Klostermeyer, J.: On the role of parametric instability of internal gravity waves in atmospheric radar observations. Radio Science 25, pp. 983 - 995 (1990)
Rüster, R.; Klostermeyer, J.: Propagation of turbulence structures detected by VHF radar. Journal of Atmospheric and Terrestrial Physics 49, pp. 743 - 750 (1987)
Rüster, R.; Klostermeyer, J.: SOUSY-VHF-Radar: Untersuchung atmosphärischer Bewegungsvorgänge zwischen 2 und 90 km. Kleinheubacher Berichte 30, p. 53 (1987)
Klostermeyer, J.; Rüster, R.: VHF radar observation of wave instability and turbulence in the mesosphere. Advances in Space Research 4 (4), pp. 79 - 82 (1984)
Klostermeyer, J.: Parametric Instabilities of Internal Gravity Waves in Boussinesq Fluids with Large Reynolds Numbers. Geophys. Astrophys. Fluid Dyn. 26, pp. 85 - 105 (1983)
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".