蒙特卡罗模拟光通过大气后的时间分布

采用蒙特卡罗方法模拟了光通过光学特性参数不同的大气后透射光时间分布.分析了大气的散射系数、吸收系数、不对称因子及折射率对透射光时间分布的影响.结果表明:透射光时间分布曲线存在两个峰,分别对应子弹光与漫射光.各光学参数界定了子弹光、蛇形光、漫射光的大小和时间范围,并从统计模拟的角度解释了折射率大的大气中难以成像的因为.     

Investigation on the flameholding mechanisms in supersonic flows: backward-facing step and cavity flameholder

Abstract  

As effective devices to extend the fuel residence time in supersonic flow and prolong the duration time for hypersonic vehicles cruising in the near-space with power, the backward-facing step and the cavity are widely employed in hypersonic airbreathing propulsive systems as flameholders. The two-dimensional coupled implicit RANS equations, the standard k-ε turbulence model, and the finite-rate/eddy-dissipation reaction model have been used to generate the flow field structures in the scramjet combustors with the backward-facing step and the cavity flameholders. The flameholding mechanism in the combustor has been investigated by comparing the flow field in the corner region of the backward-facing step with that around the cavity flameholder. The obtained results show that the numerical simulation results are in good agreement with the experimental data, and the different grid scales make only a slight difference to the numerical results. The vortices formed in the corner region of the backward-facing step, in the cavity and upstream of the fuel injector make a large difference to the enhancement of the mixing between the fuel and the free airstream, and they can prolong the residence time of the mixture and improve the combustion efficiency in the supersonic flow. The size of the recirculation zone in the scramjet combustor partially depends on the distance between the injection and the leading edge of the cavity. Further, the shock waves in the scramjet combustor with the cavity flameholder are much stronger than those that occur in the scramjet combustor with the backward-facing step, and this causes a large increase in the static pressure along the walls of the combustor.     

甘氨酸燃烧法合成纳米ZnO-MgO及其紫外光发射

利用甘氨酸燃烧法制备了ZnOMgO纳米复合材料,并在不同温度进行热处理.通过X射线衍射、扫描电子显微镜和傅里叶变换红外吸收谱,对其升温过程中的结构变化进行了表征,研究了热处理温度对样品室温光致发光行为的影响.结果表明,复合材料的发光性能与纯ZnO相比有很大改善,经900℃热处理的纳米复合材料,其发射谱由一个强紫外发射带(峰值385nm)构成;当热处理温度低于900℃时,发光强度随热处理温度的升高而增强,进一步将热处理温度升至1000℃时发光强度又明显降低.发光强度主要受ZnO、MgO纳米晶的粒子尺寸、结晶完善程度,尤其是受两相纳米粒子之间相互作用的影响.同时发现选择合适的甘氨酸与硝酸根离子的摩尔比,对改善样品紫外发光特性也很重要.     

线性常微分方程的保线性变换及其应用

研究了线性常微分方程的保线性变换，得到任意两个二阶线性常微分方程等价的条件，并用于求解一类二阶线性变系数齐次常微分方程．对数学物理方法教学中怎样通过适当的变换把给定的二阶线性变系数齐次常微分方程化为可解的方程给出了合理解释。     

Four-wave mixing based 10-Gb/s tunable wavelength conversion in dispersion-flattened microstructure fibers

All-optical wavelength conversion of 10-Gb/s signal based on four-wave mixing is experimentally demonstrated in a 30-m-long dispersion-flattened microstructure fiber with small positive dispersion. For an average pump power of 26 dBm, the conversion efficiency was around -19.5 dB with the fluctuation less than ±1.4 dB, covering a conversion bandwidth of 20 nm. The eye diagram of the converted signal shows good eye opening.     

Coherent Scattering of Light by Bose-Einstein Condensation in a Tight Confinement

We have observed strong scattering of a probe light by dilute Bose-Einstein condensate （BEC） ^87Rb gas in a tight magnetic trap. The scattering light forms fringes at the image plane. It is found that we can infer the real size of the condensation and the number of the atoms by modelling the imaging system. We present a quantitative calculation of light scattering by the condensed atoms. The calculation shows that the experimental results agree well with the prediction of the generalized diffraction theory, and thus we can directly observe the phase transition of BEC in a tight trap.     

二极管泵浦Nd:YAG棒双通放大器技术

二极管泵浦NdYAG棒双通放大器采用两个峰值功率6.5 kW激光泵浦模块作为泵浦源.每个激光泵浦模块由81个二极管激光器组成,NdYAG棒直径为6 mm,Nd掺杂质量分数1%.在两个封装方式和结构一致的激光泵浦模块之间采用光学像传递和插入90°石英旋转片进行退偏补偿.在重复频率400 Hz,谐振腔输出单脉冲能量6 mJ时,双通输出400 mJ,激光器光-光转换效率为12.3%,光束质量4.6,脉宽15 ns.     

基于针孔目标物的调制传递函数测试

为了有效测试物镜或光学系统的调制传递函数，采用CCD自动扫描针孔像，并分析系统及环境对目标像的影响因素；系统通过连续采集多幅目标物图像进行平均后，再减去当时的背景图像进行图像处理，选取包含目标物所有信息的合适积分区域，然后通过子午和弧矢方向的积分得到一维的线扩散函数，再经数据处理后由离散傅里叶变换求模得到较可靠的调制传递函数。结果表明：该方法能够快速测量出被测物镜的调制传递函数。     

CsI(Tl)晶体探测器APD读出的温度效应

对中国科学院近代物理研究所自行生长的铊激活碘化铯闪烁晶体CsI(Tl)光输出及Hamamtsu公司生产的S8664-1010型雪崩光二极管(APD)增益对温度的依赖关系做了系统研究. 结果表明, CsI(Tl)晶体光产额在室温范围内随着温度的增加而增加, 在－2℃—8℃温度范围内的平均温度系数为0.67%/℃, 在8℃—25℃温度范围内的平均温度系数为0.33%/℃. 而对所使用的APD, 其增益在室温范围内的温度系数为－3.68%℃(工作电压400V). APD结合CsI(Tl)晶体在室温下对¹³⁷Cs的662keV γ射线的能量分辨可达5.1%.     

MOD法在双轴织构Ni-W合金基片上制备SrTiO3缓冲层

MOD(金属有机化合物沉积)方法被认为是制备第二代高温超导带材最有应用前景的方法之一。文中采用MOD方法在具有双轴织构的Ni基带上制备SrTiO3薄膜作为高温超导带材的缓冲层,并研究了种子层前驱溶液和退火工艺对SrTiO3薄膜的微观结构及表面形貌的影响。通过这种方法,在Ni-5at.%W基带上获得了具有良好择优取向和表面平整的SrTiO3薄膜。