Han, X.; Fraenz, M.; Dubinin, E.; Wei, Y.; Andrews, D. J.; Wan, W.; He, M.; Rong, Z. J.; Chai, L.; Zhong, J.et al.; Li, K.; Barabash, S.: Discrepancy between ionopause and photoelectron boundary determined from Mars Express measurements. Geophysical Research Letters 41, pp. 8221 - 8227 (2014)
Han, X.; Fraenz, M.; Andrews, D.; Dubinin, E.; Wan, W.; Barabash, S.: The control of Martian ionopause altitude by the crustal and induced magnetic field strength. European Geosciences Union General Assembly 2014, Vienna, Austria (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).