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Sauer, K.; Dubinin, E.; McKenzie, J. F.: Solitons and oscillitons in complex plasmas. In: Dusty Plasmas in the New Millenium, pp. 220 - 223 (Eds. Bharuthram, R.; Hellberg, M. A.; Shukla, P. K.; Verheest, F.). UPAP, ICTP, Melville, New York (2002)
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Grigorenko, E.; Shuvalov, S.; Malova, H.; Dubinin, E.; Popov, V.; Zelenyi, L.: Influence of quasi-adiabatic ion dynamics on the current sheet structure observed in the Martian magnettail by MAVEN. Mars Aeronomy Conference, Boulder, Colorado, USA (2017)
Shuvalov, S.; Vaisberg, O.; Ermakov, V.; Zelenyi, L.; Znobishchev, A.; Dubinin, E.: Analysis of solar wind-Mars interaction region and pick-up ions from MAVEN measurements on January 04, 2015. Mars Aeronomy Conference, Boulder, Colorado, USA (2017)
Vaisberg, O.; Ermakov, V.; Shuvalov, S.; Zelenyi, L.; Znobishchev, A.; Dubinin, E.: Analysis of the magnetic barrier of Mars as observed on MAVEN on January 4, 2015. Mars Aeronomy Conference, Boulder, Colorado, USA (2017)
Dubinin, E.; Fraenz, M.; Andrews, D.; Morgan, D.: Ionosphere of Mars observed by Mars Express. European Geosciences Union General Assembly, Vienna, Austria (2016)
Dubinin, E.; Fraenz, M.; Modolo, R.: Distribution and dynamics of plasma in the magnetospheres of Venus and Mars. International Venus Conference, Oxford, U.K. (2016)
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".