Structure of Callisto and Ice Holes on Its Surface

The discovery of the induced magnetic field of Callisto that is a satellite of Jupiter has been interpreted as evidence for a subsurface salty liquid-water ocean,so we consider a layered structure of callisto,i.e.,a rock-metal core,an outer layer of ice and a middle layer of ocean.For the rock-metal core we try to indicate how the temperature,pressure and mass density depend on the depth.Due to motionn across the magnetic field of Jupiter in a plasma environment,the ice shell of Callisto must be broken down by electric current.     

Gamow—Teller Resonance of 90Zr in a Relaztivistic Approach

We establish the formalism of nuclear spin-isospin excitations,especially the Gamow-Teller resonance in a fully consstent relativistic random-phase approximation.A relativistic form of the Landau-Migdal parameter g‘ is adopted as a residual spin-isospin correlation force.In the non-relativistic limit it reproduces the excitation energy of the giant Gamow-Teller resonance state obtained in the non-relativistic model.The Gamow-Teller resonance for finite nuclei is investigated in a relativistic approach for the first time.It is found that the Ikeda sum rule of 90Zr is quenched about 8% in the Hartree as well as the correlated strengths due to the poles of the negative Dirac states at energies above 1 GeV.     

Multiple—Scattering of Near—Edge x—ray Absorption Fine Structure of Sulphur—Passivated InP（100） Surface

We use the multiple-scattering cluster method to calculated the sulphur 1s near-edge x-ray absorption fine structure (NEXAFS) of S-passivated InP(100) surface.The physical origins of the resonances in the NEXAFS have been unveiled.It is shown that the most important resonance is attributed to the photoelectron scattering between the central sulphur and the nearest indium atoms.The studies show that two S-S dimers with the bond lengths of 2.05A and 3.05A coexist in the surface,meanwhile the bridge and antibridge site adsorption of single S could not be ruled out.We support the scanning tunnelling microscopy result that the S-passivated InP(100) surface exhibits significant discorder.     

电磁能的军用展望

本文简要介绍了电磁能在发射和输能技术方面的研究现状，预测21世纪电磁能的军事应用前景．     

164Lu的三轴超形变核态的研究

利用TRS方法对双奇核¹⁶⁴Lu的位能面进行了计算,确认了¹⁶⁴Lu核的一条三轴超形变带,结果与实验较好地符合,同时指出了三轴超形变带的一个具体的组态     

X射线相衬成像

本文介绍了近年来X射线位相衬度成像技术的发展状况，详细论述了X射线干涉相衬、衍射增强相衬，类同轴相衬和数字位相重构等几种典型的成像原理，讨论了影响成像衬度与分辨率的若干因素，并对位相成像的发展趋势作了展望。     

基于CCD采集的Mach-Zehnder干涉条纹图的处理算法

Mach-Zehnder干涉仪适用于研究气体密度迅速变化的状态。由于气体折射率的变化与其密度的变化成正比,而折射率的变化将使通过气体的光线有不同的光程,因此可通过干涉臂变化对干涉条纹图像效果的影响得到气体密度。实测中,采用图像采集卡和CCD来接收Mach-Zehnder干涉仪产生的条纹图像,再通过计算机对条纹图像的条纹间距进行处理,从而得到气体密度的变化状态。从光干涉理论出发,对Mach-Zehnder干涉条纹图像特征进行了分析,建立了Mach-Zehnder干涉条纹的数学模型,并根据此模型设计了处理Mach-Zehnder干涉条纹图像的算法。算法包括图像的预处理(即图像的噪声提取)、图像的二值化及图像的细化。     

黑土腐殖酸的近红外光谱测定

研究了我国黑土腐殖酸碳含量及其光化学性质,并探索了利用近红外光谱分析法(near infrared spectroscopy, NIRS)对其进行预测的潜力。针对东北典型黑土带土壤样品,利用偏最小二乘法(PLSr)建立定量模型,并用独立样本对模型进行检验。结果表明,模型对腐殖酸碳、胡敏酸碳和富里酸碳含量的预测效果很好,NIRS对富里酸碳和胡敏酸碳的465 nm(E₄)和预测结果也较好,665 nm光密度(E₆)的预测达到可接受水平。胡敏酸碳和富里酸碳含量与SOC的相关性,高于其与NIRS模型预测值的相关性,二者光化学性质与SOC的相关性则低于其与模型预测值的相关性。NIRS在简化黑土腐殖酸碳、胡敏酸碳和富里酸碳含量和光密度测定领域具有很好的应用前景,且能够反映SOC性质方面的信息。     

186,188,^190Pb低位长椭球带的理论研究

将角动量投影壳模型应用到１８６ Ｐｂ ,１８８ Ｐｂ 和１９０ Ｐｂ 核, 对它们的低位长椭球带进行了理论计算并与实验结果进行了比较, 对这三个核从理论上预言了该带带头, 并把壳模型应用到１８６ Ｈｇ 核, 得到与实验较好地符合验证了这种理论预言的可靠性．     

全彩色LED显示屏的色度计算

全彩色ＬＥＤ显示屏可以用来显示电视画面。目前没有专门用于ＬＥＤ彩色大屏幕的图像源及其标准,所以都是将送给ＣＲＴ显像管的图形信号源送到ＬＥＤ彩色大屏幕进行显示。针对把送给ＣＲＴ的信号送到ＬＥＤ屏进行显示会引起彩色失真这种情况,本文给出ＬＥＤ大屏幕系统的色度公式,为准确控制ＬＥＤ管的发光亮度提供理论依据,并给出产例。