大地等效电容量及其测量方法     

朱旭 《地震》2015,35(4):76-82

在脉冲供电和正弦交流供电地电阻率观测研究中, 大地容性效应会引起测量误差。 本文按照电子学等效电路的方法提出了大地等效电容量的概念, 研究了大地等效电容量的测量方法, 为合理确定脉冲供电参数和减小交流地电阻率测量误差奠定了基础。  相似文献   

一种利用共振声谱法检测气液两相介质中气体含量的新方法   总被引：1，自引：0，他引：1       下载免费PDF全文

丛健生  王秀明  陈德华  徐德龙  车承轩  马水龙 《地球物理学报》2008,51(1):280-284

根据共振声谱原理,建立了气液两相介质中圆柱共振腔共振声谱的实验测量系统,研究了共振腔体中不同含量的气体对共振声谱的幅度和共振频率的影响.实验结果表明：共振幅度和共振频率随着气体流量的增加都呈指数衰减变化趋势,但共振幅度比共振频率的衰减速度快,都可反映气体流量的变化.另外,在理论上,推导了均匀流体模型气液两相介质中的圆柱共振腔的共振频率计算公式,并模拟计算了共振频率和气体含量的变化规律曲线.理论研究结果表明,随着持气率的增加,共振频率减小;当持气率较小时,共振频率衰减较快.这一结论已经被本文实验测量结果所验证.理论和实验研究表明,利用共振声谱法可以检测气液混相介质中气体含量,它为发展生产井中气液两相流分相含量检测方法提供一种可能的途径.  相似文献   

大鼠肝炎性假瘤模型的建立与影像学表现   总被引：1，自引：0，他引：1  

许乙凯  冯文兰  刘杏元  俞志坚  张嘉宁 《CT理论与应用研究》1998,7(4):25-27

本研究的目的是建立一种可供于影像学研究的大鼠肝炎性假瘤（ＩＰＬ）模型,并研究其影像学的特征。所用的材料和方法是将弗氏佐剂０１ｍｌ／只作大鼠深部注射,１０天后观察大鼠病灶的影像学特征;并取标本做病理检查。结果发现了ＩＰＬ发生率为９０％,大小分别是０３２±０１８ｃｍ。ＩＰＬ的影像学特征表现为强回声结节;ＣＴ平扫为低度圆形影,无强化或仅轻微强化;Ｔ１ＷＩ则呈等或高信号,Ｔ２ＷＩ为略高信号。病理学证实局部肝组织片状坏死并有纤维组织增生及炎细胞浸润。结论是本文研究的大鼠肝炎性假瘤模型具有易建立、容易复制、成功率高、制备周期短和影像学的表现较典型等特点,对今后探讨大鼠肝炎性假瘤的形成机制及影像学特征将发挥积极作用  相似文献   

Exploring the 7:4 mean motion resonance—I: Dynamical evolution of classical transneptunian objects     

Patryk Sofia Lykawka  Tadashi Mukai 《Planetary and Space Science》2005,53(11):1175-1187

In the transneptunian classical region (), an unexpected orbital excitation in eccentricity and inclination, dynamically distinct populations and the presence of chaotic regions are observed. For instance, the 7:4 mean motion resonance () appears to have been causing unique dynamical excitation according to observational evidences, namely, an apparent shallow gap in number density and anomalies in the colour distribution, both features enhanced near the 7:4 mean motion resonance location. In order to investigate the resonance dynamics, we present extensive computer simulation results totalizing almost 10,000 test particles under the effect of the four giant planets for the age of the solar system. A chaotic diffusion experiment was also performed to follow tracks in phase space over 4-5 Gyr. The 7:4 mean motion resonance is weakly chaotic causing irregular eccentricity and inclination evolution for billions of years. Most 7:4 resonant particles suffered significant eccentricities and/or inclinations excitation, an outcome shared even by those located in the vicinity of the resonance. Particles in stable resonance locking are rare and usually had 0.25<e<0.3. For other regions, 7:4 resonants had quite large mobility in phase space typically leaving the resonance (and being scattered) after reaching a critical e∼0.2. The escape happened in 10⁸-10⁹ yr time scales. Concerning the inclination dependence for 7:4 resonants, we found strong instability islands for approximately i>10°. Taking into account those particles still locked in the resonance at the end of the simulations, we determined a retainability of 12-15% for real 7:4 resonant transneptunian objects (TNOs). Lastly, our results demonstrate that classical TNOs associated with the 7:4 mean motion resonance have been evolving continuously until present with non-negligible mixing of populations.  相似文献   

Coupling of linear waves and a hybrid porous TLP     

Chung-Pan Lee  Wen-Kuei Ker 《Ocean Engineering》2002,29(9):1049-1066

An analytical solution has been developed in this paper to quantify the flow field and the surge motion of a porous tension leg platform with an impermeable top layer induced by linear waves. The porous layer of the TLP is considered to be anisotropic but homogeneous. The nonlinear form drag in the porous layer is replaced by a linear drag according to Lorentz’s hypothesis of equivalent work. The convergence of the series solution is verified. The dependence of the flow field, the surge motion of the platform, and its resonant frequency on wave and structure properties has been studied.  相似文献   

On the tuning of a wave-energy driven oscillating-water-column seawater pump to polychromatic waves     

Ramiro Godoy-Diana  Steven P.R. Czitrom   《Ocean Engineering》2007,34(17-18):2374-2384

Performance of wave-energy devices of the oscillating water column (OWC) type is greatly enhanced when a resonant condition with the forcing waves is maintained. The natural frequency of such systems can in general be tuned to resonate with a given wave forcing frequency. In this paper we address the tuning of an OWC sea-water pump to polychromatic waves. We report results of wave tank experiments, which were conducted with a scale model of the pump. Also, a numerical solution for the pump equations, which were proven in previous work to successfully describe its behavior when driven by monochromatic waves, is tested with various polychromatic wave spectra. Results of the numerical model forced by the wave trains measured in the wave tank experiments are used to develop a tuning criterion for the sea-water pump.  相似文献   

Evolution of the obliquities of the giant planets in encounters during migration     

Man Hoi Lee  S.J. Peale  William R. Ward 《Icarus》2007,190(1):103-109

Tsiganis et al. [Tsiganis, K., Gomes, R., Morbidelli, A., Levison, H.F., 2005. Nature 435, 459-461] have proposed that the current orbital architecture of the outer Solar System could have been established if it was initially compact and Jupiter and Saturn crossed the 2:1 orbital resonance by divergent migration. The crossing led to close encounters among the giant planets, but the orbital eccentricities and inclinations were damped to their current values by interactions with planetesimals. Brunini [Brunini, A., 2006. Nature 440, 1163-1165] has presented widely publicized numerical results showing that the close encounters led to the current obliquities of the giant planets. We present a simple analytic argument which shows that the change in the spin direction of a planet relative to an inertial frame during an encounter between the planets is very small and that the change in the obliquity (which is measured from the orbit normal) is due to the change in the orbital inclination. Since the inclinations are damped by planetesimal interactions on timescales much shorter than the timescales on which the spins precess due to the torques from the Sun, especially for Uranus and Neptune, the obliquities should return to small values if they are small before the encounters. We have performed simulations using the symplectic integrator SyMBA, modified to include spin evolution due to the torques from the Sun and mutual planetary interactions. Our numerical results are consistent with the analytic argument for no significant remnant obliquities.  相似文献   

基于自适应遗传算法的MRS-TEM联合反演方法研究   总被引：2，自引：2，他引：0       下载免费PDF全文

万玲  林婷婷  林君  蒋川东  嵇艳鞠 《地球物理学报》2013,56(11):3728-3740

地面磁共振法(MRS)因具有定性、定量分析地下水能力,而备受关注.传统磁共振地层含水量反演多采用均匀半空间模型,忽略电阻率分布信息对结果的影响.针对这一问题,本文基于多层电介质中磁共振响应理论,提出MRS与瞬变电磁(TEM)联合反演方法,通过电阻率分布信息对含水量反演过程的实时修正,提高了解释结果的准确度.反演算法采用自适应遗传算法(AGA)进行,基于繁殖规则,动态调整交叉概率和变异概率,解决了标准遗传算法易未成熟收敛而难以得到全局最优解问题.模型数据表明,含噪10%情况下,联合反演仍能较准确地反映地下含水单元模型结构,对比MRS单独反演优势明显.同时,内蒙古白旗野外观测数据联合反演结果与钻井资料基本一致,充分验证了AGA反演算法的实用性及MRS-TEM联合反演的实际意义.  相似文献   

A numerical and experimental study of hollow steel pile in layered soil subjected to lateral dynamic loading     

《Soil Dynamics and Earthquake Engineering》2013

The present study aims at investigating the nonlinear behavior of single hollow pile in layered soil subjected to varying levels of horizontal dynamic load. A finite element model has been developed using commercially available FEM based software. Mohr–Coulomb plasticity model is used to simulate the soil plasticity whereas the pile-material is idealized as elastic. Numerical results are validated comparing with the experimental results. The experimental investigations were carried out in the field located at IIT Kharagpur. Two types of motion: horizontal and rocking are studied. The effects of various influencing parameters, namely, exciting moment, length and diameter of the pile etc. on the nonlinear dynamic response of piles are investigated. It is found that separation of pile from the surrounding soil considerably affects the resonance frequency and amplitude of the pile foundations.  相似文献   

Impact of tidal power dams upon tides and environmental conditions in the Sea of Okhotsk     

A.V. Nekrasov  D.A. Romanenkov 《Continental Shelf Research》2010

The transformation of natural tidal sea-level and currents is studied resulting from large-scale tidal power plant (TPP) dams in bays of the Sea of Okhotsk (SO). Some effects due to this transformation are estimated based on predictive modelling and a number of expected changes in amplitudes and phases, and spectral composition of tidal oscillations are described. Changes of morphometric properties of basins change the character of tidal motions even on significant distance from a dam. That is why, it is impossible to estimate this impact as usual boundary-value problems. The problem is solved based on “impedance” conditions on the open boundary of the model area, allowing to take into account the radiation of the additional perturbations induced by both waves reflected from the dam and nonlinear effects inside the area. In general, the transformation effects are proportional to the dam size and depend essentially on the dam location, the creation of which can change dissipative and resonance properties of the bays. The changes in tidal energetics of SO due to the dam construction are also considered to show noticeable reconstruction of horizontal energy fluxes and changes in the energy dissipation. Possible environmental consequences are related mainly to the transformation of tidal currents.  相似文献