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)
Yu, J.; Khanna, S.; Themessl, N.; Hekker, S.; Dréau, G.; Gizon, L.; Bi, S.: Revised Extinctions and Radii for 1.5 Million Stars Observed by APOGEE, GALAH, and RAVE. The Astrophysical Journal Supplement Series 264, p. 41 (2023)
Baumgartner, C.; Birch, A. C.; Schunker, H.; Cameron, R. H.; Gizon, L.: Impact of spatially correlated fluctuations in sunspots on metrics related to magnetic twist. Astronomy and Astrophysics 664, p. A183 (2022)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation. Astronomy and Astrophysics 666, p. A135 (2022)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone. Astronomy and Astrophysics 662, p. A16 (2022)
Fournier, D.; Gizon, L.; Hyest, L.: Viscous inertial modes on a differentially rotating sphere: Comparison with solar observations. Astronomy and Astrophysics 664, p. A6 (2022)
Gottschling, N.; Schunker, H.; Birch, A.; Cameron, R. H.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, A6 (2022)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)
IMPRS alumn Yuto Bekki is given a honourable mention by the IAU Division E Sun and Heliosphere for his PhD thesis “Theory of solar oscillations in the inertial frequency range”
IMPRS alumn Yuto Bekki is awarded the European Physical Society’s (EPS) European Solar Physics Division (ESPD) Patricia Edwin PhD Thesis Prize 2023 for the outstanding collection of original results about modes of solar oscillation in the inertial frequency range and for the development of numerical models to classify and study the various families of inertial modes that permeate the solar convection zone