东昆仑三维重力异常解释方法研究

小波变换是一种广泛应用的信号处理技术,它具有良好的时—频局部化特性。本文探讨了小波变换在分解重力异常中的应用。同时,利用计算机对重力资料的三维定量解释,进行了初步试算。通过东昆仑地区实际资料处理,认为这二种方法在重力资料处理解释中,具有快速、简捷的特点。     

The formation of wind curl in the marine atmosphere boundary layer over the East China Sea Kuroshio in spring

Various data are used to investigate the characteristics of the surface wind field and rainfall on the East China Sea Kuroshio (ESK) in March and April, 2011. In March, the wind speed maximum shows over the ESK front (ESKF) in the 10 meter wind field, which agrees with the thermal wind effect. A wind curl center is generated on the warm flank of the ESKF. The winds are much weaker in April, so is the wind curl. A rainband exists over the ESKF in both the months. The Weather Research and Forecasting (WRF) model is used for further researches. The winds on the top of the marine atmosphere boundary layer (MABL) indicate that in March, a positive wind curl is generated in the whole MABL over the warm flank of the ESKF. The thermal wind effect forced by the strong SST gradient overlying the background wind leads to strong surface northeasterly winds on the ESKF, and a positive shearing vorticity is created over the warm flank of the ESKF to generate wind curl. In the smoothed sea surface temperature experiment, the presence of the ESKF is responsible for the strong northeast winds in the ESKF, and essential for the distribution of the rainfall centers in March, which confirms the mechanism above. The same simulation is made for April, 2011, and the responses from the MABL become weak. The low background wind speed weakens the effect of the thermal wind, thus no strong Ekman pumping is helpful for precipitation. There is no big difference in rainfall between the control run and the smooth SST run. Decomposition of the wind vector shows that local wind acceleration induced by the thermal wind effect along with the variations in wind direction is responsible for the pronounced wind curl/divergence over the ESKF.     

Deep crustal structures of eastern China and adjacent seas revealed by magnetic data

Through reduction to the North Pole and upward continuation of the total field magnetic anomalies, we analyze magnetic patterns and spatial distributions of different tectonic blocks and crustal faults in eastern China and adjacent seas. Depths to the Curie isotherms are further estimated from radially averaged amplitude spectra of magnetic data reduced to the pole. Data reductions effectively enhance boundaries of regional tectonic belts, such as the Dabie ultra-high metamorphic belt, the Tanlu Fault, and the Diaoyudao Uplift. Curie depths are estimated at between 19.6 and 48.9 km, with a mean of 31.7 km. The Subei Basin and the south Yellow Sea Basin in the lower Yangtze block show relatively deep Curie isotherms, up to about 35 km in depth, whereas in the surrounding areas Curie depths are averaged at about 25 km. This implies that the lower Yangtze Block has experienced a unique tectonic evolution and/or has unique basement lithology and structures. From a regional perspective, sedimentary basins, such as the Subei Basin, the south Yellow Sea Basin, and the East China Sea Basin, normally show deeper Curie isotherms than surrounding uplifts such as the Diaoyudao Uplift and the Zhemin Uplifts. Curie isotherms also upwell significantly in volcanically active areas such as the Ryukyu Arc and the Cheju Island, confirming strong magmatic and geothermal activities at depth. Supported by National Natural Science Foundation of China (Grant Nos. 40776026 and 40876022) and National Basic Research Program of China (Grant No. 2007CB411702)     

火山沉积岩及其矿床研究中伽马测井曲线解释的误区

根据酸性凝灰岩和酸性火山事件粘土岩的自然伽马测井曲线,对当前流传的"沉积岩层的放射性强度(或放射性核素的含量)随泥质含量的增加而增高"的概念和用自然伽马值及经验公式求泥质含量提出质凝。酸性凝灰岩的自然伽马曲线有高异常响应,若解释为泥岩显然是误解,故将沉积岩伽马曲线高异常一律解释为泥岩是片面的。各类火山事件粘土岩的伽马值相差悬殊,但其泥质含量几乎相等,用它们的伽马值计算泥质含量误差甚大。最后对铝土矿层的伽马曲线稍加解释,指出核测井应用的远景。     

黄骅坳陷地热资源研究

黄骅坳陷在勘探石油过程中发现了丰富的地下热水。根据实际资料对黄烨坳陷大港探区的地热资源进行了初步评价,提出了黄骅场陷储热系统和热异常区的分布规律,通过水化学分析,指出坳陷补给条件差,可实行人工回灌,增加地下热水资源。     

Local Similarity Relationships of Non-Dimensional Wind and Temperature Gradient in the Tower-Layer Atmosphere over Beijing City

Micrometeorological data for wind and temperature from a 325 m high tower in Beijing City are analyzed by use of local similarity theory. Non-dimensional wind and temperature gradients, Фm and Фh, are determined by three techniques called, respectively, eddy-correlation, mean profiles and inertia-subrange cospectra (ISC) method for a wide range of atmospheric stratification from unstable to stable conditions. Average dissipation rate Фε of turbulent kinetic energy (TKE) is evaluated from u-spectrum, as a quantity required in the last technique. Ratio of the eddy transfer coefficients. α (= Kh / Km,), is calculated from Фm and Фh estimations. The results from various techniques are compared with each other and with some available empirical results in the tower-layer. It is shown that the empirical relationships determined by mean profiles and ISC methods in the tower-layer turbulence are in agreement with each other and with some other results.     

INTEGRAL observations of TeV plerions

Amongst the sources seen in very high gamma-rays several are associated with Pulsar Wind Nebulae (“TeV plerions”). The study of hard X-ray/soft gamma-ray emission is providing an important insight into the energetic particle population present in these objects. The unpulsed emission from pulsar/pulsar wind nebula systems in the energy range accessible to the INTEGRAL satellite is mainly synchrotron emission from energetic and fast cooling electrons close to their acceleration site. Our analyses of public INTEGRAL data of known TeV plerions detected by ground based Cherenkov telescopes indicate a deeper link between these TeV plerions and INTEGRAL detected pulsar wind nebulae. The newly discovered TeV plerion in the northern wing of the Kookaburra region (G313.3+0.6 powered by the middle aged PSR J1420-6048) is found to have a previously unknown INTEGRAL counterpart which is besides the Vela pulsar the only middle aged pulsar detected with INTEGRAL. We do not find an INTEGRAL counterpart of the TeV plerion associated with the X-ray PWN “Rabbit” G313.3+0.1 which is possibly powered by a young pulsar.     

湛江港邻近海域台风浪的模拟研究

对第三代近岸海浪数值模式SWAN及包含的物理过程进行了简要介绍，利用该模式对影响南海湛江港海域的二次台风浪过程进行了模拟研究：由藤田台风风场模型同化相应时刻的台风要素、NCAR/NCEP网格点资料、单站观测资料后，提供模式所需风场；利用自嵌套的方式，提供模式波谱边界条件；两次模拟结果与实际海浪观测资料相符较好，可以为该海域台风浪的模拟预报提供较为重要的参考。     

利用重力/GPS联合观测数据计算地壳垂向构造应力的新方法

本文提出一种基于重力/GPS联合观测数据计算垂向构造应力的新方法.计算步骤如下:(1) 通过重力/GPS联合观测数据计算布格重力异常;(2) 依据布格重力异常数据推算莫霍面深度;(3) 依据GPS观测数据,通过均衡理论计算均衡面深度;(4) 依据莫霍面与均衡面之间剩余物质(壳幔物质密度差)所承受的附加浮力,计算地壳承载的垂向构造应力.本文利用上述构造应力新算法,计算了巴颜喀拉块体东边界及周边地区垂向构造应力分布,发现龙泉山断裂带以东地区垂向构造应力基本为零,龙泉山断裂带与龙门山断裂带之间地区垂向构造应力为正值,巴颜喀拉地块东部垂向构造应力为负值.鲜水河断裂带东南段周边蓄积了-40~-50 MPa的垂向构造应力,且梯度变化剧烈;松潘高原蓄积的垂向构造应力大约为-10~-20 MPa,相对较小.     

祁连东部西格拉高Sr/Y型花岗岩LA-ICP-MS锆石U-Pb定年及其地球化学特征

西格拉花岗岩体位于祁连东部的米屈花岗岩带上,空间上呈NW-NWW向展布,岩体由花岗闪长岩-花岗岩-正长岩组成,主要岩性为花岗闪长岩。LA-ICP-MS锆石U-Pb定年结果表明,西格拉花岗闪长岩存在两期岩浆作用,年龄分别为465.6±6.5Ma、443.2±4.8Ma,其中,前者与祁连洋俯冲极性发生转变的时限(~463Ma)相近,而后者与祁连洋闭合的时间(~445Ma)相似。早期淡色花岗闪长岩具正铕异常(δEu=2.44),晚期暗色花岗闪长岩则为弱负/正铕异常(δEu=0.94~1.32),两者均显示出高Si、Al,富Na贫K,富集Ba、Sr、LREE,高Sr/Y值,低Y、HREE含量,亏损HFSE(Nb、Ta、Ti、P)的特征,与Martin et al.(2005)划分的高硅埃达克岩(HSA)相似。其源区可能均残留石榴子石、普通角闪石及少量金红石,而斜长石则大量参与部分熔融过程,推测早期花岗闪长岩的源区深度可能超过50km;整体上,由早期→晚期反映出加厚地壳减薄、地幔组分贡献增强的趋势;两者可能均为加厚下地壳物质部分熔融的产物。