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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...