Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar irradiance variability and the Earth's climate. SCOSTEP's 13th Quadrennial Solar-Terrestrial Physics Symposium, Xi'an, China (2014)
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)
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).