牛血清白蛋白在NVP/HEMA无规共聚物水凝胶上的吸附研究

合成了不同含水量的N-乙烯吡咯烷酮(NVP)／甲基丙烯酸-β-羟乙酯(HEMA)共聚物水凝胶．研究了温度、pH值，蛋白质初浓度及离子强度等因素对牛血清白蛋白吸附性能的影响．采用紫外分光光度法测定BSA的吸附量．结果表明，蛋白质初浓度越高．温度越高，离子强度越大；蛋白质内部更多的疏水性氧基酸残基暴露于外部．吸附量增加：在等电点pH=4．7附近蛋白质沉积量最大．     

基于MATLAB的矢量光束聚焦光场仿真

偏振是光的基本属性之一,也是光学课程教学中的重点内容。但由于课时限制等原因,光学课程对于光的偏振介绍比较简单,内容也局限于老旧内容。随着光学的发展,矢量偏振光束由于其独特的特性已经被广泛的研究和应用,因此,在光学课程中引入偏振发展的前沿知识,有助于学生探索新的光学发展领域,从而激发他们的学习兴趣,为推动教研融合作出积极贡献。本文以矢量偏振光束通过高数值孔径物镜的衍射为例,基于矢量衍射理论和MATLAB模拟仿真展示偏振态对光场传播过程和聚焦光场的影响。首先根据矢量衍射理论推导了聚焦场分布积分表示;然后借助MATLAB仿真给出了矢量偏振光束入射情况下聚焦光场分布;最后通过与常见的线偏振光和圆偏振光对比,对矢量偏振光束聚焦场分布进行了分析和总结。     

斜孔结构装甲设计及抗弹性能研究

设计了一种斜孔结构装甲,利用有限元方法研究高速弹体冲击下斜孔结构装甲的弹道力学行为,重点分析孔倾角对孔结构装甲不同典型弹着点侵彻破坏的影响.计算结果表明:弹着点位于孔结构中心(弹着点Ⅰ)时,斜孔结构设计导致弹体发生了严重侵蚀、偏航以及折断,有效降低了弹体的侵彻速度,使孔结构中心不再是最薄弱部位;随着孔倾角的增加,位于倾...     

Ge BEAM TREATMENT OF Si SUBSTRATE FOR MOLECULAR BEAM EPITAXY

A new surface cleaning method for Si MBE is described in which a very weak Ge beam flux is deposited on the surface for removing the thin passivative layer of SiO₂ on the Si subetrate. It has proved that the SiO₂ will react with Ge at a relatively low temperature (620℃), and as a result, the oxide layer becomes volatile. Here the high temperature annealing in the conventional Shiraki method is no longer required, and since the oxide layer is removed in ultra high vacuum, only very little carbon contamination may occur. Furthermore, to reduce the excessive Ge on the substrate surface, Ge is deposited at 620℃ and then the sample is annealed at 700℃; the residual Ge atoms on Si substrate can be reduced to less than 0.1 monolay-er (ML). Ge beam treatment turns out to be an effective low-temperature Si surface-cleaning method, especially for the heteroepitaxial growth of Ge_xSi_1-x/Si.     

赤霉酸甲酯及其类似物的2D NMR研究

应用¹H-¹H COSY,NOESY,¹³C-¹H COSY等2DNMR和DEPT技术,完成了赤霉酸甲酯(2),13-O-乙酰基赤霉素甲酯(3)及其3位差向异构体(4)的¹H和¹³CNMR化学位移的全指定,并探讨了它们的相对构型,相关质子间的偶合常数也支持所得结果。     

基于InP材料的纳米光栅耦合器的耦合效率分析

设计了一种基于InP材料的纳米光栅耦合器,运用FDTD算法分析了周期长度、刻蚀深度以及占空比变化时该光栅耦合器的耦合效率。计算结果表明,周期长度为800nm,刻蚀深度为0.3μm,占空比接近0.5时,耦合效率可以达到13%。本文所设计的光栅耦合器对构建基于InP材料的谐振腔、激光器和陀螺结构具有一定的理论指导意义。     

水波实验装置的改进

水波实验装置,一般由投影仪、消波水槽、闪频器和水波振动器等组成。该实验效果的好坏,水波振动器振动顿率的稳定性是个关键。常用的振动器是用杠杆与偏心轮组成的机械式振动器;也有用低频振荡源来策动电磁铁振动的电磁振动器。由于上述装置中机械结构的问题,往往使振动器的振动频率,达不到应有的稳定性,造成振动频率与闪频器的开放频率不能同步,观察到的波阵图就不能保持稳定。特别是演示水波的干涉现象,若两者达不到同步,要清晰地观察到波的加强与减弱的位置就比较困难。笔者改用电子振动器,解决了振动器振动频率的稳定性和闪频器同步的问题,使实验效果得到明显的改善。     

小型内窥镜干涉型光纤陀螺仪装配质量控制系统（英文）北大核心CSCD

提出一种用于干涉型光纤陀螺仪(IFOG)装配质量控制的内窥镜系统设计及相关图像分析方法。同时采用1.0mm与2.4mm工业内窥镜系统采集IFOG内部图像与视频数据;并利用多自由度运动控制平台调节内窥镜工作姿态以保证图像的顺利采集。在此基础上,设计了基于db4小波基的图像增强方法,基于灰度共生矩阵的图像纹理特征估计方法以及图像几何形状特征的计算方法等,用以进行内窥镜图像的分析。通过上述系统与方法的应用,能够有效检测出IFOG产品在装配过程中出现的多余物颗粒、光纤断纤或异常胶粘等质量问题,有效提高了IFOG产品的装配质量。     

Dynamic control of retrieval contrast in a Λ-type atomic system

We propose an efficient scheme for optimizing the optical memory of a sequence of signal light pulses in a system of ultracold atoms in Λ configuration. The memory procedure consists of write-in, storage, and retrieval phases. By applying a weak microwave field in the storage stage, additional phase-dependent terms are included, and the contrast of the output signal pulses can be dynamically controlled (enhanced or suppressed) through manipulating the relative phase φ between optical and microwave fields. Our numerical analysis shows that the contrast is enhanced to the most extent when φ=1.5π. In addition, the contrast is in proportion to the Rabi frequency of the microwave field with a certain relative phase.     

Mass Fraction of 13C-Pocket in Metal-Poor AGB Stars and the Primary Nature of Neutron Source

Chemical abundances of very metal-poor s-rich stars contain excellent information to set new constraints on models of neutron-capture processes at low metallicity. Using the parametric approach based on the radiative s-process nucleosynthesis model, we obtain the mass fraction q of 13 C-pocket, the overlap factor r, the neutron exposure per interpulse △τ, and the component coefficients of the s-process and the r-process for 25 s-rich stars, respectively. We find that q deduced for the lead stars is comparable to the overlap factor r, which is larger than the standard case （hereafter ST case） of the AGB model （q - 0.05） about 10 times, and AT are about 10 times smaller than the ST case （AT = 7.0 mbarn^-1）. Although the two parameters obtained for the lead stars are very different from the ST case of the AGB stellar model, it is worth noting that the total amounts of 13 C in metal-poor condition are close to the ST case. The above relation is a significant evidence for the primary nature of the neutron source and the lead stars could be polluted by low-mass AGB stars. Because interpulse period declines with increasing stellar mass, for high-mass AGB star, the neutron irradiation may be terminated due to their shorter interpulse period. Thus the neutron exposure per interpulse of the larger AGB stars should be about 10 times smaller than the ST case. In this ease, the primary nature of the neutron source also exists.