超大型矿床全球分布规律和岩石圈形成与太阳系起源和早期演化的成因联系     

《浙江国土资源》1996,(1)

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Exhumation History of the Xining Basin Since the Mesozoic and Its Tectonic Significance     

WANG Yannan  ZHANG Jin  QI Wenhu  GUO Shan 《《地质学报》英文版》2015,89(1):145-162

The Xining Basin is located in the northeastern Qinghai–Tibetan Plateau, and its continuous Cenozoic strata record the entire uplift and outgrowth history of the Tibetan Plateau during the Cenozoic. The newly obtained apatite fission track data presented here shows that the Xining Basin and two marginal mountain ranges have experienced multiphase rapid cooling since the Jurassic, as follows. In the Middle–Late Jurassic, the rapid exhumation of the former Xining Basin resulted from collision between the Qiangtang Block and the Tarim Block. During the Early–Late Cretaceous, the former Xining Basin underwent a tectonic event due to marginal compression, causing the angular unconformity between the Upper and Lower Cretaceous. In the Late Cretaceous to the Early Cenozoic, collision between the Qiangtang Block and the Lhasa Block may have resulted in the rapid exhumation of the Xining Basin and the Lajishan to the south. In the Early Cenozoic(ca. 50–30 Ma), collision between the Indian and Eurasia plates affected the region that corresponds to the present northeastern Qinghai–Tibetan Plateau. During this period, the central Qilian Block rotated clockwise by approximately 24° to form a wedge-shaped basin(i.e., the Xining Basin) opening to the west. During ca. 17–8 Ma, the entire northeastern Qinghai–Tibetan Plateau underwent dramatic deformation, and the Lajishan uplifted rapidly owing to the northward compression of the Guide Basin from the south. A marked change in subsidence occurred in the Xining Basin during this period, when the basin was tectonically inverted.  相似文献   

Dust production from the hypervelocity impact disruption of the Murchison hydrous CM2 meteorite: Implications for the disruption of hydrous asteroids and the production of interplanetary dust     

G.J. Flynn  D.D. Durda  J.W. Kreft 《Planetary and Space Science》2009,57(2):119-6210

More than half of the C-type asteroids, the dominant type of asteroid in the outer half of the main-belt, show evidence of hydration in their reflectance spectra. In order to understand the collisional evolution of asteroids and the production of interplanetary dust and to model the infrared signature of small particles in the Solar System it is important to characterize the dust production from primary impact disruption events, and compare the disruption of hydrous and anhydrous targets. We performed a hypervelocity impact disruption experiment on an ∼30 g target of the Murchison CM2 hydrated carbonaceous chondrite meteorite, and compared the results with our previous disruption experiments on anhydrous meteorites including Allende, a CV3 carbonaceous chondrite, and nine ordinary chondrites. Murchison is significantly more friable than the ordinary chondrites or Allende. Nonetheless, on a plot of mass of the largest fragment versus specific impact energy, the Murchison disruption plots within the field of the anhydrous meteorites points, suggesting that Murchison is at least as resistant to impact disruption as the anhydrous meteorites, which require about twice the energy for disruption as terrestrial anhydrous basalt targets. We determined the mass-frequency distribution of the debris from the Murchison disruption over a nine order-of-magnitude mass range, from ∼10⁻⁹ g to the mass of the largest fragment produced in the disruption. The cumulative mass-frequency distribution from the Murchison disruption is fit by three power-law segments. For masses >10⁻² g the slope is only slightly steeper than that of the corresponding segment from the disruption of most anhydrous meteorites. Over the range from ∼10⁻⁶ to 10⁻² g the slope is significantly steeper than that for the anhydrous meteorites. For masses <10⁻⁶ g the slopes of both the Murchison and the anhydrous meteorites are almost flat. Thus the Murchison disruption significantly over-produced small fragments (10⁻⁶-10⁻³ g) compared to anhydrous meteorite targets. If the Murchison results are representative of hydrous asteroids, the hydrous asteroids may dominate over anhydrous asteroids in the production of interplanetary dust >100 μm in size, the size of micrometeorites recovered from the polar ices, while both types of asteroids might produce comparable amounts of ∼10 μm interplanetary dust. This would explain the puzzle that polar micrometeorites (>100 μm in size) are similar to hydrous meteorites, while the majority of the ∼10 μm interplanetary dust particles are anhydrous.  相似文献   

Classification of 24 New Ordinary Chondrites from the Grove Mountains, Antarctica   总被引：1，自引：0，他引：1  

LU Ren  MIAO Bingkui  WANG Guiqing  DAI Deqiu  LIN Yangting  OUYANG Ziyuan  LI Chunlai Institute of Geochemistry  Chinese Academy of Sciences  Guiyang  Guizhou  Graduate School  Chinese Academy of Sciences  Beijing Institute of Geology  Geophysics  Chinese Academy of Sciences  Beijing Guangzhou Institute of Geochemistry  Chinese Academy of Sciences  Guangzhou  Guangdong National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《《地质学报》英文版》2004,78(5):1052-1059

Petrography and mineral chemistry of 24 ordinary chondrites from the Grove Mountains, Antarctica, have been studied in order to identify their chemical-petrographic types. These samples were selected from a total of 4448 Grove Mountains (GRV) meteorites collected during the 19th Chinese Antarctic Research Expedition so as to make an estimation of the large GRV meteorite collection. The chemical-petrographic types of these meteorites are presented below: 1 H3,2 H4, 4 H5, 2 H6, 1 L4, 7 L5, 5 L6, 1 LL4 and 1 LL6. The new data weaken the previous report that unequilibrated ordinary chondrites are unusually abundant in the Grove Mountains region. However, this work confirms significant differences in distribution patterns of chemical-petrographic types between the Grove Mountains and other  相似文献   

Acoustic-Gravity Waves from Bolide Sources     

Douglas O. ReVelle 《Earth, Moon, and Planets》2008,102(1-4):345-356

We have developed a new approach to modeling the acoustic-gravity wave (AGW) radiation from bolide sources. This first effort involves entry modeling of bolide sources that have available satellite data through procedures developed in ReVelle (Earth Moon Planets 95, 441–476, 2004a; in: A. Milani, G. Valsecchi, D. Vokrouhlicky (eds) NEO Fireball Diversity: Energetics-based Entry Modeling and Analysis Techniques, Near-earth Objects: Our Celestial Neighbors (IAU S236), 2007b). Results from the entry modeling are directly coupled to AGW production through line source blast wave theory for the initial wave amplitude and period at (at 10 blast wave radii and perpendicular to the trajectory). The second effort involves the prediction of the formation and or dominance of the propagation of the atmospheric Lamb, edge-wave composite mode in a viscous fluid (Pierce, J. Acoust. Soc. Amer. 35, 1798–1807, 1963) as a function of the source energy, horizontal range and source altitude using the Lamb wave frequency that was deduced directly during the entry modeling and that is used as a surrogate for the source energy. We have also determined that Lamb wave production by bolides at close range decreases dramatically as either the source energy decreases or the source altitude increases. Finally using procedures in Gill (Atmospheric-Ocean Dynamics, 1982) and in Tolstoy (Wave Propagation, 1973), we have analyzed two simple dispersion relationships and have calculated the expected dispersion for the Lamb edge-wave mode and for the excited, propagating internal acoustic waves. Finally, we have used the above formalism to fully evaluate these techniques for four large bolides, namely: the Tunguska bolide of June 30, 1908; the Revelstoke bolide of March 31, 1965; the Crete bolide of June 6, 2002 and the Antarctic bolide of September 3, 2004. Due to page limitations, we will only present results in detail for the Revelstoke bolide.  相似文献   

西宁市老年人口分布与养老资源错位研究     

马晓帆  张海峰  高子轶  孙骜 《世界地理研究》2021,30(1):213-222

健康中国战略下,积极应对老龄化、建立健全养老和医疗等相关设施,成为许多城市关注的问题。目前相关研究很少关注西北城市的老龄人口的空间分布及养老资源错位的现象。本研究以西宁市主城区为研究区域,基于2010—2018年西宁市公安局各街镇人口数据和兴趣点（POI）数据,选用老年人口系数、赡养率、增长率和地理集中率四个指标,利用综合老龄化指数（CAI）模型、核密度函数模型和空间错位指数模型对西宁市主城区人口老龄化空间分布及养老资源（医疗资源、老年设施）空间错位现象进行探索分析,结果表明：（1）9年间西宁市主城区人口老龄化程度不断加深,已步入老年型社会。（2）通过老龄化综合指数可知：主城区外围街镇人口老龄化增长速度大于城区中心的街道,其中小桥街道、朝阳街道、马坊街道与乐家湾镇人口老龄化最为严重,2018年综合老龄化指数增长速度超过中心城区街道,西宁市主城区人口老龄化严重程度已从中心街道向外围街镇扩散。（3）通过空间错位指数计算可得知：城中区的养老资源数量充足但过于集中,城北区的养老资源分布合理但是数量较少,行政区之间的养老资源与老年人口分布存在较大空间错位问题。  相似文献   

时间地理学视角下西宁城市回族居民时空间行为分析     

谭一洺  柴彦威  王小梅 《地域研究与开发》2017,36(5)

从回族居民群体特征出发,基于时间地理学的视角理解其时空间行为,提出少数民族行为的行为选择与制约效应框架,并以西宁市回族居民为例,从微观行为视角解读少数民族的城市时空间行为与特征。结果表明:(1)回族居民受工作活动制约相对较弱,活动时间安排上自主性更强,活动具有丰富性、细碎性的特点;(2)回族居民活动空间范围存在局限性,出行需求相对较低;(3)宗教活动对回族居民时空间行为存在制约。  相似文献   

寒旱环境盐胁迫条件下两种草本植物的根系力学特性研究          下载免费PDF全文

李淑霞  刘亚斌  胡夏嵩  余冬梅  祁兆鑫 《盐湖研究》2018,26(1)

本项研究选取适宜于西宁盆地及其周边地区生长的2种优势草本植物垂穗披碱草(Elymus nutans Griseb)和细茎冰草(Agropyron trachycaulum (Linn.) Gaertn.)作为供试种,通过室内种植培育方式,采用浓度梯度分别为50mmol/L、100mmol/L、150mmol/L、200mmol/L的Na₂SO₄溶液对2种植物进行盐胁迫处理。在盐胁迫试验处理后的第15d、30d和45d时,分别测定2种植物单根抗拉力和单根抗拉强度。试验结果表明：相同盐胁迫浓度时,2种植物单根抗拉力随生长期增长呈逐渐增大,单根抗拉强度随生长期增加表现为逐渐降低的变化规律;相同生长期时,2种植物单根抗拉力随着胁迫液浓度由0mmol/L增加至200mmol/L时表现为逐渐减小趋势,单根抗拉强度则随着胁迫液浓度增加呈逐渐增大的变化规律;进一步研究表明,在相同胁迫浓度和相同生长期条件下,细茎冰草单根抗拉力和单根抗拉强度分别较垂穗披碱草高0.008N~0.025N和9.646MPa~72.807MPa;2种草本植物单根抗拉力与根径之间呈指数函数关系;2种草本单根抗拉强度分别随根径的增加而逐渐减小,且均与根径呈幂函数关系。本该研究成果对于进一步探讨寒旱环境盐胁迫条件下,草本植物根系力学强度特征及其变化规律具有重要理论研究价值,同时对于有效防治研究区水土流失、浅层滑坡等地质灾害的发生具有实际指导意义。  相似文献   

南极GRV 98003和其它3个铁陨石的化学组成及分类   总被引：3，自引：3，他引：0       下载免费PDF全文

王道德  林杨挺 《极地研究》2004,16(2):81-90

用仪器中子活化测定了从南极回收的GRV98003铁陨石和乌珠穆沁铁陨石Cr,Co,Ni,Cu,Ga,Ge,As,Sb,W,Re,Ir,Pt及Au的浓度。根据化学组成,重新对这两个未分群的铁陨石进行了分类工作,其中将GRV98003铁陨石划分为IAB群,乌珠穆沁铁陨石划分为与IAB群相关的单独铁陨石。GRV98003铁陨石的元素丰度模式、元素对相关性(如NiAu,CoAu,AsAu,WAu,CuAu,SbAu)等与NWA468铁陨石(IAB)相似,但前者具有明显的难熔亲铁元素(Re,Ir)和中等挥发性元素(Ga,Ge)的贫化。此外,本文还对南丹铁陨石(IIICD)和邕宁铁陨石(IA)的化学群重新进行了讨论,提出将前者划分为IAB复合群的主群,而将后者划分为与IAB复合群相关的单独铁陨石的新观点。  相似文献   

南极格罗夫山陨石岩石学特征Ⅰ:非平衡L3型普通球粒陨石   总被引：6，自引：0，他引：6       下载免费PDF全文

缪秉魁  林杨挺  欧阳自远  周新华 《极地研究》2002,14(4):276-287

我国第16次南极科学考察队在格罗夫山区域的蓝冰表面回收到28块陨石,其中有6块属于非平衡型(即3型)普通球粒陨石。它们保存了原始的岩石矿物学特征,包括非常清晰的球粒结构、基质未重结晶和不透明、橄榄石和低钙辉石颗粒具有明显的成分环带和极不均一的化学组成等。Fe-Ni合金含量、含Fe总量和橄榄石成分综合分析表明这6块陨石全部属于低铁群(L)。因为非平衡普通球粒陨石橄榄石成分变化的PMD(Fa)值与岩石类型亚型有良好的相关性,因此,根据橄榄石Fa的PMD标准这6块陨石被划分为如下亚型:GRV 99019为3.6型,GRV99020、GRV 99021和GRV 99026为3.5型,GRV 99001为3.4型,GRV 99022为3.0—3.4型。  相似文献