海原断裂带库仑应力积累

用中国地壳运动观测网络区域站在海原断裂带附近的所有观测数据及跨断裂GPS剖面观测数据作为约束, 用Smith3D体力模型反演了海原断裂带断层滑动速率和断层闭锁深度, 计算了库仑应力积累率和地震矩积累率.采用遗传算法拟合GPS水平运动速度场, 拟合的最后残差均方根为1.2mm/a.反演结果为: 第一段毛毛山断裂左旋走滑运动速率为3.6mm/a, 闭锁深度为22km; 第二段老虎山断裂左旋走滑速率为10.5mm/a, 闭锁深度为11.4km; 第三、四、五段(海原断裂带西段、中段和东段) 滑动速率依次为3.5mm/a、5.8mm/a、5.7mm/a, 闭锁深度依次为8.5km、3.6km、4.3km.海原断裂带库仑应力积累率为0.48~1.59MPa/100a, 毛毛山断裂地震矩积累率较大, 但库仑应力积累率较小; 老虎山断裂库仑应力积累率和地震矩积累率均比较大; 海原断裂带(狭义) 中西段库仑应力积累率最大.      

Strategies for managing reservoir sedimentation

Sediment deposition in reservoirs has caused the loss of 66% of the reservoir capacity in China. The main sedimentation control strategies are： 1） storing the clear water and releasing the turbid water; 2） releasing turbidity currents; 3） Draw-down flushing and empty flushing; and 4） dredging, The paper summarizes these strategies with examples. Sediment transport in many Chinese rivers occurs mostly during the 2-4 month flood season, that is, 80-90% of the annual sediment load is transported with 50-60% of the annual runoff. By storing the clear water after the flood season and releasing the turbid water during the flood season, less sediment deposits in the reservoir while the reservoir is still able to store enough water for power generation in the low flow season. The Three Gorges and Sanmenxia reservoirs apply this strategy and control sedimentation effectively. Turbidity currents have become the main sedimentation control strategy for the Xiaolangdi Reservoir. Empty flushing involves reservoir draw-down to temporarily establish riverine flow along the impound reach, flushing the eroded sediment through the outlets. Case studies with the Hengshan Reservoir and Zhuwo Reservoir are presented. Jet dredgers have been used to agitate the reservoir deposit so that the deposit is released from the reservoir with currents. The sediment releasing efficiency is 30-100% for storing the clear and releasing the turbid; 6-40 % for turbidity current; and 2,400-5,500% for empty flushing. Empty flushing causes high ecological stress on the ecosystem to the downstream reaches. Storing the clear and releasing the turbid is the best strategy to control reservoir sedimentation while achieving hydro-power benefit and maintain ecological stability.     

伊犁盆地油气与地浸砂岩型铀矿成矿关系研究

伊犁盆地南缘中、下侏罗统水西沟群产有数个可地浸的砂岩型铀矿床。前人对这些铀矿床的成因认识基本上都是层间氧化带成因观点,但对铀矿化的富集机理研究不够深入,普遍认为铀成矿富集机理是含矿层沉积时堆积的有机质及沉积成岩阶段形成的硫化物对层间渗入氧化水中铀的还原吸附作用。油气包裹体及其气相色谱特征研究表明,盆地至少发育过一期石油和一期天然气运移、聚集过程;铀矿床含矿砂岩中的油气来源于深部二叠纪或更老地层的较成熟的烃源层。油气一方面消耗了含矿含水层中的大量氧气,造就了含矿层较强的还原环境;另一方面也参与了铀成矿过程的氧化还原反应,加速了铀还原、沉淀、富集成矿的速度。结合盆地断裂构造研究,本文推断深部油气主要沿近EW向东曼里塔勒迪深大断裂和NWW—SEE向霍城托开深大断裂向上运移,造成断裂附近形成较强的还原障,进而控制了盆地砂岩型铀矿床(点)的空间分布。     

准噶尔盆地北部新生代构造活动特征及其对砂岩型铀矿的控制作用

准噶尔盆地北部顶山地区是我国寻找地浸砂岩型铀矿远景区段之一。本文在野外实地考察的基础上,结合遥感卫片解译分析,发现本区新生代构造活动主要表现为基底逆冲断裂的复活,致使地表呈现张性破裂,形成了洼地、峡谷等特殊的构造地貌形态;并根据擦痕、节理的测量统计,结合电子自旋共振测年分析,推断本区在上新世—更新世期间存在两期构造活动:早期为近似南北向的挤压作用为主,晚期(0.14~0.43Ma)为北东北东东的挤压作用;根据盆地新生代沉积物质充填规律和新生代构造特征,结合区域资料分析,恢复了盆地北部新生代构造演化历史,认为新生代构造活动控制了区域的构造地貌演化和地下水流向的改变,进而控制了地浸砂岩型铀矿成矿作用,并由此指出了三个泉斜坡带为有利的区域找矿远景区段。     

遥感岩性识别研究的发展趋势--遥感与航空放射性信息集成

岩石的吸收光谱主要是由杂质、包体、蚀变及替代成分产生的,每种岩石都难以形成象它的组成成分那样具有可分辨的很清晰的光谱特征;不同类型的岩石放射性元素的含量和分布特征是不同的,岩石放射性信息是岩性识别研究的重要判据。遥感与航空放射性信息的集成．既能提取光谱图像中的光语信息和空间纹理信息。又可利用航空放射性信息常常具有的甚至是诊断性的岩性识别能谱标志。能明显提高识别岩性的精度,更重要的是能谱不受值被的影响,有利于识别植被覆盖区的岩性。因此,这可能是遥感岩性识别研究的发展趋势之一。     

A TEM study of exsolution in Ca-rich pyroxenes from the Paris and Renazzo chondrites: Determination of type I chondrule cooling rates

We conducted a transmission electron microscope study of the exsolution microstructures of Ca-rich pyroxenes in type I chondrules from the Paris CM and Renazzo CR carbonaceous chondrites in order to provide better constraints on the cooling history of type I chondrules. Our study shows a high variability of composition in the augite grains at a submicrometer scale, reflecting nonequilibrium crystallization. The microstructure is closely related to the local composition and is thus variable inside augite grains. For compositions inside the pyroxene miscibility gap, with a wollastonite (Wo) content typically below 40 mole%, the augite grains contain abundant exsolution lamellae on (001). For grain areas with composition close to Wo₄₀, a modulated texture on (100) and (001) is the dominant microstructure, while areas with compositions higher than Wo₄₀ do not show any exsolution microstructure development. To estimate the cooling rate, we used the spacing of the exsolution lamellae on (001), for which the growth is diffusion controlled and thus sensitive to the cooling rate. Despite the relatively homogeneous microstructures of augite grains with Wo < 35 mole%, our study of four chondrules suggests a range of cooling rates from ~10 to ~1000 °C h⁻¹, within the temperature interval 1200–1350 °C. These cooling rates are comparable to those of type II chondrules, i.e., 1–1000 °C h⁻¹. We conclude that the formation of type I and II chondrules in the proto-solar nebula was the result of a common mechanism.     

Cooling rates of type I chondrules from Renazzo: Implications for chondrule formation

Cooling rates are one of the few fundamental constraints on models of chondrule formation. In this study, we used Cu and Ga diffusion profiles in metal grains to determine the cooling rates of type I chondrules in the Renazzo CR2 chondrite. To improve previous estimations of cooling rates obtained using this method, we used CT scanning and serial polishing of our sections to analyze equatorial sections of large metal grains. Through the cores of these metal grains situated at the surface of chondrules, the cooling rates calculated range from 21 to 86 K h⁻¹ for a peak temperature T_p ~ 1623–1673 K. A metal grain embedded in the core of a chondrule exhibits a cooling rate of 1.2 K h⁻¹ at a T_p ~ 1573 K. We also measured Cu-Ga diffusion profiles from nonequatorial sections of metal grains and calculated a lower range of cooling rates of 15–69 K h⁻¹ for T_p ~ 1473–1603 K compared to our results from equatorial sections. The high cooling rates inferred from the lightning model (several thousand K h⁻¹) are clearly at odds with the values obtained in this work. The X-wind model predicts cooling rates (~6–10 K h⁻¹) lower than most of our results. The cooling rates calculated here are in close agreement with those inferred from shock wave models, in particular for temperatures at which olivine crystallizes (from ~10 to several hundreds K h⁻¹ between 1900 and 1500 K). However, the chemical compositions of metal grains in Renazzo are consistent with the splashing model, in which a spray of metal droplets originated from a partially molten planetesimal. Volatile siderophile element depletion is explained by evaporation before metal was engulfed within silicate droplets. Liquid metal isolated from the liquid silicate crystallized during cooling, reacted with the ambient gas, and then re-accreted within partially molten chondrules.     

新疆玛因鄂博断裂带中花岗质糜棱岩锆石U-Pb SHRIMP和黑云母40Ar-39Ar年龄及意义

玛因鄂博断裂带具有左型剪切活动特征,分布其中的花岗质糜棱岩呈脉状、条带状产出,展布方向与剪切拉伸方向一致,为同构造花岗岩。其岩石化学为高钾钙碱性系列,属后碰撞“I”型花岗岩;稀土元素含量较高,ΣREE为(239.14~266.31)×10-6;具有中等程度的铕负异常,δEu为0.45~0.66,轻稀土明显富集。其锆石U-PbSHRIMP年龄为281±4Ma,黑云母40Ar-39Ar等时线年龄为236.1±1.2Ma。二者分别代表岩石的侵入年龄和后期的剪切变形年龄。其形成与早二叠世区域性大规模剪切活动有关,而黑云母40Ar-39Ar等时线年龄代表中三叠世早期的剪切变形活动。结合前人资料分析,玛因鄂博断裂的剪切活动持续时间较长,高峰期可能为290~270Ma,而其最后结束时间为230Ma左右。     

Tectonics and Petroleum Potential of the East China SeaShelf Rift Basin

There are two Cenozoic sedimentary basins in the East China Sea. They are the East China Sea shelf basin and the Okinawa Trough basin. The former can be divided into a western and an eastern rift region. The development of the shelf basin underwent continental-margin fault depression, post-rift and then tectonic inversion stages. Available exploration results show that the distribution of source rocks is controlled by the basin architecture and its tectonic evolution. In the Xihu depression, mudstones and coals are the main source rocks. The eastern rift region has good geological conditions for the formation of large oil and gas fields.     

新疆罗布泊K1孔磁性地层及古纬度初析

Ｋ１孔位于罗布泊“耳轮”构造的北缘。磁性地层初步研究得知,在孔深６１～６２ｍ处为界,以上为布容正向极性时（Ｂｒ）,以下为松山反向极性时（Ｍａ）。在孔底９７～１００ｍ处的正向极性偏移应属Ｃｏｂｂ Ｍｏｕｎｔａｉｎｓ事件,对照Ｓ．Ｃ．Ｃａｎｄｅ和Ｄ．Ｖ．Ｋｅｎｋ修定的古地磁极性年表,氏地层的年代为１．２Ｍａ,归属早更新世中期。中更新世地层厚５０余米,晚更新世地层厚１０ｍ左右,全新世地层厚度小于５ｍ。根