硅中离子注入硼的异常扩散

本工作用不同的Si~+预注入能量,改变注入损伤分布与离子注入硼杂质分布的相对位置,观察快速热退火中注入损伤对硼异常扩散的影响.结果表明,引起注入硼异常扩散的是点缺陷,而不是硼间隙原子的快扩散.而注入损伤中的点缺陷和簇团分解释放的点缺陷是驱动硼异常扩散的因素之一.如果注入损伤形成了扩展缺陷,那么扩展缺陷重构和分解将发射点缺陷,这是驱动硼异常扩散的另一个因素.     

Widely and continuously tunable optical parametric generator based on MgO-doped periodically poled LiNbO3 crystal

A widely and continuously tunable optical parametric generator (OPG) pumped by a 1064-nm acoustooptically Q-switched diode-end-pumped Nd:YAG laser based on MgO-doped periodically poled LiNbO3 crystal with a multigrating structure (29.2-30.4 μm) is reported.A broad continuous signal spectrum of 1513-1700 nm is obtained by changing the crystal grating periods from 29.2 to 30.4μm and by tuning the crystal temperature from 30 to 180 ℃ simultaneously.When the average pump power is 1.82 W with pulse duration of about 70 ns operating at a repetition rate of 10 kHz,the maximum signal output power of the periodically poled MgO-doped lithium niobate (PPMgLN) OPG is about 210 mW corresponding to the idler and total powers of 118.4 and 328.4 mW respectively.     

n—型聚乙炔复合膜电极性能的研究

自MacDiarmid等将聚乙炔(PA)做为二次电池的电极材料以来,其电化学特性和行为引起了人们的极大兴趣.随后的研究表明,p-型PA[(CH)~(y )Ay~-]_x在电解液中不稳定,用ClO_4~-掺杂的PA充放循环时有降解发生.n-型PA[My~ (CH)~(y-)]_x(y≤0.10)在THF/LiClO_4电解质中较稳定,电化学还原完全可逆,目前已实现1100次充放循环.因此,它既可做电池的正极材料(碱金属为负极),又可做负极材料(TiS_2为正极).我们发现     

非自持和非麦氏分布情况下托卡马克堆芯等离子体功率平衡

本文给出一组托卡马克堆芯等离子体功率平衡方程,它描述了在非自持和非麦氏分布情况下等离子体功率平衡的问题,计算结果表明。在现实可行的聚变堆工程和相应的等离子体参数情况下,堆芯中每秒可产生聚变中子PN大于10~19。     

Nearby source interpretation of differences among light and medium composition spectra in cosmic rays

Recently the AMS-02 reported the precise measurements of the energy spectra of medium-mass compositions (Neon, Magnesium, Silicon) of primary cosmic rays, which reveal different properties from those of light compositions (Helium, Carbon, Oxygen). Here we propose a nearby source scenario, together with the background source contribution, to explain the newly measured spectra of cosmic ray Ne, Mg, Si, and particularly their differences from that of He, C, O. Their differences at high energies can be naturally accounted for by the element abundance of the nearby source. Specifically, the abundance ratio of the nearby source to the background of the Ne, Mg, Si elements is lower by a factor of ∼ 1.7 than that of the He, C, O elements. Such a difference could be due to the abundance difference of the stellar evolution of the progenitor star or the acceleration process/environment, of the nearby source. This scenario can simultaneously explain the high-energy spectral softening features of cosmic ray spectra revealed recently by CREAM/NUCLEON/DAMPE, as well as the energy-dependent behaviors of the large-scale anisotropies. It is predicted that the dipole anisotropy amplitudes below PeV energies of the Ne, Mg, Si group are smaller than that of the He, C, O group, which can be tested with future measurements.     

Effect of boundary layer losses on 2D detonation cellular structures

We evaluate the effect of boundary layer losses on two-dimensional H2/O2/Ar cellular detonations obtained in narrow channels. The experiments provide the details of the cellular structure and the detonation speed deficits from the ideal CJ speed. We model the effect of the boundary layer losses by incorporating the flow divergence in the third dimension due to the negative boundary layer displacement thickness, modeled using Mirels’ theory. The cellular structures obtained numerically with the resulting quasi-2D formulation of the reactive Euler equations with two-step chain-branching chemistry are found in excellent agreement with experiment, both in terms of cell dynamics and velocity deficits, provided the boundary layer constant of Mirels is modified by a factor of 2. A significant increase in the cell size is found with increasing velocity deficit. This is found to be very well captured by the induction zone increase in slower detonations due to the lower temperatures in the induction zone.     

基于飞秒激光引导高压放电的SF6分解物原位检测

气体绝缘开关设备(GIS)绝缘缺陷引发的放电会导致SF₆分解,分解产生的低氟硫化物与设备内的微量H₂O和O₂反应生成具有腐蚀性的物质,影响设备正常运行,因此,研究SF₆分解机理对GIS的安全运行具有重要意义。由于部分分解物在采样过程中发生转化,因此,实现SF₆分解物的原位检测对于研究SF₆分解机理是十分必要的。采用飞秒激光引导高压放电实现了高压放电空间和时间的精确控制,并利用飞秒激光引导高压放电产生的空间分辨光谱实现了SF₆分解物的原位测量。首先研究证明了飞秒激光不会引起SF₆的分解;其次,利用飞秒激光产生的等离子体通道实现了放电空间和时间的精确控制;最后,发现分解物中包含由于高能电子碰撞直接或间接产生的大量S和F的离子和原子。研究证明了基于飞秒激光引导高压放电可以实现SF₆分解物的原位检测,为开展高压放电下SF₆分解机理研究提供了一种新的研究手段。     

基于非线性最小二乘法的多光谱拟合程序：应用于12CH4谱线参数分析

精确的甲烷分子实验光谱参数在大气科学和天文探测等领域有着广泛的应用,特别是谱线的展宽系数及其温度依赖系数对于甲烷分子浓度廓线的研究尤为重要。精密的实验测量是获得准确谱线参数的重要手段。采用实验测量获取谱线参数时,需要在已知实验条件（浓度,温度,总压力,吸收光程以及气体分子种类的混合比等）的情况下,多次扫描同一波段范围得到多组实验室吸收光谱,然后利用基于非线性最小二乘法的拟合程序处理这些光谱,反演获得所需要的光谱参数。然而,一般常用的单光谱拟合程序处理实验光谱既费时又容易引起拟合过程中的误差传递。针对此问题,采用最小二乘拟合技术和Levenberg-Marquardt迭代算法编写了一款适用于处理由可调谐半导体激光吸收光谱技术（TDLAS）所获得的吸收光谱的多光谱拟合程序。该程序可同时处理多张实验光谱,并基于全局拟合方法获得一套光谱参数。详细介绍了该程序的原理、使用方法及数据处理过程。利用多光谱拟合程序中的Voigt线型处理了2 958～2 959 cm-1波数内甲烷（12CH₄）分子6条跃迁谱线的实验光谱,获得了296.0,251.0,223.0,198.0和173.0 K共5组温度下12CH₄分子6条谱线的空气展宽系数。与之前文献报道的该波段内采用单光谱拟合程序得到的相应数据对比结果表明：获得的各温度下的空气展宽系数与参考文献中相应数据差值的百分比处在-4.97%~1.58%之间,两者数据整体符合较好,并且在30组对比数据中,有4组由单光谱拟合程序得到的空气展宽系数的误差值小于由多光谱拟合程序得到的相应数值,有2组数据显示由两种方法获得的误差值相等,其余24组由多光谱拟合程序获得的数据拟合误差小于由单光谱拟合程序获得的相应数值,表明多光谱拟合程序具有良好的可靠性,适用于气体分子吸收光谱的处理。     

HL-2M 装置烘烤系统管路应力的仿真分析与优化

根据 HL-2M 装置烘烤系统管路设计,建立烘烤系统的管道应力计算模型。对烘烤系统管路作初始 支架设计,并采用系统内的最高温度分布,对烘烤系统进行热应力计算,分析管道应力及设备管口载荷。以热应 力计算结果为依据,对管路布置进行优化,并改善支架的设计,对烘烤系统进行应力校核计算,完成烘烤系统可 靠性验证计算,完成了管口位移量计算。