Oxygen isotope compositions of quartz grains (4–16 μm) from Chinese eolian deposits and their implications for provenance     

Shengshan?HouEmail author  Shiling?Yang  Jimin?Sun  Zhongli?Ding 《中国科学D辑(英文版)》2003,46(10):1003-1011

Oxygen isotope compositions were measured in quartz grains extracted from a 7.0 Ma red clay-loess sequence at Lingtai and six late Pleistocene loess sediments (Malan loess). Results show that the changes in oxygen isotope compositions of Malan loess are basically controlled by the geochemical characteristics of the source materials, while the effect of weathering process after dust deposition could be minor. The oxygen isotope distribution of quartz grains from red clay at Lingtai is similar to that of the overlying loess-paleosol sequence, thus indicating that the red clay at Lingtai has the same eolian origin as the loess-paleosol deposits. Furthermore, the oscillations of the isotope compositions in 4–16 μm-sized quartz grains may reflect the changes, to some extent, of the climatic systems of the source region.  相似文献   

Solar ultraviolet transfer in the Martian atmosphere: biological and geological implications     

C Córdoba-Jabonero  L.M LaraA.M Mancho  A MárquezR Rodrigo 《Planetary and Space Science》2003,51(6):399-410

  相似文献   

纤粒矿物粉尘体外细胞毒性研究   总被引：6，自引：0，他引：6  

邓建军  董发勤  吴逢春  蒲小允  John Huang  赵世泉 《岩石矿物学杂志》2000,19(3):249-253

采用体外细胞培养技术,观察兔肺泡巨噬细胞死亡率,用丙二醛（ＭＤＡ）的含量变化、乳酸脱氢酶（ＬＤＨ）及超氧化物歧化酶（ＳＯＤ）的活性变化来评价来自１２个矿６床的６种矿物的１２种结晶习性的矿物粉尘的细胞毒性,探讨其使巨噬细胞受损的机制。结果显示：沸石、硅灰石无细胞毒性,而其他的纤维状及片粒状矿物粉尘则表现出不同程度的细胞毒性,说明矿物粉尘的细胞毒性与矿物粉尘的形态有一定关系,但主要由矿物粉尘的特性所决  相似文献   

GIS辅助的吴淞工业区铺设道路扬尘估算     

黄嫣旻  束炯  魏海萍  王强 《测绘科学》2006,31(6):133-136

本文以上海市的吴淞工业区为研究对象,借鉴美国EPA提出的AP-42方法,利用动力学粒径谱仪的粒径分析结果对公式系数进行修正,在GIS手段的辅助下对吴淞工业区铺设道路不同粒径的扬尘量进行估算,最终由V isualBasic语言和MapObjects2.0组件建立的铺设道路扬尘管理信息系统表明GIS的使用有利于加强扬尘污染的研究和控制。  相似文献   

Mass Concentration and Mineralogical Characteristics of Aerosol Particles Collected at Dunhuang During ACE-Asia     

沈振兴  曹军骥  李旭祥  王亚强  张小曳 《大气科学进展》2006,23(2):291-298

Measurements were performed in spring 2001 and 2002 to determine the characteristics of soil dust in the Chinese desert region of Dunhuang, one of the ground sites of the Asia-Pacific Regional Aerosol Characterization Experiment (ACE-Asia). The mean mass concentrations of total suspended particle matter during the spring of 2001 and 2002 were 317 μg m?3 and 307 μg m?3, respectively. Eleven dust storm events were observed with a mean aerosol concentration of 1095 μg m?3, while the non-dusty days with calm or weak wind speed had a background aerosol loading of 196 μgm?3 on average in the springtime. The main minerals detected in the aerosol samples by X-ray diffraction were illite, kaolinite, chlorite, quartz, feldspar, calcite and dolomite. Gypsum, halite and amphibole were also detected in a few samples. The mineralogical data also show that Asian dust is characterized by a kaolinite to chlorite (K/C) ratio lower than 1 whereas Saharan dust exhibits a K/C ratio larger than 2. Air mass back-trajectory analysis show that three families of pathways are associated with the aerosol particle transport to Dunhuang, but these have similar K/C ratios, which further demonstrates that the mineralogical characteristics of Asian dust are different from African dust.  相似文献   

土壤、大气尘中晶体的组成及其物源指示意义——以长沙、株洲和湘潭地区为例     

张广平吴堑虹  戴塔根方建武张建新  徐海珍苏调红 《地质通报》2007,26(11):1459-1462

基于长沙、株洲和湘潭地区大气尘(可吸入颗粒和近地表积尘)和表层土壤的X-射线衍射(XRD)分析数据,采用微量相鉴定方法获得的结果显示,大气尘和表层土壤中包含石英、石膏、方解石、白云石、硫酸镉等自然矿物及SiS_2、NiTi、Cd_3As_2、FeOCl等非自然源晶体。比较了长沙、株洲、湘潭地区大气尘与表层土壤的晶体组成,分析了大气尘矿物及非自然源晶体的空间分布,探讨了其环境指示意义。  相似文献   

Variations in dust event frequency over the past century reflected by ice-core and lacustrine records in north China   总被引：1，自引：0，他引：1  

WANG NingLian    YAO TanDong    YANG XiangDong  SHEN Ji & WANG Yong Key Laboratory of Cryosphere  Environment  Cold  Arid Regions Environmental  Engineering Research Institute  Chi- nese Academy of Sciences  Lanzhou  China  Institute of Tibetan Plateau Research  Chinese Academy of Sciences  Beijing  China  Nanjing Institute of Geography  Limnology  Chinese Academy of Sciences  Nanjing  China 《中国科学D辑(英文版)》2007,50(5):736-744

In this paper, we analyzed the variations of dust proxies in the Dunde, Malan and Chongce ice cores from the northern Tibetan Plateau and the Hongjiannao lacustrine sediment core from north Shaanxi Province, and found that they all showed a general decrease trend over the past century. Owing to the fact that all these ice cores and lacustrine core were retrieved from the margins and/or the leeward sides of the major areas of dust events in north China, their records could suggest that the dust event frequency in north China declined over the study period. This decrease trend might be attributed to increasing precipitation and weakening westerly. However, human activities have made the areal extent of desertification expand acceleratingly in north China. This status could make it possible that dust events would occur on a large spatial scale under the future climate change, which would be a big environmental issue we shall face.  相似文献   

塔克拉玛干沙漠腹地沙尘暴发生条件分析   总被引：4，自引：0，他引：4       下载免费PDF全文

李生宇雷加强  徐新文 《应用气象学报》2007,18(4):490-496

利用塔中气象站1997—2002年的气象资料, 从沙尘源丰富程度、风动力条件和空气稳定度等方面分析了塔克拉玛干沙漠腹地沙尘暴的成因。结果表明:在塔克拉玛干沙漠腹地, 沙尘源极为丰富, 为沙尘暴发生提供了必要条件, 降水基本不能改变沙面的湿润状况, 沙尘源丰富度不是沙尘暴发生的限制因子; 风动力是沙尘暴发生的重要条件, 而月平均风速和大风日数是风动力的重要定量表征指标; 空气稳定性也是沙尘暴发生的重要条件, 温度和天气过程是其重要标志, 沙尘暴发生与温度呈正相关, 沙尘暴多发生在夏季和午后; 降水是沙漠腹地天气过程的重要指标, 月降水日数和降水总量与沙尘暴日数呈正相关; 20世纪90年代以来沙尘暴逐年减少, 这种变化趋势可能与全球气候变化有关。  相似文献   

The expulsion and retention of dust grains by galactic discs     

J. I. Davies  P. Alton  S. Bianchi  & M. Trewhella 《Monthly notices of the Royal Astronomical Society》1998,300(4):1006-1014

We have constructed a numerical model of a galaxy that consists of a stellar, gas and dust disc imbedded within a dark halo. We have used this model to assess the radiation, gravitational and viscous forces on dust grains and to trace their motion through the interstellar medium over a period of 10⁹ yr. We conclude that the disc opacity is a crucial factor in understanding the motion of the grains. Large grains (≈0.1 μm) with low disc opacity will lead to dust expulsion from the stellar disc, while high opacity leads to dust retention. Reasonable disc opacities lead to the recycling of the larger grains from the outer to the inner regions of the galaxy. The larger grains travel at higher velocities than small grains (0.01−0.001 μm), and so the smaller grains remain relatively close to their formation sites. Dust can 'leak' out over the entire surface of the disc because of the imbalance of radiation and gravitational forces. The dust is dynamically coupled to the gas and so although the gas lags behind the dust it is carried along with it. This explains the close correlation between the far-infrared emission from dust and the gas column density. We use a simple analytical model to show how the dust mass of a galaxy may evolve with time and how a significant fraction (90 per cent) of the total dust mass produced may have been expelled into the intergalactic medium.  相似文献   

太阳系尘埃等离子体研究   总被引：1，自引：0，他引：1  

石志东  李中元 《天文学进展》1998,16(3):227-236

综述了太阳系尘埃等离子体中的充电机制和波动过程以及与之有关的若干空间物理现象,内容包括太阳系等离子体中尘埃表面的平衡电势,带电尘埃在空间环境中的受力与运动,行星环内沿的弥漫扩散,轮辐结构的成困,彗星环境中尘埃的静电爆裂,尘埃彗尾的形态演化,天王星窄环的稳定性等问题．  相似文献