Crovisier, J.; Brooke, T. Y.; Hanner, M. S.; Keller, H. U.; Lamy, P. L.; Altieri, B.; Bockelée-Morvan, D.; Jorda, L.; Leech, K.; Lellouch, E.: The infrared spectrum of comet C/1995 O1 (Hale-Bopp) at 4.6 AU from the Sun. Astronomy and Astrophysics 315, pp. L385 - L388 (1996)
Thomas, N.; Jorda, L.; Sicardy, B.: CCD imaging of Jupiter during the comet Shoemaker-Levy 9 impact using the Danish 1.54-m telescope at ESO. The ESO Messenger 77, pp. 42 - 44 (1994)
Thomas, N.; Eggers, S.; Ip, W.-H.; Lichtenberg, G.; Fitzsimmons, A.; Jorda, L.; Keller, H. U.; Williams, I. P.; Hahn, G.; Rauer, H.: Detection of thermal emission from 1993 SC - First results, Proceedings of the workshop. In: On Minor Bodies of Outer Solar System, pp. 25 - 31 (Eds. Fitzsimmons, A.; Jewitt, D.; West, R. M.). SpringerVerlag, Heidelberg (2000)
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.