Modolo, R.; Chanteur, G.; Dubinin, E.; Matthews, A.: Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary. Annales Geophysicae 24, pp. 3403 - 3410 (2006)
Dubinin, E.; Sauer, K.; McKenzie, J. F.: Differential ion streaming in the solar wind as an equilibrium state. Journal Geophysical Research 110, A07101, p. 12 (2005)
McKenzie, J. F.; Dubinin, E. M.; Sauer, K.: Relativistic whistler oscillitons - do they exist? Nonlinear Processes in Geophysics 12 (3), pp. 425 - 431 (2005)
Modolo, R.; Chanteur, G. M.; Dubinin, E.; Matthews, A. P.: Influence of the solar EUV flux on the Martian plasma environment. Annales Geophysicae 23 (2), pp. 433 - 444 (2005)
Webb, G. M.; McKenzie, J. F.; Dubinin, E. M.; Sauer, K.: Hamiltonian formulation of nonlinear travelling Whistler waves. Nonlinear Processes in Geophysics 12 (5), pp. 643 - 660 (2005)
Dubinin, E.; Sauer, K.; McKenzie, J. F.: Nonlinear stationary waves and solitons in ion beam-plasma configuration. Journal Geophysical Research 109 (A2), A02208 (2004)
Verheest, F.; Cattaert, T.; Dubinin, E.; Sauer, K.; McKenzie, J. F.: Whistler oscillitons revisited: the role of charge neutrality? Nonlinear Processes in Geophysics 11 (4), pp. 447 - 452 (2004)
Dubinin, E.; Sauer, K.; McKenzie, J. F.: Solitons and oscillitons in cold bi-ion plasmas: a parameter study. Journal of Plasma Physics 68, pp. 27 - 52 (2002)
Dubinin, E.; Sauer, K.; McKenzie, J. F.; Chanteur, G.: Nonlinear waves and solitons propagating perpendicular to the magnetic field in bi-ion plasma with finite plasma pressure. Nonlinear Processes in Geophysics 9, pp. 87 - 99 (2002)
Dubinin, E.; Skalsky, A.; Song, P.; Savin, S.; Kozyra, J.; Moore, T. E.; Russell, C. T.; Chandler, M. O.; Fedorov, A.; Avanov, L.et al.; Sauvaud, J. A.; Friedel, R. H. W.: Polar-Interball coordinated observations of plasma and magnetic field characteristics in the regions of the northern and southern distant cusps. Journal Geophysical Research 107 (A5), 1053 (2002)
McKenzie, J. F.; Dubinin, E.; Sauer, K.: Nonlinear waves propagating transverse to the magnetic field. Journal of Plasma Physics 65, pp. 213 - 233 (2001)
McKenzie, J. F.; Sauer, K.; Dubinin, E.: Stationary waves in a bi-ion plasma transverse to the magnetic field. Journal of Plasma Physics 65, pp. 197 - 212 (2001)
Sauer, K.; Dubinin, E.; McKenzie, J. F.: New type of soliton in bi-ion plasmas and possible implications. Geophysical Research Letters 28, pp. 3589 - 3592 (2001)
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).
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.
The launch was successful; the ESA’s space probe JUICE is now on its way to the Jupiter system. There, it will primarily study the gas giant's icy moons.
ESA's space probe is on the move: First it heads for the launch site in Kourou - and in April it will begin its long journey to Jupiter and its icy moons.