Wu, C.-J.; Usoskin, I.; Krivova, N.; Kavoltsov, G.; Solanki, S.: Solar Spectral Irradiance Reconstruction over 9 Millennia from a Composite 14C and 10Be series. AGU Fall Meeting, New Orleans, USA (2017)
Chatzistergos, T.; Ermolli, I.; Solanki, S. K.; Krivova, N. A.: The potential of historical spectroheliograms for Sun-climate studies. 9th IAGA - ICMA/IAMAS - ROSMIC/VarSITI/SCOSTEP workshop on long-term changes and trends in the atmosphere, Kühlungsborn, Germany (2016)
Chatzistergos, T.; Usoskin, I.; Kovaltsov, G. A.; Krivova, N. A.; Solanki, S. K.: Non-linear re-calibration of group sunspot number series back to 1739. AGU Fall Meeting, San Francisco, USA (2016)
Wu, C.-J.; Krivova, N.; Solanki, S. K.; Usoskin, I.: Reconstructions of Solar Irradiance on the Millennial Timescale. European space weather week 13, Oostende, Belgium (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Why do measurements and models of UV SSI variability not agree? 9th IAGA - ICMA/IAMAS - ROSMIC/VarSITI/SCOSTEP workshop on Long-Term Changes and Trends in the Atmosphere, Kühlungsborn, Germany (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: UV SSI variability Why do measurements and models not agree? 6th International HEPPA-SOLARIS Workshop, Helsinki, Finland (2016)
Chatzistergos, T.; Ermolli, I.; Solanki, S. K.; Krivova, N. A.: Exploiting historical Ca II K spectroheliogram archives: preliminary results from four archives. Coimbra Solar Physics Meeting, Coimbra, Portugal (2015)
Krivova, N.: Solare Variabilität und Klima. Bundesweite Lehrerfortbildung zur Astronomie der Wilhelm und Else Heraeus-Stiftung, Heidelberg,Germany (2015)
Shapiro, A.; Solanki, S.; Krivova, N.: Solar brightness variability in the stellar context. Second SOLARNET Meeting on "Solar and stellar magnetic activity, Palermo, Italy (2015)
Shapiro, A.; Solanki, S.; Krivova, N.: Brightness variations of the Sun and Sun-like stars. Solar-Stellar Connection Workshop, Sandbjerg, Denmark (2015)
Usoskin, I.; Arlt, R.; Asvestari, E.; Kovaltsov, G.; Krivova, N.; Lockwood, M.; Käpylä, M.; Owens, M.; Sokoloff, D. D.; Solanki, S.et al.; Soon, W.; Vaquero, J.; Scott, C.: The Maunder minimum: A reassessment from multiple dataset. XXIX IAU General Assembly, Honolulu, USA (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Measurements and models of solar irradiance variability in the satellite-era. Conference on Sun-Climate Connections, Kiel, Germany (2015)
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).