Classification of 24 New Ordinary Chondrites from the Grove Mountains, Antarctica

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     

The unification of RBLs with XBLs

Many astronomers have discussed the property of BL Lacertae objects, including the variation of spectrum, the correlation of multi-wave bands and the property of polarization, which could give good information for studying intrinsic correlation of components and position of BL Lacertae objects. In the paper, we investigated the properties of RBLs and XBLs and RBLs/XBLs (these objects can also be found by radio survey as by X-ray survey). Firstly, we collected the light curve of 28 BL Lacertae objects, and gained their short timescales by Structure Function (SF). Secondly, we analyzed the distribution of the short timescales of some BL Lacertae objects, including 28 objects’ timescales calculated by SF, as well as the distribution of the redshift and the black hole mass and the flux densities of the multi-wavebands (radio, near-infrared, optical and Gamma-ray). Based on statistical analysis, the result of the paper support the unification model of RBLs and XBLs.     

Formation of Transient Coronal Holes during the Eruption of a Quiescent Filament and its Overlying Sigmoid

By using Hα, He I 10830, EUV and soft X-ray (SXR) data, we examined a filament eruption that occurred on a quiet-sun region near the center of the solar disk on 2006 January 12, which disturbed a sigmoid overlying the filament channel observed by the GOES-12 SXR Imager (SXI), and led to the eruption of the sigmoid. The event was associated with a partial halo coronal mass ejection (CME) observed by the Large Angle and Spectrometric Coronagraphs (LASCO) on board the Solar and Heliospheric Observatory (SOHO), and resulted in the formation of two flare-like ribbons, post-eruption coronal loops, and two transient coronal holes (TCHs), but there were no significantly recorded GOES or Hα flares corresponding to the eruption. The two TCHs were dominated by opposite magnetic polarities and were located on the two ends of the eruptive sigmoid. They showed similar locations and shapes in He Ⅰ 10830, EUV and SXR observations. During the early eruption phase, brightenings first appeared on the locations of the two subsequent TCHs, which could be clearly identified on He Ⅰ 10830, EUV and SXR images. This eruption could be explained by the magnetic flux rope model, and the two TCHs were likely to be the feet of the flux rope.     

1979-2016年我国东北地区空中水汽状况及变化趋势分析

水汽是形成云和降水的物质基础,与全球水分循环和能量平衡密切相关,对天气和气候具有重要影响。基于NCEP/NCAR月值再分析资料,综合分析我国东北地区上空不同高度层位比湿的气候学特征和长期趋势变化,同时分析了整层积分水汽通量的季节变化。结果表明：东北地区空中水汽集中分布于500 hPa以下,1979年至20世纪末低层比湿呈增加趋势,2000年后转为缓慢下降,但2012年以来波动回升。此外,东北地区比湿及水汽通量季节差异明显,夏季水汽含量最多,冬季最少,秋季多于春季;东北地区水汽含量最大值出现于7月,最低值出现在每年12月至次年1月。水汽来源受东亚季风系统影响明显,夏季水汽源地主要为南海,渤海和黄海对东北地区夏季水汽也有一定贡献;其他季节水汽主要来源于西风带输送。     

利用深地震反射剖面开展矿集区深部结构的探测:现状与实例

深地震反射剖面技术以其探测精度高的优势被作为岩石圈精细结构研究的先锋技术,并在全球典型矿集区结构探测中发挥了重要作用.为深入研究青藏高原碰撞造山成矿系统深部结构与成矿过程,本文系统总结了深地震反射技术发展现状,梳理了该技术在加拿大、澳大利亚、中国、俄罗斯、瑞典等全球多个国家的典型矿集区的应用实例,归纳总结了地壳深部结构对矿集区控矿因素的影响,阐述了地壳、上地幔深部结构与深部成矿过程的关系.从全球实例看,深地震反射剖面探测成果为大型矿集区的形成提供了深部线索,反射透明区可能是地幔流体向上运移通道,形成矿集区的成矿物质与能量来源,表明地幔物质参与了成矿作用;具有很强反射特征的断裂系统,包括大型断层、滑脱面和剪切带,是成矿流体从下地壳向上迁移的通道;矿集区深地震反射剖面中“亮点”反射可能是火山活动的深部岩浆上涌至中地壳后而形成的残余岩浆囊的反映.揭露精细的矿集区深部结构不但对矿集区构造历史演化的重建具有重要作用,还对未来成矿潜力和前景靶区的确定具有重要指导意义.     

东天山同成铅矿地球化学特征及找矿意义

同成地区位于东天山阿齐山-长城山岛弧带(觉罗塔格岛弧),南部有彩霞山铅锌矿,东部有红柳沟铜铅锌多金属矿及维山铅锌矿等。该地区处于新疆重要的铜、镍、金等多金属成矿带,是新疆重要成矿带,成矿条件有利。研究区内元素异常受地层控制明显,主成矿元素Pb、Zn富集度高、范围广,且元素异常整体重叠,所圈定的化探异常与地表发现的铅矿化带走向一致。根据目前取得的化探及找矿成果,认为同成地区具有寻找新型铅矿的较大潜力。     

滇黔北威信凹陷晚二叠世沉积环境与层序地层格架下的聚煤规律浅析

针对滇黔北威信凹陷晚二叠世含煤岩系的“海相-海陆过渡相-陆相”三相变化地带,利用地层剖面上的沉积构造、岩石组合、古生物特征等沉积相判别标志分析研究区的沉积环境及其空间演化,并总结煤质变化规律。在此基础上,通过识别层序与体系域关键界面,建立研究区晚二叠世含煤岩系的层序地层格架,充分讨论研究区厚煤层在层序地层格架下的聚煤规律。研究区自西向东依次为河流冲积平原体系、三角洲-潮坪体系及碳酸盐岩台地体系,成煤环境主要为河流冲积平原中的泛滥盆地河漫沼泽和三角洲-潮坪沉积体系中的上三角洲平原;厚煤层在层序地层中的位置与古地理背景有关,研究区C15,C19煤层形成于最大海泛面附近,C25煤层形成于初始海泛面附近;根据煤质变化规律和煤厚变化特征,在研究区西部的彝良-盐津一带有寻找优质煤炭资源的潜力。     

载体桩在陕南粉质黏土地区的适用性研究

以陕南粉质黏土地区某住宅楼施工现场为试验场地,开展了灌注桩和载体桩复合地基的现场静载试验,结合经验法理论计算,从承载力和建设成本两个方面,对比分析了两种地基基础方案的优劣。结果显示:灌注桩和载体桩复合地基荷载-沉降曲线均为缓变型,两种方案均能提供较高的抗压承载力;当载体桩桩长超过10 m,且作为复合地基增强体时,经验法计算过程未考虑桩端阻力的扩大头效益,计算结果明显低于现场试验结果;在相同桩身用料投入条件下,载体桩复合地基较灌注桩能够提供更高承载力。在陕南的类似粉质黏土地区,建议优先考虑选用载体桩复合地基方案。     

地表暖化影响下温度示踪地下水流速方法

为构建温度示踪方法测算地下水流速技术体系,并应用于区域地下水资源评价,基于最小二乘法和垂向一维非稳定流水-热运移方程数值解法,提出地表暖化情形下地下水流速计算方法,并对雷州半岛东北部地下水流速进行测算。结果表明:研究区域地下水补给速度为0.796m/a,入渗以西北部降水和运河渗漏为主;地下水排泄速度为0.269m/a,排泄入海主要发生在东海岛、南三岛和硵州岛附近。温度示踪解析区域地下水流动情况与地下水位分布情况基本一致,观测和计算地温数据具有较强相关性(R^2>0.50)和较低均方根误差(均值0.748),表明提出方法率定得到的地下水流速具有较强的可靠性。参数敏感性分析结果表明,地质体热扩散率和地表温度均对地温计算结果产生较明显的影响,参数的准确率定对利用地温计算地下水流速十分重要。     

时间域航空电磁系统探测深度研究

时间域航空电磁系统探测深度与采样时间、发射磁矩、大地电导率、仪器背景噪声和灵敏度等诸多因素相关。本文基于时间域航空电磁一维正演对时间域航空电磁系统探测深度进行研究。正演算法从麦克斯韦方程出发,结合准静态近似条件,得到一维层状介质上空中心回线频率域电磁场响应的垂直分量,并采用汉克尔积分进行计算,进而通过时-频变换获得时间域电磁场响应。探测深度研究参考仪器背景噪声水平,通过设定最小可识别信号阈值（本文设定为系统背景噪声三倍）获取最大可探测分离时间,进而利用该分离时间结合平均电导率求取最大探测深度。最后本文以VTEM系统为例,对不同层状介质模型以及不同发射磁矩、背景噪声、发射脉宽和飞行高度下的时间域航空电磁系统最大探测深度进行分析和讨论。