Verscharen, D.: Schwach kompressive, hochfrequente Wellen im inhomogenen Multifluid-Plasma. Mitteilungen der Deutschen Geophysikalischen Gesellschaft e.V. 3, pp. 5 - 9 (2011)
Verscharen, D.; Marsch, E.: Compressive high-frequency waves riding on an Alfvén/ion-cyclotron wave in a multi-fluid plasma. Journal of Plasma Physics 77, pp. 693 - 707 (2011)
Fahr, H.-J.; Chashei, I. V.; Verscharen, D.: Injection to the pick-up ion regime from high energies and induced ion power-laws. Astronomy and Astrophysics 505, pp. 329 - 337 (2009)
Fahr, H.-J.; Verscharen, D.: Spectral intensities of Anomalous Cosmic Rays derived from the injection rate at the solar wind termination shock. Astrophysics and Space Sciences Transactions 5, pp. 21 - 30 (2009)
Verscharen, D.; Fahr, H.-J.: Solar wind proton reflection and injection to the ACR regime at the parallel termination shock. Astrophysics and Space Sciences Transactions 5, pp. 15 - 19 (2009)
Verscharen, D.: On convected wave structures and spectral transfer in space plasmas - applications to solar corona and solar wind. Dissertation, Technische Universität Braunschweig (2012)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
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).