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)
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)
Yang, D.; Gizon, L.; Barucq, H.: Imaging individual active regions on the Sun's far side with improved helioseismic holography. Astronomy and Astrophysics 669, p. A89 (2023)
Yang, D.; Gizon, L.; Barucq, H.: Imaging individual active regions on the Sun's far side with improved helioseismic holography. Astronomy and Astrophysics 669, p. A89 (2023)
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
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).