Bebesi, Z.; Krupp, N.; Szego, K.; Fränz, M.; Nemeth, Z.; Krimigis, S. M.; Mitchell, D. G.; Erdos, G.; Young, D. T.; Dougherty, M. K.: Analysis of energetic electron drop-outs in the upper atmosphere of Titan during flybys in the dayside magnetosphere of Saturn. Icarus 218, pp. 1020 - 1026 (2012)
Bebesi, Z.; Szego, K.; Balogh, A.; Krupp, N.; Erdos, G.; Rymer, A. M.; Lewis, G. R.; Kurth, W. S.; Young, D. T.; Dougherty, M. K.: Response to ``Comment on `Slow-mode shock candidate in the Jovian magnetosheath' by Bebesi et al.''. Planetary and Space Science 59 (5-6), pp. 445 - 446 (2011)
Roussos, E.; Krupp, N.; Paranicas, C. P.; Mitchell, D. G.; Müller, A. L.; Kollmann, P.; Bebesi, Z.; Krimigis, S. M.; Coates, A. J.: Energetic electron microsignatures as tracers of radial flows and dynamics in Saturn's innermost magnetosphere. Journal Geophysical Research 115, A03202 (2010)
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".
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.