Wenzler, T.; Solanki, S. K.; Krivova, N. A.; Fröhlich, C.: Reconstruction of solar irradiance variations in cycles 21-23 based on surface magnetic fields. Astronomy and Astrophysics 460, pp. 583 - 595 (2006)
Balmaceda, L.; Solanki, S. K.; Krivova, N.: A cross-calibrated sunspot areas time series since 1874. Memorie della Societa Astronomica Italiana 76, pp. 929 - 932 (2005)
Haberreiter, M.; Krivova, N. A.; Schmutz, W.; Wenzler, T.: Reconstruction of the solar UV irradiance back to 1974. Advances in Space Research 35 (3), pp. 365 - 369 (2005)
Krivova, N. A.; Solanki, S. K.: Modelling of irradiance variations through atmosphere models. Memorie della Societa Astronomica Italiana 76, pp. 834 - 841 (2005)
Wenzler, T.; Solanki, S. K.; Krivova, N. A.: Can surface magnetic fields reproduce solar irradiance variations in cycles 22 and 23? Astronomy and Astrophysics 432, pp. 1057 - 1061 (2005)
Krivov, A. V.; Krivova, N. A.; Solanki, S. K.; Titov, V. B.: Towards understanding the β Pictoris dust stream. Astronomy and Astrophysics 417, pp. 341 - 352 (2004)
Krivova, N. A.; Solanki, S. K.: Effect of spatial resolution on estimating the Sun's magnetic flux. Astronomy and Astrophysics 417, pp. 1125 - 1132 (2004)
Krivova, N. A.; Solanki, S. K.: Solar variability and global warming: A statistical comparison since 1850. Advances in Space Research 34, pp. 361 - 364 (2004)
Wenzler, T.; Solanki, S. K.; Krivova, N. A.; Fluri, D. M.: Comparison between KPVT/SPM and SoHO/MDI magnetograms with an application to solar irradiance reconstructions. Astronomy and Astrophysics 427 (3), pp. 1031 - 1043 (2004)
Krivova, N. A.; Solanki, S. K.: A stream of particles from the β Pictoris disc: A possible ejection mechanism. Astronomy and Astrophysics 402, pp. L5 - L8 (2003)
Krivova, N. A.; Solanki, S. K.; Fligge, M.; Unruh, Y. C.: Reconstruction of solar irradiance variations in Cycle 23: Is solar surface magnetism the cause? Astronomy and Astrophysics 399, pp. L1 - L4 (2003)
Krivova, N. A.; Solanki, S. K.: The 1.3-year and 156-day periodicities in sunspot data: wavelet analysis suggests a common origin. Astronomy and Astrophysics 394, pp. 701 - 706 (2002)
Solanki, S. K.; Krivova, N. A.; Schüssler, M.; Fligge, M.: Search for a relationship between solar cycle amplitude and length. Astronomy and Astrophysics 396, pp. 1029 - 1035 (2002)
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.