井周钻孔补砾工艺在修井中的应用          下载免费PDF全文

杨立斌  王国瑞 《探矿工程》2007,34(3):9-11

提出了通过井周钻孔恢复旧井填砾层，提高管井涌水量的方法，通过在某电厂供水管井中的实践，证明效果良好。  相似文献   

万丰路桥大吨位矩形截面桩成孔施工技术     

王宏坤 《探矿工程》2007,34(2):10-12

针对在卵石及基岩地层中桩孔施工时成孔难、渗漏大的问题，以液压抓斗为成孔设备，采用合理的机械结构、钻进方法、泥浆配方进行矩形截面桩的施工。  相似文献   

水下收缩裂隙形成过程及裂缝充填模式研究     

赵振宇  周瑶琪  马晓鸣  冀国盛 《地学前缘》2007,14(4):215-221

通过野外实地考察测试,对水下收缩裂隙整体形成过程、裂隙内充填物沉积模式、影响因素等进行了详细讨论,并且建立了相应的地质理论模型。水下收缩裂隙的形成共分4个阶段,依次为:泥水混合物进入低洼地带的初始混浊状态;沉积压实稳定阶段;水位线下降,盐度增大,裂隙形成阶段;沉积裂隙充填阶段。其中“异常高压作用”,对于初始裂隙的形成、沉积物孔隙水的有效排出以及主要渗流通道的发育起到了重要作用。单一泥质地层裂隙内充填物沉积模式与沙泥互层的多旋回地层略有差异,主要表现为沙层的润滑作用以及对早期裂隙内充填物类型的影响。上述两种地层裂隙内充填物沉积特征均与后期充注期次相对应,表现出很好的韵律性。裂隙纵剖面中生物发育层的出现,对裂隙内充填物的物理、化学性质将产生重要影响。  相似文献   

挤土类桩的挤土效应及其防治方法     

陈锦麟 《中国煤田地质》2007,19(A01):59-60

挤土效应是所有挤土类桩面临的共同问题，它可能造成临近建筑物破坏，地下管线断裂，道路隆起以及工程质量事故。依据挤土类桩挤土效应的形成机理，结合工程实例，提出了减少挤土效应的措施，如预钻排水孔、开挖防挤沟、设置观测点、控制压桩速度等措施，并根据施工地区不同的环境条件提出了合理的压桩顺序。  相似文献   

长河煤矿充水因素分析及防治水措施     

朱德强 《中国煤田地质》2007,19(6):42-44

长河煤矿为地质构造中等复杂区，其矿区地质及水文地质条件表明，地表水、直接充水含水层煤系砂岩裂隙水、老窑水、构造断裂带水都可构成该矿井开采的充水因素，且其涌水量大小与大气降水关系密切。针对矿井开采的具体情况提出了一系列的防治措施，并取得了良好的效果，对煤矿水害的防治有一定的指导意义。  相似文献   

磁铁矿采空区处理施工工艺与技术方法探讨   总被引：3，自引：0，他引：3  

闵卫鲸  曾德礼 《中国地质灾害与防治学报》2007,(Z1)

文章系统地介绍了采用地质钻机成孔,高压注浆机进行充填注浆的施工方法。为了将水泥砂浆及水泥粉煤灰浆填入采空区,采用能施加高压的输送泵及高压注浆设备、铸铁注浆管、水泥封孔的注浆工艺处理采空区铁路路基。在信息化施工过程中,通过试验不断地调整设计方法、改进施工工艺,在处理巨型磁铁矿采空区工程实践中达到了预期的目标。施工中,在控制充填边界、封孔方法及施工工艺等方面有一定的创新。提出的采空区施工技术控制、质量检测与评价方法,对同类工程勘察、设计及施工具有一定的参考价值。  相似文献   

深厚堆积体地层钻进工艺方法研究     

朱国平  段宏 《中国地质灾害与防治学报》2007,(Z1)

太钢(集团)有限公司矿业公司峨口铁矿是一个从20世纪60年代就开始开采的老矿区,经过长期开采储量已严重不足。为了延长矿山寿命,需要进一步扩大勘探范围,在原有矿山周边地区进行勘探。最初采用岩心勘探钻机进行常规回转钻进加套管护壁,历时3个月。在上部堆积体地层最大钻孔深度达到约20m,再也无法继续钻进,使勘探工作被迫停止。针对深厚堆积体地层钻孔施工遇到的具体困难,介绍了风动潜孔锤双管跟管钻进在工程施工中的应用,在对深厚堆积体地层进行分析的基础上,探讨进行深厚堆积体地层钻孔施工的工艺方法及技术措施;在钻孔结构基础上选择钻孔设备及钻孔机具的一般原则,对深厚堆积体地层的钻孔工程施工具一定指导意义。  相似文献   

A simple mass estimate for central black holes in cuspy galaxies     

Herwig Dejonghe  Anne Mathieu  Veronique De Bruyne  Sven De Rijcke 《Celestial Mechanics and Dynamical Astronomy》1998,72(3):219-233

We argue that the temperature of the stellar phase is likely a monotically decreasing function of radius in the central regions of elliptical galaxies with cusps. We show that it requires the presence of a central mass concentration. An estimate of its minimum mass based on few parameters is given. This lower bound is consistent with current mass values of the central objects in galaxies derived from detailed models. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

High-redshift galaxies, their active nuclei and central black holes     

Martin G. Haehnelt  Priyamvada Natarajan  & Martin J. Rees 《Monthly notices of the Royal Astronomical Society》1998,300(3):817-827

We demonstrate that the luminosity function of the recently detected population of actively star-forming galaxies at redshift z  = 3 and the B -band luminosity function of quasi-stellar objects (QSOs) at the same redshift can both be matched with the mass function of dark matter haloes predicted by standard variants of hierarchical cosmogonies for lifetimes of optically bright QSOs anywhere in the range 10⁶ to 10⁸ yr. There is a strong correlation between the lifetime and the required degree of non-linearity in the relation between black hole and halo mass. We suggest that the mass of supermassive black holes may be limited by the back-reaction of the emitted energy on the accretion flow in a self-gravitating disc. This would imply a relation of black hole to halo mass of the form M _bh ∝  v ⁵_halo ∝  M ^5/3_halo and a typical duration of the optically bright QSO phase of a few times 10⁷ yr. The high integrated mass density of black holes inferred from recent black hole mass estimates in nearby galaxies may indicate that the overall efficiency of supermassive black holes for producing blue light is smaller than previously assumed. We discuss three possible accretion modes with low optical emission efficiency: (i) accretion at far above the Eddington rate, (ii) accretion obscured by dust, and (iii) accretion below the critical rate leading to an advection-dominated accretion flow lasting for a Hubble time. We further argue that accretion with low optical efficiency might be closely related to the origin of the hard X-ray background and that the ionizing background might be progressively dominated by stars rather than QSOs at higher redshift.  相似文献   

Line emission from accretion discs around black holes: the analytic approach     

Andrej ?ade?  Claudio Fanton  Massimo Calvani 《New Astronomy》1998,3(8):528-654

The broad X-ray iron line observed in many active galactic nuclei spectra is thought to originate from the accretion disc surrounding the putative supermassive black hole. We show here how to perform the analytical integration of the geodesic equations that describe the photon trajectories in the general case of a rotating black hole (Kerr metric), in order to write a fast and efficient numerical code for modelling emission line profiles from accretion discs.  相似文献