川西坳陷源内油气成藏主控因素及模式:以孝泉-丰谷构造带须家河组五段为例

上三叠统须家河组是四川盆地川西坳陷的主力烃源岩系,而孝泉-丰谷构造带须家河组五段则是川西坳陷致密砂岩气勘探开发的新领域.利用地质、录井、钻井、分析化验等资料,结合盆地模拟技术,在须五段内部烃源岩、储集层特征以及其发育构造-沉积背景分析的基础上,探讨了孝泉-丰谷构造带须家河组五段源内成藏的主控因素,并建立了相应模式.须五段泥页岩连续稳定分布,有机质丰度高,有机质类型以Ⅲ为主,总体上处于成熟-高成熟阶段;砂岩储层总体为特低孔特低渗致密储层;沉积相以三角洲前缘亚相为主.须五段源内成藏主控因素为烃源岩控制气藏范围和规模,有利相带决定了优质储层发育位置,源储配置关系控制油气富集程度,异常高压有效保存和改造;总结其成藏模式为源内短距离垂向叠覆运聚模式.      

东昆仑造山带索拉沟地区三叠纪赞岐质闪长岩的成因机制及其对古特提斯造山作用的启示

具有特殊成因机制的赞岐岩是探究深部岩浆动力学过程与区域构造演化的重要岩石探针之一.以东昆仑索拉沟地区赞岐质闪长岩为研究对象,开展系统的岩石学、年代学、元素地球化学和Lu-Hf同位素分析,厘定其岩石成因,揭示其对古特提斯造山作用的启示.锆石U-Pb年代学分析表明,索拉沟闪长岩形成于中三叠世（~243 Ma）.岩石具有较低含量的SiO₂（50.26%~57.40%）,较高的全碱成分（Na₂O+K₂O=3.5%~6.3%）、MgO（6.0%~7.1%）和Mg#值（50.1~60.9）,属于高镁钙碱性准铝质岩石.索拉沟闪长岩具有较高的Sr（622×10-6~1 041×10-6）、Cr（30×10-6~161×10-6）和Ni（19×10-6~79×10-6）以及中等的Y（7.6×10-6~24.3×10-6）和Yb（0.62~1.87）含量,与典型的高镁安山质赞歧岩成分类似.岩石富集轻稀土和大离子亲石元素（如Rb、K和Pb）,亏损高场强元素（如Ta、Nb和Zr）,具有弧岩浆岩的化学属性.Lu-Hf同位素研究揭示,索拉沟闪长岩起源于富集岩石圈地幔（ε_Hf（t）=-2.4~-0.4,T_DM=0.89~0.99 Ga）.岩石成因分析表明,东昆仑索拉沟中三叠世赞岐质高镁闪长岩形成于陆缘弧背景,岩浆起源于富集岩石圈地幔,且岩浆经历了以角闪石和黑云母为主的分离结晶作用.中三叠世是东昆仑造山带古特提斯洋壳俯冲和地体碰撞的构造转换阶段,索拉沟赞岐质高镁闪长岩可能是俯冲作用结束时板片断离的岩浆响应.      

地球外部扰动重力严密改化模型及分析检验

直接积分模型是计算地球外部扰动重力的主要数学工具,将全球积分模型改化为局域积分模型是实现地球外部重力场赋值的前提条件.相比表层积分模型和向上延拓积分模型,Stokes积分模型要求的输入信息种类最少,故在减轻数据保障压力方面具有比较明显的优势.在实施Stokes积分模型工程化应用过程中,我们发现扰动重力径向分量积分模型从...     

产业有序转移与区域产业协调发展——基于广东产业有序转移的经验

阐明了产业有序转移、区域产业协调发展的内涵,构建了产业有序转移对区域产业协调发展作用机制的分析框架。根据这个分析框架,从理论和广东产业转移经验两个方面进一步揭示了产业有序转移促进区域产业协调发展的机制。结果表明,产业有序转移是在政府有效干预下所形成的有利于区域产业协调发展的一种产业转移形式。产业有序转移通过诱致或促进区域产业结构优化调整、区际产业合理分工、区际产业关联互动,以及提高区域产业发展总体效率等路径,促进区域产业协调发展。     

Lithium depletion in late-type dwarfs

Using a self-consistent dynamic theory of non-local convection, the atmospheric lithium-abundance depletion values of a series of stellar evolutionary models with     are calculated, and the results show that the general observed properties of lithium abundance in lower-main-sequence stars can be reproduced by overshooting mixing and gravitational settling. After a careful study of the mechanisms of lithium depletion in stars, it is concluded that overshooting mixing and microdiffusion induced by gravitational settling and radiative acceleration are the two primary depletion mechanisms: for warm stars with     (or     ) microdiffusion dominates, while it is the other way round for cooler objects with     (or     ).     

Calculating the Light Period of BL Lac Object S5 0716+714 by Wavelet Analysis Method

A kind of wavelet analysis method for identifying the light period of the BL Lac object S5 0716+714 is introduced. The rather complete observed data in the four optical wavebands B, V, R, I are collected, and the long-term light curves based on 10-day averaging are obtained. On these light curves, the periodicity analysis is performed by using a wavelet analysis method. The result demonstrates that the wavelet analysis method is preferable for searching and identifying the light periods of BL Lac objects. From the contour map of the real part of the wavelet transform coefficient, the periodical light variations of the BL Lac object S5 0716+714 can be precisely identified. By analyzing the wavelet variance curves at the 4 wavebands, it is found that the BL Lac Object S5 0716+174 has a stable light period of 1160 days. This result is consistent with the 3.3-year period given by Raiteri et al. It is predicted that the next outburst in this object will happen around the August of 2011.     

A Study of the γ-ray and X-ray Radiations of BL Lac Objects

The X-ray and γ-ray flux densities of 18 γ-loud BL Lac objects as well as their average spectral indices of X-ray wave band (1 keV) and γ-ray wave band (>100 MeV) are collected, and the correlations among the various quantities are examined. The results indicate: (1) The X-ray flux density and the γ-ray flux density exhibit rather strong correlations in all the states, high, low or mediate. (2) Between the mean spectral indices in X-ray and γ-ray wave bands there is a comparatively intense anti-correlation. (3) Between the average spectral indices and the X-ray and γ- flux densities there is no evident correlation either in the high or the mediate state. (4) Between the average spectral index of γ-ray wave band and the flux density of X-rays in low state there is a rather strong anticorrelation. Between the mean spectral index of X-ray wave band and the γ-flux density in low state there also exists a weak correlation. The results of our analysis support the viewpoint that both the X-ray and γ-ray emissions of BL Lac objects come from the synchrotron radiation and synchrotron self Compton (SSC) radiation with one and the same distribution of relativistic electrons.     

雷电临近预警系统的运行试验

介绍了中国气象科学研究院研发的雷电临近预警系统(CAMSLNWS)在北京地区开展的业务运行试验.通过运行测试以及预警结果与闪电监测结果的对比评估,表明:CAMS.LNWS能够稳定运行,定时读取多种探测资料、自动生成并循环显示雷电发生概率、雷电活动区域移动趋势和重点区域雷电危险度等级三种雷电临近预警产品;CAMS.LNWS的雷电发生概率预警产品具有较高的命中率,能够较好地对0～30min内可能发生闪电的区域进行有效预警;随着预警时间的延长,CAMS.LNWS的预警效果会有所降低.     

1980年地面气象观测规范变更对能见度资料连续性影响研究

为探讨1980年地面气象观测规范变更对能见度资料连续性,采用累积百分率法、Ridit分析法、"非常好"能见度分析法等工具,对1951—2006年南宁、桂林城市大气能见度变化进行了分析。分析显示:南宁、桂林能见度高值在1980年相对1979年迅速下降,并导致平均Ridit值,"非常好"能见度天数迅速降低,其原因是1980年采用新《地面气象观测规范》的结果,采用能见度高值、Ridit值、"非常好"能见度对比分析1980年前后的能见度变化是不可信的;南宁、桂林能见度中、低值受1980年采用新的《地面气象观测规范》的影响较小,保持了很好的连续性,资料跨越1980年是连续可靠的,可以用来进行对比分析1980年前后的能见度变化。     

我国飞机观测气象资料概况及质量分析

为全面了解我国飞机观测气象资料的时空分布特征和质量状况,该文介绍了AMDAR(Aircraft MeteorologicalData Relay)计划的发展及我国通过AMDAR计划实施获取的飞机观测气象资料(又称AMDAR资料)的时空分布特征,分析了起飞和降落阶段飞机观测所获廓线资料的可用性,并分别对全球AMDAR资料和我国AMDAR资料进行极值检查、空间位置检验和时间一致性检验,对我国AMDAR资料错误率的月值变化和垂直分布特征进行了分析。结果表明:我国三分之二的AMDAR资料集中在飞机的起飞和降落阶段,并主要集中在我国中东部地区;利用我国AMDAR资料制作的廓线垂直分辨率大部分高于10 hPa。我国AMDAR资料的气温错误率低于全球水平,但风速错误率高于全球水平,错误资料主要集中在近地面层。从2008年开始,我国AMDAR资料的质量状况较往年有了明显改善,风速错误率一直维持在1.3%以下,气温错误率维持在0.2%以下。总体来说,我国AMDAR资料已成为我国高空气象观测资料的重要组成部分,资料质量稳定,具有较高的应用价值。