Bučík, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R.: Long-lasting 3He-rich solar energetic particle sources. STEREO SEP meeting, Laurel, Maryland, USA (2014)
Bučík, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E.: Observations of a blast EUV wave in 3He-rich solar energetic particle sources. 14th Annual International Astrophysics Conference, Tampa, USA (2015)
Park, J.; Innes, D. E.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: Study of solar energetic particle associations with extreme-ultraviolet waves. The 3rd Asia-Pacific Solar Physics Meeting, Seoul, Rep. of Korea (2015)
Chen, N.-H.; Bučík, R.; Innes, D. E.; Mason, G. M.: The relation between solar jets and 3He-rich solar energetic particle events at 1 AU. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Park, J.; Innes, D.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: The study of solar energetic protons associated with EUV waves. 224th AAS Meeting, Boston, MA, USA (2014)
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).