Feng, L.; Inhester, B.; Gan, W.: 3D reconstructions of CMEs from SECCHI COR and HI1 data and their link to in-situ observations. Solar Information Workshop 7, La Roche-en-Ardenne, Belgium (2014)
Feng, L.; Inhester, B.; Wang, Y.; Shen, F.; Shen, C.; Gan, W.: On the mass evolution of CMEs. European Solar Physics Meeting 14, Dublin, Ireland (2014)
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).