Dubinin, E.; Chanteur, G.; Fraenz, M.; Woch, J.: Field-aligned currents and parallel electric field potential drops at Mars. Scaling from the Earth aurora. Planetary and Space Science 56, pp. 868 - 872 (2008)
Dubinin, E.; Fraenz, M.; Woch, J.; Winningham, D.; Frahm, R.; Lundin, R.; Barabash, S.: Suprathermal electron fluxes on the nightside of Mars: ASPERA-3 observations. Planetary and Space Science 56, pp. 846 - 851 (2008)
Dubinin, E.; Modolo, R.; Fraenz, M.; Woch, J.; Duru, F.; Akalin, F.; Gurnett, D.; Lundin, R.; Barabash, S.; Plaut, J. J.et al.; Picardi, G.: Structure and dynamics of the solar wind/ionosphere interface on Mars. MEX-ASPERA-3 and MEX-MARSIS observations. Geophysical Research Letters 35, L11103 (2008)
Lundin, R.; Barabash, S.; Holmstrom, M.; Nilsson, H.; Yamauchi, M.; Fraenz, M.; Dubinin, E.: A comet-like escape of ionospheric plasma from Mars. Geophysical Research Letters 35, L18203 (2008)
Roussos, E.; Fraenz, M.; Dubinin, E.; Martinecz, C.; Woch, J.; Motschmann, U.; Winningham, J. D.; Frahm, R.; Barabash, S.; Lundin, R.: Energetic electron asymmetries at Mars: ASPERA-3 observations. Planetary and Space Science 56, pp. 836 - 839 (2008)
Baumgaertel, K.; Sauer, K.; Mjolhus, E.; Dubinin, E.: Fluid versus simulation model of solitons in solar wind: Application to Ulysses observations. Journal Geophysical Research 112, A12101 (2007)
Dubinin, E.; Fraenz, M.; Woch, J.; Barabash, S.; Lundin, R.; Yamauchi, M.: Hydrogen exosphere at Mars: Pickup protons and their acceleration at the bow shock. Geophysical Research Letters 33 (22), L22103 (2006)
Fränz, M.; Dubinin, E.; Roussos, E.; Woch, J.; Winningham, J. D.; Frahm, R.; Coates, A. J.; Fedorov, A.; Barabash, S.; Lundin, R.: Plasma Moments in the Environment of Mars. Space Science Reviews 126, pp. 165 - 207 (2006)
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".
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.