Muñoz, P. A.; Told, D.; Kilian, P.; Büchner, J.; Jenko, F.: Gyrokinetic and kinetic particle-in-cell simulations of guide-field reconnection. I. Macroscopic effects of the electron flows. Physics of Plasmas 22 (8), 082110 (2015)
Skála, J.; Baruffa, F.; Büchner, J.; Rampp, M.: The 3D MHD code GOEMHD3 for astrophysical plasmas with large Reynolds numbers Code description, verification, and computational performance. Astronomy and Astrophysics 580, A48 (2015)
Zhou, X.; Büchner, J.; Bárta, M.; Gan, W.; Liu, S.: Electron Acceleration by Cascading Reconnection in the Solar Corona. I. Magnetic Gradient and Curvature Drift Effects. Astrophysical Journal 815 (1), 6 (2015)
Jain, N.; Büchner, J.: Nonlinear evolution of three-dimensional instabilities of thin and thick electron scale current sheets: Plasmoid formation and current filamentation. Physics of Plasmas 21 (7), 072306 (2014)
Santos, J. C.; Sibeck, D. G.; Büchner, J.; Gonzalez, W. D.; Ferreira, J. L.: Three-dimensional MHD simulation of FTEs produced by merging at an isolated point in a sheared magnetic field configuration. Journal Geophysical Research 119 (3), pp. 2009 - 2023 (2014)
Yang, S.; Büchner, J.; Sanos, J. C.; Zhang, H.: Evolution of relative magnetic helicity: method of computation and application to a simulated solar corona above an Active Region. Solar Physics 283, pp. 369 - 382 (2013)
Doctoral candidates joining the Solar System School are offered attractive funding, clear prospects and optimal career conditions. IMPRS-funded students receive a three-year doctoral support contract at 65% pay level. Additional funds are available for travel to international conferences. Following their PhD period, graduates are offered postdoc wrap-up funding.