Becker, G.; Knapmeyer-Endrun, B.: Moho depth across the Trans-European Suture Zone from ambient vibration autocorrelations. European Geosciences Union General Assembly, Vienna, Austria (2017)
Dimech, J.-L.; Knapmeyer-Endrun, B.; Weber, R. C.: A new moonquake catalog from Apollo 17 geophone data. 48th Lunar and Planetary Science Conference, The Woodlands, Texas (2017)
Becker, G.; Knapmeyer-Endrun, B.: Crustal thickness in central Europe from single-station seismic noise autocorrelation analysis. European Geosciences Union General Assembly, Vienna, Austria (2016)
Knapmeyer-Endrun, B.; Golombek, M.; Ohrnberger, M.: Shallow structure of the InSight 2018 landing site in Elysium Planitia, Mars, from ambient vibration Rayleigh wave ellipticity: A modeling study. AGU Fall Meeting, San Francisco, USA (2016)
Becker, G.; Knapmeyer-Endrun, B.: Moho depth from single-station seismic noise autocorrelations in preparation of the InSight SEIS installation on Mars. 41. Sitzung der AG Seismologie, Wildbad-Kreuth, Germany (2015)
Knapmeyer-Endrun, B.; Hammer, C.: Applying a Hidden Markov Model-based event detection and classification algorithm to Apollo lunar seismic data. AGU Fall Meeting, San Francisco, USA (2014)
Krueger, F.; Knapmeyer-Endrun, B.; Group, t. P. W.: Crustal and lithospheric structure across the boundary of the East European Craton from receiver functions. AGU Fall Meeting, San Francisco, USA (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.