Kosch, M. J.; Ishii, M.; Kohsiek, A.; Rees, D.; Schlegel, K.; Hagfors, T.; Cierpka, K.: A comparison of vertical thermospheric winds from Fabry-Perot interferometer measurements over a 50 km baseline. Advances in Space Research 26, pp. 985 - 988 (2000)
Kosch, M. J.; Ishii, M.; Nozawa, S.; Rees, D.; Cierpka, K.; Kohsiek, A.; Schlegel, K.; Fujii, R.; Hagfors, T.; Fuller-Rowell, T. J.et al.; Lathuillere, C.: A comparison of thermospheric winds and temperatures from Fabry-Perot interferometer and EISCAT radar measurements with models. Advances in Space Research 26, pp. 979 - 984 (2000)
Liu, H.; Ma, S.; Schlegel, K.: Magnetic storm effects in the auroral ionosphere observed with EISCAT radar - two case studies. Wuhan University Journal of Natural Sciences 5 (2), pp. 181 - 186 (2000)
Liu, H.; Schlegel, K.; Ma, S.-Y.: Combined ESR and EISCAT observations of the dayside polar cap and auroral oval during the May 15, 1997 storm. Annales Geophysicae 18 (9), pp. 1067 - 1072 (2000)
Liu, P.; Ma, S.; Schlegel, K.: EISCAT observations of main ionization troughs in the high-latitude ionosphere. Wuhan University Journal of Natural Sciences 5 (2), pp. 187 - 193 (2000)
Ma, S. Y.; Liu, P.; Schlegel, K.: EISCAT observations of a high latitude ionization trough associated with a reversed westward plasma flow. Geophysical Research Letters 27, pp. 3269 - 3272 (2000)
Mikhailov, A. V.; Schlegel, K.: A self-consistent estimate of O+, N2-rate coefficient and total EUV flux with λ < 1050 Å using EISCAT observations. Annales Geophysicae 18 (9), pp. 1164 - 1171 (2000)
Robinson, T. R.; Schlegel, K.: The generation of non aspect sensitive plasma density irregularities by field aligned drifts in the lower ionosphere. Annales Geophysicae 18 (7), pp. 799 - 806 (2000)
Schlegel, K.; Füllekrug, M.: Diurnal harmonics in Schumann resonance parameters observed on both hemispheres. Geophysical Research Letters 27 (17), pp. 2805 - 2808 (2000)
Voiculescu, M.; Haldoupis, C.; Pancheva, D.; Ignat, M.; Schlegel, K.; Shalimov, S.: More evidence for a planetary wave link with midlatitude E region coherent backscatter and sporadic E layers. Annales Geophysicae 18 (9), pp. 1182 - 1196 (2000)
Koehler, J. A.; Haldoupis, C.; Schlegel, K.: Coherent backscatter cross-section ratio measurements in the midlatitude E region ionosphere. Journal Geophysical Research 104, pp. 4351 - 4359 (1999)
Murayama, Y.; Igarashi, K.; Nishimuta, I.; Yamazaki, R.; Oyama, K.-I.; Tsuda, T.; Nakamura, T.; Fukao, S.; Widdel, H.-U.; Schlegel, K.: Wind observations in the MLT region over southern Japan, by using foil chaff technique, Yamagawa MF radar and the MU radar. Advances in Space Research 24, pp. 575 - 578 (1999)
Oyama, K.-I.; Abe, T.; Schlegel, K.; Nagy, A.; Kim, J.; Marubashi, K.: Electron temperature probe onboard Japan's Mars orbiter. Earth Planets Space 51, pp. 1309 - 1317 (1999)
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".