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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...