Rüster, R.; Czechowsky, P.; Schmidt, G.: VHF Radar Observations of Tides at Polar Latitudes in the Summer Mesosphere. Journal of Atmospheric and Terrestrial Physics 50, pp. 1041 - 1046 (1988)
Meyer, W.; Philbrick, C. R.; Röttger, J.; Rüster, R.; Widdel, H. U.; Schmidlin, F. J.: Mean winds in the winter middle atmosphere above northern Scandinavia. Journal of Atmospheric and Terrestrial Physics 49, pp. 675 - 687 (1987)
Meyer, W.; Philbrick, C. R.; Röttger, J.; Rüster, R.; Widdel, H.-U.; Schmidlin, F. J.: Mean state of winds in the winter middle atmosphere above northern Scandinavia. Journal of Atmospheric and Terrestrial Physics 49, pp. 675 - 687 (1987)
Reid, I. M.; Rüster, R.; Schmidt, G.: VHF Radar Observations of Cat's-eye-like Structures at Mesospheric Heights. Nature 327 (6117), pp. 43 - 45 (1987)
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)
Hocking, W. K.; Rüster, R.; Czechowsky, P.: Absolute reflectivities and aspect sensitivities of VHF radio wave scatterers measured with the SOUSY radar. Journal of Atmospheric and Terrestrial Physics 48, pp. 131 - 144 (1986)
Maekawa, Y.; Aso, T.; Röttger, J.; Czechowsky, P.; Rüster, R.; Schmidt, G.; Hirota, I.; Woodman, R. F.; Kato, S.: A cooperative synchronous observation of winds and tides in the equatorial lower stratosphere and mesosphere using VHF radars at Jicamarca and Arecibo. J. Geomag. Geoelectr. 38, pp. 81 - 97 (1986)
Thomas, L.; Winder, R. J.; Rüster, R.: The characteristics of VHF radar echoes from the tropopause region near a jet stream. Journal of Atmospheric and Terrestrial Physics 48, pp. 261 - 265 (1986)
Czechowsky, P.; Rüster, R.; Schmidt, G.: First results of VHF-radar measurements during the MAP/WINE Campaign. Advances in Space Research 4 (4), pp. 47 - 50 (1984)
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)
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".