Jockers, K.: Astronomical observations of comets and the Io torus using Fabry-Perot-Interferometry. In: Tridimensional Optical Spectroscopic Methods in Astrophysics, IAU Colloquium 149, A. S. P. Conf. Ser. Vol. 71, pp. 182 - 187 (Eds. Comte, G.; Marcelin, M.). Astron. Soc. Pacific, San Francisco (1995)
Schleicher, H.; Balthasar, H.; Jockers, K.; Knölker, M.; Schmidt, W.: Observation at 892 nm of impact L with the solar vacuum tower telescope at Tenerife. In: Proc. Eur. SL-9/Jupiter Workshop, pp. 171 - 174 (Eds. West, R.; Böhnhardt, H.). European Southern Observatory, Garching (1995)
Jockers, K.: Solomon Borisovich Pikel’ner, how I remember him 55 years after his untimely death. Ideas of S. B. Pikel’ner and S.A. Kaplan and contemporary astrophysics, a conference on occasion of the hundredth birthday of S.B. Pikel’ner (1921-1975) and S.A. Kaplan (1921 – 1978), Moscow, Russia (2021)
Jockers, K.: The early evolution of our solar system and of nascent planetary systems: hints for the origin of comets? Comet Workshop 2017: Comet formation paradigm after Rosetta. What is the hallmark of cometary nuclei formation in protoplanetary discs inherited from Rosetta? , Sofia, Bulgaria (2017)
Jockers, K.: Observations of scattered light from cometary dust and their interpretation. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1998)
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".