Numerical analysis of a dual-pass pumping laser with weak absorption

A model for a laser with dual-pass pumping is established, and an equation expressing the mode matching for this structure is presented. Through the numerical analysis of this equation, under the conditions of weak-absorption and effective absorption efficiency, the optimum radius of the pump beam waist as well as the optimum location is fitted to simple formulas, considering the quality of the pump beam, absorption coefficient, and beam waist of the cavity mode.Using these formulas, the laser with dual-pass pumping could be optimized to obtain a high slope efficiency. To test the utility of this model, an Nd:YVO_4 laser with dual-pass pumping and weak-absorption was built and optimized according to the results of the calculation. A good agreement between the results of the calculations and the experiment verified the model and the numerical analysis.     

C@Fe3O4磁性微孔球的制备及性能研究

利用活性炭良好的吸附性能,在低温碳化的基础上碳球液态造孔剂制备C@Fe3O4磁性微孔球,在磁性碳球表面形成大量微孔结构,磁性Fe3O4核心也能起到快速分离的特点.通过制备C@Fe3O4复合材料并对其形貌性能进行分析研究,C@Fe3O4磁性微孔球复合材料对于水中重金属离子及芳香烃分子的吸附性能较好,可在污水净化处理中得以应用.     

基于多分辨率融合距离的低质量星系光谱红移测量方法

星系光谱红移测量是大规模天体光谱巡天项目中的一个重要研究内容,其目的是从在光谱中测量出对应星系由于多普勒效应引起的红移。随着银河系外巡天项目的开展,观测目标距离(红移)越来越远,其星等越来越暗,光谱的质量也随之越来越差,如何能够有效准确地从这些低质量的光谱测量出红移是河外巡天面临的一个重要问题。基于此问题,充分考虑到低质量星系光谱的特点及数据特征,新定义了一种针对低质量巡天光谱数据的多分辨率融合距离,以此为基础提出一种针对低质量星系光谱的红移测量方法。该方法充分结合不同分辨率下光谱的特征,计算距离时首先将模板光谱和待测光谱同时降到多个相同分辨率下,该分辨率下所有波长采样点都计算一个偏差进而得到一个距离,然后将多个分辨率下得到的距离通过加权得到一个融合距离。基于多分辨率融合距离提出的星系红移测量方法,能够有效的解决低质量星系光谱的红移无法准确测量的问题。研究了不同信噪比下红移测量的精度,在信噪比大于5之后,该方法测量准确率可以达到90%以上。大量实验表明,提出的方法在星系光谱质量较低的情况可以非常准确地从中测量出红移,测量误差和红移大小无关,可以很好地应用于大规模巡天数据的星系光谱红移测量中。     

Design of LD in-band direct-pumping side surface polished micro-rod Nd:YVO_4 laser

To diminish the thermal load, two ways, that is, in-band direct pumping and micro-rod crystal, could be adopted at the same time. The efficiency of LD in-band direct-pumping side surface polished micro-rod Nd:YVO_4 laser is numerically analyzed. By optimizing parameters such as crystal length, laser mode radius, pump beam radius, doping concentration and crystal cross-section size, the overall efficiency can reach over 50%. It is found that with micro-rod crystal implemented in the laser oscillator, high overall efficiency LD in-band direct-pumping Nd:YVO_4 laser could be realized. High efficiency combined with low thermal load makes this laser an outstanding scheme for building high-power Nd:YVO_4 lasers.     

Theory of noise in a kilo-Hz cascaded high-energy Yb-doped nanosecond pulsed fiber amplifier

A theoretical analysis of noise in a high-power cascaded fiber amplifier is presented. Unlike the noise theory in low power communication, the noise of a high power system is redefined as the leaked output energy between pulses with coherent beat noise uncounted. This definition is more appropriate for high power usage in which the pulse energy receives more attention than the pulse shape integrity. Then the low power pre-amplifying stages are considered as linear amplification and analyzed by linear theory. In the high-power amplification stages, the inversion is assumed to recover linearly in the time interval between pulses. The time shape of the output pulse is different from that of the input signal because of different gains at the front and back ends of the pulse. Then, a criterion is provided to distinguish the nonlinear and linear amplifications based on the signal-to-noise ratio （SNR） analysis. Then, an experiment that shows that the output SNR actually drops off in nonlinear amplification is performed. The change in the noise factor can be well evaluated by pulse shape distortion.     

227-W output all-fiberized Tm-doped fiber laser at 1908 nm

In this paper, we report that a diode-pumped thulium-doped double clad silica fiber laser can provide powers of up to 227 W at 1908 nm, corresponding to a slope efficiency of 54.3%, and an optical-to-optical efficiency of 51.2%. The output power, to the best of our knowledge, is the highest output at 1908 nm. The beam quality M2 factor is about 1.56. Also discussed in this paper is the dependence of the laser performance on fiber length.     

基于聚合物网络液晶的近红外波段快响应相位调制器

相位型液晶空间光调制技术已经广泛应用于自适应光学、信息光学等领域,然而一直存在着响应速度较低的问题。为了提高相位型液晶空间光调制器的响应速度,采用聚合物网络液晶制备近红外波段亚毫秒响应相位调制器,并对其光散射特性和瞬态响应特性进行了研究。通过降低聚合反应温度并提高紫外(UV)固化照度,可以降低器件的光散射强度,实现较好的相位调制。在此基础上,初步研究了聚合物网络形貌对最大光散射强度的影响。在高电压加载下,聚合物网络的电致伸缩效应会极大降低聚合物网络液晶的响应速度,使其达到秒级,经分析认为通过采用高介电各向异性的液晶材料可以降低阈值电压,提高器件的响应速度。     

SKLOF:一种新的超新星候选范围约减算法

超新星是宇宙学中的“标准烛光”, 其在星系中爆发的概率很低, 是一种特殊、稀少的天体, 只有在大量观测的星系数据中才有机会遇到, 而正处于爆发期的超新星会照亮其整个星系从而在观测获得的星系光谱中具有较明显的特征。但是, 目前已发现的超新星数量相对于大量的天体而言又是非常稀少的, 搜寻它们所用的计算时间成为能否进行后续观测的关键, 因此需要寻找高效率的超新星搜寻方法。对超新星候选范围进行约减的LOF算法的时间复杂度较高, 计算量大, 不适用于大规模数据集。为此通过对LOF算法进行改进, 提出了一种在海量星系光谱中快速约减超新星候范围的新方法(SKLOF)。首先对光谱数据集中离中心点近的数据点进行数据剪枝, 剪掉那些肯定不是超新星候选体的光谱数据对象, 然后利用改进的LOF算法计算剩余的光谱数据的孤立性因子并降序排列进行离群搜索, 最后获得超新星候选体的较小的搜索范围以便进行后续的证认。实验结果表明, 该算法十分有效, 不仅在精确度上有所提高, 而且相比于LOF算法还进一步缩短了算法的运行时间, 提高了算法的执行效率。     

磁驱动飞片的三维数值模拟及分析

磁驱动准等熵加载和超高速飞片发射是一种全新的冲击动力学和高能量密度物理实验加载技术。利用三维磁流体动力学软件,模拟了磁驱动飞片的物理过程,计算得到的飞片自由面速度与实验结果符合较好。通过计算飞片横断面的温度、密度和磁场分布,得到了加载过程中磁扩散速度和飞片的剩余厚度。飞片加载过程中飞片边缘的卷曲变形严重,分析认为是由电流和磁场分布的不均匀导致飞片边侧受斜上方较大的加载力所致,并且电流分布的不均匀是主要因素。实验设计时,可利用极板构型的变化调节加载面的电流分布,从而提高飞片的平面性,减小边侧的卷曲变形。     

成像型速度干涉仪散斑成因的研究

在冲击波过程中,利用成像型速度干涉仪探测样品自由面的速度时,散斑的叠加使得干涉曲线被严重干扰,影响了速度信息的精密提取。在理论上从光路的角度分析了系统中可能造成散斑的两种因素:靶面粗糙度和多模光纤。在实验上设计了三种照明方式分别对这两种因素进行验证。离线实验的结果表明,多模光纤的引入对散斑的产生起了主要的作用,这对抑制乃至遏制散斑的产生具有很好的指导性意义。