Barta, M.; Büchner, J.; Karlicky, M.; Skala, J.: Role of plasmoids in energy cascade in magnetic reconnection in solar corona. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Büchner, J.: Collisionless reconnection in the solar corona. International E. Parker Workshop on magnetic reconnection, Sao Jose dos Campos, Brazil (2014)
Büchner, J.: Collisionlesss reconnection at the Sun for strong guide fields. R2014 -International Workshop on Magnetic Reconnection, Tokyo, Japan (2014)
Büchner, J.: Sub-Grid-Scale (SGS) Approach to the Turbulent Dynamo and Magnetic Reconnection. Zeldovich-100, International Astrophysical Conference, Moscow, Russia (2014)
Büchner, J.: Influence of turbulence on reconnection by SGS MHD models and their calibration on plasma models beyond MHD: Hybrid and PIC code kinetic simulations. Max-Planck-Princeton Center for Plasma Physics Annual Meeting, Berlin, Germany (2014)
Muñoz, P. A.; Kilian, P.; Büchner, J.: PIC-code simulation of spontaneous instabilities of current sheets: anisotropic heating and guide field influence on magnetic reconnection. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Savin, S.; Amata, E.; Büchner, J.; Klimov, S.; Kronberg, E.; Zelenyi, L.; others: Study of Discrete and Turbulent Cascades in the Outer Magnetosphere: Resonances and Transport. Annual Meeting of the Asia Oceania Geosciences Society , Sapporo, Japan (2014)
Yang, S.; Büchner, J.; Santos, J. C.; Zhang, H.: Modeling the relative magnetic helicity in MHD simulations and its application to solar activity. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Widmer, F.; Büchner, J.; Yokoi, N.; Schmidt, W.: Turbulent MHD Magnetic Reconnection using Sub-grid Scale Modelling. Turbulence, magnetic fields and self organization in laboratory and astrophysical plasmas, Les Houches, France (2015)
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, ...