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)
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)
Asvestari, E.; Usoskin, I. G.; Krivova, N. A.; Cameron, R. H.: Semi-empirical long-term reconstruction of the heliospheric parameters validated by cosmogenic radionuclide records. Coimbra Solar Physics Meeting CSPM-2015: Ground-based Solar Observations in the Space Instrumentation Era, Coimbra, Portugal (2015)
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)
Kopp, G.; Krivova, N.; Lean, J.; Wu, C.-J.: The Impact of the Revised Sunspot Record on Solar Irradiance Reconstructions. AGU Fall Meeting, San Francisco, USA (2015)
Espuig, M. D.; Jiang, J.; Krivova, N. A.; Solanki, S. K.: Total solar irradiance reconstruction since 1700 using a flux transport model. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Wen, G.; Cahalan, R. F.; Rind, D. H.; Jonas, J.; Pilewskie, P.; Harder, J. W.; Krivova, N.: GISS GCMAM Modeled Climate Responses to Total and Spectral Solar Forcing on Decadal and Centennial Time Scales. American Geophysical Unions 47th annual Fall Meeting, San Francisco, USA (2014)
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".