Steinhagen, H.; Christoph, A.; Czechowsky, P.; Görsdorf, U.; Gube-Lenhardt, M.; Lippmann, J.; Neisser, J.; Rüster, R.; Schmidt, G.; Wergen, W.et al.; Yoe, J. G.: Field campaign for the comparison of SOUSY radar wind measurements with rawinsonde and model data. Annales Geophysicae 12 (8), pp. 746 - 764 (1994)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Spatial variability of the aspect sensitivity of VHF radar echoes in the troposphere and lower stratosphere during jet stream passages. Annales Geophysicae 12 (8), pp. 733 - 745 (1994)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Temporal and Spatial Variability of Aspect Sensitivity of VHF Radar Echoes in the Lower Atmosphere. Annales Geophysicae 12, pp. 733 - 745 (1993)
Yoe, J. G.; Rüster, R.: VHF Doppler Radar Opservations of Vertical Velocities in the Vicinity of the Jet Stream. Monthly Weather Rev. 120 (10), pp. 2378 - 2382 (1992)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Spatial and temporal variability of the aspect sensitivity of VHF radar echoes in the troposphere and lower stratosphere during jet stream passages. In: Solar-Terrestrial Energy Program, Proc. 6th Workshop on Techhnical and Scientific Aspects of MST Radar, Chung-Li/Taiwan 1993, pp. 66 - 70 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1994)
Yoe, J. G.; Rüster, R.; Schmidt, G.: Measurement of momentum fluxes in the troposphere and stratosphere during jet sream passages using the SOUSY VHF. In: Proc. 5th Workshop on Technical and Scientific Aspects of MSt Radar,, Aberystwyth, United Kingdom 1991, pp. 150 - 155 (Ed. Edwards, B.). SCOSTEP, Secret., Boulder (1992)
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.