Chilson, P. B.; Czechowsky, P.; Schmidt, G.: VHF aspect sensitivity measurements using frequency domain interferometry. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, p. 18 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
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)
Chilson, P. B.; Muschinski, A.; Schmidt, G.: Simultaneous observations of a jet stream passage using VHF FDI and a microbarometer. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 113 - 116 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Muschinski, A.; Chilson, P. B.; Schmidt, G.; Hollmann, R.: FDI measurements with the SOUSY VHF Radar: A comparison between the time series of layer altitudes and Doppler shifts. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 407 - 410 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Singer, W.; Keuer, D.; Hoffmann, P.; Czechowsky, P.; Schmidt, G.: The ALOMAR SOUSY radar: Technical design and further developments. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 473 - 476 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Singer, W.; Keuer, D.; Hoffmann, P.; Czechowsky, P.; Schmidt, G.: The ALOMAR-SOUSY Radar: Technical design and further developments. In: Proc. 12th ESA Symp. on Rocket and Balloon Programmes & Related Research, Lillehammer/Norway 1995, pp. 409 - 415. ESA Publ. Div., Noordwijk (1995)
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)
Czechowsky, P.; Inhester, B.; Klostermeyer, J.; Rüster, R.; Schmidt, G.: Simultaneous radar and lidar observations during the DYANA-campaign. In: Proc. 10th ESA Symposium on European Rocket and Balloon Programmes and Related Research, pp. 399 - 405. ESA Publ. Div., Noordwijk (1991)
Schmidt, G.; Rüster, R.; Czechowsky, P.: Complementary code and digital filtering for detection of weak VHF radar signals from the mesosphere. In: Handbook for MAP, p. 338. (1983)
Czechowsky, P.; Rüster, R.; Schmidt, G.: VHF-radar observations of structures and their dynamics in the stratosphere and mesosphere. Am. Met. Soc., pp. 588 - 592 (1980)
Schmidt, G.; Brekke, A.; Czechowsky, P.; Hall, C. M.; Widdel, H. U.: Spatial Extent and Persistance of Mesospheric Turbulent Layers. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1985)
Czechowsky, P.; Schmidt, G.; Rüster, R.: The mobile SOUSY-Doppler Radar - Technical design and first results. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (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".