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)
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.
Bewerbungsfrist 1 November 2022. Promotionsprojekte in Planetenwissenschaft, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
First Light für die wissenschaftlichen Instrumente von Sunrise III: Das ballongetragene Sonnenobservatorium bereitet sich auf den nächsten Forschungsflug vor.