Narita, Y.; Glassmeier, K.-H.; Motschmann, U.: High-resolution wave number spectrum using multi-point measurements in space - the Multi-point Signal Resonator (MSR) technique. Annales Geophysicae 29 (2), pp. 351 - 360 (2011)
Plaschke, F.; Glassmeier, K.-H.: Properties of standing Kruskal-Schwarzschild-modes at the magnetopause. Annales Geophysicae 29 (10), pp. 1793 - 1807 (2011)
Takahashi, K.; Glassmeier, K.-H.; Angelopoulos, V.; Bonnell, J.; Nishimura, Y.; Singer, H. J.; Russell, C. T.: Multisatellite observations of a giant pulsation event. Journal Geophysical Research 116, A11223 (2011)
Turner, D. L.; Eriksson, S.; Phan, T. D.; Angelopoulos, V.; Tu, W.; Liu, W.; Li, X.; Teh, W.-L.; McFadden, J. P.; Glassmeier, K.-H.: Multispacecraft observations of a foreshock-induced magnetopause disturbance exhibiting distinct plasma flows and an intense density compression. Journal Geophysical Research 116, A04230 (2011)
Wiehle, S.; Motschmann, U.; Gortsas, N.; Glassmeier, K.-H.; Müller, J.; Koenders, C.: Simulation of cometary jets in interaction with the solar wind. Advances in Space Research 48 (6), pp. 1108 - 1113 (2011)
Wiehle, S.; Plaschke, F.; Motschmann, U.; Glassmeier, K.-H.; Auster, H. U.; Angelopoulos, V.; Mueller, J.; Kriegel, H.; Georgescu, E.; Halekas, J.et al.; Sibeck, D. G.; McFadden, J. P.: First lunar wake passage of ARTEMIS: Discrimination of wake effects and solar wind fluctuations by 3D hybrid simulations. Planetary and Space Science 59 (8), pp. 661 - 671 (2011)
Auster, H. U.; Richter, I.; Glassmeier, K. H.; Berghofer, G.; Carr, C. M.; Motschmann, U.: Magnetic field investigations during ROSETTA's 2867 Steins flyby. Planetary and Space Science 58 (9), pp. 1124 - 1128 (2010)
Baumjohann, W.; Blanc, M.; Fedorov, A.; Glassmeier, K.-H.: Current Systems in Planetary Magnetospheres and Ionospheres. Space Science Reviews 152 (1-4), pp. 99 - 134 (2010)
Liu, W.; Sarris, T. E.; Li, X.; Ergun, R.; Angelopoulos, V.; Bonnell, J.; Glassmeier, K. H.: Solar wind influence on Pc4 and Pc5 ULF wave activity in the inner magnetosphere. Journal Geophysical Research 115, A12201 (2010)
Mueller, J.; Simon, S.; Motschmann, U.; Glassmeier, K.-H.; Saur, J.; Schuele, J.; Pringle, G. J.: Magnetic field fossilization and tail reconfiguration in Titan's plasma environment during a magnetopause passage: 3D adaptive hybrid code simulations. Planetary and Space Science 58 (12), pp. 1526 - 1546 (2010)
Narita, Y.; Glassmeier, K.-H.: Anisotropy evolution of magnetic field fluctuation through the bow shock. Earth, Planets and Space 62 (2), pp. E1 - E4 (2010)
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".