Warnecke, J.: Connecting the solar dynamo below the surface with ejection of twisted magnetic fields above the surface. Forecasts and Warnings of Extreme Storms at the Sun, Lund, Sweden (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Understanding the equatorward migration of the Sun's magnetic field, 2nd Solarnet meeting. 2nd Solarnet meeting, Solar and Stellar Activity, Palermo, Italy (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Understanding the equatorward migration of the Sun's magnetic field. Sunspot formation: theory, simulations and observation, Stockholm, Sweden (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Understanding the equatorward migration of the Sun's magnetic field. Stellar and Planetary Dynamos, Göttingen, Germany (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Magnetic field generation in the Sun driven by rotating Rayleigh-Bénard convection in spherical wedges. International Conference on Rayleigh-Benard Turbulence, Göttingen, Germany (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Understanding the equatorward migration of the Sun's magnetic field. NASA LWS Workshop on Solar Dynamo Frontiers, Boulder, Colorado, USA (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding the solar dynamo form global dynamo simulations. 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity, Bad Honnef, Germany (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding Solar and Stellar Dynamos with numerical simulations. Annual Meeting of the Astronomische Gesellschaft, Kiel, Germany (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding Solar and Stellar Activity with Numerical Simulations. CS Forum, School of Science, Aalto University, Finland (2015)
Warnecke, J.; Losada, I. R.; Brandenburg, A.; Kleeorin, N.; Rogachevskii, I.: Bipolar region formation in stratified two-layer turbulence. Sunspot formation: theory, simulations and observations, Stockholm, Sweden (2015)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Recent results of global convective dynamo simulations. HELASVI, Göttingen, Germany (2014)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: The importance of a coronal envelope for modeling the global turbulent dynamo of the Sun. Coupling and dynamics of the solar atmosphere , Pune, India (2014)
Warnecke, J.; Peter, H.: Magnetic field lines in 3D MHD models of the solar corona. Max-Planck/Princeton Center for Plasma Physics, General Meeting, Berlin, Germany (2014)
Viviani, M.; Cole, E.; Käpylä, P. J.; Käpylä, M. J.; Olspert, N.; Warnecke, J.: Studying the transition from axi- to nonaxisymmetric dynamos using semi-global convection models. MHD Days , Göttingen, Germany (2016)
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".