Poulier, P.-L.; Gizon, L.; Duvall, T.; Fournier, D.: Multiple scattering of acoustic waves. AG2017 The many Scales of Universe: Galaxies, theirs Suns and their Planets, Göttingen, Germany (2017)
Pourabdian, M.; Fournier, D.; Gizon, L.: Comparison Between Travel-time and Amplitude Measurements Using Deep-focusing Time-distance Helioseismology. AG Meeting 2017, Göttingen, Germany (2017)
Yang, D.; Gizon, L.; Fournier, D.: A Possible Improvement on Helioseismic Holography. the many Scales of the Universe: Galaxies, their Suns, and their Planets - Annual Meeting of the Astronomische Gesellschaft 2017, Göttingen, Germany (2017)
Hanson, C. S.; Leguebe, M.; Fournier, D.; Brich, A. C.; Gizon, L.: Computational Local Helioseismology in the Frequency Domain. Seismology of the Sun and the Distant Stars 2016, Angra do Heroísmo, Portugal (2016)
Löptien, B.; Birch, A. C.; Duvall Jr, T. L.; Gizon, L.; Schou, J.: Measuring active region inflows with local correlation tracking. Seismology of the Sun and the Distant Stars 2016, Angra do Heroísmo, Portugal (2016)
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".