Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on the depth of an average supergranule through forward modeling in time-distance helioseismology. Rocks \& Stars II, Göttingen, Germany (2017)
Cameron, R. H.; Schüssler, M.: The Babcock-Leighton solar dynamo. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Jiang, J.; Cameron, R. H.; Schüssler, M.: The cause of the weak solar cycle 24. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on supergranular depth obtained through the resolution of the forward problem in local helioseismology. Astronomische Gesellschaft Meeting, Göttingen, Germany (2017)
Asvestari, E.; Usoskin, I. G.; Krivova, N. A.; Cameron, R. H.: Semi-empirical long-term reconstruction of the heliospheric parameters validated by cosmogenic radionuclide records. Coimbra Solar Physics Meeting CSPM-2015: Ground-based Solar Observations in the Space Instrumentation Era, Coimbra, Portugal (2015)
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".