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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.