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)
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".
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.