Engrand, C.; Duprat, J.; Bardin, N.; Dartois, E.; Leroux, H.; Quirico, E.; Benzerara, K.; Rémusat, L.; Dobrica, E.; Delauche, L.et al.; Bradley, J.; Ishii, H.; Hilchenbach, M.; The COSIMA Team: The asteroid-comet continuum from laboratory and space analyses of comet samples and micrometeorites. IAU General Assembly Meeting, Honolulu, USA (2015)
Hilchenbach, M.: Rosetta Philae - Impact on a Comet as Envisioned by Multibody Simulations. The 2015 SIMULIA Community Conference, Berlin, Germany (2015)
Hilchenbach, M.; Hornung, K.; Kissel, J.; Langevin, Y.; Merouane, S.; The COSIMA Team: Mechanical properties of cometary dust particles as observed in the inner coma of 67P/Churyumov-Gerasimenko. IAU General Assembly Meeting, Honolulu, USA (2015)
Hilchenbach, M.; Kissel, J.; Langevin, Y.; Briois, C.; Koch, A.; Schulz, R.; Silen, J.; Rynö, J.: Dust particles in the inner coma of Comet 67P/Churyumov-Gerasimenko. European Geosciences Union General Assembly, Vienna, Austria (2015)
Langevin, Y.; Hilchenbach, M.; Ligier, N.; Merouhane, S.; Hornung, K.: Typology of dust particles collected by the COSIMA mass spectrometer in the inner coma of 67P/Churyumov Gerasimenko from Rendez-Vous to perihelion. European Planetary Science Congress, Nantes, France (2015)
Levasseur-Regourd, A.-C.; Rotundi, A.; Bentley, M.S.; DellaCorte, V.; Fulle, M.; Hadamick, E.; Hilchenbach, M.; Hines, D.; Lasue, J.; Merouane, S.et al.; Renard, J.-B.: Physical properties of dust particles in cometary comae: from clues to evidence with the Rosetta mission. European Planetary Science Congress, Nantes, France (2015)
Apathy, I.; Hilchenbach, M.; Remizov, A.; Auster, H.-U.; Berghofer, G.: Envisaged plasma and magnetic field measurements onboard the Rosetta Lander Philae on comet 67P/Churyumov-Gerasimenko. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Fray, N.; Bardyn, A.; Briois, C.; Cottin, H.; Engrand, C.; Le Roy, L.; Siljeström, S.; Thirkell, L.; Varmuza, K.; Hilchenbach, M.: The organic content of comets: How to get prepared for the COSIMA TOF-SIMS measurements onboard the ROSETTA spacecraft. European Planetary Science Congress, Cascais, Portugal (2014)
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".
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.