微地震监测技术在秦家屯地区的应用

详细阐述了微地震注水前缘监测的原理。应用微地震注水前缘监测系统,通过微地震信息的现场监测和解释,结合生产动态及其他监测资料综合分析,并以秦家屯地区的QK 3-5井为例,描述了秦家屯地区注水开发状态下水井水驱前缘位置,研究了地下油水运动规律,证明了方法的可靠性和实用性。结果表明,对于油田注水分析与研究微地震监测技术可以取得很好的效果。     

陆相沉积的天文地层研究方法简介——以井下地层为例

通过对我国大陆三十余口井的测井资料研究成果,归纳出对陆相地层进行天文地层研究的方法。介绍了所用的新的天文周期理论值、测井资料的选取及预处理方法,重点说明谱分析的数据点数的选定、不同参数(自然伽玛、自然电位和岩屑)的测井资料谱分析结果的对比,以实例说明如何选定主要优势旋回和AR值,以及FIR数字滤波器的基本性质和数字滤波结果,小波分析的特点和通过小波图进行调频的方法,并介绍了地层单位的延续时间计算和年龄确定方法。     

东营凹陷牛庄地区沙三段层序地层分析

山东济阳坳陷东营凹陷牛庄地区沙三段层序地层分析是在三级层序划分的基础上,通过对沉积体系发育特征和气候旋回单元的识别和解剖,建立了高精度层序地层单元的基本构型。气候旋回包含了从干旱枯水期到潮湿湖泛期的完整过程,沉积响应为受湖平面变化、沉积物供给等因素控制的多种方式叠置的湖底扇和前积体等,多期气候旋回叠合构成了湖泊层序的基本面貌。通过气候旋回的识别,可以对不同级别层序间的包含关系,以及高精度层序的内部构成进行分析和讨论。     

ENVIRONMENTAL MIGRATION AND SUSTAINABLE DEVELOPMENT——A Case Study of Southwest China

Ｉ．ＩＮＴＲＯＤＵＣＴＩＯＮＩｔｉｓｇｅｎｅｒａｌｙａｃｃｅｐｔｅｄｔｈａｔｔｈｅｄｅｇｒａｄａｔｉｏｎｏｆｒｅｎｅｗａｂｌｅｒｅｓｏｕｒｃｅｓａｎｄｆｒａｇｉｌｅｅｎｖｉｒｏｎｍｅｎｔｓｉｎｄｅｖｅｌｏｐｉｎｇｃｏｕｎｔｒｉｅｓｉｓｂｅｃｏｍｉｎ...     

南京伏牛山铜矿脉状矽卡岩稀土元素地球化学特征

介绍了南京伏牛山铜矿与成矿有关的花岗闪长斑岩及脉状矽卡岩的稀土元素组成模式及稀土元素地球化学特征。并据两者的相似性及变异性特征,探讨了脉状矽卡岩的成因。     

爆炸影响降水的观测分析

本文对“炮响雨落”的现象进行了实验验证。初步结果表明:在一定云雨条件下,炮击后可能促使未降水积状云产生降水,也可能促使已降水云的降水参量增大,这些变化发生迅速,但维持时间不长。并指出炮击促进云体降水的作用可能是通过改变支托水滴的气流造成的。在适当条件下,通过炮击影响气流的瞬时作用,可能触发云内不稳定能量释放,造成持续下沉,破坏云的发展,从而防止冰雹灾害。     

夏季青藏高原流场三维结构的模拟实验

本文用流体模拟实验的方法,研究了我国夏季青藏高原及邻近地区环流的三维结构和成因,主要结果为: 无转动因素时,高原加热作用能引起流体在低层径向地朝高原辐合,在高原上层放射状向周围辐散.高层辐散流体的一部分在高原内部开始下沉,形成高原上空的对流环,在有转动的实验中也观察到.辐散流体中还出现波动. 高原内部经常出现两个对流上升中心,中心附近的温度有较大脉动,两个对流上升区之间有时为下沉运动,构成高原内部独特的对流环. 通过高原中部的南北垂直剖面上,可观察到方向相反的两个对流环,流体在高原中部上升,在南北高原范围内下沉.在高原外部为高原加热引起的下沉运动. 实验表明,包括基本东西风和高原以外热源的环境背景条件,对高原流场有重要作用. 实验结果为解决夏季青藏高原环流的三维结构提供了依据,文中列举了一些说明的现象。     

l0舰船科学技术Ship Science and

青岛266071潜艇;;定深旋回;;控制定深等速直航潜艇操方向舵后将逐渐进入并保持圆周运动,要实现潜艇定深旋回,可同时操纵尾升降舵、首升降舵或者首尾升降舵配合操舵。通过仿真分析各种操纵方案的优劣,得到实现定深旋回的最佳控制方式。Modeling and analysis on the control of submarine's certain depth and gyration motionCHEN Jun-feng, TIAN Wei,CHE Meng-hu (Navy Submarine Academy, Qingdao 266071, China)Submarine will go into and keep the states of circular motion under the contro     

Characteristics of convection and overshooting in RGB and AGB stars

Based on the turbulent convection model (TCM) of Li & Yang, we have studied the characteristics of turbulent convection in the envelopes of 2 and 5M⊙ stars at the red giant branch and asymptotic giant branch phases. The TCM has been successfully applied over the entire convective envelopes, including the convective unstable zone and the overshooting regions. We find that the convective motions become progressively stronger when the stellar models are located farther up along the Hayashi line. In the convect...     

Cassini SAR, radiometry, scatterometry and altimetry observations of Titan’s dune fields

Large expanses of linear dunes cover Titan’s equatorial regions. As the Cassini mission continues, more dune fields are becoming unveiled and examined by the microwave radar in all its modes of operation (SAR, radiometry, scatterometry, altimetry) and with an increasing variety of observational geometries. In this paper, we report on Cassini’s radar instrument observations of the dune fields mapped through May 2009 and present our key findings in terms of Titan’s geology and climate. We estimate that dune fields cover ∼12.5% of Titan’s surface, which corresponds to an area of ∼10 million km², roughly the area of the United States. If dune sand-sized particles are mainly composed of solid organics as suggested by VIMS observations (Cassini Visual and Infrared Mapping Spectrometer) and atmospheric modeling and supported by radiometry data, dune fields are the largest known organic reservoir on Titan. Dune regions are, with the exception of the polar lakes and seas, the least reflective and most emissive features on this moon. Interestingly, we also find a latitudinal dependence in the dune field microwave properties: up to a latitude of ∼11°, dune fields tend to become less emissive and brighter as one moves northward. Above ∼11° this trend is reversed. The microwave signatures of the dune regions are thought to be primarily controlled by the interdune proportion (relative to that of the dune), roughness and degree of sand cover. In agreement with radiometry and scatterometry observations, SAR images suggest that the fraction of interdunes increases northward up to a latitude of ∼14°. In general, scattering from the subsurface (volume scattering and surface scattering from buried interfaces) makes interdunal regions brighter than the dunes. The observed latitudinal trend may therefore also be partially caused by a gradual thinning of the interdunal sand cover or surrounding sand sheets to the north, thus allowing wave penetration in the underlying substrate. Altimetry measurements over dunes have highlighted a region located in the Fensal dune field (∼5° latitude) where the icy bedrock of Titan is likely exposed within smooth interdune areas. The hemispherical assymetry of dune field properties may point to a general reduction in the availability of sediments and/or an increase in the ground humidity toward the north, which could be related to Titan’s asymmetric seasonal polar insolation. Alternatively, it may indicate that either the wind pattern or the topography is less favorable for dune formation in Titan’s northern tropics.