甘肃老虎山闪长岩的地球化学特征及其成因

位于北祁连造山带东端的老虎山闪长岩侵位在晚奥陶统阴沟群砂板岩中,闪长岩的单颗粒锆石Ｕ－Ｐｂ年龄为４２３．５±２．８Ｍａ,是中志留世侵位的。老虎山闪长岩属于钙碱性岩系,富集ＬＲＥＥ和大离子亲石元素（ＬＩＬＥ）,Ｃｅ／Ｙｂ比值大于１３,Ｔｈ／Ｔａ比值大（１３～４２）,在微量元素分布图中呈现明显的Ｎｂ负异常,具岛弧或活动陆缘环境的特征。虽然老虎山闪长岩具有岛弧地球化学特征,但并不能认为它就产于岛弧环境,因为,在奥陶纪末期,早古生代的北祁连洋盆已经发生闭合,华北板块与柴达木板块已发生碰撞。因此,老虎山闪长岩是造山后侵位的,其成因可能与岩石圈拆沉作用有关。     

Modelling the January and July Climate of 9000 Years before Present

ＭｏｄｅｌｌｉｎｇｔｈｅＪａｎｕａｒｙａｎｄＪｕｌｙＣｌｉｍａｔｅｏｆ９０００ＹｅａｒｓｂｅｆｏｒｅＰｒｅｓｅｎｔ￥ＷａｎｇＨｕｉｊｕｎ（王会军）（ＬＡＳＧ，ＩｎｓｔｉｔｕｔｅｏｆＡｔｍｏｓｐｈｅｒｉｃＰｈｙｓｉｃｓ，ＣｈｉｎｅｓｅＡｃａｄｅｍｙｏｆ...     

汛期短历时强降水过程的闪电特征

对2011年3次短历时强降水天气过程的闪电特征分析结果表明:①3次短时强降水都以负闪为主,负闪占总闪电的比例都在92﹪以上;②小时闪电频数峰值超前降雨峰值1h或同相;③5min闪电频数超前雨量峰值5~60min;④负闪电密集区主要发生在40dBZ以上的回波区,偶尔发生的正闪一般在较弱回波处;闪电大部分发生在回波顶高大于5km以上的区域;多分布在速度不均匀场附近;闪电密集区与VIL大值区对应关系不太好;⑤不同云体,闪电特征不尽相同,闪电频数高峰有的发生在强回波阶段,有的并不是回波最强阶段,而是减弱阶段。强回波前沿出现闪电密集区或前方无回波处发生闪电,预示未来强回波移动的方向;有的云体发展、成熟阶段闪电分布密集,负闪电主要集中在强回波中心附近,云体减弱阶段闪电分散,集中在单体的不同部位。     

二维小波变换在消除相干噪声中的应用

相干噪声常使地震记录中的反射同相轴模糊不清,使得处理解释难以进行。而常规的各种ｆ－ｋ滤波技术不能对其有效地消除,且每种技术都有其局限性,容易产生人为假象,使信号发生很大畸变。我们的技术是利用二维小波变换,把二维地震信号变换到有关频率、时间、波数、空间的一个四维函数。根据信号和相干噪声在频率、时间、波数、空间等方面的局部差异来达到滤波的目的。经过对实际炮集数据的处理表明该方法比ｆ－ｋ滤波技术消除噪声的效果要好,信号的畸变程度更低,并且没有任何限制条件。     

Crustal structure beneath the central Tien Shan from ambient noise tomography

Through analysis of seismic ambient noise recorded by the GHENGIS array, we constructed a high‐resolution 3‐D crustal shear‐wave velocity model for the central Tien Shan. The obtained shear‐wave velocity model provides insight into the detailed crustal structure beneath the Tien Shan. The results obtained at shallow depths are well correlated with known subsurface geological features. Low velocities are found mainly beneath sedimentary basins, whereas high velocities are mainly associated with mountain ranges. At greater depths of ~43–45 km, high velocities were observed beneath the Tarim Basin and Kazakh Shield; these high velocities extend forward in opposite directions and tilt down towards the central Tien Shan to a depth of in excess of 50 km, most likely reflecting lateral variations in crustal thickness beneath the Tien Shan and surrounding platforms.     

Observations of Low-Latitude Coronal Plumes

Using Fe ix/x 17.1 nm observations from the Extreme-Ultraviolet Imaging Telescope (EIT) on the Solar and Heliospheric Observatory (SOHO), we have identified many coronal plumes inside low-latitude coronal holes as they transited the solar limb during the late declining phase of cycle 23. These diffuse, linear features appear to be completely analogous to the familiar polar plumes. By tracking them as they rotate from the limb onto the disk (or vice versa), we confirm that EUV plumes seen against the disk appear as faint, diffuse blobs of emission surrounding a brighter core. When the EIT images are compared with near-simultaneous magnetograms from the SOHO Michelson Doppler Imager (MDI), the low-latitude, on-disk plumes are found to overlie regions of mixed polarity, where small bipoles are in contact with unipolar flux concentrations inside the coronal hole. The birth and decay of the plumes are shown to be closely related to the emergence of ephemeral regions, their dispersal in the supergranular flow field, and the cancellation of the minority-polarity flux against the dominant-polarity network elements. In addition to the faint polar and nonpolar plumes associated with ephemeral regions, we note the existence of two topologically similar coronal structures: the giant plume-like features that occur above active regions inside coronal holes, and the even larger scale “pseudostreamers” that separate coronal holes of the same polarity. In all three cases, the basic structure consists of open field lines of a given polarity overlying a photospheric region of the opposite polarity; ongoing interchange reconnection at the X-point separating the open field domains from the underlying double-arcade system appears to result in the steady evaporation of material from the closed into the open region.     

利用遗传算法和最小二乘联合反演共和地震位错参数

中国地震局第二地形变监测中心已监测到与1990年4月26日青海共和7.0级地震有关的大幅度隆起垂直形变资料．基于这些形变资料,本研究首先利用全局搜索性能优良的遗传算法和弹性半空间单一矩形均匀滑动模型,对该地震的震源位错参数进行了初步反演;然后以遗传算法的反演结果为初始值,利用拟牛顿阻尼最小二乘方法对该地震的震源位错参数进行了更精细的反演．结果表明,共和7.0级地震的发震断层为一走向NW60左右、倾向SW、倾角37左右的右旋走滑逆冲断层,同震断层破裂长度约37 km,宽度约6 km,错动幅度约2.7 m．反演结果还同时表明,遗传算法与最小二乘方法相结合是一种行之有效的联合反演方法,它既可以保证实现全局最优解,防止最小二乘方法的局部极值解问题,又可以有效地解决遗传算法达到全局最优解区域后收敛速度过慢的问题．     

Geothermal potential evaluation and development prioritization based on geochemistry of geothermal waters from Kangding area,western Sichuan,China

Kangding geothermal area is located in the western Sichuan, belonging to southeastern margin of Tibetan Plateau. Similar to world-renowned south Tibetan and western Yunnan geothermal belt, western Sichuan has intensive surface thermal manifestations including boiling and hot springs. The emerging temperature of thermal waters ranges from 47 to 79 °C with total dissolved solids lying between 899 and 2550 mg/L. δ²H–δ¹⁸O isotopes indicate a meteoric source for the thermal waters and a significant positive oxygen-18 shift in the southern region. It is suggested that southern thermal waters experienced stronger water–rock interaction and are closer to thermodynamic equilibrium, which is also proved by the water type classification. The reservoir temperature calculated by empirical and theoretical chemical thermometry is 180–225 °C for the north and 225–310 °C for the south. Evidences of hydrogeochemistry, stable isotopes, geothermometry and radiocarbon dating indicate that southern region of Kangding area shows greater geothermal potential than the northern region. In addition, based on the hydrogeochemical modeling of mineral saturation, underlying problem of scaling is likely to occur in the study area. According to the results of reservoir temperature, south Kangding sub-district has greater potential in geothermal power generation and development than northern Kangding. Therefore, further exploration and drilling work should give priority to the south Kangding area.     

Sm–Nd geochronology and petrography of garnet pyroxene granulites in the northern Sulu region of China and their geotectonic implication

Abundant garnet-bearing granulite lenses are widely distributed in the northern part of the Sulu region and adjacent areas. They are possibly re-metamorphosed high-pressure metamorphic rocks. On the basis of detailed petrographic study, samples WD01, WD04 and ML06 from Laixi and Wendeng were identified as high-pressure granulites, and WH1 from Weihai as an original coesite-bearing eclogite. Three high-pressure granulite samples give mineral-WR isochron ages of 1846±76, 1743±79 and 1752±30 Ma. TDM ages are 3.3, 3.0 and 2.8 Ga. The Sm–Nd mineral-WR isochron ages are interpreted to date as the metamorphic resetting within the medium-pressure granulite facies, representing an isotopic re-homogeneity during uplifting of the high-pressure granulites from deep continent crust. It is important that Sm–Nd chronological characteristics are the same as Archaean high-pressure granulites in the North China craton. However, sample WH1 from Weihai demonstrates abnormal Sm–Nd characteristics. Its whole rock _Nd (0) value is +129. TDM age is 1.3 Ga, and constrains the minimum age of re-metamorphosed eclogite protolith formation to the mid-Proterozoic. This result is identical to those reported by Jahn (1994), showing complicated processes of metamorphism and metasomatism. The data in this paper provide further evidence to define the boundary between the North China craton and UHPM belt in eastern Shandong and to understand the geotectonic nature of the boundary.