电葫吊车数控化的原理与设计

本文结合一应用实例，具体介绍用微机对电葫吊车进行控制。文中也论述了实现电葫吊车数控化的原理及设计方法。     

粉末烧结Nd15Fe77B8永磁合金的矫顽力特征

通过测量粉末烧结Ｎｄ１５Ｆ３７７Ｂ８永磁合金的充磁和退磁曲线，结合金相组织及磁畴观察分析，证明该合金的矫顽力是由畴壁的钉扎来控制。     

A magnetic explanation for the rapid burster

The observations of X-ray Type II bursts from the low-mass X-ray binary MXB 1730-335 can be explained by a particular form of magnetic gating in the presence of steady external accretion. The requirements are a strong magnetic field of the neutron star (7×10¹¹–2×10¹² gauss at the surface), rotational symmetry and alignment of the field axis with the axis of a steadily accreting disk to within 6°.     

国际贸易对国家创新能力影响的实证分析

长期以来,国际贸易一直被视为创新能力扩散和转移的重要渠道,文章选取我国进出口总额和国内专利授权数作为衡量国际贸易和国家创新能力的指标,利用协整分析和Granger因果检验对其进行实证研究。研究发现,国际贸易和国家创新能力之间存在着长期的均衡关系;国际贸易是提升国家创新能力的原因,但不是国家创新能力的结果;并在此基础上分析了作为一个贸易大国,我国创新能力对国际贸易影响不大的原因。     

平视显示器的瞬时视场计算

瞬时视场是平视显示器的重要技术指标之一。平均应有尽可能大的瞬时视场，平显的瞬时社场应叠合于平显总视场的下部区域。平视显示器的瞬时视场由半径大小可知，圆心坐标可控的6圆交接而成。本文论证实现平显瞬时视场正确占位的设计途径，并给出数字实例。     

基于四边形网格细分曲面的生成

基于Catmull-Clark细分模式，提出了一种有效的四边形网格的细分曲面生成方法。对细分算法的数据结构特点进行了详细的分析，根据细分规则，给出了算法的生成矩阵以及连接规律。该方法具有局部性好、简单、易操作的特点，可成功应用于工程实际，解决细分曲面的生成问题。     

The optical to X-ray spectrum of the broad-line ultrasoft AGN RE J2248-511

We present a series of monitoring observations of the ultrasoft broad-line Seyfert galaxy RE J2248-511 with XMM-Newton. Previous X-ray observations showed a transition from a very soft state to a harder state five years later. We find that the ultrasoft X-ray excess has re-emerged, yet there is no change in the hard power-law. Reflection models with a reflection fraction of 15, and Comptonisation models with two components of different temperatures and optical depths (kT₁ = 83 keV, T₁ = 30 eV, τ₁ = 0.8; KT₂ = 3.5 keV, T₂ = 60 eV, τ₂ = 2.8) can be fit to the spectrum, but cannot be constrained. The best representation of the spectrum is a model consisting of two blackbodies (kT₁ = 0.09 ± 0.01 keV, kT₂ = 0.21 ± 0.03 keV) plus a power-law (Γ = 1.8 ± 0.08). We also present simultaneous optical and infrared data showing that the optical spectral slope also changes dramatically on timescales of years. If the optical to X-ray flux comes primarily from a Comptonised accretion disk we obtain estimates for the black hole mass , accretion rate and inclination cos(i)  0.8 of the disk.     

Orbital phase spectroscopy of X-ray pulsars to study the stellar wind of the companion

High Mass X-ray Binary Pulsars (HMXBP), in which the companion star is a source of supersonic stellar wind, provide a laboratory to probe the velocity and density profile of such winds. Here, we have measured the variation of the absorption column density along with other spectral parameters over the binary orbit for two HMXBP in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. In 4U 1538-52, we find the model corroborating the observations; whereas in GX 301-2, the stellar wind appears to be very clumpy and a smooth symmetric wind model seems to be inadequate in explaining the variation in column density.     

Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.     

PC—DIO─96接口板在大尺寸计量标准中的应用

介绍了美国NI公司的数据采集板PC—DIO—96的功能,及其在Windows95下软硬件的安装,描述了如何使用其随板软件包,并给出了其三种主要功能（线功能、口功能和组功能）的程序框图。详细介绍了在“建立大尺寸计量标准”题目中应用该板进行环境参数的采集和电机控制。