Wenzler, T.; Solanki, S. K.; Krivova, N. A.: Reconstructed and measured total solar irradiance: Is there a secular trend between 1978 and 2003? Geophysical Research Letters 36, L11102 (2009)
Unruh, Y. C.; Krivova, N. A.; Solanki, S. K.; Harder, J. W.; Kopp, G.: Spectral irradiance variations: comparison between observations and the SATIRE model on solar rotation time scales. Astronomy and Astrophysics 486, pp. 311 - 323 (2008)
Balmaceda, L.; Krivova, N. A.; Solanki, S. K.: Reconstruction of solar irradiance using the Group sunspot number. Advances in Space Research 40, pp. 986 - 989 (2007)
Krivova, N. A.; Balmaceda, L.; Solanki, S. K.: Reconstruction of solar total irradiance since 1700 from the surface magnetic flux. Astronomy and Astrophysics 467, pp. 335 - 346 (2007)
Mathew, S. K.; Martínez Pillet, V.; Solanki, S. K.; Krivova, N. A.: Properties of sunspots in cycle 23. I. Dependence of brightness on sunspot size and cycle phase. Astronomy and Astrophysics 465, pp. 291 - 304 (2007)
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)
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".
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.