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標(biāo)題: Titlebook: Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles; O. D. Rode,A. V. Ivanov,В. Гейл Book 1979 Springer Scienc [打印本頁(yè)]

作者: Alacrity    時(shí)間: 2025-3-21 18:00
書目名稱Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles影響因子(影響力)




書目名稱Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles影響因子(影響力)學(xué)科排名




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書目名稱Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles讀者反饋




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作者: 指耕作    時(shí)間: 2025-3-21 21:50
Atlas of Photomicrographs of the Surface Structures of Lunar Regolith Particles978-94-009-9359-4
作者: 切碎    時(shí)間: 2025-3-22 02:09
Book 1979 three-dimensional description of rocks was replaced by the study of thin sections, since the optical microscope does not permit examination of an uneven surface as a result of a restricted depth of observation field. The art of ancient naturalists of conceiving the object in its entirety, with all
作者: 過渡時(shí)期    時(shí)間: 2025-3-22 06:06

作者: Ingest    時(shí)間: 2025-3-22 12:17

作者: 無目標(biāo)    時(shí)間: 2025-3-22 16:46
https://doi.org/10.1007/1-84628-252-7h 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
作者: CAJ    時(shí)間: 2025-3-22 20:05

作者: 匯總    時(shí)間: 2025-3-23 00:24

作者: Defense    時(shí)間: 2025-3-23 01:46
https://doi.org/10.1007/978-94-009-9359-4evolution; geomorphology; mineral; petrography
作者: 通便    時(shí)間: 2025-3-23 06:17

作者: 驚奇    時(shí)間: 2025-3-23 10:20
http://image.papertrans.cn/b/image/164431.jpg
作者: INERT    時(shí)間: 2025-3-23 16:24
https://doi.org/10.1007/1-84628-252-7Surfaces of lunar regolith particles were studied with a JEOL JXM-2 scanning electron microscope and a JEOL JXA-50A instrument, combining a scanning electron microscope and X-ray microanalyzer.
作者: 龍卷風(fēng)    時(shí)間: 2025-3-23 19:59
https://doi.org/10.1007/1-84628-252-7Scanning electron microscopy enabled the surface morphology of lunar regolith particles to be studied in detail. Its thorough examination contributed to the recognition of the principal processes that led to the origin and evolution of the regolith.
作者: 大漩渦    時(shí)間: 2025-3-23 22:17

作者: 魯莽    時(shí)間: 2025-3-24 03:07

作者: 溫和女人    時(shí)間: 2025-3-24 06:36

作者: 致命    時(shí)間: 2025-3-24 12:40
https://doi.org/10.1007/1-84628-252-7cesses 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.
作者: 進(jìn)步    時(shí)間: 2025-3-24 17:12
Book 1979ic 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
作者: ineluctable    時(shí)間: 2025-3-24 20:42
https://doi.org/10.1007/1-84628-252-7d 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.
作者: 北京人起源    時(shí)間: 2025-3-24 23:46
f scientific 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 characteristi
作者: 雕鏤    時(shí)間: 2025-3-25 06:36
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.
作者: acrobat    時(shí)間: 2025-3-25 08:22

作者: JIBE    時(shí)間: 2025-3-25 13:02
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.
作者: wall-stress    時(shí)間: 2025-3-25 18:54
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.
作者: triptans    時(shí)間: 2025-3-25 23:04

作者: 大方一點(diǎn)    時(shí)間: 2025-3-26 04:08
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
作者: Hiatal-Hernia    時(shí)間: 2025-3-26 08:08
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
作者: 遵循的規(guī)范    時(shí)間: 2025-3-26 08:28
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.
作者: 草率女    時(shí)間: 2025-3-26 15:08

作者: Nonthreatening    時(shí)間: 2025-3-26 19:35
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