Kronberg, E. A.; Smirnov, A. G.; Latallerie, F.; Daly, P. W.; Aseev, N.; Shprits, Y. Y.; Kellerman, A.; Kasahara, S.; Turner, D.; Taylor, M. G. G. T.: Evolution of energetic electron intensities in the radiation belts measured by Cluster/RAPID during 1.5 solar cycles. 29th Cluster workshop, Lanzarote, Canary Islands, Spain (2019)
Kronberg, E. A.: On the role of heavy energetic ions for the dynamics of the magnetosphere: Cluster observations. Ion Composition in the Sun Earth System (ICSES), Durango, USA (2019)
Kronberg, E. A.; Grigorenko, E.; Kozak, L.; Gorman, J.; Malykhin, A.; Petrenko, B.; Smirnov, A.; Daly, P. W.; Malova, H.: Energy transformation, turbulence and acceleration in space plasmas: why it is cool to be together? VWS Symposium, Dresden, Germany (2019)
Kellerman, A.; Kronberg, E. A.: Cluster RAPID data computed in adiabatic invariant coordinates: A long-term data product for radiation belt research and data assimilation. 24th Cluster Cross-Calibration Workshop, Maspalomas, Gran Canaria, Spain (2018)
Smirnov, A.; Kronberg, E. A.; Daly, P. W.: Electron intensity measurements in the radiation belts. 24th Cluster Cross-Calibration Workshop, Maspalomas, Gran Canaria, Spain (2018)
Kronberg, E. A.; Luo, H.; Nykyri, K.; Trattner, K. J.; Daly, P. W.; Grigorenko, E.: The energetic particle properties in the magnetosphere: results based on statistics from Cluster/RAPID observations. 5th Cluster-Themis Workshop, Chania, Greece (2018)
Kronberg, E. A.: Sources of Soft X-rays in the magnetosphere. ISSI meeting “Soft Protons in the Magnetosphere focused by X-ray Telescopes”, Bern, Switzerland (2018)
Kronberg, E. A.; Grigorenko, E.; Turner, D.; Daly, P. W.; Khotyaintsev, Y.; Kozak, L.: Comparing and contrasting dispersionless injections at geosynchronous orbit during a substorm event. COSPAR 2018, Pasadena, CA, USA (2018)
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.