偏振光的干涉场分布特征数值模拟及实验研究

从偏振光的产生出发,对不同偏振态的偏振光的干涉场分布进行了数值模拟,得出了不同偏振态干涉场的特征分布,并对不同情况进行了实验,分析讨论了实验结果,为偏振光实验的教学和实验结果的分析提供了依据.     

基于ARM和CPLD的NMR谱仪前放控制设计

提出了一种基于ARM（Advanced RISC Machine,先进精简指令计算机）和CPLD（Complex Programmable Logic Device, 复杂可编程逻辑器件）的NMR（Nuclear Magnetic Resonance,核磁共振）谱仪前放控制系统设计方案. 该控制系统以ARM为控制核心、 CPLD为控制命令执行单元, 控制前置放大器和混频器的工作状态. 本电路包括以下主要功能：1) 前置放大器收发切换的门控信号电平转换;2) 氘梯度匀场时身频通道自动切换;3) 探头调谐的信息显示;4) 锁前放和混频器的配置. 该设计方案具有系统运行速度高、 控制灵活和成本低的优点,并且可以有效减小系统噪声,降低控制部件对前置放大器和混频器的干扰.     

532-nm picosecond pulse generated in a passively mode-locked Nd:YVO_4 laser

A diode-pumped continuous-wave （CW） mode-locked Nd：YVO4/KTP green laser with semiconductor saturable absorber mirror （SESAM） is demonstrated. The maximum output power of CW mode-locked green laser is obtained to be 552 mW at the incident pump power of 7.25 W, corresponding to an opticai-optical conversion efficiency of about 7.6%. The 532-nm CW mode-locked pulse duration is estimated to be about 8.4 ps with the repetition rate of 87 MHz.     

不同微场分布函数对Stark加宽和频移的影响

分别采用Holtsmark,Neutral Point,Nearest-Neighbor和Mayer模型微场分布函数对Stark线型进行了研究,进而得到相应微场函数下的Stark加宽和频移,研究了4种不同的微场分布函数对Stark加宽和频移的影响。研究结果表明,在电子加宽参数不变时,4种微场分布函数对Stark加宽和频移的影响随离子加宽参数的增加而增加;在离子加宽参数不变时,4种微场分布函数对Stark加宽和频移的影响随电子加宽参数的增加而增加;特别是,当离子加宽参数较大时,Mayer模型微场分布函数对Stark加宽和频移的影响异常明显。这说明,微场分布函数对谱线的加宽和频移的影响在离子与离子碰撞剧烈的等离子体环境中尤其显著, 在这样的等离子体环境中,进行等离子体诊断时,选择合适的微场分布函数非常重要。结果对等离子体诊断有一定参考价值。     

喷墨打印垂直有机光晶体管及其性能优化

通过旋涂透明源极并在其上采用喷墨打印的方式制备有源层及源漏电极,从而得到一种垂直结构光晶体管,并获得了较好的光电性能,其响应率为～1 500A/W,探测率可达1.6×10~(14) Jones。向有源层中掺杂一定比例的电子捕获材料PCBM,使有源层中光生空穴复合减小,光生电流增大,从而进一步提高其光探测性能。研究发现当掺杂5wt%电子捕获材料时,垂直结构光晶体管性能达到最优,响应率为～6 000A/W,探测率可达1.4×10~(15) Jones.     

Research on the cyclostationary nearfield acoustic holography based on boundary element method

Cyclostationary sound field is a special kind of nonstationary sound field, in which the pressure signal is modulated seriously and sidebands exist in its spectrum. The reconstructed sound field can＇t figure the cyclostationary features in conventional Nearfield Acoustic Holography （NAH） procedure. On the basis of planar cyclostationary NAH, the cyclostationary NAH based on boundary element method is proposed which can be utilized to analyze radiators with complicated surface. Replacing the Fourier＇s transform with the second-order cyclic statistics, the Cyclic Spectral Density （CSD） functions is used as the reconstructed physical quantity in the proposed NAH technique, instead of the spectrum or power spectral density of pressure signal. By virtue of the demodulation ability of CSD function, the reconstructed CSD can effectively express the information of modulating and carrier wave respectively. The simulation and experiment illustrate that the validity and accuracy of this cyclostationary NAH technique satisfy the request of engineering.     

Intensity Distribution and Phase Vortices of Speckle Fields Generated by Multi-Aperture Random Scattering Screens

The intensity distribution and phase vortices of the speckle fields generated by multi-aperture random scattering screens are simulated, and it is found that the vortices exhibit layer-like structures and the dislocation phenomena occur in the local phase patterns produced by the two-pinhole aperture, whose phase distributions appear as striped structures. For three- or four-pinhole aperture, there are many circular bright spots appearing in the speckle grains, and there is one vortex between the neighboring circular bright spots. The positive and negative phase vortex lattices appear in the phase distributions, and the regions circled by the isothetic phase lines form irregular quadrilaterals or hexagons. Moreover, the relative positions of the vortices or bright spots can be adjusted by changing those of the pinhole apertures.     

多模光纤模式场群速与相速的关系

为了从理论上统一射线光学和导波光学关于多模光纤中各模式场传播过程中时延的论述,试从介质波导理论出发,根据模式的特征根U随光纤归一化频率R的变化关系,在弱波导近似下导出了描述模式场相速Vp与群速Vg关系的重要结果:Vp*Vg=(c/n1)2。根据这一结果可以得出结论:对于低阶模式,由于相速Vp慢,所以群速快;高阶模式其相速Vp快,所以群速慢。对于给定的光纤,利用射线光学和波导光学进行了带宽估计,2种理论计算结果的一致性,印证了上述关系的正确性。     

环境卫星HJlA超光谱成像仪在轨辐射定标及光谱响应函数敏感性分析

环境卫星HJIA搭载的超光谱成像仪HSI是我国第一个对地观测的星载高光谱传感器,针对超光谱成像仪缺乏各通道光谱响应函数这一问题,对传统的反射率基法予以改进,提出一种不使用光谱响应函数的场地定标方法.利用敦煌场地2009年8月定标实验数据,实现超光谱成像仪在轨辐射定标.通过构建不同形状的光谱响应函数,分析光谱响应函数形状对最终辐射定标结果产生的误差.结果表明,利用新提出的场地定标方法可以实现超光谱成像仪绝对辐射定标,除水汽和氧气吸收通道外,光谱响应函数对定标结果的影响小于3%,采用新定标方法得到的定标系数可以满足应用的需求.