非均匀月壤介质的被动微波辐射传输模拟   总被引：1，自引：1，他引：0  

孟治国  陈圣波  刘财  杜晓娟  吕航 《吉林大学学报(地球科学版)》2008,38(6)

基于非均匀月壤物理模型和辐射传输方程,模拟月壤介质中的微波辐射传输特性,探讨频率、月壤厚度等与月表亮温的关系。结果表明:在低频段,月壤微波辐射亮温的动态变化范围较大,可探测的月壤厚度大,3 GHz时的最大可探测月壤厚度达12.4 m;在高频段对应的可探测月壤厚度较小,特别是从50GHz往后的频率段内,最大可探测月壤厚度均小于2 m。不同频率的亮温-厚度变化曲线没有交叉点,且频率越高,所能探测的月壤厚度越小。根据模拟结果,建立了月壤厚度与亮温的查找表。基于查找表,利用单个波段的亮温数据即可得到月壤厚度信息。  相似文献   

月球某些资源的开发利用前景   总被引：18，自引：0，他引：18  

欧阳自远  邹永廖等 《地球科学》2002,27(5):498-503

21世纪月球探测的主要趋势是建立月球基地，开发利用月球的矿产资源，能源和特殊环境，为人类社会的可持续发展发挥长期而有效的支撑作用，通过对月海玄武岩中的钛铁矿，克里普岩中的U，Th,REE和月壤中的拟－3在月面的含量与分布的系统分析，月海玄武碉中蕴藏有极丰富的钛铁矿，TiO2总资源量超过70万亿t，钛铁矿还是月球基地生产水和火箭燃料的主要原料；克里普岩是未来月球探测与研究的热点之一，其蕴藏有巨量的铀，钍，钾，磷和稀土元素资源；月壤长期受到太阳风的辐射，使其蕴藏有极其丰富的氢，氦，氧，氮等气体资源，其中氦－3的资源量大于100万t，它是一种可供人类社会长期使用的，安全，清洁，高效，廉价的核聚变发电燃料，其含量与月壤的化学成分，矿物组分，颗粒大小等有密切的关系。  相似文献   

月壤中的氦-3     

徐琳  邹永廖  刘建忠 《矿物学报》2003,23(4):374-378

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。  相似文献   

Noble Gases in the Lunar Regolith     

邹永廖  徐琳  欧阳自远 《中国地球化学学报》2003,22(4):361-368

The most fundamental character of lunar soil is its high concentrations of solar-wind-implanted elements, and the concentrations and behavior of the noble gases He, Ne, Ar, and Xe, which provide unique and extensive information about a broad range of fundamental problems. In this paper, the authors studied the forming mechanism of lunar regolith, and proposed that most of the noble gases in lunar regolith come from the solar wind. Meteoroid bombardment controls the maturity of lunar soil, with the degree of maturation decreasing with grain size; the concentrations of the noble gases would be of slight variation with the depth of lunar soil but tend to decrease with grain size. In addition, the concentrations of noble gases in lunar soil also show a close relationship with its mineral and chemical compositions. The utilization prospects of the noble gas ^3He in lunar regolith will be further discussed.  相似文献   

月壤的物理和机械性质   总被引：46，自引：0，他引：46  

郑永春  欧阳自远  王世杰  邹永廖 《矿物岩石》2004,24(4):14-19

月壤是在O2、水、风和生命活动都不存在的情况下，由陨石和微陨石撞击、宇宙射线和太阳风轰击、月表温差导致岩石热胀冷缩破碎等因素的共同作用下形成的。月壤独特的形成过程，加上独特的月表环境，使月壤在粒度分布、颗粒形态、颗粒比重、孔隙比和孔隙率、电性和电磁性质、压缩性、抗剪性、承载力等方面均与地球土壤存在较大差异，这些参数的平均值和最佳估计值，可以作为月表机械设计和操作、宇航员装备设计、月球着陆场选址的主要依据，对月球资源开发和利用以及月球基地建设具有极其重要的意义。  相似文献   

Origin of sandplains in Western Australia: A review of the debate and some recent findings     

D. Newsome 《Australian Journal of Earth Sciences》2013,60(4):695-706

Views on the origin of sandplains in Western Australia remain controversial with debate focusing around three different models of formation. These are in situ, aeolian and in situ formation with local remobilisation by wind or colluvial transport. The only recent work on the subject to date espouses a dominantly aeolian origin. New work from a detailed study on the Victoria Plateau is described and demonstrates the applicability of utilising a range of evidence in understanding the origin of sandplains in Western Australia. Field investigations show a strong association of sandplain with sandstone and an absence of sand on non‐arenaceous geology in similar and adjacent topographic settings. Grainsize, mineral magnetic analysis and heavy‐mineral spectra show the Victoria Plateau to be a heterogeneous body of sand. These findings coupled with a lack of internal sedimentary structures are not consistent with an aeolian origin for the sandplain. Furthermore, scanning electron microscopy, grainsize and heavy minerals also demonstrate a clear link between bedrock and overlying sandplain. These data support the hypothesis that Western Australian sandplains are mostly the product of in situ weathering. Such findings question whether the origin of sandplains can be satisfactorily deduced without such a range of data.  相似文献   

Vanadium in magnetite gabbros and its behaviour during lateritic weathering,Windimurra Complex,Western Australia     

M. M. Habteselassie  C. I. Mathison  R. J. Gilkes 《Australian Journal of Earth Sciences》2013,60(5):555-566

Shephards Discordant Zone is a 500–600 m thick interlayered sequence of deformed, altered and metamorphosed magnetite metagabbro and about 50 layers or lenses of magnetitite (> 80–90% magnetite). The sequence shows progressive magmatic fractionation upwards: Ti and Ti/Fe increase, and V, V/Ti and Cr decrease upwards in magnetite and in whole‐rock compositions. The main magnetite‐rich sequence (about 400 m thick) is deeply weathered, with 40 m of saprolite showing vertical zonation of weathering minerals due to progressive weathering. Magnetitites (average 1% V₂O₃) are resistant to weathering and show little chemical change, but magnetite gabbros (average 0.27% V₂O₃) are extensively weathered and show progressive loss of Ca, Na, Mg and S. Plagioclase, magnetite (1.37% V₂O₃), chlorite (up to 0.35% V₂O₃), actinolite, epidote and minor sulfides in unweathered rocks weather to kaolinite, hematite, goethite and minor vermiculite, ilmenite remaining largely unaffected. Vanadium is essentially immobile during weathering and is unaffected during weathering of magnetitites (1% V₂O₃), but is slightly depleted during weathering of magnetite gabbros (0.23% V₂O₃).  相似文献   

滇西菲红超基性岩风化壳铂族元素地球化学行为   总被引：4，自引：0，他引：4  

杨竹森  高振敏  罗泰义  陶琰  李红阳  饶文波 《矿物学报》2001,21(4):625-630

近年来在世界不同地区进行了风化过程中铂族元素的地球化学行为研究。作为中国西南部的第一个实例，本文研究了云南西部菲红超基性岩体上发育的红土风化剖面。矿物学和微量元素地球化学研究证明该风化壳是超基性岩风化的结果。文中详细讨论了风化壳的地质、矿物学、红土化和铂族元素地球化学特征。结果表明，风化壳的红土化程度不高，仍处于红色粘土阶段；风化壳上部的表层土壤带和铁质粘土带中铂族元素总量至少富集了3．57－7．87倍，其中Ru和Pd的富集程度较大,Ir的富集程度中等，Pt和Rh的富集程度较小，使得铂族元素的配分模式由基岩的Pt富集型转变为风化壳的Ru-Pt富集型，证明红土化过程中铂族元素发生了分异。  相似文献   

青藏高原东北部古喀斯特过程与环境   总被引：6，自引：0，他引：6  

崔之久  陈怀录 《地理学报》1996,51(5):408-417,T001

本文介绍了青藏高原东北部地区的古喀斯特现象，并对相关沉积进行了化学成、粘土矿物的Ｘ－射线衍射以及石英砂表面结构等气候代用指标的分析。分析结果一致，指示了温暖湿润的亚热带气候条件。重结晶方解石的裂变径迹测年结果表明，该地区古喀斯特发育于中中新世。  相似文献   

荒漠戈壁区地表疏松层中元素的分布规律   总被引：2，自引：0，他引：2  

赵善定  王学求 《物探与化探》2006,30(6):517-520

通过对荒漠戈壁区不同矿区地表疏松层中元素的分布规律研究发现:主要成矿元素和指示元素均在近地表疏松层中富集,同时,在粒级分布上又倾向于细粒级(-160目)富集,可见,在对荒漠戈壁区进行区域地球化学调查中,采集弱胶结层(10~40 cm)细粒级样品(-160目)为最佳采样介质,这样能有效地捕捉深部含矿信息。  相似文献