Bazot, M.; Nielsen, M. B.; Mary, D.; Christensen-Dalsgaard, J.; Benomar, O.; Petit, P.; Gizon, L.; Sreenivasan, K. R.; White, T. R.: Butterfly diagram of a Sun-like star observed using asteroseismology. Astronomy and Astrophysics 619, L9 (2018)
Benomar, O.; Goupil, M.; Belkacem, K.; Appourchaux, T.; Nielsen, M. B.; Bazot, M.; Gizon, L.; Hanasoge, S.; Sreenivasan, K. R.; Marchand, B.: Asymmetry of Line Profiles of Stellar Oscillations Measured by Kepler for Ensembles of Solar-like Oscillators: Impact on Mode Frequencies and Dependence on Effective Temperature. The Astrophysical Journal 857 (2), 119 (2018)
Fournier, D.; Hanson, C. S.; Gizon, L.; Barucq, H.: Sensitivity kernels for time-distance helioseismology: Efficient computation for spherically symmetric solar models. Astronomy and Astrophysics 616, A 156 (2018)
Langfellner, J.; Birch, A.; Gizon, L.: Evolution and wave-like properties of the average solar supergranule. Astronomy and Astrophysics 617, A97 (2018)
Liang, Z.-C.; Gizon, L.; Birch, A.; Duvall, T.; Rajaguru, S. P.: Solar meridional circulation from twenty-one years of SOHO/MDI and SDO/HMI observations: Helioseismic travel times and forward modeling in the ray approximation. Astronomy and Astrophysics 619, A99 (2018)
Pourabdian, M.; Fournier, D.; Gizon, L.: Comparison of Travel-Time and Amplitude Measurements for Deep-Focusing Time–Distance Helioseismology. Solar Physics 293, 66 (2018)
Rodenbeck, K.; Heller, R.; Hippke, M.; Gizon, L.: Revisiting the exomoon candidate signal around Kepler 1625 b. Astronomy and Astrophysics 617, A49 (2018)
Bhattacharya, J.; Hanasoge, S. M.; Birch, A.; Gizon, L.: Recovery of subsurface profiles of supergranular flows via iterative inversion of synthetic travel times. Astronomy and Astrophysics 607, A 129 (2017)
Centeno, R.; Blanco Rodriguez, J.; Del Toro Iniesta, J. C.; Solanki, S. K.; Barthol, P.; Gandorfer, A.; Gizon, L.; Hirzberger, J.; Riethmüller, T. L.; van Noort, M.et al.; Orozco Suarez, D.; Berkefeld, T.; Schmidt, W.; Pillet, V. M.; Knoelker, M.: A Tale of Two Emergences: SUNRISE II Observations of Emergence Sites in a Solar Active Region. Astrophysical Journal, Suppl. Ser. 229 (1), 3 (2017)
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".