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)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).