地震测井在煤炭地震地质勘探中的作用     

屈学贤  于树旺 《地质与资源》2004,13(3):187-188

地震测井是求取地震波在地层中的传播速度的一种有效的方法,其主要用途是标定地震地质层位,判定终孔深度.该技术在龙家堡南部地区准确地标定了TY1、TY地震地质层位,确定了M12的终孔深度.  相似文献   

泡沫增压技术在煤矿瓦斯抽放长钻孔施工中的应用前景     

高科  孙荣军  孙友宏 《吉林大学学报(地球科学版)》2005,35(4):543-544

为了解决在煤矿瓦斯抽放长钻孔施工中由于冲洗介质对孔壁的冲刷作用而出现塌孔、埋钻等难题,采用泡沫增压技术通过提供高压泡沫流压力来解决。论述了应用泡沫增压技术解决煤矿瓦斯抽放长钻孔施工问题的可行性和经济性。  相似文献   

Epicyclic oscillation modes of a Newtonian,non‐slender torus     

E. &#x;rmkov 《Astronomische Nachrichten》2005,326(9):835-837

All normal modes of oscillations of slender tori have been expressed analytically in the classic work by Blaes (1985). We adopt his approach in order to calculate the eigenfunctions and eigenfrequencies of a particular class of epicyclic modes for slightly non‐slender tori, and present results of our numerical simulation of torus epicyclic modes of oscillations, which will be compared with the analytical results. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

The onset of General Relativity: gravitationally redshifted emission lines     

A. Müller 《Astronomische Nachrichten》2006,327(10):1024-1027

We study and quantify gravitational redshift by means of relativistic ray tracing simulations of emission lines. The emitter model is based on thin, Keplerian rotating rings in the equatorial plane of a rotating black hole. Emission lines are characterised by a generalized fully relativistic Doppler factor or redshift associated with the line core. Two modes of gravitational redshift, shift and distortion, become stronger with the emitting region closer to the Kerr black hole. Shifts of the line cores reveal an effect at levels of 0.0015 to 60% at gravitational radii ranging from 10⁵ to 2. The corresponding Doppler factors range from 0.999985 to 0.4048. Line shape distortion by strong gravity, i.e. very skewed and asymmetric lines occur at radii smaller than roughly ten gravitational radii. Gravitational redshift decreases with distance to the black hole but remains finite due to the asymptotical flatness of black hole space–time. The onset of gravitational redshift can be tested observationally with sufficient spectral resolution. Assuming a resolving power of ∼100000, yielding a resolution of ≈0.1 Å for optical and near‐infrared broad emission lines, the gravitational redshift can be probed out to approximately 75000 gravitational radii. In general, gravitational redshift is an indicator of black hole mass and spin as well as for the inclination angle of the emitter, e.g. an accretion disk. We suggest to do multi‐wavelength observations because all redshifted features should point towards the same central mass. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

光照碾压混凝土大坝渗控分析     

荣冠  周创兵 《岩土力学》2006,27(Z2):429-434

基于光照水电站坝基水文地质条件及坝体渗透特性的研究,建立了大坝三维有限元模型,模型较详细地考虑了坝体大坝不防渗结构和排水系统及坝基地质和防排渗结构。分析研究了薄层单元、排水孔幕的模拟方法,采用合适的方法计算了同条件下的渗控情况。通过综合对比分析,对该坝的渗流规律及相应渗控措施进行了初步地探讨。  相似文献   

第四系深厚洪积物内成洞条件工程地质研究     

李院忠 《岩土力学》2006,27(Z2):601-606

经过对不同时期洪积物的成因、物质组成、结构、构造等的分析,以及对第一期洪积物内能否成洞的试验性模拟开挖、观察、分析,并在大量室内外物理力学性质试验的基础上,分析、量化出洪积物内成洞工程地质特性参数。在精心设计和施工下,深厚洪积物内开挖大跨度洞室顺利成功。  相似文献   

金沙峡电站闸坝区渗流场有限体积法数值模拟   总被引：2，自引：0，他引：2  

杨海英  陈刚  柴军瑞  张志昌 《岩土力学》2005,26(3):461-464

为实现泄冲闸、进水闸和土坝结合部位三维渗流场真实区域的数值模拟,采用有限体积法对含排水孔在内的闸坝区三维渗流场进行了网格划分。根据计算结果可知,闸基处防渗墙效果微弱,溢出点垂直坡降大于允许值,对工程不利,并提出了相应的改进措施。  相似文献   

单轴压缩下含孔脆性材料的力学行为研究   总被引：3，自引：1，他引：2  

段进超  唐春安  常旭  陈奇栓 《岩土力学》2006,27(8):1416-1420

运用材料破裂过程分析MFPA2D系统,在单轴压缩条件下对含单孔和双孔脆性材料破坏过程进行数值模拟。结果表明：原始的萌生裂纹不一定是最后形成宏观贯通破坏的主裂纹。岩石等脆性材料破坏的局部化特征,说明非均匀性是岩石类脆性材料发生局部破裂的根本原因。分析了孔的分布对材料强度以及破坏模式的影响,并给出破坏过程的应力-应变关系。指出了有的孔洞分布会增加应力的集中程度,而有的孔洞分布可以降低应力集中。数值模拟与试验结果具有较好的一致性。  相似文献   

阳泉矿区瓦斯抽放方式及优选原则   总被引：3，自引：1，他引：2  

张吉林  卫东  蔡锋光 《煤田地质与勘探》2001,29(4):17-19

针对阳泉矿区瓦斯赋存特点,通过对比分析各类瓦斯抽放方式指标,从而得出经济、技术可行的最优抽放方式;阳泉矿区单一煤层采用U+L型通风方式的工作面,大口径钻孔抽放方式是最佳选择和发展方向;15#煤层综放工作面采用U型通风方式和走向顶板岩巷抽放方式比较优越。   相似文献   

Measuring solar irradiance profiles in the Arctic sea ice using fiber optic spectrometry via inclined holes     

Zexia Qiu  Hangzhou Wang  Tao Li  Hong Song  Yuanqian Wu  Tingting Yan  Ying Chen 《海洋学报(英文版)》2021,40(3):134-141

An irradiance profile measurement approach and profiling system were developed to measure the solar irradiance profile of the Arctic sea ice using fiber optic spectrometry. The approach involved using a miniature spectrometer to sense light signals collected and transmitted from a fiber probe. The fiber probe was small, and could thus move freely in inclined bore holes drilled in sea ice with its optical entrance pointing upward. The input-output relationship of the system was analyzed and built. Influence factors that determined the system output were analyzed. A correctional system output approach was proposed to correct the influence of these factors, and to obtain the solar irradiance profile based on the measurements outputted by this system. The overall performance of the system was examined in two ice floes in the Arctic during the 9 th Chinese National Arctic Research Expedition. The measured solar irradiance profiles were in good agreement with those obtained using other commercially available oceanographic radiometers. The derived apparent optical properties of sea ice were comparable to those of similar sea ice measured by other optical instruments.  相似文献