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)
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)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.