导向钻机液压管路的优化设计

导向钻机液压管路的尺寸直接影响着能量损失以及管路体积、质量的大小。采用优化设计方法,综合考虑能量损失及管路体积2方面的影响,建立了导向钻机吸油管路的目标函数,经编程求解,确定了管路的合理尺寸。     

长营岭—龙门冲原生晕异常及找矿预测

通过对珊瑚矿田长营岭－龙门冲地区岩石地球化学测量,圈定了该区Ｗ、Ｓｎ、Ｃｕ、Ｚｎ、Ａｓ、Ｂ、Ｆ等元素异常,原生晕严格受ＮＥ和ＮＷ两组断裂控制。综合评价认为处于长营岭钨锡矿带南延带的南风井多元素组合异常是矿异常,该异常明显地受ＮＥ（Ｆ９）断裂和ＮＷ（Ｆ１０）断裂控制,浓集中心位于Ｆ９断裂下盘,与长营岭矿区矿体在ＮＷ断裂下盘富集的规律相同。测区内,异常形态与北区具连续性,异常强度弱于北区,组分分带显示以隐伏花岗岩为成矿中心,但沿矿带由ＮＥ到ＳＷ并无明显的组分分带和元素组合变化,矿田内不仅矿带南延并向ＳＷ方向倾伏,而且很有可能深部隐伏花岗岩体亦分枝向南延伸。     

地层不整合遮挡油气藏地质储量计算新方法及其应用

从几何学的观点出发,针对纯油藏和具有气顶的油气藏,采用单储系数、横截面面积与油层横向分布长度三者乘积的方式改进采用单储系数、含油面积与油层厚度三者乘积方式的传统容积法,提出相应的地层不整合遮挡油气藏地质储量计算新公式,并根据油气藏的特点提出水平井钻遇油气藏厚度的预测公式。地层不整合遮挡油气藏的地质储量计算目前主要采用容积法,这类方法不仅计算繁琐,而且不确定因素较多;改进后的新方法计算简单方便,理论性更强,存在的不确定因素显著减少。采用新方法在高青油田高424块高424-1井区进行了实践应用。实践表明:改进的新方法适用于地层不整合遮挡油气藏的地质储量计算及预测水平井钻遇油气藏厚度。     

Distant field blue horizontal branch stars – III. Identification of a probable outer halo stream at Galactocentric distance r= 70 kpc

We present FOcal Reducer/low dispersion Spectrograph-1 spectra (from the European Southern Observatory's Very Large Telescope) of a sample of 34 faint  20.0 < g * < 21.1  A-type stars selected from the Sloan Digital Sky Survey Early Data Release, with the goal of measuring the velocity dispersion of blue horizontal branch (BHB) stars in the remote Galactic halo,   R ∼ 80 kpc  . We show that colour selection with  1.08 < u *− g * < 1.40  and  −0.2 < g *− r * < −0.04  minimizes contamination of the sample by less luminous blue stragglers. In classifying the stars we confine our attention to the 20 stars with spectra of signal-to-noise ratio >15 Å⁻¹. Classification produces a sample of eight BHB stars at distances  65–102 kpc  from the Sun (mean 80 kpc), which represents the most distant sample of Galactic stars with measured radial velocities. The dispersion of the measured radial component of the velocity with respect to the centre of the Galaxy is  58 ± 15 km s⁻¹  . This value is anomalously low in comparison with measured values for stars at smaller distances, as well as for satellites at similar distances. Seeking an explanation for the low measured velocity dispersion, further analysis reveals that six of the eight remote BHB stars are plausibly associated with a single orbit. Three previously known outer halo carbon stars also appear to belong to this stream. The velocity dispersion of all nine stars relative to the orbit is only  15 ± 4 km s⁻¹  . Further observations along the orbit are required to trace the full extent of this structure on the sky.     

A new method for determining physical parameters of fundamental mode RR Lyrae stars from multicolour light curves

We present a new method for determining physical parameters of RRab variables exclusively from multicolour light curves. Our method is an inverse photometric Baade–Wesselink analysis which, using a non-linear least-squares algorithm, searches for the effective temperature ( T _eff) and pulsational velocity ( V _p) curves and other physical parameters that best fit the observed light curves, utilizing synthetic colours and bolometric corrections from static atmosphere models. The T _eff and V _p curves are initially derived from empirical relations then they are varied by the fitting algorithm. The method yields the variations and the absolute values of the radius, the effective temperature, the visual brightness and the luminosity of individual objects. Distance and mass are also determined. The method is tested on nine RRab stars subjected to Baade–Wesselink analyses earlier by several authors. The physical parameters derived by our method using only the light-curve data of these stars are well within their possible ranges defined by direct Baade–Wesselink and other techniques. A new empirical relation between the I _C magnitude and the pulsational velocity is also presented, which allows to construct the V _p curve of an RRab star purely from photometric observations to an accuracy of about 3.5 km s⁻¹.     

基于弹性地基梁理论的土工格室加筋体变形分析

在土工格室处理软土路基加固机制研究的基础上,针对土工格室加筋体的受力变形特点,将格室体视为置放于Winkler地基上的连续长梁,基于传统的弹性地基梁理论,建立考虑水平摩阻力影响的土工格室加筋体的挠曲变形微分方程,并给出其幂级数解答,从而得到了土工格室加筋体在集中荷载作用下的变形计算方法,为土工格室加固处理后的软土路基沉降计算提供了依据。理论与试验结果对比分析表明,在格室体变形分析中不计水平摩阻力的影响将夸大格室体在荷载作用下的竖向变形,计入水平摩阻力影响后理论与实测曲线吻合更好。     

环保型弱凝胶护壁护心钻井液研究与应用

海域浅层气地质调查和盐湖环境科学钻探在松散砂岩钻探取样工程中,存在孔壁易坍塌、成孔率低等技术难题,为此开展了松散砂岩地层环保型弱凝胶护壁护心钻井液技术研究。通过弱凝胶结构研究及成胶剂、交联剂及抗盐降滤失剂等材料优选,研发了一套环保型弱凝胶护壁护心钻井液,评价了钻井液的流变性、滤失性、抑制性、护心性能、环保性能等性能,并在山西某盐湖环境科学钻探工程进行现场应用。室内及现场应用结果表明：研制的弱凝胶护壁护心钻井液具有良好的流变性、降滤失性、抑制性（岩屑回收率96.3%）、护壁护心性能及环保性能（BOD5/COD比值24.6%,EC50值47950 mg/L）,能有效解决松散砂岩类地层孔壁坍塌、岩屑不易携带等问题,在松散地层钻探工程中具有广阔的应用前景。     

新型热压WC-Fe基金刚石钻头钻进试验

为满足硬岩钻探的需要,将传统的热压碳化钨(WC)基金刚石钻头胎体中一部分WC用Fe代替,用Excel中的回归分析和非线性规划求解计算出的最优胎体配方,试制了新型热压WC-Fe基金刚石钻头,在可钻性为8级以上的岩石上进行了室内、外钻进试验,取得了较好的效果。      

新型电磁式孔底冲击器工作机理研究

冲击回转钻进是一种提高硬岩钻探效率的有效方法,实现冲击回转钻进的关键设备是冲击器。针对现有液动、风动冲击器在应用中存在的不足,提出了利用可充电电池组为动力的新型电磁式孔底冲击器的设计思路。详细介绍了新型电磁式孔底冲击器的结构和工作原理,对冲击器的控制系统、电磁驱动部分及电池组供电方案等关键设计技术进行了阐述。研究表明,新型电磁式孔底冲击器能够克服液动、风动冲击器的众多不足、优点显著,具有广泛的推广应用前景。     

非开挖三维轨迹设计软件的应用与优化

文章对非开挖导向孔三维轨迹设计软件的功能和使用方法进行了介绍,对该系统近两年的工程应用进行了总结,并通过一个典型工程实例介绍了软件模拟施工环境和设计轨迹的过程。通过用户反馈信息的搜集,介绍了软件存在的部分问题及其改进方案,并对软件的进一步开发的思路进行了展望。