Dubinin, E.; Fraenz, M.; Andrews, D.; Morgan, D.: Ionosphere of Mars observed by Mars Express. European Geosciences Union General Assembly, Vienna, Austria (2016)
Dubinin, E.; Fraenz, M.; Modolo, R.: Distribution and dynamics of plasma in the magnetospheres of Venus and Mars. International Venus Conference, Oxford, U.K. (2016)
Dubinin, E.; Fraenz, M.; Modolo, R.: Magnetic fields and currents at Mars and Venus. AGU Chapman Conference "Currents in Geospace and Beyond", Dubrovnik, Croatia (2016)
Dubinin, E.; Fraenz, M.; Paetzold, M.; McFadden, J.; Eparvier, F.; Brain, D.; Jakosky, B.; Andrews, D.; Barabash, S.: Effects of solar irradiance on the upper ionosphere and ion fluxes at Mars, Mars Express and MAVEN observations. 8th MUAN meeting, Leicester, UK (2016)
Huybrighs, H.; Futaana, Y.; Barabash, S.; Wieser, M.; Wurz, P.; Krupp, N.; Roussos, E.; Fränz, M.; Glassmeier, K.-H.; Vermeersen, B.: Feasibility study of the in-situ detectability of Europa's neutral and plasma plumes from a flyby mission. Europa-Enceladus Plumes Workshop, Pasadene, Caltech, USA (2016)
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)
Fränz, M.; Krupp, N.; Roussos, E.; Wang, X.-D.: Plasma Energization in the Jovian System. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Krupp, N.; Roussos, E.; Fränz, M.; Palmaerts, B.; Bagenal, F.; Wilson, R.; Paranicas, C.: Global Flow Patterns in the Jovian Magnetosphere: Galileo/EPD and Galileo/PLS measurements. European Planetary Science Congress EPSC, Cascais, Portugal (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)
De Oliveira, I.; Echer, E.; Franco, A.; Fränz, M.: Study of Mars' crustal magnetic field displacements due to its interaction with the solar wind. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.