Gent, F. A.; Mac Low, M.-M.; Korpi-Lagg, M. J.: Transition from Small-scale to Large-scale Dynamo in a Supernova-driven, Multiphase Medium. The Astrophysical Journal 961, p. 7 (2024)
Hackman, T.; Kochukhov, O.; Viviani, M.; Warnecke, J.; Korpi-Lagg., M.J.; Lehtinen, J. J.: From convective stellar dynamo simulations to Zeeman-Doppler images. Astronomy and Astrophysics 682, p. A156 (2024)
Snellman, J.; Barrio, R.; Kaski, K.; Korpi-Lagg., M.J.: A modelling study to explore the effects of regional socio-economics on the spreading of epidemics. JOURNAL OF COMPUTATIONAL SOCIAL SCIENCE (3), pp. 2535 - 2562 (2024)
Warnecke, J.; Korpi-Lagg, M.; Gent, F. A.; Rheinhardt, M.: Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers. Nature Astronomy 7, pp. 662 - 668 (2023)
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".