Fränz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Barabash, S.; Fedorov, A.: Cold Ion Escape from the Martian Ionosphere. European Planetary Science Congress, Nantes, France (2015)
Barabash, S.; Holmsrtom, M.; Futaana, Y.; Fedorov, A.; Frahm, R.; Fraenz, M.; Dubinin, E.: Phobos-solar wind interaction: Results from Mars Express for the closest-ever fly-by. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Dubinin, E.; Fraenz, M.; Mazelle, C.; Barabash, S.: Large-amplitude coherent structures in plasma near Mars. The 5th Moscow Solar System Symposium (5M-S3), Moscow, Russia (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields and currents at Venus and Mars. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields at Venus and Mars and their effect on plasma flow in the near planet wakes. EPSC, Estoril, Portugal (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.; Barabash, S.: Asymmetrical response of the ionospheric magnetization and the plasma sheet formation on the IMF orientation. 6th Alfven Conference: Plasma Interactions with Solar System Objects anticipating Rosetta, MAVEN and Mars Orbiter Mission, London, UK (2014)
Wei, Y.; Fränz, M.; Dubinin, E.; Wan, W.; Jarvinen, R.; Zhang, T.-L.; Barabash, S.; Lundin, R.: Ablation of Venusian oxygen ions by unshocked solar wind. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Fan, K.; Wei, Y.; Fränz, M.; Dubinin, E. M.; Mcfadden, J.: Efficiency of Solar wind electric field in accelerating planetary ions. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
Fränz, M.; Dubinin, E. M.; Fan, K.; Maes, L.; Halekas, J.; McFadden, J.; Connerney, J.: Mars in the Solar Wind - Simulations and Observations. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
Fränz, M.; Dubinin, E. M.; Fan, K.; Maes, L.; Halekas, J.; McFadden, J.: Mars in the Solar Wind. 21st EGU General Assembly, EGU2019, Vienna, Austria (2019)
Chai, L.; Wei, Y.; Wan, W.; Zhang, T.; Fraenz, M.; Dubinin, E.; Zhang, H.; Rong, Z.; Barabash, S.: An induced global magnetic field looping around the magnetotail of Venus. European Geosciences Union General Assembly, Vienna, Austria (2016)
Han, Q.; Wei, Y.; Chai, L.; Rong, Z.; Fraenz, M.; Dubinin, E.; Wan, W.; Rong, Z.; Futaana, Y.: EUV0dependence of Venusian ionopause height over the dayside high-latitude region: VEX and PVO observations. European Geosciences Union General Assembly, Vienna, Austria (2016)
Dubinin, E.; Fraenz, M.; Andrews, D.; Witasse, O.; Barabash, S.: Ionosphere of Mars as seen by Mars Express. Effect of crustal fields. European Planetary Science Congress, Nantes, France (2015)
Fränz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Barabash, S.; Fedorov, A.: Cold Ion Escape from the Martian Ionosphere - 2007-2014. European Geosciences Union General Assembly, Vienna, Austria (2015)
Fraenz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Fedorov, A.: Cold ion escape from the Martian ionosphere. European Geosciences Union General Assembly 2014, Vienna, Austria (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 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).