Yeo, K. L.; Krivova, N. A.; Solanki, S. K.; Glassmeier, K. H.: Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations. Astronomy and Astrophysics 570, A85 (2014)
Yeo, K. L.; Shapiro, A. I.; Krivova, N. A.; Solanki, S. K.: Modelling solar and stellar brightness variabilities. In: Coimbra Solar Physics Meeting: Ground-based Solar Observations in the Space Instrumentation Era, Vol. 504, pp. 273 - 286. (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Solar radiative forcing. IAPSO-IAMAS-IAGA Joint Assembly. Good Hope for Earth Sciences - IAPSO-IAMAS-IAGA Joint Assembly 2017, Cape Town, South Africa (2018)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Why do measurements and models of UV SSI variability not agree? 9th IAGA - ICMA/IAMAS - ROSMIC/VarSITI/SCOSTEP workshop on Long-Term Changes and Trends in the Atmosphere, Kühlungsborn, Germany (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: UV SSI variability Why do measurements and models not agree? 6th International HEPPA-SOLARIS Workshop, Helsinki, Finland (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Measurements and models of solar irradiance variability in the satellite-era. Conference on Sun-Climate Connections, Kiel, Germany (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Measurements and models of solar irradiance variability in the satellite-era. Conference on Sun-Climate Connections, Kiel, Germany (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Solar irradiance variability since 1978 Reconciling measurements and models. AOGS 12th Annual Meeting, Singapore (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Discrepancy between the various UV SSI records and reconstructions, and the underlying causes. SOLARIS-HEPPA Working Group Meeting, Boulder, Colorado, USA (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: SATIRE-S reconstruction of TSI and SSI since 1974. 2015 Sun-Climate Symposium, Savannah, Georgia, USA (2015)
Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar magnetic activity and solar irradiance variability since 1978. 2nd SOLARNET Meeting, Palermo, Italy (2015)
Ball, W. T.; Yeo, K. L.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Haigh, J. D.; Mortlock, D.; Egerton, J. S.: Spectral solar irradiance and limits on understanding the effect on stratospheric ozone. seminar, Kiel, Germany (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".