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)
Büchner, J.; Nikutowski, B.; Bedrich, S.; Griethe, H.: SCHWARM - Small satellites for the investigation of collisionless plasma turbulence and magnetic reconnection. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (2001)
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.