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  • Other Sources  (4)
  • NUCLEAR ENGINEERING  (3)
  • ASTRONAUTICS (GENERAL)  (1)
  • 1
    Publication Date: 2019-06-27
    Description: Horn and Von Oertzen (1967) have shown that tracks in mica are produced by an irradiation with 32-MeV O-16 ions. These tracks were attributed to K and Fe recoils produced by elastic scattering of the incident oxygen beam. In the present work an alternate explanation of their observations is provided. The measured characteristics of the tracks are shown to be compatible with theoretical predictions for production of tracks by inelastic (mostly compound nucleus) reactions with silicon and to be inconsistent with the previously proposed elastic scattering process. The possibility that the tracks are produced by contaminant ions in the beam cannot be ruled out.
    Keywords: NUCLEAR ENGINEERING
    Type: Radiation Effects; 19; 1973
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  • 2
    Publication Date: 2019-07-13
    Description: Heavy ion tracks in silicate minerals, using thermal annealing to identify origins
    Keywords: NUCLEAR ENGINEERING
    Type: INTERNATIONAL TOPICAL CONFERENCE ON NUCLEAR TRACK REGISTRATION IN INSULATING SOLIDS AND APPLICATIONS; May 01, 1969; CLERMONT-FERRAND, PUY-DE DOME; FRANCE|; VUE SCIENTIFIQUE ET
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  • 3
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    In:  Other Sources
    Publication Date: 2019-07-13
    Description: Heavy ion track registration in nonconductor minerals, discussing radiation damage and atomic species along trajectory
    Keywords: NUCLEAR ENGINEERING
    Type: INTERNATIONAL TOPICAL CONFERENCE ON NUCLEAR TRACK REGISTRATION IN INSULATING SOLIDS AND APPLICATIONS; May 01, 1969; CLERMONT-FERRAND, PUY-DE DOME; FRANCE|; VUE SCIENTIFIQUE ET
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  • 4
    Publication Date: 2019-07-12
    Description: In connection with the establishment of a lunar base, it would be necessary to provide water, and the feasibility to obtain water from solar wind (SW) implanted lunar soils has been considered. In this context, a project involving the examination of materials under conditions of simulated SW irradiation has been initiated. A description is presented of initial results on oligoclase, ilmenite, and simulated lunar glass (SLG). Attention is given to the reaction chamber, the target materials, the saturation concentrations, aspects of water release, depth profiles, thermal release, effects from helium-3 preimplants, mechanisms of possible water release related to direct emission and thermal release, and lunar soil components enriched in trapped SW hydrogen. It is found that ilmenite stores about twice as much deuterium as the other target materials. However, it is unknown whether the small enrichment factor will be sufficient to make the material a potential source of lunar water.
    Keywords: ASTRONAUTICS (GENERAL)
    Type: Journal of Geophysical Research (ISSN 0148-0227); 91; D467-D47
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