Zhou, X.; Buechner, J.; Barta, M.; Gan, W.; Liu, S.: Electron Acceleration by Cascading Reconnection in the Solar Corona. II. Resistive Electric Field Effects. Astrophysical Journal 827 (2), 94 (2016)
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)
Büchner, J.; Muñoz, P. A.; Zhou, X.: Electron Energization in the Solar Corona in Current Concentrations and by Magnetic Reconnection. 14th Annual International Astrophysics Conference, Tampa, USA (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).