组合式面板双绞合六边形钢丝网加筋土挡墙现场试验研究

为研究双绞合六边形钢丝网加筋土挡墙的受力、变形特性,对潭衡（湘潭－衡阳）西线高速公路K124+340断面组合式面板双绞合六边形钢丝网加筋土挡墙进行了现场试验,测试了竖向土压力、水平土压力、筋材拉应变分布规律和格宾箱变形规律。结果表明：在筋材长度方向上,竖向土压力在挡墙下部呈双峰型分布,而在上部呈单峰形分布;墙背水平土压力沿墙高呈非线性分布,最大值发生在墙高约1.5 m处,实测水平土压力小于主动压力;筋材应变在筋长方向上呈非线性分布,各层筋材的应变分布模式不相同;筋材的变形主要发生在施工期,格宾箱的变形呈鼓胀式     

基于电偶极子近似的多边形回线源瞬变电磁响应

针对大回线源中心装置在回线内场非中心位置处场点响应表达式复杂,视电阻率计算困难,只能套用中心回线装置计算公式,导致解释精度下降问题,给出了圆回线的响应公式。提出对发射回线沿边框进行电偶极子源分解,通过对各个边框的偶极子源产生的响应进行叠加;讨论了圆回线与圆内接多边形发射回线的等效性问题;完成了大回线内任意点的场值计算,并对基于电偶极子近似的大回线内场的分布特征进行了分析,得出了大回线源内非中心点探测的可行性结论。研究成果具有理论价值和实际指导意义。     

综合物探解决黄土区煤田复杂地质问题

山西某矿位于构造堆积盆地，属黄土匠陵地貌，区内被第四系黄土覆盖，为解决该矿地质构造及水文地质问题，采用三维地震勘探与瞬变电磁法、直流电测深法相结合的勘探方案。利用三维地震勘探解决目的层赋存形态及其地质构造问题，再利用瞬变电磁法进行平面控制，以使平面及深度解释误差达到勘探要求；应用直流电测深法及瞬变电磁进行勘探，在正反演解释的基础上对其资料综合分析、对比，并结合三维地震资料，确定地质构造的富水及导水性。     

MT方法在冀东迁安铁矿区深部找矿中的异常识别

文章叙述了通过MT方法在已知矿体上的剖面试验,结合钻探验证的3个钻孔的见矿情况,以及电偶极子人工场源对观测数据影响的对比、分析,指出依据航磁异常布设、采集的大地电磁剖面测深数据,尽管测点位于生产矿区,数据受到较严重的人文噪声干扰,且其部分频段异常形态与近区特征非常相似,实际上应为数据反演过程中所用软件未曾考虑铁矿石磁导率所致,而非近区效应;当一维视电阻率和相位曲线自几千赫兹以上即出现类似近区特征,二维反演剖面中的假象视电阻率异常高达几千至几万欧姆米时,应为有较强磁性的岩石和磁铁矿的反映;具有一定磁性的岩石和磁铁石英岩（包括磁铁石英辉石岩）在假象视电阻率异常强度、异常梯度变化上具有不同特征,可结合岩、矿石的电性、磁性特征予以识别.     

层状含水系统R—C电网络模拟方法

本文论述了R-C电网络模型的基本原理及模拟装置,分析了不同类型的层状含水系统。根据榴似性原理,建立了不同类型的电网络模型。在此基础上,预测了内蒙古某露天煤矿的矿坑疏干涌水量,取得了比较满意的结果。     

三维复杂域非结构化六面体网格全自动生成方法

使用自适应有限单元法在三维复杂域内求解水工及岩土工程问题,讨论了应用行波法在多介质三维复杂块体内六面体单元网格的自动生成过程。其特点是对不规则区域具有较强的适应性,并考虑了节理单元的自动生成。     

Letter to the editor Electric field fluctuations (25–35 min) in the midnight dip equatorial ionosphere

Measurements with a HF Doppler sounder at Kodaikanal (10.2°N, 77.5°E, geomagnetic latitude 0.8°N) showed conspicuous quasi-periodic fluctuations (period 25/35 min) in F region vertical plasma drift, V_z in the interval 0047/0210 IST on the night of 23/24 December, 1991 (A_p = 14, K_p < 4^–). The fluctuations in F region vertical drift are found to be coherent with variations in B_z (north-south) component of interplanetary magnetic field (IMF), in geomagnetic H/X components at high-mid latitude locations both in the sunlit and dark hemispheres and near the dayside dip equator, suggestive of DP2 origin. But the polarity of the electric field fluctuations at the midnight dip equator (eastward) is the same as the dayside equator inferred from magnetic variations, contrary to what is expected of equatorial DP2. The origin of the coherent occurrence of equatorial electric field fluctuations in the DP2 range of the same sign in the day and night hemispheres is unclear and merits further investigations.     

A high order Godunov scheme with constrained transport and adaptive mesh refinement for astrophysical and geophysical MHD

We propose to extend the well-known MUSCL-Hancock scheme for Euler equations to the induction equation modeling the magnetic field evolution in kinematic dynamo problems. The scheme is based on an integral form of the underlying conservation law which, in our formulation, results in a “finite-surface” scheme for the induction equation. This naturally leads to the well-known “constrained transport” method, with additional continuity requirement on the magnetic field representation. The second ingredient in the MUSCL scheme is the predictor step that ensures second order accuracy both in space and time. We explore specific constraints that the mathematical properties of the induction equations place on this predictor step, showing that three possible variants can be considered. We show that the most aggressive formulations reach the same level of accuracy than the other ones, at a lower computational cost. More interestingly, these schemes are compatible with the Adaptive Mesh Refinement (AMR) framework. It has been implemented in the AMR code RAMSES. It offers a novel and efficient implementation of a second order scheme for the induction equation. The scheme is then adaptated to solve for the full MHD equations using the same methodology. Through a series of test problems, we illustrate the performances of this new code using two different MHD Riemann solvers (Lax–Friedrich and Roe) and the need of the Adaptive Mesh Refinement capabilities in some cases. Finally, we show its versatility by applying it to the ABC dynamo problem and to the collapse of a magnetized cloud core.     

相空间相似预报的一种新方法

本文针对相空间相似预报方法应用过程中存在需要同时确定时滞和维数的困难,引入历史预报准确率最高原则,提出了一种相空间相似预报的新方法。应用昆明站近百年（1901年～1992年）逐月雨量和气温时间序列对该方法进行了检验。计算结果表明此方法是可行的。     

An Economical Consistent Dissipation Operator and Its Applications to the Improvement of AGCM

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