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)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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).
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.