Werner, S.; Keller, H. U.; Korth, A.; Lauche, H.: UVIS/HDAC Lyman-alpha observations of the geocorona during Cassini's Earth swingby compared to model prediction. Advances in Space Research 34 (8), pp. 1647 - 1649 (2004)
Østgaard, N.; Mende, S. B.; Frey, H. U.; Gladstone, G. R.; Lauche, H.: Neutral hydrogen density profiles derived from geocoronal imaging. Journal Geophysical Research 108 (A7), 1300 (2003)
Mende, S. B.; Heetderks, H.; Frey, H. U.; Stock, J. M.; Lampton, M.; Geller, S. P.; Abiad, R.; Siegmund, O. H. W.; Habraken, S.; Renotte, E.et al.; Jamar, C.; Rochus, P.; Gerard, J.-C.; Sigler, R.; Lauche, H.: Far ultraviolet imaging from the IMAGE spacecraft: 3. Spectral imaging of Lyman alpha and OI 135.6 nm. Space Science Reviews 91, pp. 287 - 318 (2000)
Boehm, M.; Paschmann, G.; Clemmons, J.; Höfner, H.; Frenzel, R.; Ertl, M.; Haerendel, G.; Hill, P.; Lauche, H.; Eliasson, L.et al.; Lundin, R.: The TESP electron spectrometer and correlator (F7) on Freja. Space Science Reviews 70, pp. 509 - 540 (1994)
Czechowsky, P.; Kochan, H.; Lange-Hesse, G.; Lauche, H.; Möller, H. G.: Simultane Beobachtungen verschiedener ionosphärischer Phänomene während des erdmagnetischen Sturmes vom 31. Oktober bis 2. November 1968. Zeitschrift für Geophysik 36 (Heft 1), pp. 77 - 103 (1970)
Czechowsky, P.; Kochan, H.; Lange-Hesse, G.; Lauche, H.; Möller, H. G.: Simultaneous Observations of Various Ionospheric Phenomena During the Geomagnetic Storm from October 31 to November 2, 1968. World Data Center A, (1970)
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".