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)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)