Gizon, L.: Presentation of Director candidate. Meeting of the Chemistry, Physics and Technology Section of the Scientific Council of the Max Planck Society, Berlin, Germany (2019)
Gizon, L.: Presentation of the Department: Solar and Stellar Interiors. ESRP Meeting; Max Planck Institute for Solar System Research, Goettingen, Germany (2018)
Gizon, L.: Helioseismology as a probe of solar turbulent convection. Max-Planck/Princeton Center for Plasma Physics Workshop 2018, Princeton, NJ, USA (2018)
Gizon, L.: Equatorial Rossby Waves in the Solar Interior. Dynamic Sun II conference: Solar Magnetism from Interior to the Corona, Siem Reap, Angkor Wat, Cambodia (2018)
Gizon, L.: Rotating turbulent convection in the Sun. Discussion Meeting on Turbulence from Angstroms to Light Years. International Centre for Theoretical Sciences (ICTS) of the Tata Institute of Fundamental Research, Bangalore, India (2018)
Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on the depth of an average supergranule through forward modeling in time-distance helioseismology. Rocks \& Stars II, Göttingen, Germany (2017)
Gizon, L.: Equatorial Rossby waves in the solar interior. Conference - "Our mysterious Sun: magnetic coupling between solar interior and atmosphere", Tbilisi, Georgia (2017)
Gizon, L.; Fournier, D.; Hohage, T.: Problems in computational helioseismology. Workshop: Computational Inverse Problems for Partial Differential Equations , Mathematical Research Institute, Oberwolfach, Germany (2017)
Langfellner, J.; Birch, A. C.; Gizon, L.: The wave-like nature of solar supergranulation - revisited. Rocks and Stars II Conference, Goettingen, Germany (2017)
Liang, Z.-C.; Birch, A. C.; Duvall Jr., T. L.; Gizon, L.; Schou, J.: Helioseismic travel-time measurements of solar meridional from SDO/HMI and SOHO/MDI. 15th European Solar Physics Meeting, Budapest, Hungary (2017)
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).