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Roussos, E.; Andriopoulou, M.; Krupp, N.; Kotova, A.; Paranicas, C.; Krimigis, S. M.; Mitchell, D. G.: Numerical simulation of energetic electron microsignature drifts at Saturn: Methods and applications. Icarus 226 (2), pp. 1595 - 1611 (2013)
Andriopoulou, M.; Roussos, E.; Krupp, N.; Paranicas, C.; Thomsen, M.; Krimigis, S.; Dougherty, M. K.; Glassmeier, K. -.: A noon-to-midnight electric field and nightside dynamics in Saturns inner magnetosphere, using microsignature observations. Icarus 220, pp. 503 - 513 (2012)
Thomsen, M. F.; Roussos, E.; Andriopoulou, M.; Kollmann, P.; Arridge, C. S.; Paranicas, C. P.; Gurnett, D. A.; Powell, R. L.; Tokar, R. L.; Young, T. D.: Saturn's inner magnetospheric convection pattern: Further evidence. Journal Geophysical Research 117, A09208 (2012)
Roussos, E.; Krupp, N.; Mitchell, D. G.; Paranicas, C.; Palmaerts, B.; Paranicas, C.; Krimigis, S. M.; Andriopoulou, M.; Kurth, W. S.; Badman, S.et al.; Masters, A.; Dougherty, M. K.: Quasi-Periodic injections of relativistic electrons in Saturn's magnetosphere. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
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).