Heller, R.; Duda, J.-P.; Winkler, M.; Reitner, J.; Gizon, L.: Habitability of the Early Earth: A Faint Young Sun and Strong Tidal Heating due to a Closer Moon. ESRP Meeting, Jena, Germany (2022)
Gizon, L.; MPS Team: Global-scale Rossby waves in the solar interior. Dynamics of the Sun and Stars: Honoring the Life and Work of Michael J. Thompson,, Boulder, USA (2019)
Nagashima, K.; Birch, A.; Schou, J.; Hindman, B.; Gizon, L.: Monte-Carlo test of an improved multi-ridge fitting code for ring-diagram analysis. Dynamics of the Sun & Stars: Honoring the Life & Work of Michael Thompson , Boulder, CO, USA (2019)
Yang, D.; Gizon, L.; Fournier, D.; Lindsey, C.: Improved helioseismic imaging of the farside. Dynamics of the Sun and Stars: Honoring the Life and Work of Michael J. Thompson,, Boulder, USA (2019)
Pourabdian, M.; Gizon, L.; Hohage, T.; Fournier, D.; Hanson, C. S.: Optimal averaging for helioseismic measurements using the singular value decomposition. XXXth General Assembly of the International Astronomical Union, Vienna, Austria (2019)
Poulier, P.-L.; Gizon, L.; Fournier, D.; Duvall, T.: On the validity of the frozen-in approximation for acoustic wave propagation through solar granulation. XXXth General Assembly of the International Astronomical Union, Vienna, Austria (2019)
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)
Nagashima, K.; Duvall, T.; Birch, A. C.; Gizon, L.: Comparison between time-distance and ring-diagram helioseismology measurements of subsurface convective flows. Annual Meeting of the Astronomische Gesellschaft 2017, Göttingen, Germany (2017)
Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on supergranular depth obtained through the resolution of the forward problem in local helioseismology. Astronomische Gesellschaft Meeting, Göttingen, Germany (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).