Knapmeyer-Endrun, B.; Krülger, F.; Geissler, W. H.; Group, t. P. W.: Upper mantle structure across the Trans-European Suture Zone imaged by S-receiver functions. Earth and Planetary Science Letters 458, pp. 429 - 441 (2017)
Knapmeyer-Endrun, B.; Hammer, C.: Identification of new events in Apollo 16 lunar seismic data by Hidden Markov Model-based event detection and classification. Journal Geophysical Research 120, pp. 1620 - 1645 (2015)
Becker, G.; Knapmeyer-Endrun, B.: Crustal thickness across Central Europe from seismic noise autocorrelation analysis. Rocks \& Stars II, Göttingen, Germany (2017)
Dimech, J.-L.; Knapmeyer-Endrun, B.; Philips, D.; Weber, R.: A new moonquake catalog from Apollo 17 geophone data. European Geosciences Union General Assembly, Vienna, Austria (2017)
Knapmeyer-Endrun, B.; the InSight Science Team: Crustal and shallow subsurface seismology on InSight. ISSI-BJ Lunar and Planetary Seismology Forum, Beijing, China (2017)
Knapmeyer-Endrun, B.: Crustal S-velocity from P-wave polarization - Tests with receiver functions from Instaseis Mars synthetics. 43. Sitzung der AG Seismologie, Bad Breisig, Göttingen (2017)
Knapmeyer-Endrun, B.; Golombek, M. P.; Ohrnberger, M.: Rayleigh wave ellipticity modeling and inversion for shallow sub-surface structure at the InSight landing site in Elysium Planitia, Mars. 42. Sitzung der AG Seismologie, Bad Salzschlirf, Germany (2016)
Knapmeyer-Endrun, B.; Krueger, F.; Geissler, W. H.: Upper mantle structure across the Trans-European Suture Zone from S-receiver functions. European Geosciences Union General Assembly, Vienna, Austria (2016)
Knapmeyer-Endrun, B.: InSight - a geophysical mission to planet Mars in 2016. Institutskolloquium Institut fur Erd- und Umweltwissenschaften, Potsdam, Germany (2015)
Knapmeyer-Endrun, B.; Hammer, C.: New events identified in Apollo 16 lunar seismic data by Hidden Markov model based event detection and classification. 41. Sitzung der AG Seismologie, Wildbad-Kreuth, Germany (2015)
Knapmeyer-Endrun, B.; Hammer, C.: New seismic events identified in the Apollo lunar data by application of a Hidden Markov Model. European Planetary Science Congress, Nantes, France (2015)
Knapmeyer-Endrun, B.: Preparing the installation of station ELYS: The InSight mission to Mars. 40. Sitzung der Arbeitsgemeinschaft Seismologie der FKPE, Gross-Doelln, Germany (2014)
Knapmeyer-Endrun, B.: Red planet, seismologically dead planet? The InSight mission to Mars. Working Group Seminar General Geophysics/Seismology, Potsdam, Germany (2014)
Knapmeyer-Endrun, B.; Geissler, W.; Krueger, F.; Legandre, C.: The outline of a cratonic margin: Mapping structure across the Trans-European Suture Zone with receiver functions. Seminar aktuelle Forschungsthemen, Kiel, Germany (2014)
Becker, G.; Knapmeyer-Endrun, B.: Crustal thickness and vp/vs-ratios from single-station auto-and cross-correlations of seismic noise. European Geosciences Union General Assembly (EGU), Vienna, Austria (2018)
Knapmeyer-Endrun, B.; Ceylan, S.; van Driel, M.; the InSight Science Team: Martian crustal S-wave velocities from apparent incidence angles - a case study for InSight. European Geosciences Union General Assembly, Vienna, Austria (2018)
Knapmeyer-Endrun, B.; Ceylan, S.; van Driel, M.: Martian crustal S-wave velocities from P-wave polarization - a test study for InSight. 49th Lunar and Planetary Science Conference, The Woodlands, Texas (2018)
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".