川南沐川地区宣威组底部铌-稀土多金属富集层富集规律、沉积环境与成矿模式

云南、贵州地区对晚二叠世宣威组底部Nb-REE多金属富集层的研究取得了重要进展,但其成因还有较大争议.为厘清沐川地区宣威组底部Nb-REE多金属富集层成因机制及富集规律,本研究开展了野外实地调查、矿物学、岩相古地理与岩石地球化学等系统性研究,探讨其物源、富集规律,建立了成矿模式.结果 表明,川南沐川地区宣威组底部Nb-...     

赣南西华山成矿花岗岩锆石U-Pb年代学和Hf同位素特征及其地质意义北大核心CSCD

赣南西华山钨矿是与侏罗纪花岗岩有关的大型石英脉型矿床,也是我国南岭成矿带赣南地区典型的钨矿床。本文选取西华山钨矿成矿花岗岩进行了锆石LA-ICP-MS U-Pb定年、微量元素和Hf同位素分析,旨在揭示花岗岩的形成时间并推断岩石成因及其对成矿的指示。锆石U-Pb测年结果表明,西华山中粒黑云母花岗岩锆石206 Pb/238 U加权平均年龄为154.8±6.0 Ma。锆石形态、激光拉曼和地球化学特征表明,该花岗岩受到岩浆热液的影响。锆石的176 Yb/177 Hf和176 Lu/177 Hf比值较高,表明源岩浆有强烈的流体出溶作用。西华山黑云母花岗岩的εHf(t)变化范围较小,呈明显负值(-12.8~-10.8),且集中在华夏地块古老基底范畴内,指示其形成于古老地壳物质的部分熔融。     

不同成因类型煤中烷基环己烷和烷基苯的特征探讨

通过对藻煤、烛煤、腐殖煤共生煤层的分析，将不同成因类型煤中的烷基环己烷和烷基苯进行了比较。结果表明，不同成因类型煤中所含的烷基环己烷和烷基苯明显不同。各种成因类型煤中烷基环己烷和烷基苯所提供的母质信息与煤岩结果吻合。氧化环境不利于烷基环己烷和烷基苯的形成。烷基环己烷和烷基苯有时可以作为沉积环境和成熟度的标志。     

渭南黄土沉积中十五万年来的古土壤及其形成时的古环境

关中盆地渭南地区十五万年来的黄土剖面记载了６个大的成壤期。本文对古土壤形成时的古环境进行了解译,并对它们在不同分类系统中的位置进行评价。全新世土壤Ｓ０是联合国土壤分类中的淋溶湿草原土。马兰黄土中包含两层古土壤,属典型黑钙土。Ｓ１古土壤由三层土壤复合组成,从上到下依次为典型黑钙土、淋溶湿草原土和深色淋溶土。成壤期与全球冰量较小的时期相对应,但古土壤的类型及发育程度与深海氧同位素所推测的全球冰量的变化有很大的不一致性,相反许多方面与北半球夏季太阳辐射的变化有较大的可比性。     

井下巷道围岩变形的散斑分析法

通过对散斑计量法原理分析、数学描述及观测实例的论述,证明激光散斑法是研究煤矿地下结构物相似模型变形状态的一种新的无损检测技术,若采用白光作为光源,该项技术可用于二维变形场的实地测试。     

规则球粒堆积体的孔隙度

以椭球堆积体为模型，求出圆球、扁球、长球、椭球４种堆积体的理论孔隙度极值相同，并导出了政府孔隙度的通式。认为理论孔隙度的大小仅与规则球粒的排列方式有关，当某一规则球粒堆积体受压而使该规则球粒变形为另一种规则球粒时，只要排列方式不变，其理论孔隙度也不变。     

Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events

During the rising phase of Solar Cycle 24 tremendous activity occurred on the Sun with rapid and compact emergence of magnetic flux leading to bursts of flares (C to M and even X-class). We investigate the violent events occurring in the cluster of two active regions (ARs), NOAA numbers 11121 and 11123, observed in November 2010 with instruments onboard the Solar Dynamics Observatory and from Earth. Within one day the total magnetic flux increased by 70 % with the emergence of new groups of bipoles in AR 11123. From all the events on 11 November, we study, in particular, the ones starting at around 07:16 UT in GOES soft X-ray data and the brightenings preceding them. A magnetic-field topological analysis indicates the presence of null points, associated separatrices, and quasi-separatrix layers (QSLs) where magnetic reconnection is prone to occur. The presence of null points is confirmed by a linear and a non-linear force-free magnetic-field model. Their locations and general characteristics are similar in both modelling approaches, which supports their robustness. However, in order to explain the full extension of the analysed event brightenings, which are not restricted to the photospheric traces of the null separatrices, we compute the locations of QSLs. Based on this more complete topological analysis, we propose a scenario to explain the origin of a low-energy event preceding a filament eruption, which is accompanied by a two-ribbon flare, and a consecutive confined flare in AR 11123. The results of our topology computation can also explain the locations of flare ribbons in two other events, one preceding and one following the ones at 07:16 UT. Finally, this study provides further examples where flare-ribbon locations can be explained when compared to QSLs and only, partially, when using separatrices.     

Authigenic iron oxide formation in the estuarine mixing zone of the Yangtze River

Estuaries are elementary geochemical fronts where river water and seawater mix. Within this mixing zone, iron and other non-conservative elements can undergo complex reactions to form new solid phases. In order to understand authigenic iron oxide formation in the Yangtze River Estuary, two onsite water-mixing sets of experiments were conducted, one by mixing variable amounts of unfiltered Yangtze River water with filtered East China Sea water of different salinity (set 1), the other by mixing variable amounts of filtered Yangtze River water with filtered East China Sea water of different salinity (set 2). In set 2, the minerals newly formed in the course of mixing were investigated by means of a scanning electron microscope fitted with an energy-dispersive X-ray analytical system. It was found that ferrihydrite and lepidocrocite were formed in these mixing experiments, coexisting in nearly equal amounts. These iron oxides appear as aggregated particles with a large grain-size range of several microns to more than 100 μm. The electrolytic properties of seawater played an important role in the formation of these authigenic iron oxides. Kaolinite and organic aggregates were also found in the experimentally mixed pre-filtered waters. Amounts of newly formed suspended matter (set 2) were one to three orders of magnitude lower than those of total suspended matter (TSM) (set 1). This implies that newly formed minerals represent only a very small proportion of TSM in the estuarine mixing zone of the Yangtze River.     

X-ray activity from different types of stars

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar Xray activity using the XMM-Newton and LAMOST data for different types of stars. We provide a sample including 1259 X-ray-emitting stars, of which 1090 have accurate stellar parameter estimations. Our sample size is much larger than those used in previous works. We find a bimodal distribution of the X-ray to optical flux ratio(log(fX/fV)) for G and K stars. We interpret that this bimodality is due to two subpopulations with different coronal heating rates. Furthermore, using the full widths at half maxima calculated from Hα and Hβ lines, we show that these stars in the inactive peaks have smaller rotational velocities. This is consistent with the magnetic dynamo theory that presumes stars with low rotational velocities have low levels of stellar activity. We also examine the correlation between log(fX/fV) and luminosity of the excess emission in the Hα line, and find a tight relation between the coronal and chromospheric activity indicators.