井下倾斜仪的定向反演问题

倾斜观测已在地球物理领域以及地震部门获得广泛应用。有时,由于种种原因井下倾斜仪难以定向,这会对倾斜观测资料的解释带来困难,本文阐明一种利用潮汐信号进行井下倾斜仪定向反演的方法。     

用套筒致裂法测试岩体应力反弹性模量与讨论

在改进套筒致裂装置性能的基础上,使压力-体积曲线的记录与处理得到改善,对潘三矿东采区的测试实践表明,得出的压力-体积曲线较好地反映了钻孔围岩随内压增加所表现出的力学性质。还探讨了如何通过改进套筒致裂技术来实现由围岩应力测试发展到原岩应力测试以及围岩损伤区的测定。     

连续变脉宽发送激电方波与自动变周期测量二次场信号

介绍一种新的激电数据采集方式。该方式的主要特点在于一次测量操作可同时获取极化二次场随时间衰减和随深度变化的信息,同时还讨论了实现该采集方式的仪器工作原理和信号测量过程中的一些技术问题。     

Recent tectonic stress field research in Shanxi graben system

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一种有效的结构动态参数识别方法

本文以优化算法中单纯形法为基础,提出了一种只有利用实测的结构模态部分信息识别其结构参数的方法。数值计算表明,该算法具有良好的精度和适用性。     

张北6.2级地震的水化前兆异常分析及有关问题讨论

张北地震前、在中期阶段,多井水氡出现负异常变化;短期阶段出现区域水氡差分异常的月频次增加;短临阶段则出现怀来４井水汞的多次突跳。大同地震前多井出现水氡的趋势性正常,是张北地震水化前兆最显著的不同之处。本文分析了张北地震水化方法预报失误的原因。讨论认为,水氡负异常做为中期前兆的信度较低;为提高水化预报地震的效能,必须与其它前兆手段相结合。     

Change in the magnetic properties of bituminous coal intruded by an igneous dike, Dutch Creek Mine, Pitkin County, Colorado

Magnetization measurements have been made on natural coke–coal samples collected at various distances from a felsic porphyry dike in a coal seam in Dutch Creek Mine, Colorado to help characterize the nature and distribution of the iron-bearing phases. The magnetization passes through a maximum at the coke-to-coal transition about 31 cm from the dike contact. The magnetic measurements support the geochemical data indicating that magmatic fluids along with a high-temperature gas pulse moved into the coal bed. Interaction of the magmatic fluids with the coal diminished the reducing power of the thermal gas pulse from the dike to a point about 24 cm into the coal. The hot reducing gas penetrated further and produced a high temperature (400–525°C) zone (at about 31 cm) just ahead of the magmatic fluids. Metallic iron found in this zone is the principal cause of the observed high magnetization. Beyond this zone, the temperature was too low to alter the coal significantly.     

Depth of the base of the Jackson aquifer, based on geophysical exploration, southern Jackson Hole, Wyoming, USA

 A geophysical survey was conducted to determine the depth of the base of the water-table aquifer in the southern part of Jackson Hole, Wyoming, USA. Audio-magnetotellurics (AMT) measurements at 77 sites in the study area yielded electrical-resistivity logs of the subsurface, and these were used to infer lithologic changes with depth. A 100–600 ohm-m geoelectric layer, designated the Jackson aquifer, was used to represent surficial saturated, unconsolidated deposits of Quaternary age. The median depth of the base of the Jackson aquifer is estimated to be 200 ft (61 m), based on 62 sites that had sufficient resistivity data. AMT-measured values were kriged to predict the depth to the base of the aquifer throughout the southern part of Jackson Hole. Contour maps of the kriging predictions indicate that the depth of the base of the Jackson aquifer is shallow in the central part of the study area near the East and West Gros Ventre Buttes, deeper in the west near the Teton fault system, and shallow at the southern edge of Jackson Hole. Predicted, contoured depths range from 100 ft (30 m) in the south, near the confluences of Spring Creek and Flat Creek with the Snake River, to 700 ft (210 m) in the west, near the town of Wilson, Wyoming. Received, May 1997 · Revised, February 1998 · Accepted, April 1998     

Sodium beacon tip–tilt determination with Rayleigh-aided auxiliary telescope technique

The usefulness of tracking the Rayleigh portion of a mesospheric sodium laser guide star as reference for absolute tip–tilt recovery in the frame of the auxiliary telescopes technique is shown. This approach leads to the reduction of the ground occupation needed to attain a given sky coverage by more than one order of magnitude. Speed, tracking precision, and the number of auxiliary telescopes are also reduced, making this new approach a more attractive one. The use of a low-altitude Rayleigh spot reinforces the fundamental limitations affecting this and other techniques, thus degrading significantly the quality of the recovered tip–tilt. However, it is shown that, provided adequate care is taken in the collection and treatment of data, an interesting tilt signal can still be retrieved.     

On the global structure of self-gravitating discs for softened gravity

The effects of gravitational softening on the global structure of self-gravitating discs in centrifugal equilibrium are examined in relation to hydrodynamical/gravitational simulations. The one-parameter spline softening proposed by Hernquist & Katz is used.
It is found that if the characteristic size of a disc, r , is comparable to or less than the gravitational softening length, ε, then the cross-section of the simulated disc is significantly larger than that of a no-softening (Newtonian) disc with the same mass and angular momentum.
We demonstrate, furthermore, that if r ≲ε/2 then the scaling relation r ∝ε^3/4 holds for a given mass and specific angular momentum distribution with mass. Finally, we compare some of the theoretical results obtained in this paper and a previous one with the results of numerical Tree-SPH simulations and find qualitative agreement.