辽东石庙沟岩体岩石地球化学特征、锆石U-Pb年龄、Hf同位素及其地质意义

辽东石庙沟地区位于华北陆块东部的辽吉造山/活动带上,该带经历了十分复杂的构造演化过程,记录了多期岩浆-构造-变质事件。石庙沟岩体为花岗斑岩,富SiO₂、Na₂O和K₂O,贫CaO、MgO及Al₂O₃,亏损高场强元素（Nb、Ti、Ta、P）,富集大离子亲石元素（K、Rb、Ba、U）,A/CNK值大于1,REE配分曲线呈"海鸥"式分布,以具有显著的负Eu异常为特征,高Ga/Al值,与典型A型花岗岩特征一致。花岗斑岩中锆石的LA-ICP-MS U-Pb测年结果表明其成岩年龄为（123.0±1.6）Ma,为早白垩世。锆石Hf同位素分析表明,ε_Hf（t）值均为负值,介于-15.72~-12.85之间,平均值为-14.14,二阶段模式年龄（T_DM2）在2 164~1 989 Ma之间,平均为2 067 Ma,反映源岩以大陆壳成分为主。结合花岗斑岩高SiO₂,低Mg、Co、Cr、Ni,且富集LREE和LILE,亏损HFSE等特征,表明早白垩世花岗斑岩岩浆应为大陆地壳物质熔融的产物。根据年代学和岩石地球化学研究认为,早白垩世花岗斑岩是古太平洋板块向欧亚大陆板块俯冲所形成的活动大陆边缘弧花岗岩。研究区早白垩世花岗斑岩的形成主要受太平洋构造域的影响,形成环境受板块俯冲造山后伸展作用和下地壳拆沉作用的联合制约,是辽东地区岩石圈减薄的直接证据。     

投影寻踪门限回归模型在年径流预测中的应用

为预测年径流这类同维复杂动力系统，提出了投影寻踪门限回归（PPTR）模型。构造了新的投影指标函数，用门限回归（TR）模型描述投影值与预测对象间的非线性关系，并用实码加速遗传算法优化投影指标指数函数和TR模型参数。实例的计算结果表明，用PPTR模型预测年径流是可行而有效的。PPRT模型简便、适用性强，克服了目前投影寻踪方法计算量大、编程实现困难的缺点，有利投影寻踪方法的推广应用，为解决高维非线性复杂预测问题提供了新途径。     

淮北海孜煤矿断层与层间滑动构造组合型式及其形成机制

煤矿中煤层断层与层间滑动构造(简称层滑构造)发育普遍,可出现不同形式的组合。进行煤层断层与层滑构造及其组合型式的研究,对分析区域构造变形史、查明和预测煤层赋存规律、研究煤的耗散流变、煤层气的开发以及预防煤与瓦斯突出都具有重要作用。本文以淮北矿区海孜煤矿为例,在现场观测的基础上,分析总结了7、8、9和10煤层的断层与层滑构造的组合型式,并探讨了其形成机制。由于7、8、9和10煤层及顶、底板岩层组合的差异,不同煤层构造变形有较大区别。由于海孜煤矿岩层和煤层经历了多次构造活动,断层和层滑构造间产生了不同的空间组合,具体表现为3种型式:断层与层滑构造的同期扩展、断层与层滑构造组成块体及断层与层滑构造间的相互切割和限制。煤层的构造组合型式在很大程度上取决于构造应力作用、含煤地层的岩石力学性质和应变环境等。     

世界海洋油气资源与勘探模式概述

描述了全球海洋油气储量的总体情况、海洋油气资源的地域分布以及海洋油气产量的状况与增长趋势。简略阐述了海洋油气勘探的阶段划分、海洋地质调查、海洋地球化学勘探、海洋非地震地球物理勘探以及海洋地震勘探各方法的基本特点、关键技术和常用手段等。对海洋油气勘探的前景,尤其是深水区和天然气水合物的勘探前景作了展望。     

Simultaneous monochromatic and spectral observations of two large loop prominence groups

Using the solar tower telescope of Nanjing University, we observed the two large loop prominence groups of 1982 Dec. 20 and 1983 Feb. 9. Hα photographs and spectra around the Hα and H and K lines were obtained simultaneously. From these data, we derived a line of sight velocity distribution, which agrees perfectly with the distribution for matter falling freely without viscosity. From the widths of the Hα and the K lines, we found the loop material to have a uniform kinetic temperature and a turbulent velocity that increases with height. From the central intensities of the lines we derived a density of n(H) ? 1.3 ? 2.6 × 10¹⁰cm^?3. A possible mechanism of the formation of loop prominence groups and their relation with flares are discussed.     

Automatic Solar Filament Detection Using Image Processing Techniques

We present an automatic solar filament detection algorithm based on image enhancement, segmentation, pattern recognition, and mathematical morphology methods. This algorithm cannot only detect filaments, but can also identify spines, footpoints, and filament disappearances. It consists of five steps: (1) The stabilized inverse diffusion equation (SIDE) is used to enhance and sharpen filament contours. (2) A new method for automatic threshold selection is proposed to extract filaments from local background. (3) The support vector machine (SVM) is used to differentiate between sunspots and filaments. (4) Once a filament is identified, morphological thinning, pruning, and adaptive edge linking methods are used to determine the filament properties. (5) Finally, we propose a filament matching method to detect filament disappearances. We have successfully applied the algorithm to Hα full-disk images obtained at Big Bear Solar Observatory (BBSO). It has the potential to become the foundation of an automatic solar filament detection system, which will enhance our capabilities of forecasting and predicting geo-effective events and space weather.     

The evolution of the Magellanic clouds

The observed maximum luminosities of AGB stars in the Magellanic Cloud clusters were compared with luminosities obtained theoretically in order to estimate the ages of the clusters. Several rates of mass loss by AGB stars are considered. The ages for 10 clusters in the SMC and 25 in the LMC are presented in the tables with the compilations of ages from the literature quoted. The discrepancies between ages derived from the AGB peak luminosities and from the Main-Sequence turn off and maximum luminosity are explained by allowing for intensive mass-loss during the AGB evolutionary phase. The method is useful only if the brightest star is on the thermally pulse AGB phase but not in the early-AGB phase.     

浅析造礁生物演化及生物绝灭事件对礁丘发育的控制作用──以中国南方震旦纪至三叠纪生物礁丘为例

造礁生物演化经历了六个主要发展阶段，具有全球性演化规律特征，其盛衰变化在中国南方礁丘的时代分布上反映较为醒目。早泥盆世至晚泥盆世早期，为生物礁发育的首次鼎盛期，已发现的礁体达９７个，而至今尚未发现晚泥盆世晚期（法门期）的生物礁；二叠纪是第二次鼎盛期，已发现该时期的礁丘达１４８个之多，生物特征明显，而至今也尚未发现早三叠世时期的礁体。中国南方这一礁丘时代分布特征恰好与 Ｆ／Ｆ和Ｔ／Ｐ两次全球性巨大生物绝灭事件相吻合。因此在南方寻找生物礁型油气藏时，除了应当重视本区构造演化的控制作用外，还应极大地注意全球性生物演化规律的控制作用。     

1961-2015年陕西省不同等级降水事件变化特征

利用19612015年陕西省70个气象观测站的逐日降水资料,采用线性倾向估计、趋势分析及Mann Kendall等方法,分析了陕西省不同等级降水量、降水日数及降水强度的气候变化特征。结果表明：无论是降水量、降水日数,还是降水强度,均呈现出南多北少的分布特征,且随着降水级别的逐级增加,地区分布差异逐渐增大;整体上降水量和降水日数呈现出减少趋势,其中降水日数的下降趋势均非常显著,全省年均降水日数的气候倾向率达到了-3.83天·10a-1,通过了0.01的显著性检验,降水强度的增加趋势通过了0.05的显著性检验,每10 a全省年均降水强度增加0.15 mm·d-1;陕西降水量及降水日数的减少主要体现在春秋两季小雨及中雨的减少上,小雨降水强度在夏、秋两季的气候倾向率分别为0.05和0.04 mm·d-1·10a-1,其上升趋势分别通过了0.01和0.1的显著性检验,这是年均降水强度上升的主要原因;陕西年均降水量及降水日数自1984年出现了突变性下降,而降水强度的突变则出现在2004年,之后一直呈现持续的上升趋势。     

The Occurrence of Oleananes in the Beibuwan Basin and Its Application to the Study of Maturity and Oil-Source Rock Correlation

The oleanane parameter, i.e., OP （oleananes/（oleananes＋C30hopanes）） in the two sedimentary columns of the Beibuwan Basin, South China Sea, can be used to delimit the top of oil generation window, with Ro （/%） of 0.53 in Well M1 and 0.55 in Wells H1/Hd1/Hd2, respectively. Comparing with vitrinite reflectance （Ro/%）, the OP features a dynamic range and can indicate the oil generation window more precisely. By using OP and other geochemical indices, the oil-source correlation is also conducted. It suggests that the oils in wells M1 and M2 are derived from the source rocks in situ. The mudstone in Huachang uplift is not the main source rocks for oils in this area, The OP is also a useful oil-source correlation parameter in some Tertiary lacustrine basins.