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)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".