Computer simulation of spectrometer magnets for some experimental installations

The significance of numerical simulation in the research of magnetic systems is determined by not only known advantages of the computing experiment, but also by the fact that the measurement of a magnetic field is a labour-consuming and expensive problem. Mathematical simulation allows one to investigate those parts of the magnet’s design where the measurements of the magnetic field are extremely complicated or even impossible. This work is aimed to generalize experience of the mathematical simulation of magnetic systems of various-type physical and electromechanical installations and to work out some recommendations of the optimal use of some software products for the numerical modeling of magnetostatic problems. This work also presents some results of a numerical analysis of the magnetic systems of the JINR’s physical installation MARUSYA with the purpose of studying an opportunity of designing magnetic systems with predetermined characteristics of the magnetic field. The article is published in the original.     

Modern microwave magnetic materials: Recent advances and trends

In recent years, a large variety of microwave magnetic materials has been developed, with different compositions, shapes, and fabrication processes. The physics of the dynamic magnetic responses of these materials is very rich, due to the interplay between the intrinsic magnetic properties of the materials, the domain structure, and dynamic shape effects. These materials are associated to a variety of applications, some of them well-established, for direct interaction with rf waves; others corresponding to etablished uses of magnetic materials, but at higher speeds or higher frequencies; and some in association with hot topics in the magnetic or rf communities including metamaterials, nanoscale structures, and nonlinear devices.     

Application of magnetic refrigeration and its assessment

Magnetic refrigeration has the potential to replace conventional refrigeration—with often problematic refrigerants—in several niche markets or even some main markets of the refrigeration domain. Based on this insight, for the Swiss Federal Office of Energy a list of almost all existing refrigeration technologies was worked out. Then an evaluation how good magnetic refrigeration applies to each of these technologies was performed. For this purpose a calculation tool to determine the coefficient of performance (COP) and the exergy efficiency as a function of the magnetic field strength and the rotation frequency of a rotary-type magnetic refrigerator was developed. The evaluation clearly shows that some application domains are more ideal for a replacement of conventional refrigerators by their magnetic counterparts than others. In the pre-study, four good examples were chosen for a more comprehensive investigation and working out of more detailed results. In this article, the calculation method is briefly described. COP values and exergy efficiencies of one very suitable technology, namely the magnetic household refrigerator, are presented for different operation conditions. Summarizing, it is stated that magnetic refrigeration is a serious environmentally benign alternative to some conventional cooling, refrigeration and air-conditioning technologies.     

Internal dynamics of a plasma propelled across a magnetic field

When a plasma is pushed across a magnetic field by some nonelectromagnetic force, ions and electrons get turned in opposite directions by the magnetic field. This creates an internal current as well as sheaths at the plasma surfaces and results in an electric field which allows the plasma to maintain some, or even most of its initial momentum in the form of E&oarr;×B&oarr; drift. An exact analysis of that process is presented for the internal region of the plasma. The energy provided by the initial push is used, in part, to create some gyrations inside the plasma. When the rest energy density of the plasma exceeds twice the magnetic energy density (or when the Alfven speed is less than c), there will be enough energy to spare for the plasma to continue across the magnetic field at half its initial momentum. Two cases are considered: an impulsive start and a gentle push such as provided by gravity. The amplitude of the resulting internal gyrations becomes small in the second case. The frequencies of the gyrations are those of extraordinary modes of very long spatial wavelength     

A neutron diffraction and magnetization study of Heusler alloys containing Co and Zr,Hf, V or Nb

Neutron diffraction, X-ray diffraction and saturation magnetization measurements have been made on a series of ferromagnetic alloys at the composition Co₂YZ, where Y is a group IVA or VA element and Z is a group IIIB or IVB element. The alloys are mainly ordered in the Heusler L2₁ type chemical structure, but some show the presence of a small amount of additional phase, or some preferential disorder.The magnetic results form two distinct groups in which the moments are confined to the Co sites but their magnitude depends on the electron concentration determined by the Y and Z atoms. Although the magnetic moments and Curie temperatures of the alloys in the same group are similar, their lattice parameters differ according to whether Z is a group IIIB or IVB element. Such behaviour indicates that, as in other alloy series with the Heusler structure, a change in lattice parameter has little effect on the magnetic properties in comparison with the effect of a change in electron concentration.     

Mössbauer effect studies of some trimeric iron compounds

Mössbauer spectra of some basic iron (III) carboxylates are reported. The zero field spectra are quadrupole doublets with a characteristic temperature dependent asymmetry. In applied magnetic fields at 4·2°K large hyperfine magnetic fields are observed. These can only result from a Hamiltonian which is not symmetric in all three sites. This asymmetry may be due to a structural asymmetry or to small intercluster magnetic interactions.     

过渡金属掺杂氧化锌团簇的物性研究

本文采用第一性原理密度泛函理论研究了过渡金属（TM）原子Cr和Fe单掺杂和双掺杂(ZnO)12团簇的结构和磁性质。我们考虑了替代掺杂和间隙掺杂。结果表明Cr 和 Fe间隙掺杂团簇结构最稳定。团簇磁矩主要来自TM原子3d态的贡献,4s 和4p 态也贡献了一小部分磁矩。由于轨道杂化,相邻的Zn和O原子上也产生少量自旋。最近邻TM原子间的磁性耦合,主要由两个TM原子之间的直接短程铁磁耦合和TM和O原子之间通过p-d杂化产生的反铁磁耦合这两种相互作用的竞争来决定。不同TM原子掺杂团簇的总磁矩与TM原子种类以及掺杂位置有关,说明在(ZnO)12团簇中掺杂不同TM原子在可调磁矩的磁性材料的领域有潜在应用价值。     

Aberrations theory of a time dependent magnetic field lens

We analyze new forms of aberrations affecting a time dependent magnetic field lens recently proposed. The lens consist of an axially symmetric ellipsoidal solenoid producing a spatially uniform but time pulsating homogeneous field. The dynamics of electrons emitted by some object and injected into this coil shows that this system is capable of focusing a parallel beam or produce images free of geometrical aberrations. The cardinal elements of this lens change periodically in positions and therefore to obtain a stationary image it is necessary to employ a chopped electron beam. Two forms of aberrations originate from the finite duration of the electron pulse and the energy dispersion of the incoming beam (chromatic aberration). Their image degradation effects are quite similar and result from recording different axially displaced images at some fixed stationary plane. We show how, by adjusting the parameters characterizing the magnetic pulse and introducing small apertures that increase the depth of focus, their effects can be reduced or in some cases eliminated. Other forms of instrumental aberrations characteristic of this time dependent magnetic field lens are briefly discussed.     

Aberrations theory of a time dependent magnetic field lens

We analyze new forms of aberrations affecting a time dependent magnetic field lens recently proposed. The lens consist of an axially symmetric ellipsoidal solenoid producing a spatially uniform but time pulsating homogeneous field. The dynamics of electrons emitted by some object and injected into this coil shows that this system is capable of focusing a parallel beam or produce images free of geometrical aberrations. The cardinal elements of this lens change periodically in positions and therefore to obtain a stationary image it is necessary to employ a chopped electron beam. Two forms of aberrations originate from the finite duration of the electron pulse and the energy dispersion of the incoming beam (chromatic aberration). Their image degradation effects are quite similar and result from recording different axially displaced images at some fixed stationary plane. We show how, by adjusting the parameters characterizing the magnetic pulse and introducing small apertures that increase the depth of focus, their effects can be reduced or in some cases eliminated. Other forms of instrumental aberrations characteristic of this time dependent magnetic field lens are briefly discussed.     

Astronomical Spectroscopy: An Introduction to the Atomic and Molecular Physics of Astronomical Spectra, 2nd edn., by Jonathan Tennyson Atomic Astrophyiscs and Spectroscopy,by Anil K. Pradhan and Sultana N. Nahar

Much of our knowledge about magnetic centres in solids haa been obtained using magnetic resonance. The experiments rely upon detecting the absorption of microwave or radio frequency radiation by the centres at charaateristic values of an applied magnetic field. The method in its conventional form is usually restricted to the ground states of systems, since, even for long-lived excited states, there are at any instant insufficient numbers of excited centres to give detectable absorption signals. It is, nevertheless, possible to observe magnetic resonance in many of these excited states provided that optical methods of detection are used, since the magnetic resonance often affects some property of the luminescence, such aa intensity or polarization. The purpose of this article is to describe how optically-detected magnetic resonance experiments are carried out and to discuss the types of system to which they may be applied. It will be seen that, as well as providing details of excited states, the technique enables one to investigate the luminescence process itself.     

生物磁铁矿的磁各向异性与磁接收器

磁铁矿是分布广泛且非常重要的亚铁磁材料,也广泛分布在生物体中。生物体中的磁铁矿具有完美的晶体结构,大多为超顺磁颗粒或单畴颗粒,且大多呈链状分布,具有明显的磁各向异性。生物体中存在“磁接收器”,生物磁铁矿是“磁接收器”的生物物理基础。本文中,从超顺磁磁铁矿颗粒和单畴磁铁矿颗粒的物理特性出发,主要是从它们的磁各向异性特性的基础上描述了生物磁铁矿和“磁接收器”的工作机制, 即在某些条件下,在外界地磁场强度量级的磁场作用下,超顺磁颗粒或单畴颗粒可以诱导产生足够强的磁场,使邻近的晶体可以相互吸引或排斥, 这些粒子间的相互作用可以改变晶体颗粒束所在的外围机体形状,而神经系统可以探测到单独的粒子束或一列粒子束的扩张或收缩,因此生物体就可以探测到磁场的方向以及强度等磁场参量。     

生物磁铁矿的磁各向异性与磁接收器

磁铁矿是分布广泛且非常重要的亚铁磁材料,也广泛分布在生物体中。生物体中的磁铁矿具有完美的晶体结构,大多为超顺磁颗粒或单畴颗粒,且大多呈链状分布,具有明显的磁各向异性。生物体中存在“磁接收器”,生物磁铁矿是“磁接收器”的生物物理基础。本文中,从超顺磁磁铁矿颗粒和单畴磁铁矿颗粒的物理特性出发,主要是从它们的磁各向异性特性的基础上描述了生物磁铁矿和“磁接收器”的工作机制,即在某些条件下,在外界地磁场强度量级的磁场作用下,超顺磁颗粒或单畴颗粒可以诱导产生足够强的磁场,使邻近的晶体可以相互吸引或排斥,这些粒子间的相互作用可以改变晶体颗粒束所在的外围机体形状,而神经系统可以探测到单独的粒子束或一列粒子束的扩张或收缩,因此生物体就可以探测到磁场的方向以及强度等磁场参量。     

Cluster of solar active regions and onset of coronal mass ejections

round-the-clock solar observations with full-disk coverage of vector magnetograms and multi-wavelength images demonstrate that solar active regions(ARs) are ultimately connected with magnetic field. Often two or more ARs are clustered, creating a favorable magnetic environment for the onset of coronal mass ejections(CMEs). In this work, we describe a new type of magnetic complex: cluster of solar ARs. An AR cluster is referred to as the close connection of two or more ARs which are located in nearly the same latitude and a narrow span of longitude. We illustrate three examples of AR clusters, each of which has two ARs connected and formed a common dome of magnetic flux system. They are clusters of NOAA(i.e., National Oceanic and Atmospheric Administration) ARs 11226 11227, 11429 11430, and 11525 11524. In these AR clusters, CME initiations were often tied to the instability of the magnetic structures connecting two partner ARs, in the form of inter-connecting loops and/or channeling filaments between the two ARs. We show the evidence that, at least, some of the flare/CMEs in an AR cluster are not a phenomenon of a single AR, but the result of magnetic interaction in the whole AR cluster. The observations shed new light on understanding the mechanism(s) of solar activity. Instead of the simple bipolar topology as suggested by the so-called standard flare model, a multi-bipolar magnetic topology is more common to host the violent solar activity in solar atmosphere.     

Magnetic guide of cold atoms using a U-shaped current-carrying conductor

We propose a new scheme to magnetically guide cold neutral atoms using a U-shaped current carrying conductor. The spatial magnetic field distribution from the U-shaped current-carrying conductor and the relationship between the magnetic field and parameters of the U-shaped conductor are analysed. Our study shows that U-shaped current-carrying conductor can be used to realize single- or double-channel magnetic guiding of cold atoms in weak-field-seeking states and to construct various atom-optical elements. By using Monte Carlo simulations, the dynamic process of the guided atomic-beam splitting in an atomic-beam splitter composed by the U-shaped current-carrying conductor is studied, and some results are presented.     

Model of magnetization in thin magnetic films with one domain and two-domain basic structures

The magnetization processes in thin magnetic films are described by a model analysing the behaviour of one domain and two-domain basic structures (BS) in the applied magnetic field. These structures include the film areas with nearly constant crystal and magnetic parameters. The minimum of BS free energy including the energy in the internal magnetic field, the energy of the induced anisotropy and the domain-wall energy are taken into account. The initial and hysteresis curves of the sample depend on the function of distribution for the BSs are calculated. A good qualitative agreement with the results of other authors is observed if the films consists of one-domain or two-domain BS only. Our experimental data give also some support of the model.     

Three-layer magnetoconvection

It is believed that some stars have two or more convection zones in close proximity near to the stellar photosphere. These zones are separated by convectively stable regions that are relatively narrow. Due to the close proximity of these regions it is important to construct mathematical models to understand the transport and mixing of passive and dynamic quantities. One key quantity of interest is a magnetic field, a dynamic vector quantity, that can drastically alter the convectively driven flows, and have an important role in coupling the different layers. In this Letter we present the first investigation into the effect of an imposed magnetic field in such a geometry. We focus our attention on the effect of field strength and show that, while there are some similarities with results for magnetic field evolution in a single layer, new and interesting phenomena are also present in a three layer system.     

基于开口环的可调谐滤波器及其电磁带隙

基于开口谐振环上加载变容二极管设计可调谐滤波器,很好地实现了电磁波带隙的可调.在单环开口谐振环缝隙处或者双环开口谐振环的两环之间加载变容二极管,改变加载变容管上得的电压,改变该结构的分布参量而达到滤波器可调性能.同时通过数值计算分析了该滤波器结构对电磁波的频率响应函数,指出其形成电磁波带隙的物理机制,为了消除开口谐振环的磁谐振效应而关闭开口谐振环的缝隙实验进行了验证.研究表明基于变容管开口环的可调谐滤波器所形成的电磁波带隙中,有的带隙是源于磁谐振机制.有的带隙是源于电谐振机制.对该滤波器形成带隙物理机制的研究,可以更好地理解开口谐振环,有助于其在光学和微波波段器件的设计.     

Behavior of neutrinos in stochastic magnetic fields

If massive neutrinos possess magnetic moments, they can undergo spin flip in a magnetic field. The magnetic fields needed for a meaningful measurement of neutrino moments could be very high and may occur in astronomical objects such as some supernovae or active galactic nuclei: they are typically chaotic ones. We develop the general theory of the passage of neutrinos through such fields. We also develop a simple model which becomes solvable in the high energy limit. Both helicities occur with equal probability, independently of the initial distribution. Observational consequences are discussed.     

微纳尺度多铁异质结中电驱动磁反转

近年来,多铁异质结中电控磁性研究引起了广泛关注,已成为多铁领域的热点.现代自旋电子学器件(如磁内存)通常利用电流产生的磁场或自旋转移扭矩效应驱动磁反转来实现数据擦写,但这带来高额能耗和热量,成为亟待解决的关键难题.而利用多铁异质结实施电场驱动磁反转则有望大幅降低能耗,从而实现高速、低能耗、高稳定性新型高密度磁存储、逻辑及其他自旋电子学器件.在当前器件发展的微型化趋势下,探索可集成化的微纳尺度电场驱动磁反转方案显得越发重要.本文针对发展新型磁电器件所面临的微型化关键问题,回顾了微纳尺度电场驱动磁反转研究的新进展,主要关注小尺度多铁异质结中电控磁的新特点、新方法及相关物理机理的实验和理论成果,讨论了进入纳米尺度将面临的挑战,并对未来研究工作提出一些展望.     

Magnetic properties of the Kondo lattice

We review the magnetic properties of the Konso lattice model using the functional integral technique: we discuss the magnetic and non-magnetic phases, and some properties of these phases. Comparison with other calculations is also made. Finally some open questions are discussed.