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Czechowsky, P.; Klostermeyer, J.; Röttger, J.; Rüster, R.; Schmidt, G.: The SOUSY-Svalbard-Radar for middle and lower atmosphere research in polar regions. In: Solar-Terrestrial Energy Program, Proc. 8th Workshop on Technical and Scientific Aspects of MST Radar, Bangalore/Indien 1997, pp. 318 - 321 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1998)
Röttger, J.; Pan, C. J.; Singer, W.; Czechowsky, P.: On the possibility to study troposphere-stratosphere exchange with ST radar. In: Solar-Terrestrial Energy Program, Proc. 8th Workshop on Technical and Scientific Aspects of MST Radar, Bangalore/India 1997, pp. 212 - 215 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1998)
Chilson, P. B.; Czechowsky, P.; Klostermeyer, J.; Rüster, R.; Schmidt, G.: A study of PMSE-like echoes at mid latitudes using VHF radar and lidar. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 88 - 91 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
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Chilson, P. B.; Czechowsky, P.; Schmidt, G.: A comparison of ambipolar diffusion coefficients near the mesopause as determined by VHF radar and UV lidar observations. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 286 - 289 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
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Hoffmann, P.; Singer, W.; Keuer, D.; Rüster, R.; Czechowsky, P.; Meek, C. E.; Lübken, F.-J.; Burrage, M.: Comparison of winds as measured by different techniques during the echo-94 campaign in northern Norway. In: Solar-Terrestrial Energy Program, Proc. 7th workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 166 - 169 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
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".