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)
Gottschling, N.; Schunker, H.; Birch, A. C.; Cameron, R.; Gizon, L.: Testing solar surface flux transport models in the first days after active region emergence. Astronomy and Astrophysics 660, p. A6 (2022)
Jiang, C.; Cunha, M.; Christensen-Dalsgaard, J.; Zhang, Q. S.; Gizon, L.: Evolution of dipolar mixed-mode coupling factor in red giant stars: impact of buoyancy spike. Monthly Notices of the Royal Astronomical Society 515, pp. 3853 - 3866 (2022)
Lampens, P.; Samadi-Ghadim, A.; Gizon, L.: KIC 6951642: A confirmed Kepler γ Doradus - δ Scuti star with intermediate to fast rotation in a possible single-lined binary system. Astronomy and Astrophysics 667, p. A60 (2022)
Nascimbeni, V.; Piotto, G.; Börner, A.; Montalto, M.; Marrese, P. M.; Cabrera, J.; Marinoni, S.; Aerts, C.; Altavilla, G.; Benatti, S.et al.; Claudi, R.; Deleuil, M.; Desidera, S.; Fabrizio, M.; Gizon, L.; Goupil, M. J.; Granata, V.; Heras, A. M.; Magrin, D.; Malavolta, L.; Mas-Hesse, J. M.; Ortolani, S.; Pagano, I.; Pollacco, D.; Prisinzano, L.; Ragazzoni, R.; Ramsay, G.; Rauer, H.; Udry, S.: The PLATO field selection process. I. Identification and content of the long-pointing fields. Astronomy and Astrophysics 658, p. A31 (2022)
Poulier, P.-L.; Liang, Z.-C.; Fournier, D.; Gizon, L.: Contribution of flows around active regions to the north-south helioseismic travel-time measurements. Astronomy and Astrophysics 664, p. A189 (2022)
Böning, V. G. A.; Birch, A.; Gizon, L.; Duvall, T.: Helioseismological determination of the subsurface spatial spectrum of solar convection: Demonstration using numerical simulations. Astronomy and Astrophysics 649, A59 (2021)
Compaire, N.; Margerin, L.; Garcia, R. F.; Pinot, B.; Calvet, M.; Orhand-Mainsant, G.; Kim, D.; Lekic, V.; Tauzin, B.; Schimmel, M.et al.; Stutzmann, E.; Knapmeyer-Endrun, B.; Lognonné, P.; Pike, W. T.; Schmerr, N.; Gizon, L.; Banerdt, W. B.: Autocorrelation of the Ground Vibrations Recorded by the SEIS-InSight Seismometer on Mars. Journal of Geophysical Research: Planets 126 (4), e2020JE006498 (2021)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".