TY - JOUR A1 - Elbers, Gereon A1 - Lehmann, G. T1 - Electron paramagnetic resonance of Vanadyl ion impurities in crystalline solids: A comment JF - Journal of Physics and Chemistry of Solids. 46 (1985), H. 6 Y1 - 1985 SN - 0022-3697 SP - 761 ER - TY - JOUR A1 - Elbers, Gereon A1 - Lehmann, G. T1 - Electron Paramagnetic Resonance and Optical Absorption Spectra of VO2+ in CsCl Single Crystals JF - Zeitschrift für Naturforschung / Section A, a journal of physical sciences. 40 (1985) Y1 - 1985 SN - 0932-0784 SP - 511 ER - TY - JOUR A1 - Elbers, Gereon A1 - Remme, S. A1 - Lehmann, G. T1 - EPR of Cr3+ in Tris(acetylacetonato)gallium(III) Single Crystals JF - Inorganic Chemistry. 25 (1986) Y1 - 1986 SN - 0020-1669 SP - 896 EP - 897 ER - TY - JOUR A1 - Elbers, Gereon A1 - Remme, S. A1 - Lehmann, G. T1 - EPR and Optical Absorption of Cr3+ in CsCl and CsBr JF - Physica Status Solidi (B). 142 (1987), H. 2 Y1 - 1987 SN - 0031-8957 SP - 367 EP - 377 ER - TY - CHAP A1 - Baader, Fabian A1 - Reiswich, M. A1 - Bartsch, M. A1 - Keller, D. A1 - Tiede, E. A1 - Keck, G. A1 - Demircian, A. A1 - Friedrich, M. A1 - Dachwald, Bernd A1 - Schüller, K. A1 - Lehmann, R. A1 - Chojetzki, R. A1 - Durand, C. A1 - Rapp, L. A1 - Kowalski, Julia A1 - Förstner, R. T1 - VIPER - Student research on extraterrestrical ice penetration technology T2 - Proceedings of the 2nd Symposium on Space Educational Activities N2 - Recent analysis of scientific data from Cassini and earth-based observations gave evidence for a global ocean under a surrounding solid ice shell on Saturn's moon Enceladus. Images of Enceladus' South Pole showed several fissures in the ice shell with plumes constantly exhausting frozen water particles, building up the E-Ring, one of the outer rings of Saturn. In this southern region of Enceladus, the ice shell is considered to be as thin as 2 km, about an order of magnitude thinner than on the rest of the moon. Under the ice shell, there is a global ocean consisting of liquid water. Scientists are discussing different approaches the possibilities of taking samples of water, i.e. by melting through the ice using a melting probe. FH Aachen UAS developed a prototype of maneuverable melting probe which can navigate through the ice that has already been tested successfully in a terrestrial environment. This means no atmosphere and or ambient pressure, low ice temperatures of around 100 to 150K (near the South Pole) and a very low gravity of 0,114 m/s^2 or 1100 μg. Two of these influencing measures are about to be investigated at FH Aachen UAS in 2017, low ice temperature and low ambient pressure below the triple point of water. Low gravity cannot be easily simulated inside a large experiment chamber, though. Numerical simulations of the melting process at RWTH Aachen however are showing a gravity dependence of melting behavior. Considering this aspect, VIPER provides a link between large-scale experimental simulations at FH Aachen UAS and numerical simulations at RWTH Aachen. To analyze the melting process, about 90 seconds of experiment time in reduced gravity and low ambient pressure is provided by the REXUS rocket. In this time frame, the melting speed and contact force between ice and probes are measured, as well as heating power and a two-dimensional array of ice temperatures. Additionally, visual and infrared cameras are used to observe the melting process. Y1 - 2018 SP - 1 EP - 6 ER -