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 Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
The Sun’s planets and small objects have undergone substantial evolution. Deciphering the history of our cosmic home is not a simple task even though we now have access to a multitude of data gathered by space missions, remote observations, and laboratory studies of diverse samples. A significant fraction of materials available for the study of planetary bodies come from meteorites.