Dasi-Espuig, M.; Unruh, Y.; Krivova, N. A.; Solanki, S. K.; Jiang, J.: Modeling of spectral irradiance based on modeled proxies. SOLID annual meeting, Bremen, Germany (2014)
Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar irradiance variability and the Earth's climate. SCOSTEP's 13th Quadrennial Solar-Terrestrial Physics Symposium, Xi'an, China (2014)
Lagg, A.; Bernasconi, P.; Katsukawa, Y.; del Toro Iniesta, J.C.; Berkefeld, T.; Solanki, S. K.: SUNRISE III: The Solar Atmosphere in 3D and High Rssolution. 2021 Scientific Ballooning Technologies Workshop, online (2021)
Albert, K.; Hirzberger, J.; Busse, D.; Rodrguez, J. B.; Castellanos Durán, J. S.; Carrascosa, J. P. C.; Fiethe, B.; Gandorfer, A. M.; Guan, Y.; Kolleck, M.et al.; Lange, T.; Michalik, H.; Solanki, S. K.; Iniesta, J. C. d. T.; Woch, J.: Performance analysis of the SO/PHI software framework for on-board data reduction. 28th annual international Astronomical Data Analysis Software & Systems (ADASS) conference, College Park, Maryland, USA (2019)
Smitha, H. N.; Anusha, L. S.; Solanki, S. K.; Riethmueller, T. L.: Flux emergence rate in the quiet Sun from SUNRISE data. SOLARNET IV, The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Wu, C.-J.; Krivova, N.; Solanki, S.; Usoskin, I.: Solar Total and Spectral Irradiance reconstruction over last 9000 years. Space Climate 6, Levi, Finland (2016)
Wu, C.-J.; Krivova, N.; Solanki, S. K.; Usoskin, I.: Solar Total and Spectral Irradiance Reconstruction over Last 9000 Years. Space Climate 6 symposium, Levi, Finland (2016)
Wu, C.-J.; Krivova, N.; Solanki, S. K.; Usoskin, I.: Solar Total and Spectral Irradiance Reconstruction over Last 9000 Years. AGU Fall Meeting, San Francisco, USA (2016)
Ball, W.; Yeo, K. L.; Krivova, N.; Solanki, S.; Unruh, Y.; Morrill, J.: Evaluation of solar irradiance models for climate studies. European Geosciences Union General Assembly, Vienna, Austria (2015)
Ball, W. T.; Yeo, K. L.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Morrill, J.: Evaluation of solar irradiance models for climate studies. European Geosciences Union General Assembly, Vienna, Austria (2015)
Tapia, A. L. S.; Solanki, S. K.; Lagg, A.; van Noort, M.: ANOMALOUS REVERSED EVERSHED FLOW IN A SUNSPOT PENUMBRA. Sunspot formation: theory, simulations and observations, Stockholm, Sweden (2015)
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".