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)
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)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).