NAOC Open IR
月壤中的氦-3
徐琳; 邹永廖; 刘建忠
2003
Source Publication矿物学报
ISSN1000-4734
Volume023Issue:004Pages:374
Abstract除了极少数非常陡峭的山脉与撞击坑和火山通道的峭壁外,整个月球表面几乎都被一层厚度不等的月尘、岩屑和岩块的混合堆积物即月壤所覆盖。由于月球无大气层等特殊环境,太阳光长驱直入,太阳风粒子直接注入到月壤细小颗粒上使月壤中富含稀有气体等太阳风粒子组分。本文在系统阐述月壤的形成过程与形成机制的基础上,分析了月壤中稀有气体的来源及其浓度与月壤的成熟度、月壤颗粒大小、月壤矿物组成和化学成分的相关关系,进而利用已有的探测数据和分析结果,对月壤中氦-3资源的开发利用前景进行了初步评估。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/40512
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
徐琳,邹永廖,刘建忠. 月壤中的氦-3[J]. 矿物学报,2003,023(004):374.
APA 徐琳,邹永廖,&刘建忠.(2003).月壤中的氦-3.矿物学报,023(004),374.
MLA 徐琳,et al."月壤中的氦-3".矿物学报 023.004(2003):374.
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