Lee, K. W.; Büchner, J.; Elkina, N.: Collisionless transport of energetic electrons in the solar corona at current-free double layers. Astronomy and Astrophysics 478, pp. 889 - 895 (2008)
Lee, K. W.; Büchner, J.; Elkina, N.: Current driven low-frequency electrostatic waves in the solar corona: Linear theory and nonlinear saturation. Physics of Plasmas 14, 112903 (2007)
Büchner, J.; Elkina, N.: Anomalous resistivity of current-driven isothermal plasmas due to phase space structuring. Physics of Plasmas 13, 082304 (2006)
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).