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Titlebook: Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles; O. D. Rode,A. V. Ivanov,В. Гейл Book 1979 Springer Scienc

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樓主: Alacrity
21#
發(fā)表于 2025-3-25 06:36:55 | 只看該作者
https://doi.org/10.1007/1-84628-252-7ds, consists of minute fragments of crystalline rocks and minerals, of welded and brecciated agglomerates and partly melted particles. The average size of regolith particles (i.e. < 1 mm) is controlled by the degree of its exogenic reworking; it varies between 60 and 100 μm as a rule.
22#
發(fā)表于 2025-3-25 08:22:17 | 只看該作者
23#
發(fā)表于 2025-3-25 13:02:55 | 只看該作者
Preface,d by laboratory analyses. The goniometric study of a crystal, for example, has developed into the determination of constants of the crystal lattice, but the examination of minerals from a specific deposit was concerned primarily with the chemical analysis of their admixtures.
24#
發(fā)表于 2025-3-25 18:54:01 | 只看該作者
https://doi.org/10.1007/1-84628-252-7clusions in rock fragments and of newly formed minerals produced by exogenic processes have also been the subject of our study. The surface morphology of lunar regolith particles is shown in 164 photographs.
25#
發(fā)表于 2025-3-25 23:04:15 | 只看該作者
26#
發(fā)表于 2025-3-26 04:08:43 | 只看該作者
Preface,ic facts. At the same time, however, in studying natural bodies, primary attention has not been paid to their total character; the body either ceased to be an individual, as in the case of mathematical methods, or has become a complex of separate, not always closely connected characteristics examine
27#
發(fā)表于 2025-3-26 08:08:58 | 只看該作者
Introduction,h was transported from the place of its original occurrence. This heterogeneous mixture, dark-gray or black in the maria and light-gray in the highlands, consists of minute fragments of crystalline rocks and minerals, of welded and brecciated agglomerates and partly melted particles. The average siz
28#
發(fā)表于 2025-3-26 08:28:34 | 只看該作者
Morphological Characteristics of the Surface of Lunar Regolith Particles,cesses that were active on the lunar surface. This chapter describes the surface features of the principal types of lunar regolith particles (from the Luna-16 and Luna-20 materials), as determined by the use of a scanning electron microscope and X-ray microprobe analysis.
29#
發(fā)表于 2025-3-26 15:08:40 | 只看該作者
30#
發(fā)表于 2025-3-26 19:35:17 | 只看該作者
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