水中电偶极子空中磁场响应的一维频率域分析

海洋电磁中浅海作业由于受到空气波的干扰而难于进行,而如果于空中接收电偶极子的磁场响应则可避免空气波的干扰,是一种新的海洋电磁勘探思路。用一维频率域程序,对水中电偶极子在空中的磁场响应进行了计算分析,比较了海底有高阻异常层和低阻异常层时空中磁场响应的变化规律。分别计算测线布置、发射信号频、海水深度、异常储层埋深、异常储层厚度、储层电阻率、空中测量高度等多种因素对空中磁场响应的影响,结果表明,海底有低阻层时空中磁场有更强的响应,归一化幅度异常变化约为10%~60%,而海底有高阻异常储层时响应较弱,归一化异幅度常变化约为2%~8%。因此海洋电磁勘探中于空中接收磁场的模式,更适合浅海区低阻矿产资源的大面积调查。     

椭球体的视电阻率特征

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。     

LiDAR 在四川某地电力选线项目中的应用

机载激光雷达（ LiDAR）技术的快速发展为获取高时空分辨率的地球空间信息提供了一种全新的技术手段。笔者在某市电力选线项目中利用机载激光雷达技术,获得高精度点云,根据点云建立三维模型,并通过大量外业采集数据进行精度检核,最后将生成产品导入电力选线软件中,实现了在室内完成电力选线工作。实验表明,在电力选线项目中,利用机载激光雷达技术提高了作业效率,具有广阔的应用前景。     

时变重力场的非各向同性高斯滤波比较

使用GRACE反演地球表层的质量异常,其结果取决于构造的平滑函数即滤波方法。本文阐述了两种在经典高斯滤波基础上构造的Fan滤波和Non-isotropic Gaussian(Non)滤波,两者均对GRACE的阶和次起作用。在同一阶下,两者的权重随着次数的升高而衰减,但衰减的趋势不同,比如在20阶时,Fan滤波呈抛物线变化,而Non滤波则为线性衰减;在40和60阶,两者均呈抛物线变化。使用CSR发布的GRACE Level-2 RL05数据反演地表质量异常,两者的结果相近。     

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

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.     

Advances in Numerical Modeling of Astrophysical and Space Plasmas

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.     

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

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.     

5000 m新型能源勘探智能钻探装备与技术研究

结合我国地下新型能源勘探工作的重大需求,开展了“5000 m新型能源勘探智能钻探装备与技术”的研究,取得了5000 m多功能交流变频电动钻机、多参数孔底自动监测装置、高温环保泥浆及泥浆性能自动测量装置、取心和无心钻进不提钻互换钻具等系列成果,填补了国内空白,推动了新型能源深部钻探技术向智能化方向发展。     

XD-10DK型小口径电动顶驱钻机的研制与应用

为了解决新疆地区铀矿勘探设备落后、劳动强度大、安全隐患多、钻效提升困难等难题,研制了XD-10DK型小口径电动顶驱钻机,该钻机采用了模块化设计、交流变频电机直驱、负载双通道、数字化检测、顶部驱动等多项先进技术。经过在准噶尔盆地车排子地区3个钻孔的现场试验,提高了铀矿勘探自动化程度和钻进效率、降低了工人的劳动强度、改善了工人的工作环境、保障了施工设备和人员安全。为新疆地区铀矿勘探乃至全国的岩心钻机更新换代提供了借鉴。