Viviani, M.; Cole, E.; Käpylä, P. J.; Käpylä, M. J.; Olspert, N.; Warnecke, J.: Axi- to nonaxisymmetric dynamo transition in semi-global convection models. 14th Potsdam Thinkshop: Stellar magnetism: Challenges, Connections and Prospects, Potsdam, Germany (2017)
Viviani, M.; Cole-Kodicara, E.; Käpylä, P. J.; Käpylä, M. J.; Olspert, N.; Warnecke, J.: The influence of rotation in the transition from axi- to nonaxisymmetric dynamos. Rocks \& Stars II, Göttingen, Germany (2017)
Viviani, M.; Cole-Kodicara, E.; Käpylä, P. J.; Käpylä, M. J.; Olspert, N.; Warnecke, J.: Axi- to nonaxisymmetric dynamo transition in stellar models with varying rotation rate. AG2017 The many Scales of Universe: Galaxies, theirs Suns and their Planets, Göttingen, Germany (2017)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding dynamo mechanisms from 3D convection simulations of the Sun. SOLARNET IV Meeting: The Physics of the Sun from the Interior to the Outer Atmosphere., Lanzarote, Spain (2017)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Brandenburg, A.: Identifying dynamo mechanism for slowly and rapidly rotating stars. 14th Potsdam Thinkshop: Stellar Magnetism: Challenges, Connections, and Prospects, Potsdam, Germany (2017)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Brandenburg, A.: Determine dynamo mechanisms and magnetic helicity fluxes in compressible convective dynamo simulations of solar-like stars. 2nd Conference on Natural Dynamos, Valtice, Czech Republic (2017)
Käpylä, M. J.: Interaction of MRI and other sources of turbulence and what does it mean for galactic dynamo. Max Planck Princeton Center for Plasma Physics Meeting, Princeton, USA (2016)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: The Test-Field Method and Its Applications. ax Planck Princeton Center for Plasma Physics Meeting, Princeton, USA (2016)
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Brandenburg, A.: Understanding dynamo mechanisms from 3D convection simulations of the Sun. MHD Days, Göttingen, Germany (2016)
Viviani, M.; Warnecke, J.; Käpylä, M. J.; Käpylä, P. J.; Olspert., N.; Cole-Kodikara, E. M.; Lehtinen, J.; Brandenburg, A.: Solar-like stars at various rotation rates: a comparison between observations and simulations. IAU Symposia 340: Long-term datasets for the understanding of solar and stellar magnetic cycles, Jaipur, India (2018)
Olspert, N.; Käpylä, M. J.; Pelt, J.: From periods to cycles: new methods applied to solar, stellar and in silico data. Physics Days 2017, the 51st annual meeting of the Finnish Physical Society, Helsinki, Finland (2017)
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)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.