Electric Discharges in the Protoplanetary Nebula as a Source of Impulse Magnetic Fields to Promote Dust Aggregation     

Túnyi  I.  Guba  P.  Roth  L. E.  Timko  M. 《Earth, Moon, and Planets》2003,93(1):65-74

Lightning discharge generated in the protoplanetary nebula is viewed as a temporally isolated surge in the flow of electrically charged particles, similar to that of terrestrial lightning. If the current is intense enough, a powerful circular impulse magnetic field is generated around the instantaneous virtual electric conductor. Such magnetic field is capable of magnetizing dust grains containing ferromagnetic components present in its vicinity to their saturation levels. As a result, dust grains attract one another, forming the aggregates. This magnetically driven attraction suggests an important process possibly operational at an early stage of the planetary accretion. Based on both a classical model for electric conductor, and the theory of Lienard–Wiechert electromagnetic potentials, our calculations show that the magnetic impulse due to a discharge channel of a few cm in diameter transferring a charge of about 10⁴ electrons reaches as high as 10 T. At these magnetic fields, the ferromagnetic dust grains, and possibly the already-formed larger aggregates as well, are easily magnetized to the saturation levels, producing compact clusters exhibiting permanent magnetic moments.  相似文献   

东营凹陷北部沙河街组四段深部储层多重成岩环境及演化模式   总被引：7，自引：0，他引：7       下载免费PDF全文

张善文  袁静  隋风贵  陈鑫 《地质科学》2008,43(3):576

主要通过薄片鉴定、扫描电镜观察、包裹体分析、粘土矿物分析、镜质体反射率测试和岩心物性分析等手段,结合构造发育史和有机质热演化史等研究成果,以揭示东营凹陷北带古近系深部碎屑岩储层成岩环境及演化模式为目的展开研究工作。结果表明:东营凹陷北带古近系深部碎屑岩储层存在酸性、碱性和酸性碱性交替等多重成岩环境。酸性成岩环境以碳酸盐矿物溶解、长石溶解蚀变为高岭石并伴生石英次生加大等为标志,碱性成岩环境以石英质颗粒及其次生加大边溶解、长石次生加大和晚期碳酸盐矿物沉淀为标志。研究区古近系深部碎屑岩储层成岩环境由浅至深大致经历了碱性—酸性—酸性碱性交替(局部碱性较强)—碱性—弱碱性的演化过程,并建立了沙河街组四段的成岩演化和储层改造模式。  相似文献   

冲绳海槽玄武岩中中酸性残余熔体研究及其岩石学意义   总被引：1，自引：0，他引：1  

陈小明  王汝成赵明 倪培赵广涛  李巍然 《岩石学报》2005,21(1):158-168

与洋壳有关的酸性岩由于对了解幔源岩浆的演化以及判别古老蛇绿岩套及其构造位置的重要意义而倍受岩石学家和构造地质学家的关注。本对发现于冲绳海槽玄武岩基质中的中酸性到酸性残余熔体进行了详细研究，它们提供了幔源玄武岩浆结晶分异形成酸性岩浆的直接证据。在细小的基质矿物间分布有一种玻璃质的残余熔体，其成分随距冷凝边距离(L)的增加而越来越酸性。在SiO2对Na2O K2O图解上，残余熔体的投影点从玄武岩到英安岩均有分布，反映了一个连续的演化系列。在AFM图解上，残余熔体表现出与Thingmuli火山岩系列类似的拉斑玄武岩系列的演化趋势。我们的研究表明：残余熔体的演化受结晶分异作用控制。在早期结晶阶段，辉石的结晶起主导作用，结果造成残余熔体中SiO2、Al2O3，Na2O的迅速增加，FeO、MgO、CaO迅速降低。在晚期结晶阶段，斜长石成为主导结晶相，导致残余熔体中Al2O3，Na2O的迅速消减。Al2O3、Na2O从增加到降低的转变出现在SiO2=62％左右。在L=27．5mm处，85～90％的基质岩浆已发生了结晶作用，导致残余熔体中SiO2含量达到69～70％，而且此处还新出现了一种富FeTi的氧化物。该玄武岩中残余熔体和基质矿物的成分及演化特征分别与Thingmuli火山岩系列中酸性端元的组成相似，在也佐证了Thingmuli火山岩系列是幔源岩浆结晶分异的产物.  相似文献   

From soil aggregates to riverine flocs: a laboratory experiment assessing the respective effects of soil type and flow shear stress on particles characteristics          下载免费PDF全文

T. Grangeon  I. G. Droppo  C. Legout  M. Esteves 《水文研究》2014,28(13):4141-4155

Particles eroded from hillslopes and exported to rivers are recognized to be composite particles of high internal complexity. Their architecture and composition are known to influence their transport behaviour within the water column relative to discrete particles. To‐date, hillslope erosion studies consider aggregates to be stable once they are detached from the soil matrix. However, lowland rivers and estuaries studies often suggest that particle structure and dynamics are controlled by flocculation within the water column. In order to improve the understanding of particle dynamics along the continuum from hillslopes to the lowland river environment, soil particle behaviour was tested under controlled laboratory conditions. Seven flume erosion and deposition experiments, designed to simulate a natural erosive event, and five shear cell experiments were performed using three contrasting materials: two of them were poorly developed and as such can not be considered as soils, whilst the third one was a calcareous brown soil. These experiments revealed that soil aggregates were prone to disaggregation within the water column and that flocculation may affect their size distribution during transport. Large differences in effective particle size were found between soil types during the rising limb of the bed shear stress sequence. Indeed, at the maximum applied bed shear stress, the aggregated particles median diameter was found to be three times larger for the well‐developed soil than for the two others. Differences were smaller in the falling limb, suggesting that soil aggregates underwent structural changes. However, characterization of particles strength parameters showed that these changes did not fully turn soil aggregates into flocs, but rather into hybrid soil aggregate–floc particles. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Response of soil aggregate disintegration to the different content of organic carbon and its fractions during splash erosion     

Hairu Li  Gang Liu  Ju Gu  Hong Chen  Hongqiang Shi  Mohamed A. M. Abd Elbasit  Feinan Hu 《水文研究》2021,35(2):e14060

Aggregate disintegration is a critical process in soil splash erosion. However, the effect of soil organic carbon (SOC) and its fractions on soil aggregates disintegration is still not clear. In this study, five soils with similar clay contents and different contents of SOC have been used. The effects of slaking and mechanical striking on splash erosion were distinguished by using deionized water and 95% ethanol as raindrops. The simulated rainfall experiments were carried out in four heights (0.5, 1.0, 1.5 and 2.0 m). The result indicated that the soil aggregate stability increased with the increases of SOC and light fraction organic carbon (LFOC). The relative slaking and the mechanical striking index increased with the decreases of SOC and LFOC. The reduction of macroaggregates in eroded soil gradually decreased with the increase of SOC and LFOC, especially in alcohol test. The amount of macroaggregates (>0.25 mm) in deionized water tests were significantly less than that in alcohol tests under the same rainfall heights. The contribution of slaking to splash erosion increased with the decrease of heavy fractions organic carbon. The contribution of mechanical striking was dominant when the rainfall kinetic energy increased to a range of threshold between 9 J m⁻² mm⁻¹ and 12 m⁻² mm⁻¹. This study could provide the scientific basis for deeply understanding the mechanism of soil aggregates disintegration and splash erosion.  相似文献   

白银厂酸性火山岩地球化学特征及成因分析          下载免费PDF全文

覃伟  陈守余  赵江南  董凯  田光礼 《地质找矿论丛》2018,33(3):425-433

甘肃白银厂矿田是我国著名的火山成因块状硫化物矿床产地,赋矿岩石主要为酸性火山岩(石英角斑岩和石英角斑凝灰岩)。文章通过对白银厂矿区酸性火山岩的岩相学和岩石地球化学特征研究,结果表明:1)岩石发生了低绿片岩相的变质作用,镜下可见明显的绢云母化、绿泥石化等蚀变作用,造成了岩石K、Ca、Na、Rb等活泼元素的迁移;2)岩石具有高硅、低钛、弱铝、贫镁,亏损高场强元素Nb、Ta,以及明显的Sr、P、Ti、Eu的负异常和Th、U、Pb正异常特征,表明本区酸性火山岩可能为下地壳基性岩重熔的产物,源区存在斜长石、磷灰石以及钛铁矿等矿物的残留,并且岩浆在演化过程中经历过围岩的混染与弱的分离结晶作用;3)结合北祁连的区域构造演化、岩浆活动以及本区火山岩的年代学资料,认为该酸性火山岩可能处于由岛弧向弧后盆地过渡的环境中。  相似文献   

阿尔泰额尔齐斯带东段酸性岩墙群地球化学特征及其地质意义     

宫红良陈正乐  胡远清李丽赖新荣  马庆佑李玉英胡博  张文贵 《岩石学报》2007,23(5):889-899

野外地质调查发现在阿尔泰南缘额尔齐斯构造带东段、额尔齐斯活动断裂与富蕴-锡泊渡断裂之间发育了一套未变形的酸性岩墙群。岩墙群侵位于海西期片麻岩化花岗岩和上石炭统深变质的额尔齐斯组岩层中,薄片鉴定和岩石地球化学分析确定为具有细晶结构的流纹斑岩。岩石的SiO_2含量为70.9%～75.38%,K_2O Na_2O含量为7.55%～8.99%;大部分样品Na_2O>K_2O,里特曼指数值为1.8～2.5之间,Al_2O_3=12.80%～14.53%,A/CNK=0.9～1.1,NK/A=0.7～0.9,具有准铝质—弱过铝质、低镁、高钾钠、低钙和锶、高(Fe)_(mol)/(Mg)_(mol)特点,具A型花岗岩类特点,属于亚碱性脉岩。岩石轻稀土富集,大离子亲石元素相对富集,具有明显的中等负铕异常,壳源特征明显。锆石U-Pb二次粒子微探针测年显示岩墙群形成于277～286Ma。推断岩墙是阿尔泰海西期造山运动结束后,在拉张构造环境下的地壳局部熔融产物。  相似文献   

Mud dispersal across a Cretaceous prodelta: Storm‐generated,wave‐enhanced sediment gravity flows inferred from mudstone microtexture and microfacies     

A. Guy Plint 《Sedimentology》2014,61(3):609-647

Determining sediment transport direction in ancient mudrocks is difficult. In order to determine both process and direction of mud transport, a portion of a well‐mapped Cretaceous delta system was studied. Oriented samples from outcrop represent prodelta environments from ca 10 to 120 km offshore. Oriented thin sections of mudstone, cut in three planes, allowed bed microstructure and palaeoflow directions to be determined. Clay mineral platelets are packaged in equant, face‐face aggregates 2 to 5 μm in diameter that have a random orientation; these aggregates may have formed through flocculation in fluid mud. Cohesive mud was eroded by storms to make intraclastic aggregates 5 to 20 μm in diameter. Mudstone beds are millimetre‐scale, and four microfacies are recognized: Well‐sorted siltstone forms millimetre‐scale combined‐flow ripples overlying scoured surfaces; deposition was from turbulent combined flow. Silt‐streaked claystone comprises parallel, sub‐millimetre laminae of siliceous silt and clay aggregates sorted by shear in the boundary layer beneath a wave‐supported gravity flow of fluid mud. Silty claystone comprises fine siliceous silt grains floating in a matrix of clay and was deposited by vertical settling as fluid mud gelled under minimal current shear. Homogeneous clay‐rich mudstone has little silt and may represent late‐stage settling of fluid mud, or settling from wave‐dissipated fluid mud. It is difficult or impossible to correlate millimetre‐scale beds between thin sections from the same sample, spaced only ca 20 mm apart, due to lateral facies change and localized scour and fill. Combined‐flow ripples in siltstone show strong preferred migration directly down the regional prodelta slope, estimated at ca 1 : 1000. Ripple migration was effected by drag exerted by an overlying layer of downslope‐flowing, wave‐supported fluid mud. In the upper part of the studied section, centimetre‐scale interbeds of very fine to fine‐grained sandstone show wave ripple crests trending shore normal, whereas combined‐flow ripples migrated obliquely alongshore and offshore. Storm winds blowing from the north‐east drove shore‐oblique geostrophic sand transport whereas simultaneously, wave‐supported flows of fluid mud travelled downslope under the influence of gravity. Effective wave base for sand, estimated at ca 40 m, intersected the prodelta surface ca 80 km offshore whereas wave base for mud was at ca 70 m and lay ca 120 km offshore. Small‐scale bioturbation of mud beds co‐occurs with interbedded sandstone but stratigraphically lower, sand‐free mudstone has few or no signs of benthic fauna. It is likely that a combination of soupground substrate, frequent storm emplacement of fluid mud, low nutrient availability and possibly reduced bottom‐water oxygen content collectively inhibited benthic fauna in the distal prodelta.  相似文献   

Amoeboid olivine aggregates and related objects in carbonaceous chondrites: records of nebular and asteroid processes     

Alexander N. Krot  Michail I. Petaev  Shoichi Itoh  Timothy J. Fagan  Hisayoshi Yurimoto  Michael K. Weisberg  Matsumi Komatsu  Klaus Keil 《Chemie der Erde / Geochemistry》2004,64(3):185-239

Amoeboid olivine aggregates (AOAs) are the most common type of refractory inclusions in CM, CR, CH, CV, CO, and ungrouped carbonaceous chondrites Acfer 094 and Adelaide; only one AOA was found in the CB_b chondrite Hammadah al Hamra 237 and none were observed in the CB_a chondrites Bencubbin, Gujba, and Weatherford. In primitive (unaltered and unmetamorphosed) carbonaceous chondrites, AOAs consist of forsterite (Fa_<2), Fe, Ni-metal (5-12 wt% Ni), and Ca, Al-rich inclusions (CAIs) composed of Al-diopside, spinel, anorthite, and very rare melilite. Melilite is typically replaced by a fine-grained mixture of spinel, Al-diopside, and ±anorthite; spinel is replaced by anorthite. About 10% of AOAs contain low-Ca pyroxene replacing forsterite. Forsterite and spinel are always ¹⁶O-rich (δ^17,18O∼−40‰ to −50‰), whereas melilite, anorthite, and diopside could be either similarly ¹⁶O-rich or ¹⁶O-depleted to varying degrees; the latter is common in AOAs from altered and metamorphosed carbonaceous chondrites such as some CVs and COs. Low-Ca pyroxene is either ¹⁶O-rich (δ^17,18O∼−40‰) or ¹⁶O-poor (δ^17,18O∼0‰). Most AOAs in CV chondrites have unfractionated (∼2-10×CI) rare-earth element patterns. AOAs have similar textures, mineralogy and oxygen isotopic compositions to those of forsterite-rich accretionary rims surrounding different types of CAIs (compact and fluffy Type A, Type B, and fine-grained, spinel-rich) in CV and CR chondrites. AOAs in primitive carbonaceous chondrites show no evidence for alteration and thermal metamorphism. Secondary minerals in AOAs from CR, CM, and CO, and CV chondrites are similar to those in chondrules, CAIs, and matrices of their host meteorites and include phyllosilicates, magnetite, carbonates, nepheline, sodalite, grossular, wollastonite, hedenbergite, andradite, and ferrous olivine.Our observations and a thermodynamic analysis suggest that AOAs and forsterite-rich accretionary rims formed in ¹⁶O-rich gaseous reservoirs, probably in the CAI-forming region(s), as aggregates of solar nebular condensates originally composed of forsterite, Fe, Ni-metal, and CAIs. Some of the CAIs were melted prior to aggregation into AOAs and experienced formation of Wark-Lovering rims. Before and possibly after the aggregation, melilite and spinel in CAIs reacted with SiO and Mg of the solar nebula gas enriched in ¹⁶O to form Al-diopside and anorthite. Forsterite in some AOAs reacted with ¹⁶O-enriched SiO gas to form low-Ca pyroxene. Some other AOAs were either reheated in ¹⁶O-poor gaseous reservoirs or coated by ¹⁶O-depleted pyroxene-rich dust and melted to varying degrees, possibly during chondrule formation. The most extensively melted AOAs experienced oxygen isotope exchange with ¹⁶O-poor nebular gas and may have been transformed into magnesian (Type I) chondrules. Secondary mineralization and at least some of the oxygen isotope exchange in AOAs from altered and metamorphosed chondrites must have resulted from alteration in the presence of aqueous solutions after aggregation and lithification of the chondrite parent asteroids.  相似文献   

人体乳腺矿化集合体类型与临床相关性分析     

张岩  李艳  程潇  鲁安怀  王长秋  梅放  柳剑英  王大翠 《岩石矿物学杂志》2019,38(6):861-870

选取123例乳腺病理性矿化样品,利用光镜、扫描电镜对乳腺矿化进行了微形貌分类研究,并利用统计学方法探讨了乳腺矿化集合体类型与患者年龄、乳腺病变类型和癌变阶段的相关性。研究发现,根据乳腺矿化在光学显微镜下的可分辨形态,将其分为两种类型:粒状集合体与块状集合体;其中粒状集合体为小于200μm的规则粒状钙化,少部分有环带结构,和有机组织结合紧密;而块状集合体则为大于200μm的片状钙化,形状不规则。统计分析数据显示,随年龄增加,块状集合体出现病理比例增加,粒状集合体出现病理比例减少,敏感年龄分区界限为50岁;粒状集合体在50岁以上和50岁以下患者中单独出现的概率分别为24%和53%;块状集合体在乳腺原位癌(71. 4%)患者中占主导,粒状集合体在乳腺纤维腺瘤(64. 5%)患者中占主导。该研究可为未来乳腺癌的诊断提供基于乳腺矿化精细矿物学特征的辅助新方法。  相似文献