Schou, J.; Löptien, B.: Interaction of Oscillations with Near Surface Convection. Joint TASC2 \& KASC9 Workshop SPACEINN \& HELAS8 Conference, Angra do Heroísmo, Portugal (2016)
Löptien, B.; Birch, A. C.; Duvall Jr., T. L.; Gizon, L.; Schou, J.: Data compression for helioseismology. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: On the depth dependence of solar equatorial Rossby waves. Solar Dynamics Observatory Workshop Catalyzing Solar Connections, Ghent, Belgium (2018)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: On the depth dependence of solar equatorial Rossby waves. XXXth General Assembly of the International Astronomical Union, Vienna, Austria (2018)
Löptien, B.; Birch, A. C.; Duvall Jr, T. L.; Gizon, L.; Schou, J.: Measuring active region inflows with local correlation tracking. Seismology of the Sun and the Distant Stars 2016, Angra do Heroísmo, Portugal (2016)
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).