Electron density measurements in a gas discharge subjected to a rotating magnetic field

Measurements of the electron density within an axial CO₂ laser discharge subjected to a transverse rotating magnetic field are presented. Experiments were performed with a single Langmuir probe. Electron density is evaluated using Su and lam's thick sheath expression for a stationary plasma. Results are presented for a 2.7 kPa (20 torr) discharge with external pre-ionization and for a 0.7 kPa (5 torr) self-sustained discharge.     

On the points of bifurcation along the sequence of rotating axisymmetric masses with magnetic fields

It is shown that the points of bifurcation belonging to the third harmonics along the sequence of Maclaurin spheroids viewed from an inertial frame are distinct from the corresponding points along the Maclaurin sequence considered stationary in a rotating frame and occur at eccentricitye=0·73113 ande=0·99608; the Maclaurin spheroids having become dynamically unstable before the second point is reached. A toroidal magnetic field leaves these points uneffected, while a general poloidal field may either raise or lower these points of bifurcation.     

NMR in pulsed magnetic field

Nuclear magnetic resonance (NMR) experiments in pulsed magnetic fields up to 30.4 T focused on ¹H and ⁹³Nb nuclei are reported. Here we discuss the advantage and limitation of pulsed field NMR and why this technique is able to become a promising research tool.     

脉冲强磁场磁特性科学测量系统及其应用

作为一种极端条件下的实验技术,脉冲强磁场下的磁化测量在磁性材料等研究领域发挥着重要作用。武汉国家脉冲强磁场科学中心建成了两套先进的脉冲强磁场磁化测量系统,并已对外开放运行。文章介绍了该测量系统的组成、测量原理和系统特点,以及该系统在量子磁性材料、功能磁性材料、强关联材料等研究领域中的应用,并对未来的发展提出了展望。     

定轴转动带电体的远区磁场分布

类比定轴转动刚体转动惯量以及电偶极子电场的计算方法，得出定轴转动带电体的磁矩及其远区磁场分布。     

Accretion onto a Kerr black hole in the presence of a dipole magnetic field

We analyze the accretion of charged matter onto a rotating black hole immersed in an aligned dipolar magnetic field. We specialize to motion in the equatorial plane and calculate the ‘Keplerian’ angular momentum distribution, the marginally stable and marginally bound orbits, and the efficiency of mass-to-energy conversion as functions of the angular momentum of the black hole and of the product of the dipole moment and the charge of the infalling matter. Although the detailed results are quite different from those previously obtained in the case of an uniform magnetic field, the astrophysically relevant results are very similar; when hydrodynamical accretion is considered, these effects of the magnetic field are always very small. But for test particles the efficiency can be significantly increased for limited ranges of the parameters.     

Compactifications of the heterotic string with unitary bundles

We describe a large new class of four‐dimensional supersymmetric string vacua defined as compactifications of the E₈ × E₈ and the SO(32) heterotic string on smooth Calabi‐Yau threefolds with unitary gauge bundles and heterotic five‐branes. The conventional gauge symmetry breaking via Wilson lines is replaced by the embedding of non‐flat line bundles into the ten‐dimensional gauge group, thus opening up the way for phenomenologically interesting string compactifications on simply connected manifolds. After a detailed analysis of the four‐dimensional effective theory we exemplify the general framework by means of a couple of explicit examples involving the spectral cover construction of stable holomorphic bundles. As for the SO(32) heterotic string, the resulting vacua can be viewed, in the S‐dual Type I picture, as a generalisation of magnetized D9/D5‐brane models. In the case of the E₈ × E₈ string, we find a natural way to construct realistic MSSM‐like models, either directly or via a flipped SU(5) GUT scenario.     

Potts models with magnetic field: Arithmetic,geometry, and computation

We give a sheaf theoretic interpretation of Potts models with external magnetic field, in terms of constructible sheaves and their Euler characteristics. We show that the polynomial countability question for the hypersurfaces defined by the vanishing of the partition function is affected by changes in the magnetic field: elementary examples suffice to see non-polynomially countable cases that become polynomially countable after a perturbation of the magnetic field. The same recursive formula for the Grothendieck classes, under edge-doubling operations, holds as in the case without magnetic field, but the closed formulae for specific examples like banana graphs differ in the presence of magnetic field. We give examples of computation of the Euler characteristic with compact support, for the set of real zeros, and find a similar exponential growth with the size of the graph. This can be viewed as a measure of topological and algorithmic complexity. We also consider the computational complexity question for evaluations of the polynomial, and show both tractable and NP-hard examples, using dynamic programming.     

电源频率可调的单相旋转磁场实验仪

设计了电源频率可调的单相交流电产生的旋转磁场实验仪,应用该仪器可测量电感、损耗电阻、转速等     

Creation or destruction of sourceless abelian gauge strings in a Robertson-Walker universe

Following Morris’s [5] consideration of a sourceless abelian gauge string in a Robertson-Walker universe with flat space sections we have generalized the treatment to the case of arbitrary spatial curvature. We find that creation or destruction of the gauge string is not possible if the spatial curvature is nonzero.     

一种重复频率脉冲导引磁场的设计

介绍了一种重复频率脉冲磁场作为高功率微波源的导引磁场的设计,该磁场电源具有功耗低、发热量小、结构紧凑等优点,符合高功率微波朝重复频率方向发展的需求。从产生脉冲磁场的电流表达式出发,根据涡流损耗不能太大、品质因数要高和电容储能要小的原则,给出了脉冲磁场产生系统的储能电容和充电电压的优化设计方法。最后将此方法应用于Ka波段返波振荡器导引磁场的设计,确定出产生脉冲磁场电路的电容和充电电压的值,并进行了仿真和实验研究,结果与理论要求吻合较好,在重复频率10 Hz条件下能稳定运行,验证了设计的合理性。     

一种重复频率脉冲导引磁场的设计

介绍了一种重复频率脉冲磁场作为高功率微波源的导引磁场的设计,该磁场电源具有功耗低、发热量小、结构紧凑等优点,符合高功率微波朝重复频率方向发展的需求。从产生脉冲磁场的电流表达式出发,根据涡流损耗不能太大、品质因数要高和电容储能要小的原则,给出了脉冲磁场产生系统的储能电容和充电电压的优化设计方法。最后将此方法应用于Ka波段返波振荡器导引磁场的设计,确定出产生脉冲磁场电路的电容和充电电压的值,并进行了仿真和实验研究,结果与理论要求吻合较好,在重复频率10 Hz条件下能稳定运行,验证了设计的合理性。     

A class of stationary rotating string cosmological models

We obtain a one parameter class of stationary rotating string cosmological models of which the well-known Gödel universe is a particular case. By suitably choosing the free parameter function, it is always possible to satisfy the energy conditions. The rotation of the model hinges on the cosmological constant which turns out to be negative. String-dust distribution in Gödel-type universes is also briefly discussed.     

Excited states of two-dimensional hydrogen atom in tilted magnetic field: Quantum chaos

The aim of the current work is the research of the influence of a tilted magnetic field direction on the spectrum and the energy level spacing distribution of a two-dimensional (2D) hydrogen atom and of an exciton in GaAs/Al_0.33Ga_0.67As quantum well. It was discovered that the quantum chaos (QC) is initiated with an increasing angle α between the magnetic field direction and the normal to the atomic plane. It is characterized by the repulsion of levels leading to the eliminating of the shell structure and by changing the spectrum statistical properties. The statement about the initiation of chaos and its dominance over regular motion with increasing angle α is confirmed by the results of our calculations of the classical dynamics presented in this paper. The evolution of the spatial distribution of the square of the absolute value of the wave function at an increasing angle α was observed. The differences of calculated dependencies of energies for various excited states on the tilt angle at a wide range of the magnetic field strength were described.     

超高速碰撞产生磁场的1维模型

为研究超高速弹丸碰撞靶板产生等离子体诱生的磁场,引用已有关于激光产生等离子体的磁场理论,结合麦克斯韦方程和法拉第电磁感应定律得到了超高速碰撞产生等离子体诱生磁场的1维理论模型。基于已有关于超高速正碰撞产生半球状等离子体云诱生磁场的偏微分方程,建立了柱坐标系下超高速斜碰撞产生部分椭球状等离子体云的偏微分方程。通过感应线圈进行了磁感应强度的实验测量,实验结果与模型预言表明,该模型可近似地描述超高速斜碰撞产生等离子体诱生的磁感应强度。     

Eddy-current loss in a rotating magnetic field

The eddy-current loss is calculated for nonferromagnetic disks in a rotating magnetic field. The power loss is found as a function of the magnetic field intensity, the field rotation velocity, and the disk dimensions. The eddy-current loss was measured experimentally in rotating fields in copper, aluminum, and zinc disks; a good agreement was found with the calculated values.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 1, pp. 38–42, January, 1971.     

超高速碰撞产生磁场的1维模型

 为研究超高速弹丸碰撞靶板产生等离子体诱生的磁场,引用已有关于激光产生等离子体的磁场理论,结合麦克斯韦方程和法拉第电磁感应定律得到了超高速碰撞产生等离子体诱生磁场的1维理论模型。基于已有关于超高速正碰撞产生半球状等离子体云诱生磁场的偏微分方程,建立了柱坐标系下超高速斜碰撞产生部分椭球状等离子体云的偏微分方程。通过感应线圈进行了磁感应强度的实验测量,实验结果与模型预言表明,该模型可近似地描述超高速斜碰撞产生等离子体诱生的磁感应强度。     

The effect of toroidal field on the rotating magnetic field current drive in rotamak plasmas

A rotamak is one kind of compact spherically shaped magnetic-confinement device. In a rotamak the plasma current is driven by means of rotating magnetic field （RMF）. The driven current can reverse the original equilibrium field and generate a field-reversed-configuration. In a conventional rotamak, a toroidal field （TF） is not necessary for the RMF to drive plasma current, but it was found that the present of an additional TF can influence the RMF current drive. In this paper the effect of TF on the RMF current drive in a rotamak are investigated in some detail. The experimental results show that addition of TF increases the RMF driven current greatly and enhances the RMF penetration dramatically. Without TF, the RMF can only penetrate into plasma in the edge region. When a TF is added, the RMF can reach almost the whole plasma region. This is an optimal strength of toroidal magnetic field for getting maximum plasma current when Bv and radio frequency generator power are fixed. Besides driving current, the RMF generates high harmonic fields in rotamak plasma. The effect of TF on the harmonic field spectra are also reported.[第一段]     

重复频率脉冲磁场初级能源

为产生重复频率脉冲磁场的螺线管,研制了一种新型的初级能源,它采用半桥串联谐振恒流充电拓扑结构,可在0~2.5 kV范围内实现输出可调,最大平均充电功率达4.7 kW。该电路最大特色在于无需使用外加谐振元件,只利用变压器的漏感和半桥桥臂电容组成谐振元件。简要分析了电路的工作过程,给出了电路参数设计方法和设计实例,并进行电路仿真和初步实验研究,结果表明,该设计基本达到要求。最后,进行了带螺线管负载的实验研究,实验证明该能源在重复频率10 Hz条件下运行稳定可靠。