Bekki, Y.; Cameron, R. H.; Gizon, L.: The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes. Science Advances 10, p. eadk5643 (2024)
Bekki, Y.; Cameron, R. H.; Gizon, L.: The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes. Science Advances 10, p. eadk5643 (2024)
Birch, A. C.; Proxauf, B. ..; Duvall, T. L.; Gizon, L.; Hanasoge, S.; Hindman, B. W.; Sreenivasan, K. R.: Solar convective velocities: Updated helioseismic constraints. Physics of Fluids 36, p. 117136 (2024)
Cloutier, S.; Cameron, R. H.; Gizon, L.: The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun. Astronomy and Astrophysics 691, p. A9 (2024)
Fournier, D.; Hohage, T.; Preuss, J.; Gizon, L.: Learned infinite elements for helioseismology: Learning transparent boundary conditions for the solar atmosphere. Astronomy and Astrophysics 690, p. A86 (2024)
Müller, B.; Hohage, T.; Fournier, D.; Gizon, L.: Quantitative passive imaging by iterative holography: the example of helioseismic holography. Inverse Problems 40, p. 045016 (2024)
Vasilyev, V.; Gizon, L.: Detecting stellar activity cycles in p-mode travel times. Proof of concept using SOHO/VIRGO solar observations. Astronomy and Astrophysics 682, p. A142 (2024)
Jiang, C.; Wu, T.; Feinstein, A. D.; Stassun, K.G.; Bedding, T. R.; Veras, D.; Corsaro, E.; Buzasi, D. L.; Stello, D.; Li, Y.et al.; Mathur, S.; García, R. A.; Breton, S. N.; Lundkvist, M. S.; Mikołajczyk, P. J.; Gehan, C.; Campante, T. L.; Bossini, D.; Kane, S. R.; Joel Ong, J. M.; Yıldız, M.; Kayhan, C.; Çelik Orhan, Z.; Örtel, S.; Zhang, X.; Cunha, M. S.; de Moura, B. L.; Yu, J.; Huber, D.; Ou, J. W.; Wittenmyer, R. A.; Gizon, L.; Chaplin, W. J.: TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting an Extremely Eccentric Exoplanet. The Astrophysical Journal 945, p. 20 (2023)
Philidet, J.; Gizon, L.: Interaction of solar inertial modes with turbulent convection. A 2D model for the excitation of linearly stable modes. Astronomy and Astrophysics 673, p. A124 (2023)
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).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...