Sauer, K.; Dubinin, E.; McKenzie, J. F.: Solitons and oscillitons in multi-ion space plasmas. Nonlinear Processes in Geophysics 10, pp. 121 - 130 (2003)
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)
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)
Dubinin, E.; Sauer, K.; Delva, M.; Grard, R.; Livi, S.; Lundin, R.; Skalsky, A.; Schwingenschuh, K.; Szegö, K.; Trotignon, J.-G.: Multi-instrument study of the upstream region near Mars: Phobos-2 observations. Journal Geophysical Research 105, pp. 7557 - 7571 (2000)
Dubinin, E.; Sauer, K.; Delva, M.; Livi, S.; Lundin, R.; Skalsky, A.; Szego, K.: Deceleration of the solar wind upstream of the Martian bow schock. Mass-loading or foreshock features? Advances in Space Research 26, pp. 1627 - 1631 (2000)
Dubinin, E.; Sauer, K.: The Martian magnetosphere - a laboratory for bi-ion plasma investigations. Astrophysics and Space Science 264, pp. 273 - 288 (1999)
Dubinin, E.; Sauer, K.; Delva, M.; Tanaka, T.: The IMF control of the Martian bow shock and plasma flow in the magnetosheath. Predictions of 3D simulations and observations. Earth, Planets and Space 50, pp. 873 - 882 (1999)
Dubinin, E.; Sauer, K.; Delva, M.; Tanaka, T.: The IMF control of the Martian bow shock and plasma flow in the magnetosheath. Predictions of 3D simulations and observations. Earth, Moon and Planets 50, pp. 873 - 882 (1999)
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".