Griessmeier, J. M.; Preusse, S.; Khodachenko, M.; Motschmann, U.; Mann, G.; Rucker, H. O.: Exoplanetary radio emission under different stellar wind conditions. Planetary and Space Science 55 (5), pp. 618 - 630 (2007)
Preusse, S.; Kopp, A.; Büchner, J.; Motschman, U.: MHD simulation scenarios of the stellar wind interaction with Hot Jupiter magnetospheres. Planetary and Space Science 55, pp. 589 - 597 (2007)
Preusse, S.; Kopp, A.; Büchner, J.; Motschmann, U.: A magnetic communication scenario for hot Jupiters. Astronomy and Astrophysics 460, pp. 317 - 322 (2006)
Preusse, S.; Kopp, A.; Büchner, J.; Motschmann, U.: Magnetic communication scenarii for close-in extrasolar planets. In: Tenth Anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies, pp. 274 - 281 (Eds. Arnold, L.; Bouchy, F.; Moutou, C.). Frontier Group, Paris (2006)
Preusse, S.; Kopp, A.; Büchner, J.; Motschmann, U.: Magnetic communication scenarios for close-in extrasolar planets. In: Status and prospects for hot Jupiter studies, Haute Provence Observatory Colloquium, August 22-25, 2005, pp. 1 - 8. (2005)
Preusse, S.: Szenarien der Plasmawechselwirkung in kurzperiodischen extrasolaren Planetensystemen. Dissertation, Technische Universität Braunschweig (2005)
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".