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1.
The anisotropy of magnetic susceptibility has been proven to be an excellent indicator for mineral fabrics and therefore deformation
in a rock or sediment. Low-field anisotropy is relatively rapid to measure so that a sufficient number of samples can be measured
to obtain a good statistical representation of the magnetic fabric. The physical properties of individual minerals that contribute
to the observed magnetic fabric include bulk susceptibility and intrinsic anisotropy of the mineral phase, its volume concentration,
and its degree of alignment. Several techniques have been developed to separate magnetic subfabrics arising from magnetization
types, i.e., ferrimagnetism, antiferromagnetism, paramagnetism, and diamagnetism. Susceptibility anisotropy can be measured
in low or high fields and at different temperatures in order to isolate a particular subfabric. Measuring the anisotropy of
a remanent magnetization can also isolate ferrimagnetic fabrics. A series of case studies are presented that exemplify the
value of isolating magnetic subfabrics in a geological context. It is particularly useful in rocks that carry a paramagnetic
and diamagnetic subfabric of similar magnitude, such that they negate one another. Further examples are provided for purely
paramagnetic subfabrics and cases where a ferrimagnetic subfabric is also identified. 相似文献
2.
在模拟含Cu2+废水中加入Mg2+和Al3+,以NaOH为沉淀剂,研究金属盐水解即时合成层状双氢氧化物去除Cu2+的可行性,同时考察了体系终点pH值、配料中Mg/Cu摩尔比值及反应温度和时间对Cu2+去除率的影响,探讨了Cu2+去除机理及层状双氢氧化物形成过程。结果表明,实验条件下体系终点pH值显著影响Cu2+去除率,在pH值8.0~11.0范围内去除效果较好,达99%以上。通过X射线衍射分析结合即时合成法特点,废水中Cu2+主要是在晶核生成阶段以Cu/Mg/Al三元层状双氢氧化物形式被去除;三元层状双氢氧化物的形成由反应体系中Al3+、Cu2+、Mg2+分步水解导致,最适pH值约为9.0。 相似文献
3.
The progressive development of mylonitic fabrics in a series of Torridonian sandstones and shales has been studied along traverses across the Kishorn Nappe. The fabrics developed have been investigated using the following techniques.
- 1. 1. Optical examination of thin sections.
- 2. 2. Measurements of the anisotropy of magnetic susceptibility.
- 3. 3. X-ray texture goniometry.
4.
Hematite is a very abundant mineral in natural rock samples. Despite being one of the most important carriers of remanent
magnetization, its magnetic anisotropy is not well understood partially due to its high coercivity and complex behavior. In
particular, the field intensity beyond which the Rayleigh relation no longer holds varies from one crystal to another. This
field threshold is usually less than the field used in most commercial instruments. The nonlinear behavior of low-field susceptibility
may thus hinder the magnetic fabric analysis. We have carried out an intensive study of the low-field bulk susceptibility
and anisotropy of magnetic susceptibility (AMS) at increasing low fields in the range of 2–450 A/m (effective value) in a
collection of hematite natural crystals. Standard rock magnetic properties, X-ray diffraction, and mass spectrometry have
also been determined in order to discover the parameters influencing the low-field susceptibility variations with field. The
AMS principal directions, the shape of the AMS ellipsoid, and the degree of anisotropy are the parameters that can vary with
different applied fields. It has been found that there is no correlation between magnetic properties like coercivity or saturation
magnetization and the range in which the Rayleigh approximation is valid. However, there seems to be a correlation with the
peak width determined from X-ray diffraction, suggesting that the Rayleigh region in hematite crystals is related to the spatial
orientation of the physical domains within the basal plane. 相似文献
5.
软土预压工程中,初始和诱发各向异性对软土力学性质的影响十分显著,而现有研究缺乏对初始和诱发各向异性的统一研究方法。采用离散单元法,以颗粒长宽比作为定量评价指标,构建真实形态的颗粒模型,生成5组不同沉积角的初始各向异性试样,并进行竖直和水平两方向加载的双轴模拟实验,研究了初始各向异性和诱发各向异性对软土力学特性影响;在细观层面,以颗粒为对象研究了颗粒接触形式和转动角度的变化规律,以接触为对象研究了配位数和接触法向各向异性的发展趋势,在此基础上探究抗剪强度指标与各向异性关系。结果表明:初始和诱发各向异性共同影响试样力学性质,当加载方向和软土沉积方向垂直时,土体有最大的峰值强度。颗粒接触形式中面面接触的比例随加载的进行逐渐增大,并影响着试样初始模量和抗剪强度,配位数和接触法向各向异性受颗粒接触形式的影响有不同的演化规律,并在加载后期趋于稳定;同时,初始各向异性试样相较各向同性试样有更大的黏聚力,诱发各向异性主要影响试样内摩擦角,进而影响试样抗剪强度。 相似文献
6.
A program for the simulation of two‐dimensional (2‐D) fluid flow at the microstructural level of a saturated anisotropic granular medium is presented. The program provides a numerical solution to the complete set of Navier–Stokes equations without a priori assumptions on the viscous or convection components. This is especially suited for the simulation of the flow of fluids with different density and viscosity values and for a wide range of granular material porosity. The analytical solution for fluid flow in a simple microstructure of porous medium is used to verify the computer program. Subsequently, the flow field is computed within microscopic images of granular material that differ in porosity, particle size and particle shape. The computed flow fields are shown to follow certain paths depending on air void size and connectivity. The permeability tensor coefficients are derived from the flow fields, and their values are shown to compare well with laboratory experimental data on glass beads, Ottawa sand and silica sands. The directional distribution of permeability is expressed in a functional form and its anisotropy is quantified. Permeability anisotropy is found to be more pronounced in the silica sand medium that consists of elongated particles. Copyright © 2001 John Wiley & Sons, Ltd. 相似文献
7.
Besides granites of the ilmenite series, in which the anisotropy of magnetic susceptibility (AMS) is mainly controlled by paramagnetic minerals, the AMS of igneous rocks is commonly interpreted as the result of the shape-preferred orientation of unequant ferromagnetic grains. In a few instances, the anisotropy due to the distribution of ferromagnetic grains, irrespective of their shape, has also been proposed as an important AMS source. Former analytical models that consider infinite geometry of identical and uniformly magnetized and coaxial particles confirm that shape fabric may be overcome by dipolar contributions if neighboring grains are close enough to each other to magnetically interact. On these bases we present and experimentally validate a two-grain macroscopic numerical model in which each grain carries its own magnetic anisotropy, volume, orientation and location in space. Compared with analytical predictions and available experiments, our results allow to list and quantify the factors that affect the effects of magnetic interactions. In particular, we discuss the effects of (i) the infinite geometry used in the analytical models, (ii) the intrinsic shape anisotropy of the grains, (iii) the relative orientation in space of the grains, and (iv) the spatial distribution of grains with a particular focus on the inter-grain distance distribution. Using documented case studies, these findings are summarized and discussed in the framework of the generalized total AMS tensor recently introduced by Cañon-Tapia (Cañon-Tapia, E., 2001. Factors affecting the relative importance of shape and distribution anisotropy in rocks: theory and experiments. Tectonophysics, 340, 117–131.). The most important result of our work is that analytical models far overestimate the role of magnetic interaction in rock fabric quantification. Considering natural rocks as an assemblage of interacting and non-interacting grains, and that the effects of interaction are reduced by (i) the finite geometry of the interacting clusters, (ii) the relative orientation between interacting grains, (iii) their heterogeneity in orientation, shape and bulk susceptibility, and (iv) their inter-distance distribution, we reconcile analytical models and experiments with real case studies that minimize the role of magnetic interaction onto the measured AMS. Limitations of our results are discussed and guidelines are provided for the use of AMS in geological interpretation of igneous rock fabrics where magnetic interactions are likely to occur. 相似文献
8.
岩石的磁性组构及其在岩石变形分析中的应用 总被引：17，自引：0，他引：17
文本总结了对采自巴彦乌拉山韧性剪切带的部分标本进行岩石组构数据测定的分析结果,并将其与用常规应变分析方法所得结果予以比较,表明了岩石磁化率各向异性椭球体能够反映总的应变椭球体,证明岩石磁化率各向异性技术做为一种岩石组构因素的研究是有发展前景的。岩石磁性组构资料可应用于变形岩石的应变分析,特别是在通常的岩石组构分析技术太费时间和粗糙的情况下更显示了其优越性。 相似文献
9.
Solar flares observed during the 24th solar-activity cycle and accompanied by fluxes of particles detected at the Earth’s orbit with intensities exceeding 10 particles cm?2 s?1 and energies of more than 10 MeV per particle mainly occurred in activity complexes (82% of cases), with 80% of these occurring no more than 20 heliographic degrees from the nearest coronal holes. The correlation between the X-ray classes of flares and the proton fluxes detected at the Earth’s orbit is weak. The work presented here supports the hypothesis that the leakage of particles into the heliosphere is due to the existence of long-lived magnetic channels, which facilitate the transport of flare-accelerated particles into the boundary regions of open magnetic structures of coronal holes. The possible contribution of exchange reconnection in the formation of such channels and the role of exchange reconnection in the generation of flares are discussed. 相似文献
10.
《Russian Geology and Geophysics》2014,55(10):1229-1238
Phase change of dielectric magnesiowustite in the lower mantle may leave signatures in geomagnetic records of the globally distributed array of observatories. The related features appear in EM induction responses of lower mantle, which are studied theoretically. The surface EM field corresponding to a response of the earth with conductivity anisotropy in a mantle spherical layer is presented as the sum of the magnetic and electric modes. Equations for the fields of both modes and their relationship in a weakly anisotropic earth are obtained by the perturbation method. The two field modes are analyzed jointly and separately to characterize the conductivity tensor of the anisotropic lower mantle. The tensor elements corresponding to the tangential components of the field can be estimated from the magnetic mode alone recorded currently by the global network of geomagnetic observatories. For the tensor data to be complete, observatory data on lateral variations of the electric field are required in addition to three-component geomagnetic records. 相似文献
11.
《Geodinamica Acta》2013,26(3-4):197-211
This work deals with the magnetic susceptibility and its anisotropy (AMS) in the Variscan Millares pluton in the Central Pyrenees. The zonation of low-field magnetic susceptibility is consistent with the concentric arrangement of rock-types, with more basic compositions at the external areas. Magnetic foliations defined from AMS strike NE-SW and dip gently towards the NW. Magnetic foliations are mainly perpendicular and oblique to the elongation of the pluton in map view (NW-SE) and show a concentric pattern at the central part, where the more acid rocks crop out. Magnetic lineations are scattered between NW-SE and NE-SW and plunge shallowly to the N. In map view magnetic lineations are distributed in domains normal to the elongation of the pluton. The contours of P' (degree of magnetic anisotropy) are oriented NE-SW and bands of oblate and prolate ellipsoids alternate perpendicular to the elongation of the pluton in map view. P' is between 1.009 and 1.055 in 93% of the specimens. Such low values are currently recorded in granites having magmatic fabrics and for which the anisotropy is mainly carried by biotite. The attitude of the magnetic foliation and the magnetic lineation, the geometry of the pluton, and their relationship with the host-rock structure suggest an intrusion contemporary with a transpressional regime, syntectonic with the late stages of the Variscan orogeny. 相似文献
12.
地球内核与地球深部动力学 总被引：11，自引：2，他引：9
地球内核由外核富含铁元素的液态物质结晶而成。经证实,内核正以约１（°）／ａ的速率相对于地幔向东转动。内核的旋转是通过穿过内核的地震波的走时随时间变化推测得到的。这种变化是最近十多年来揭示出的内核各向异性在空间方位的改变所造成。内核的各向异性被认为起因于各向异性的铁晶体的有序排列,但这种有序排列的机制还不清楚。内核在地球发电机中起着重要的作用。利用大型的并行计算机,人们已得到能产生像地磁场一样的三维发电机数值模拟。地震学观测到的内核差速旋转为最近的发电机数值模拟提供了支持。这种数值模拟曾预测：导体内核与外核产生的磁场的电磁耦合驱动了内核每年几度向东旋转。地核通过核幔边界的接触及内核与地幔的引力耦合与地幔存在强烈的相互作用。多学科领域的突破为认识地球的深部动力过程提供了极好的机会和手段。 相似文献
13.
通过对青峰韧性剪切带中糜棱岩的磁性组构研究,同时与常规主应变分析方法所测结果比较,表明岩石磁化率各向异性椭球体与应变椭球体之间有一定的对应关系。磁性组构的特征为构造岩变形机制,以及断裂带的运动学、动力学等的研究提供了一种比较可靠、准确、方便的方法。 相似文献
14.
用变差函数研究重磁场的区域变化特征.变差函数的变程反映重磁场的相干范围, 块金效应反映随机干扰, 基台值反映变异程度.重磁场的理论模拟说明: 重力场的相干范围大于磁场, 重磁场变程主要取决于场源深度, 浅源重磁场变差函数近似为球状模型或指数模型, 深源重磁场近似为连续性更好的高斯模型.磁场场源深度近似等于变程的一半, 重力场场源深度近似等于变程的四分之一.湖北大冶铁矿垂直分量磁异常具有几何各向异性, 北西-南东走向, 变差函数推测磁铁矿平均深度为250m.磁异常小波多尺度分解细节和逼近部分磁场具有协调几何各向异性, 变差函数的各阶场源深度估计结果与功率谱估计结果吻合. 相似文献
15.
浅析北方红粘土对碳酸盐岩溶蚀作用的影响 总被引：1，自引：0，他引：1
田级生 《吉林大学学报(地球科学版)》1986,(3)
北方碳酸盐岩发育的红色风化壳大都是第Ⅰ、Ⅱ间冰期湿热气候条件下溶蚀与风化作用的结果,形成硅铝—铁型风化壳。风化壳中红粘土化学成分R_2O_3(Al_2O_3+Fe_2O_3)含量达20—30％。当降水或地表水的垂直下渗、红粘土的氢离子浓度加大,溶蚀性增强,沿红粘土和碳酸盐岩接触面产生溶蚀作用,形成石芽、溶沟、溶槽、溶痕等岩溶地形,并在它们的表面保留有红粘土痕迹。 相似文献
16.
This paper examines the mechanisms for the acceleration of electrons, protons, and ions during solar flares. The acceleration is assumed to occur in two steps. The particles are first pre-accelerated by the electric field of a high-temperature current sheet undergoing magnetic reconnection. A collapsing magnetic trap in the solar corona provides further acceleration. It is shown that the Fermi mechanism accelerates trapped protons and ions even more efficiently than it does electrons. The particles escaping from the trap have energies reaching several GeV. The energy distribution of the accelerated ions is essentially independent of their mass and degree of ionization. 相似文献
17.
R.S. Bhathal 《Earth》1971
In any rock six kinds of magnetic anisotropy can be distinguished, viz.: (1) shape alignment of grains; (2) alignment of crystals with magneto-crystalline anisotropy; (3) alignment of magnetic domains; (4) the stringing-together of magnetic grains, which is a special case of (1); (5) stress-induced anisotropy; and (6) exchange anisotropy. Each of these anisotropies, together with the method of measurement and practical uses in the fields of geology and geophysics, is discussed. 相似文献
18.
Abstractthe effect of the large-scale magnetic fields generated by the solar dynamo on the radiation flux issuing from the convection zone is studied. A governing equation describing convective heat transfer is obtained in the framework of mean-field magnetohydrodynamics, with account for the influence of magnetic fields and differential rotation on the energy budget of the convection zone. The principal effects are illustrated using a one-dimensional numerical model. Calculations indicate that the influence of large-scale magnetic fields can modulate the solar irradiance with a relative amplitude of ～0.07%. 相似文献
19.
Óscar Pueyo Anchuela Antonio M. Casas‐Sainz Emilio L. Pueyo Andrés Pocoví Juan Andrés Gil Imaz 《地学学报》2013,25(4):307-314
Magnetic susceptibility in rocks is the sum of the contributions of different magnetic particles (paramagnetic, diamagnetic and ferromagnetic s.l.). These contributions can be measured at variable temperatures or at variable fields (hysteresis loops). Both are time‐consuming techniques that cannot be routinely used in magnetic fabrics analysis. In this study, we propose a simplified method to determine the ferro‐ and paramagnetic contributions to the susceptibility, based on the discrete measurement of susceptibility at two different fields (near 0 and 2.5 T). The results obtained in samples from the Southern Pyrenees and Ebro Basin indicate that the ferromagnetic contribution vary considerably within homogeneous susceptibility values and within the expected range of paramagnetic values. Standard bulk susceptibilities higher than 200 10?6 SI contribute significantly to the ferromagnetic fraction (>50% on average). 相似文献
20.
G. A. Shul’man 《Astronomy Reports》2011,55(8):718-723
The quantum motion of non-relativistic and relativistic electrons in the presence of constant magnetic fields at the surfaces of magnetic stars, magnetic white dwarfs, and pulsars is considered. The quantizing magnetic-field strengths for charged particles with specified energies are determined. The quantum motion of these particles in a plane perpendicular to the magnetic field is accompanied by spontaneous radiation due to electron transitions from higher to lower discrete energy levels, right down to the ground state. In the non-relativistic case, this emission is monochromatic. In the non-relativistic case, various frequencies are emitted, but lie within an order of magnitude of each other. The electron kinetic energy along the magnetic field varies from zero to a maximum value, due to the one-dimensional character of the motion along the field, between each pair of potential barriers corresponding to the discrete energy levels. The results may be relevant to describing gamma-ray flares of pulsars. 相似文献