeter observation of CO in the stratosphere of Uranus with Herschel-HIFI. European Planetary Science Congress, London, UK (2015)
Cavalié, T.; Hue, V.; Hartogh, P.; Lellouch, E.; Cassidy, T.; Dobrijevic, M.; Jarchow, C.; Moreno, R.: Is Enceladus Saturn's source of water? European Planetary Science Congress , Cascais, Portugal (2014)
Cavalié, T.; Venot, O.; Selsis, F.; Hersant, F.; Hartogh, P.: The Deep O/H Ratio in Uranus and Neptune from CO Spectroscopy and Thermochemical Modeling. Workshop on the Study of the Ice Giant Planets, Laurel, Maryland, USA (2014)
Orton, G.; Fletcher, L. N.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Encrenaz, T.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Cavalié, T.et al.; Moses, J.; Burgdorf, M.; Hammel, H.; Line, M.; Mainzer, A. K.; Hofstadter, M.; Sandell, G. H.; Dowell, C. D.; Pantin, E.; Fujiyoshi, T.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. American Astronomical Society, DPS meeting #46, Tucson, AZ, USA (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New Determination of the HCN Profile in the Stratosphere of Neptune from Millimeter-wave Spectroscopy. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
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".