熔融织构Y0．8Ca0．2Ba2Cu3Oy的电子比热

采用热驰豫方法在0到9T范围内测量了熔融织构Y0．8Ca0．2Ba2Cu3Oy的比热．零场下，2-180K的比热结果可以用Einstein模型来描述．通过4-Einstein峰拟合声子谱的方法，我们分别处理了不同磁场下超导转变附近的比热，获得了晶格比热和不同磁场下的电子比热，并将实验结果与London模型的计算结果进行对比，发现London模型能够很好地模拟出我们的实验结果．     

本征Josephson单结的电流-电压特性

采用光刻蚀和Ar离子刻蚀技术成功地在Bi-2212单晶表面制备出台阶型本征Josephson单个结，并在5-65K范围内用四引线法测量了该结零场下的Ⅰ～Ⅴ特征曲线．结果表明，临界电流几乎保持不变，但返回电流随温度增加而增大；与此同时，Mccumber参数βc随着温度增加而减小．临界温度附近，跳跃电压△V明显偏离BCS理论．     

瞄准制导仪中的调制盘光学系统分析

瞄准制导仪中的调制盘光学系统包含有光束投射系统、光束投影系统和旋转调制盘。基于旋转调制盘图案设计的原理,分析了瞄准制导仪中内、外调制图案与光学系统的配合问题。较详细地分析了激光束投射系统和投影系统。     

人参中锗的分光光度法测定

采用灰化法分解人参样品，用分光光度法测定人参中的有机锗含量，方法简便，快捷，回收率为98．90％－99．78％。     

实验室天体物理研究进展

近年来,随着高功率激光实验装置的广泛应用,成像技术和模拟分析技术水平的进一步提高,实验室天体物理研究取得了一些新的重要进展,如激光等离子体实验中对流等离子体磁场结构,冲击波中磁场的湍流放大效应,实验室模拟原恒星喷流中磁场的准直效应和太阳风与偶极磁场之间相互作用等方面的研究。这些研究加深了人们对原恒星以及Herbig—Haro天体喷流、超新星遗迹冲击波、地球磁层中磁场活动等天体物理现象的理解。文章对上述几个方向进行了介绍,并对未来研究方向做一些展望。     

Spatial Carrier Bi-frequency Fourier Transform Profilometry for the 3-D Shape Measurement of Object with Discontinuous Height Steps

1 IntroductionProjecting a single frequency lfringe pattern upon an Object and observing itsdeformation from a different view angle has been a common method for various threedimensional shape measurement techniques. An autpmatic analysis of the fringepatterns is normally carried out either by the FOurier transform method[IJ or by phasestepping['] of the fringe patterns. HOWever, these techniques have a disadvantage ofprincipal importance, the so-called indetedrinaCy tO a factor Of Zap, or …     

Evolution of Hyperbolic-Secant Pulses Towards Cross-Phase Modulation Induced Optical Wave Breaking and Soliton or Soliton Trains Generation in Quintic Nonlinear Fibers

The approximate analytical frequency chirps and the critical distances for cross-phase modulation induced optical wave breaking (OWB) of the initial hyperbolic-secant optical pulses propagating in optical fibers with quintic nonlinearity (QN) are presented. The pulse evolutions in terms of the frequency chirps, shapes and spectra are numerically calculated in the normal dispersion regime. The results reveal that, depending on different QN parameters, the traditional OWB or soliton or soliton pulse trains may occur. The approximate analytical critical distances are found to be in good agreement with the numerical ones only for the traditional OWB whereas the approximate analytical frequency chirps accords well with the numerical ones at the initial evolution stages of the pulses.     

研究性核反应堆的现状、应用和发展

回顾了世界过去50多年研究堆的发展历程,分析了世界研究堆的现状以及未来的应用发展趋势,同时结合我国脉冲堆的实际情况,对其应用发展前景进行了初步展望。     

行星重力的后牛顿近似对卫星作用的估计

将行星重力的广义相对论后牛顿近似应用于木星系统和撞击木星的彗星Shoe maker Levy 9,计算了木星重力的后牛顿改正和它的卫星的进动效应,并与地球月球系统作比较,进行分析和讨论 关键词： 重力的后牛顿近似 木星及其卫星 彗星Shoe maker-Levy 9 广义相对论     

Estimating Magic Numbers Larger Than 126 by Fermi—Yang Liming Method

The Fermi-Yang Liming method is followed and developed to estimate new magic numbers in nuclei with a Woods-Saxon density function.The calculated results predict that the magic number next to 126 should be around 184 and 258.