Ishikawa, R. T.; Nakata, M.; Katsukawa, Y.; Masada, Y.; Riethmüller, T. L.: Multi-scale deep learning for estimating horizontal velocity fields on the solar surface. Astronomy and Astrophysics 658, p. A142 (2022)
Guglielmino, S. L.; Pillet, V. M.; Cobo, B. R.; Rubio, L. R. B.; Iniesta, J. C. d. T.; Solanki, S. K.; Riethmüller, T.; Zuccarello, F.: On the Magnetic Nature of an Exploding Granule as Revealed by Sunrise/IMaX. The Astrophysical Journal 896 (1), 62 (2020)
Kahil, F.; Riethmüller, T.; Solanki, S. K.: Intensity contrast of solar plage as a function of magnetic flux at high spatial resolution. Astronomy and Astrophysics 621, A78 (2019)
Riethmüller, T.; Solanki, S. K.: The potential of many-line inversions of photospheric spectropolarimetric data in the visible and near UV. Astronomy and Astrophysics 622, A36 (2019)
Kianfar, S.; Jafarzadeh, S.; Mirtorabi, M. T.; Riethmüller, T.: Linear Polarization Features in the Quiet-Sun Photosphere: Structure and Dynamics. Solar Physics 293, 123 (2018)
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)
Gorobets, A. Y.; Berdyugina, S. V.; Riethmüller, T.; Rodríguez, J. B.; Solanki, S. K.; Barthol, P.; Gandorfer, A. M.; Gizon, L.; Hirzberger, J.; van Noort, M.et al.; Del Toro Iniesta, J. C.; Orozco Suárez, D.; Schmidt, W.; Martínez Pillet, V.; Knölker, M.: The Maximum Entropy Limit of Small-scale Magnetic Field Fluctuations in the Quiet Sun. The Astrophysical Journal Supplement Series 233, 5 (2017)
Kahil, F.; Riethmüller, T.; Solanki, S.: Brightness of Solar Magnetic Elements As a Function of Magnetic Fux at High Spatial Resolution. Astrophysical Journal, Suppl. Ser. 229 (1), 12 (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".