Ball, W.; Yeo, K. L.; Krivova, N.; Solanki, S.; Unruh, Y.; Morrill, J.: Evaluation of solar irradiance models for climate studies. European Geosciences Union General Assembly, Vienna, Austria (2015)
Ball, W. T.; Yeo, K. L.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Morrill, J.: Evaluation of solar irradiance models for climate studies. European Geosciences Union General Assembly, Vienna, Austria (2015)
Tapia, A. L. S.; Solanki, S. K.; Lagg, A.; van Noort, M.: ANOMALOUS REVERSED EVERSHED FLOW IN A SUNSPOT PENUMBRA. Sunspot formation: theory, simulations and observations, Stockholm, Sweden (2015)
Espuig, M. D.; Jiang, J.; Krivova, N. A.; Solanki, S. K.: Total solar irradiance reconstruction since 1700 using a flux transport model. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
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).