椭球体的视电阻率特征     

张超  汤井田  强建科 《物探化探计算技术》2014,(2):158-163

椭球体是最具代表性的典型三维地电体之一,它三个轴的长短经过变化后可以和多种形状的地电体相似。因此,实现了椭球体电阻率的求解,就可以模拟绝大多数三维地电体的电阻率曲线。从拉普拉斯方程的求解出发,得到了均匀空间中存在的水平椭球体异常表达式,并用简单加倍的方法得到了均匀半空间中水平椭球体的视电阻率公式,结合倾斜旋转椭球体的视电阻率公式的规律,得到了倾斜椭球体的视电阻率公式,再进行一系列简化得到板状体。最后分析对比了均匀电场中旋转椭球体和板状体的视电阻率曲线的形态和规律。结论表明:旋转椭球体与板状体的视电阻率曲线的走向大体相似,且板状体的曲线相比旋转椭球体较缓和。对于低阻情况,在异常体顶部附近的视电阻率异常为零,异常体的倾向一侧有极小值,反倾向一侧有极大值,曲线随倾角α的增大而逐渐变陡。对于高阻情况,视电阻率的极大值出现在异常体顶部附近,两侧有极小值,倾向一侧的曲线较缓和而反倾向一侧的曲线较陡峭,随着倾角α的增大,视电阻率异常变大。  相似文献   

全球锂资源供需前景与对策建议   总被引：4，自引：0，他引：4  

周平  唐金荣  张涛 《地质通报》2014,33(10):1532-1538

随着信息技术和新能源汽车等新兴产业的兴起,金属锂的地位和作用与日俱增。通过分析全球锂资源及其分布、供需现状及锂电发展对未来锂的供需影响,认为全球锂市场在中短期内将由供过于求向供需趋紧转变;长远来看,全球锂资源量大,且随着进入社会领域的锂产品规模扩大,锂的二次资源回收循环利用也将增加,理论上可以满足人类本世纪需求。锂的生产集中度过高、国内盐湖提锂工艺有待改进、锂电安全性问题等是制约中国锂业可持续发展的重要因素。因此,提出要将锂作为中国的新能源关键矿产,适时建立并启动锂的战略储备,加强高Mg/Li值盐湖卤水提锂工艺的科技公关,加强高性能锂电技术研发等对策建议。  相似文献   

双巷三维并行电法数值及物理模型试验研究     

张成乾  杨伐  谭磊  吴荣新  张平松 《中国煤炭地质》2014,(6):60-62,68

电法勘探是一种以研究地下探测目标体与周围介质之间的电性差异的地球物理探测方法,通常采用的二维电法勘探只能得到一条垂直于测线的视电阻率剖面,如果不能确定测线位置正好在异常体的正上方,这时就难给出较准确的结论。三维电阻率法采集数据量大,可获得三维电性数据体,而且可方便地根据需要实现水平及垂直切片,有着二维电法探测不能比拟的优点,实现对目标体的准确定位及全面透视。通过对构建的三维地质模型体进行数值模拟和物理模拟,表明双巷并行三维电法对地质异常体可以进行有效的探查并获得良好的探测效果。  相似文献   

On the possibility of investigation of the magnetic field structure in subphotospheric layers of the Sun according to observations of sunspot torsional oscillations     

O. S. Gopasyuk  S. I. Gopasyuk 《Bulletin of the Crimean Astrophysical Observatory》2008,104(1):52-58

A method of investigation of the magnetic field structure in subphotospheric layers of the Sun has been developed. The method is based on observations of the torisonal oscillations of single sunspots. Characteristics of the torsional oscillations have been obtained from observations of the longitudinal magnetic field and radial velocities of seven single sunspots in the photospheric line Fe I λ5253 Å. The parameters of the torsional oscillations and magnetic tubes in the deep layers have been determined. The radius of the cross section of a magnetic flux tube forming a sunspot is greatest near the Sun’s surface and is approximately equal to the radius of a sunspot umbra. Down to the deeper layers, it decreases quite quickly. The longitudinal electric current appearing in the magnetic tube changes direction. The typical time of the current changes is determined by the period of the torsional oscillations. The intensity of the longitudinal magnetic field in the tube increases with depth. The Alfven wave velocity averaged over the length of a magnetic tube is tens or hundreds of times less than this velocity in a sunspot umbra. It decreases with an increase in the period of oscillations. A decrease in the Alfven wave velocity leads to an increase in the twisting angle of magnetic field lines.  相似文献   

Effect of parallel electric field on electrostatic ion-cyclotron instability in anisotropic plasma in the presence of ion beam and general distribution function—Particle aspect analysis     

Ruchi Mishra 《Planetary and Space Science》2006,54(2):188-199

Dispersion relation, resonant energy transferred, growth rate and marginal instability criteria for the electrostatic ion-cyclotron wave with general loss-cone distribution in low-β anisotropic, homogeneous plasma in the auroral acceleration region are discussed by investigating the trajectories of the charged particles. Effects of the parallel electric field, ion beam velocity, steepness of the loss-cone distribution and temperature anisotropy on resonant energy transferred and growth rate of the instability are discussed. It is found that the effect of the parallel electric field is to stabilize the wave and enhance the transverse acceleration of ions whereas the effect of steepness of loss-cone, ion beam velocity and the temperature anisotropy is to enhance the growth rate and decrease the transverse acceleration of ions. The steepness of the loss-cone also introduces a peak in the growth rate which shifts towards the lower side of the perpendicular wave number with the increasing steepness of the loss-cone.  相似文献   

Experimental Radar Studies of Anisotropic Diffusion of High Altitude Meteor Trails     

W. K. Hocking 《Earth, Moon, and Planets》2004,95(1-4):671-679

At altitudes above 93 km in the atmosphere, magnetic and electric fields can affect the modes and rates of non-turbulent diffusion of ionized meteor trails. Anisotropic diffusion is expected. Most theories of anisotropic diffusion, and indeed most experimental studies, have concentrated on the effects of the magnetic field in producing this anisotropy, and different rates of expansion are expected in directions parallel to and perpendicular to the magnetic field lines. In this study, we use interferometric meteor radars to investigate the dependence of the ambipolar diffusion coefficient on viewing direction relative to the magnetic field, and show that the dependence is at best weak when daily averages are used. We then demonstrate that the reason for this effect is that the positions of maximum and minimum diffusion rates varies as a function of time of day, and that daily averaging masks the anisotropy. One possibility to account for the observations is that this strong diurnal variation is a consequence of the electric fields in the upper atmosphere, which are often tidally driven. An alternative possibility is a diurnal cycle in mean meteor entrance speeds. We lean towards the first hypothesis, but both possibilities are discussed. We demonstrate our results with data from several sites, but particularly using the Clovar radar near London, Ontario, Canada.  相似文献   

ICE, the electric field experiment on DEMETER   总被引：9，自引：0，他引：9  

J.J. Berthelier  M. Godefroy  M. Malingre  D. Lagoutte  F. Colin  C. Legendre  D. Benoist  J. Artru 《Planetary and Space Science》2006,54(5):456-471

  相似文献   

On the acceleration of solar-flare charged particles in a collapsing magnetic trap with an electric potential     

V. A. Kovalev  B. V. Somov 《Astronomy Letters》2002,28(7):488-493

We consider the kinetic problem of charged-particle acceleration in a magnetic trap with converging magnetic mirrors. We show that for a positive electrostatic potential of the trap plasma relative to the mirrors, the efficiency of confinement and acceleration increases for electrons and decreases for ions.  相似文献   

Advances in Numerical Modeling of Astrophysical and Space Plasmas     

Anthony L. Peratt 《Astrophysics and Space Science》1997,256(1-2):51-75

Advances in the simulation of astrophysical and cosmic plasmas are the direct result of advances in computational capabilities, today consisting of new techniques such as multilevel concurrent simulation, multi-teraflop computational platforms and experimental facilities for producing and diagnosing plasmas under extreme conditions for the benchmarking of simulations. Examples of these are the treatment of mesoscalic plasma and the scaling to astrophysical and cosmic dimensions and the Accelerated Strategic Computing Initiative whose goal is to construct petaflop (10¹⁵ floating operations per second) computers, and pulsed power and laser inertial confinement plasmas where megajoules of energy are delivered to highly-diagnosed plasmas. This paper concentrates on the achievements to date in simulating and experimentally producing plasmas scaled to both astrophysical and cosmic plasma dimensions. A previous paper (Part I, Peratt, 1997) outlines the algorithms and computational growth.  相似文献   

电测深ρ＿s差值法的应用效果     

杨昌桂 《湖南地质》1994,(1)

用电测深研究地电断面、寻找隐伏多金属矿体时，以往采用ρ＿ｓ（或η＿ｓ）等值线断面图进行地质推断解释，因受浅源信号的干扰，效果差。本文提出了采用ρ＿ｓ（或η＿ｓ）差值法，能排除浅源干扰信号，反映出地电断面的相对变化，突出了深部微弱信息，取得了较好的地质解释效果。  相似文献