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We simulate the OH/H2O production from the action of keV protons on the lunar regolith using a vacuum chamber and a mass analyzer to examine the molecular products released from olivine and SiO2 powders during their irradiation by deuterium ions. The measured mass spectra, showing the OD/D2O signature, confirm the possibility of OH/H2O formation on the lunar surface by solar-wind hydrogen. 相似文献
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G. G. Managadze R. Z. Sagdeev A. E. Chumikov V. T. Cherepin G. Z. Saralidze 《Solar System Research》2010,44(5):385-392
The onboard time-of-flight mass reflectron MANAGA-F is described which is aimed at measuring the elemental and isotopic composition
of the secondary ion fluxes generated under the influence of solar wind. It is shown that by using this apparatus, the composition
of the surface regolith layer averaged over a considerable area can be determined while approaching Phobos. After the landing
of the spacecraft on the surface of Phobos, the measurements will be aimed at examining the local characteristics of the regolith
and a new mechanism for water synthesis in the process of ion collisions. The apparatus allows for the mass of the secondary
molecular ions to be detected and determined, including organic ones which arise during the bombardment of the regolith by
ions of different origins. The main scientific problems to be solved using the given apparatus are considered in the paper.
The working principle of the apparatus together with its analytical and technical characteristics and design particularities
are presented. Information concerning the range of its applications for solving a number of challenging tasks of contemporary
science is given. The MANAGA-F apparatus is shown to be the first realization of an original new-generation onboard device
that has been invented, developed, and produced at the Space Research Institute of the Russian Academy of Sciences (SRI RAS). 相似文献
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