多波束测量系统在长江潜坝工程中的应用

通过叙述多波束测量系统在长江水下工程中的应用实践和体会，说明多波束测量系统和单波束等常规测量仪器相比，具有测深点多、测量迅速快捷、全覆盖等优点。     

热敏电阻测温电桥的一种线性化方法

热敏电阻因温度系数大,尺寸小和价格低而得到广泛的应用。但其电阻和温度呈非线性关系 (1)式中T和T_0为绝对温度,R_(T_0)为参考温度T_0时的热敏电阻阻值。这给测量工作带来不便和限制。 不少作者研究过热敏电阻温度计的线性化问题。Beakley分析了负温度系数热敏电阻作为惠斯     

川北地区飞仙关组储层特征及其主控因素

采用宏观和微观相结合的方法,对川北地区飞仙关组鲕粒滩储层的研究表明,其储集岩类型主要有鲕粒白云岩和鲕粒灰岩,储集空间以次生孔隙为主,储集物性较差,多为低孔、低渗的裂缝-孔隙型和孔隙-裂缝型储层。研究区飞仙关组储层是海平面下降形成的一套产物,储层的发育及演化受到沉积作用和成岩作用的共同控制。二叠纪长兴组生物礁古地貌高地和龙门山岛链的形成,为飞仙关组的沉积提供了高能沉积环境,而相对海平面的下降促进了高能滩体的形成,位于台地边缘的高能鲕粒滩体是储层发育的有利部位;混合水白云化作用和埋藏溶解作用为次生孔隙的形成提供了有利条件,改善了储层的储集性能。     

Analytical solution for two-phase flow in a wellbore using the drift-flux model

This paper presents analytical solutions for steady-state, compressible two-phase flow through a wellbore under isothermal conditions using the drift flux conceptual model. Although only applicable to highly idealized systems, the analytical solutions are useful for verifying numerical simulation capabilities that can handle much more complicated systems, and can be used in their own right for gaining insight about two-phase flow processes in wells. The analytical solutions are obtained by solving the mixture momentum equation of steady-state, two-phase flow with an assumption that the two phases are immiscible. These analytical solutions describe the steady-state behavior of two-phase flow in the wellbore, including profiles of phase saturation, phase velocities, and pressure gradients, as affected by the total mass flow rate, phase mass fraction, and drift velocity (i.e., the slip between two phases). Close matching between the analytical solutions and numerical solutions for a hypothetical CO₂ leakage problem as well as to field data from a CO₂ production well indicates that the analytical solution is capable of capturing the major features of steady-state two-phase flow through an open wellbore, and that the related assumptions and simplifications are justified for many actual systems. In addition, we demonstrate the utility of the analytical solution to evaluate how the bottomhole pressure in a well in which CO₂ is leaking upward responds to the mass flow rate of CO₂-water mixture.     

逐次最优插值方案及其试验

本文介绍了“空军中尺度数值预报业务系统”前期处理模块中采用的逐次最优插值方案及相关处理技术，通过个例和一个月统计结果分析表明：本方案的插值效果较好，能够满足日常业务预报和数值式对资料分析精度的要求。     

测井资料解释煤成气层方法研究

本文在应用计算机对测井曲线进行分层的基础上,利用孔隙差异法、声波差值法、空间模量差比法和电阻率比值法逐层综合解释煤成气层,并对这几种方法在解释煤成气层时可能出现的问题进行了探讨．     

断层相互作用对中国川滇地区地震危险评估的意义

研究了1904年以来发生在中国四川、云南地区的强烈地震所伴生的库仑应力变化. 研究区涉及了中国大陆最活动的地震带. 由于欧亚板块与印度板块沿喜马拉雅会聚带的碰撞, 菱形区域的构造运动受到西藏高原向东扩展的影响,在东——西方向上受到主要板内走滑断裂运动的调节. 在研究区,断层顺时针逐步旋转,转动角达90deg;, 造成了应力场的复杂性. 计算了由强地震(MSge;6.5) 的同震滑动和连续构造加载在主要断裂上产生的库仑破裂函数变化(Delta;CFF). 在应力评估模型的每一步, 对是否能触发下一次地震的可能性都进行了判断. 最后,模型给出了下一次地震中断层易于破裂的证据,对未来危险性进行了评估.      

49种大气科学类期刊创刊及更名情况分析

收集、整理49种大气科学类期刊的创刊、中外文刊名变更、刊期变更、期刊网站等情况,并分析了存在的问题。结果表明:1)49种期刊中,《气象学报》创刊最早,《气象科技进展》创刊最晚,创刊、复刊的高峰期是20世纪70、80年代。2)25种期刊变更过刊名,其中18种期刊在2000年之后更名;著录参考文献时,应注意正确著录更名期刊的中外文刊名。3)25种期刊更改过刊期,其中20种期刊由季刊变更为双月刊。4)38种期刊建有自主网站,但尚需加强网站维护。     

东尼日尔盆地Tenere坳陷上白垩统海相烃源岩评价及勘探潜力

东尼日尔盆地是中西非裂谷系中典型的中—新生代裂谷盆地。Tenere坳陷位于盆地西北部,包括西部凹陷、东Ⅰ凹陷和东Ⅱ凹陷。对Saha-1井上白垩统岩屑样品的分析揭示,干酪根显微组分以不发荧光或弱荧光的无定形体为主,岩石抽提物中C29甾烷优势明显,说明该井上白垩统泥岩有机质输入以陆源植物为主。岩石热解分析表明上白垩统Yogou组泥岩大多数为中等—好烃源岩,有机质以Ⅱ2-Ⅲ型为主,Donga组泥岩大部分为差—中等烃源岩,以Ⅲ型为主;岩石热解峰温指示烃源岩成熟门限深度为2300 m左右。生烃史模拟显示,Saha-1井Yogou组泥岩尚未开始生烃,Donga组在白垩纪末期开始生烃,下部已进入生气阶段。综合研究认为Tenere坳陷的西部凹陷勘探潜力较大,而东Ⅰ凹陷和东Ⅱ凹陷潜力有限。     

DWT Power Spectrum of the Two-Degree Field Galaxy Redshift Survey

The power spectrum of the two-degree Field Galaxy Redshift Survey (2dFGRS) sample is estimated with the discrete wavelet transform (DWT) method. The DWT power spectra within 0.035 < k < 2.2 h Mpc-1 are measured for three volume-limited samples de-fined in consecutive absolute magnitude bins -19 ～-18, -20～ -19 and -21～-20. We show that the DWT power spectrum can effectively distinguish ACDM models of σs = 0.84 and σ8 = 0.74. We adopt maximum likelihood method to perform three-parameter fitting of the bias parameter b, pairwise velocity dispersion σpv and redshift distortion parame-ter β = Ω0.6m/b to the measured DWT power spectrum. The fitting results state that in a σ8= 0.84 universe the best-fit values of σm given by the three samples are mutually consis-tent within the range 0.28 ～ 0.36, and the best fitted values of σpv are 398 35-27475 37-29 and 550 ± 20km s-1 for the three samples, respectively. In the model of σ8 = 0.74, our three samples give very different values of Ωm. We repeated the fitting using the empirical formula of redshift distortion. The result of the model of low σ8 is still poor, especially, one of the best-fit values of σpv is as large as 103 km s-1. We also repeated our fitting by incorporating a scale-dependent galaxy bias. This gave a slightly lower value of Ωm. Differences between the models of σ8 = 0.84 and σ8 = 0.74 still exist in the fitting results. The power spectrum of 2dFGRS seems to disfavor models with low amplitude of density fluctuations if the bias parameter is assumed to be scale independent. For the fitting value of Ωm to be consistent with that given by WMAP3, strong scale dependence of the bias parameters is needed.