Westlake, J.; McNutt, R.; Kasper, J.; Battista, C.; Case, A.; Cochrane, C.; Grey, M.; Jia, X.; Kivelson, M.; Kim, C.et al.; Korth, H.; Khurana, K.; Krupp, N.; Paty, C.; Roussos, E.; Rymer, A.; Stevens, M.; Slavin, J.; Smith, H.; Saur, J.; Coren, D.: The Plasma Instrument for Magnetic Sounding (PIMS) on the Europa Clipper Mission. AGU Fall Meeting, New Orleans, USA (2017)
Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Galactic Cosmic Rays access to the upper atmosphere and rings of Saturn. AGU Fall Meeting, San Francisco, USA (2016)
Regoli, L. H.; Roussos, E.; Luhmann, J.; Dialynas, K.; Krupp, N.; Jones, G. H.; Coates, A. J.: Energetic environment at Titan's orbit. AGU Fall Meeting, San Francisco, USA (2016)
Lee-Payne, Z.; Grande, M.; Krupp, N.; Paranicas, C.; Roussos, E.; Kollmann, P.: Re-evaluating Galileo Energetic Particle Detector data based on radiation detector decay; for use in estimating Sputtering Erosion rates on Europa. European Planetary Science Congress EPSC , Nantes, France (2015)
Palmaerts, B.; Roussos, E.; Krupp, N.; Kurth, W. S.; Mitchell, D. G.; Dougherty, M. K.: Statistical analysis and multi-instrument overview of the quasi-periodic 1-hour pulsations in Saturn's outer magnetosphere. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Coates, A.; Thomsen, M.; Feyerabend, M.; Jones, G.; Roussos, E.; Krupp, N.: Pickup Ion Signatures in the Vicinity of Titan. AGU Fall Meeting, San Francisco, USA (2015)
Roussos, E.; Krupp, N.; Fraenz, M.; Kollmann, P.; Truscott, P.; Futaana, Y.: Hot Plasma Environment Model (HPEM): A empirical model for describing time-dependent processes of the jovian energetic electron environment. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Tracing of energetic particles in the vicinity of Titan. European Geosciences Union General Assembly, Vienna, Austria (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. 10 years of Cassini-Huygens in the Saturnian system, London, UK (2014)
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".