宁夏中北部地区沙尘暴频率气候影响指数模型的建立   总被引：2，自引：0，他引：2  

李艳春 《干旱气象》2004,22(1):13-16

从形成沙尘暴天气的动力机制、热力条件及物质基础入手,定性地分析了月平均风速、湿润度指数、月地面温差及下垫面沙化程度对沙尘暴频率的影响,在此基础上借鉴最新研究进展,建立适合宁夏中北部地区沙尘暴频率气候影响指数模型,比较深入地分析了宁夏中北部地区气候因素对沙尘暴频率的影响。  相似文献   

如何开展老矿山后备资源的寻找与定位预测--工作程序与实例分析   总被引：4，自引：4，他引：0  

刘红涛  杨秀瑛  刘建明  曾庆栋  于昌明  叶杰 《地球物理学进展》2004,19(3):573-582

在老矿山的深部与外围寻找新的可用资源,要求勘探者具备新的找矿思路、行之有效的深部探测手段与合理的工作程序、新的找矿思路来自于研究者的相关知识储备和创新能力,使其不墨守成规,用新的视角重新认识矿化规律和控矿要素。进而在老矿区优选出潜在的有利成矿区段．行之有效的深部探测手段以其高分辨的数字图像,不仅可以客观地反映深部地质结构的各种变化及矿化信息,以验证地质推测的可靠性,而且借助属地化的解释模型对矿区深部和外围开展真正意义的矿体定位预测、同时还可以大大降低工程验证的盲目性和巨大浪费．根据我们目前拥有的先进地球物理深部探测手段和大量老矿山找矿的经验与教训,逐渐形成了一套实用的工作程序。  相似文献   

A reanalysis of the Apollo light scattering observations, and implications for lunar exospheric dust     

David A. Glenar  Timothy J. Stubbs  James E. McCoy  Richard R. Vondrak 《Planetary and Space Science》2011,59(14):1695-1707

Conspicuous excess brightness, exceeding that expected from coronal and zodiacal light (CZL), was observed above the lunar horizon in the Apollo 15 coronal photographic sequence acquired immediately after orbital sunset (surface sunrise). This excess brightness systematically faded as the Command Module moved farther into shadow, eventually becoming indistinguishable from the CZL background. These observations have previously been attributed to scattering by ultrafine dust grains (radius ∼0.1 microns) in the lunar exosphere, and used to obtain coarse estimates of dust concentration at several altitudes and an order-of-magnitude estimate of ∼10⁻⁹ g cm⁻² for the column mass of dust near the terminator, collectively referred to as model “0”.We have reanalyzed the Apollo 15 orbital sunset sequence by incorporating the known sightline geometries in a Mie-scattering simulation code, and then inverting the measured intensities to retrieve exospheric dust concentration as a function of altitude and distance from the terminator. Results are presented in terms of monodisperse (single grain size) dust distributions. For a grain radius of 0.10 microns, our retrieved dust concentration near the terminator (∼0.010 cm⁻³) is in agreement with model “0” at z=10 km, as is the dust column mass (∼3–6×10⁻¹⁰ g cm⁻²), but the present results indicate generally larger dust scale heights, and much lower concentrations near 1 km (<0.08 cm⁻³ vs. a few times 0.1 cm⁻³ for model “0"). The concentration of dust at high altitudes (z>50 km) is virtually unconstrained by the measurements. The dust exosphere extends into shadow a distance somewhere between 100 and 200 km from the terminator, depending on the uncertain contribution of CZL to the total brightness. These refined estimates of the distribution and concentration of exospheric dust above the lunar sunrise terminator should place new and more rigorous constraints on exospheric dust transport models, as well as provide valuable support for upcoming missions such as the Lunar Atmosphere and Dust Environment Explorer (LADEE).  相似文献   

Mitigation of lunar dust adhesion by surface modification   总被引：2，自引：0，他引：2  

Adrienne Dove  Genevieve Devaud  Xu Wang  Mark Crowder  Anna Lawitzke  Christina Haley 《Planetary and Space Science》2011,59(14):1784-1790

Dust has been recognized as one of the greatest hazards in continued lunar exploration due to its tenacious adhesion to everything with which it comes into contact. Unfortunately, there is little known about the mechanisms of adhesion on widely varying surface types: van der Waals and electrostatic forces are the dominant forces under consideration here. Surface energy, roughness, mechanical properties and electronic properties are all known to contribute to the adhesion characteristics. An optimal solution to mitigate dust adhesion would be to identify the dominant components of the adhesive force and to reduce that force by surface modification. In this study, an ion beam process was used to modify (treat) the surfaces of three dramatically different materials spanning the range of conductor (black Kapton), semiconductor (silicon), and insulator (quartz). Adhesive forces between less than JSC-1 lunar simulants and these virgin/treated surfaces were measured in vacuum using a centrifugal force detachment method. We found that JSC-1 particles adhered less to treated silicon and quartz surfaces, correlated with a reduction in van der Waals force due to a reduced surface energy. The large reduction in adhesion for treated black Kapton is mainly due to the large decrease in the electrostatic (image) force that results from reduced contact charging. Materials in space and on the lunar surface will be directly exposed to high-energy ultraviolet radiation prior to being covered by dust, so the UV irradiation effects on surface adhesion were also examined. Both virgin and treated quartz surfaces are most affected by the UV-irradiation, showing dramatically increased adhesion.  相似文献   

Using X‐shooter to measure the extinction in long GRB host galaxies from emission lines     

K. Wiersema 《Astronomische Nachrichten》2011,332(3):295-296

The spectra of the host galaxies of gamma‐ray bursts at low redshift generally show strong hydrogen lines of the Balmer, Paschen and Brackett series, in addition to strong nebular metal lines. In special cases the hosts can be resolved in separate star forming regions, and spatially resolved spectroscopy can be obtained. Generally, the three strongest Balmer lines are used to derive the reddening experienced by the emission lines of the host gas, assuming a Milky Way extinction curve, case B recombination and a fixed electron temperature. We demonstrate how the wide wavelength range of X‐shooter, in combination with a rigorous calibration strategy, can be used to fit explicitly for R_V, T_e, and A_V simultaneously using a large number of H and He I recombination lines, explicitly corrected for stellar atmosphere absorption. This increases our understanding of extinction and absorption in starforming regions in GRB hosts. We use two GRB hosts as examples of the methods, outlining the advantages of using X‐shooter over other instruments (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Recycling of Coastal Dredged Sediments from the Northern Nile Delta,Egypt, for Heavy Minerals Exploitation     

Omran Frihy  Essam Deabes  Wahid Moufaddal  Adam El-Shahat 《Marine Georesources & Geotechnology》2013,31(5):408-418

Mineralogical and textural analyses of 45 undisturbed short cores and 80 grab sediment samples, collected from five frequently dredged navigational areas within harbors and water pathways of the Nile delta littoral system, were utilized for evaluation of these sediments as potential source of economic heavy minerals (EHMs). Results of mineralogical characterization indicate that the average total heavy mineral (HM) concentrations are as follows: Abu Qir Bay (1.7%), Rosetta estuary (3.1%), Burullus fishing port (4.5%), Damietta Harbor (2.9%), and El Gamil lagoon inlet (1.9%). Assessment of HM grades indicates predominance of magnetite, ilmenite, hematite, leucoxene, garnet, zircon, and rutile. Results of the feasibility analysis indicate that dredged sediments at these study areas are considered as a potential source of EHMs and economically promising to be mined for HMs. The present study suggests a practical operative plan of two successive phases for HMs recycling: (1) in-situ initial separation of HMs on the dredger deck using wet-gravity spirals, then (2) transportation of the recovered HM concentrates to an onshore processing plant to selectively separate individual HMs via wet and dry magnetic and electrostatic separators. Alternatively, dredged sediments can be directly pumped to a nearby onshore area as stockpile to be recycled afterward in inland processing plant.  相似文献   

GIS在矿产资源潜力评价中的应用     

孙元 《地理空间信息》2012,(3):57-60

GIS技术的广泛应用为矿产资源潜力评价提供了新的思路和手段,并对其产生了深远的影响。简要介绍了GIS、矿产资源潜力评价及GIS在矿产资源潜力评价中的应用现状,并根据基于GIS矿产资源潜力评价的3个步骤,详细阐述了GIS在矿产资源潜力评价中的具体应用及其优越性。  相似文献   

南方红土磁性地层年代学研究进展          下载免费PDF全文

刘彩彩  邓成龙 《地学前缘》2011,18(4):158-170

南方红土是中国分布最广的第四纪土状堆积,蕴含丰富的古气候、古地理以及古人类演化的信息。然而,南方红土地区长期高温多雨的气候造成许多定年材料的缺乏,导致其年代学研究进展比较缓慢。磁性地层学方法是一种适合于中、新生代海陆相沉积物定年的快捷、有效的方法,近年来南方红土的磁性地层年代学研究取得了很好的结果。文中比较系统地总结了近年来南方红土磁性地层年代学研究方面的进展。这些研究显示南方红土中的载磁矿物包括赤铁矿、磁赤铁矿、磁铁矿和针铁矿,其中磁铁矿和赤铁矿是特征剩磁的主要载体。磁性地层结果表明南方红土记录了Matuyama负极性时晚期至Brunhes正极性时早-中期的沉积,其沉积起始年龄不晚于Jaramillo正极性亚时,即早于11 Ma。这些磁性地层学结果为揭示南方红土记录的环境变化和中国南方亚热带地区早期人类演化提供了年代学基础。  相似文献   

黔东南天锦黎地区矿田级金矿定位预测——兼论勘查及研究程度较低地区的矿产预测方法     

陶平  陈启飞  王亮  胡从亮 《吉林大学学报(地球科学版)》2013,43(4):1235-1245

黔东南天柱-锦屏-黎平地区金矿勘查及研究程度较低,在进行矿产预测时必须有针对性地进行成矿地质背景、成矿规律、物化遥信息、找矿标志、预测要素等专题研究,更多关注成矿地质背景、成矿规律对矿产预测的主导作用,找准影响矿产预测的主要因素,客观适度地赋予物化遥信息对矿产预测的权重。同时,在条件不成熟时可将预测精度降至矿田-矿床级的定位预测,从整体上评价每个金矿田的找矿远景,并对某些部位找到矿床的可能性作进一步评述。采用了多种预测要素权重的简单相加法进行定位预测,而未具体开展基于GIS的定量预测,意在强调地质勘查及研究程度较低地区开展各项专题研究的重要性,并探讨简化矿产预测程序的可行性。经尝试,适宜于该类地区矿田级定位预测的简化流程为：a.相关专题研究;b.预测要素研究及赋值;c.各矿田成矿概率的计算及找矿远景分类;d.各矿田资源潜力评价。通过该方法尝试,该区获得找矿远景区A类4个、B类3个、C类3个。  相似文献   

冰尘结构特征及形成分析——以乌鲁木齐河源1号冰川为例     

许慧  李忠勤  Nozomu Takeuchi  张晓宇  张国飞 《冰川冻土》2013,35(5):1118-1125

利用2007-2010年夏季在乌鲁木齐河源1号冰川采集的5个冰样, 对冰样中冰尘的特征、冰尘中蓝藻的种类及冰尘中无机矿物颗粒的粒度特征进行了分析研究. 研究表明: 冰尘为棕色球状聚合体, 粒径为0.27~3.5 mm, 分布在冰川消融区表面, 其组成成分为有机质、无机矿物颗粒和微生物. 冰尘有4种主要的内部结构: 类型Ⅰ, 具有同心层结构的冰尘;类型Ⅱ, 带有亚颗粒的冰尘;类型Ⅲ, 内部无明显结构的冰尘;类型Ⅳ, 中心位置处具有较大无机颗粒的冰尘. 冰尘中无机矿物颗粒的数量主要分布在d<3.5 μm的范围内, 且体积分布的粒径众数介于3~25 μm之间. 同时, 对冰尘中的蓝藻进行了16S rRNA基因序列的系统发育分析, 共从蓝藻16S rRNA基因文库中筛选了247个阳性克隆, RFLP分型得到10个不同的OTUs. BLAST比对, 系统发育分析将这10个OTUs归为颤藻目(Oscillatoriales)、色球藻目(Chroococcales)、未定种(Unclassified). 颤藻目为绝对优势类群, 占整个基因克隆文库的91%. 经估算, 冰尘中存在大量的有机物质和微生物, 无机矿物颗粒只占了很小的比例, 表明影响冰川消融区表面反照率的主要因素为冰尘中的有机部分, 包括有机物质和微生物.  相似文献