采用新型谐振腔镜的高效可调谐波光器

采用波长变以反射率镜作为可调谐激光器谐振腔的输出镜,大大提高了可调谐激光器的整体运转效率和时间特性参数。     

不同谐振腔分步合成法制备的固态染料P567可调谐激光器

利用新型分步合成法制备的激光染料P567掺杂有机改性凝胶玻璃,建立了基于全息光栅的两种不同腔型可调谐激光器.采用光栅零级作为输出的激光器,调谐范围近70nm (543～610nm), 获得的最高斜效率为17%;采用腔镜耦合输出方式,调谐范围超过30 nm (553～585 nm),获得的最高斜效率为9.7%.并对激光器的可调谐范围、阈值、斜效率及线宽等参数进行了深入的分析比较.     

基于光纤平移的窄线宽可调谐Er3+/Yb3+共掺光纤激光器

针对输出耦合镜旋转调谐时输出光束方向变化问题,设计了一种光纤位置平移、而调谐输出光束方向不变的光纤激光器系统。运用光栅方程,分析了光纤平移的调谐机理;采用输出与反馈光束耦合模型,分析了输出增益线宽随光纤位置、光束半径的变化。理论分析表明:该光纤激光器可获得线宽小于0.2 nm的调谐激光输出。实验结果表明,该激光器在波长为1543.446 nm处获得的调谐输出功率最大,达到470 mW,计算的斜率效率为23.9 %;整个调谐区域达到36 nm,调谐范围内激光的3 dB线宽小于0.08 nm。     

48-波长线形腔多波长掺铒光纤激光器

采用两个光纤环镜作为腔镜构成线形腔可调谐多波长掺铒光纤激光器.将铒光纤浸入77 K的液氮中,选择可调谐光纤环镜作为输出腔镜,利用Mach-Zehnder干涉仪的滤波特性和输出端光纤环镜反射率的宽带可调特性,获得了波长间隔～0.4 nm、最大波长数目48个的多波长激光的稳定输出,同时实现了在1525～1555 nm范围内,多波长激光运转区域的灵活调节.     

波长无啁啾调谐窄线宽掺Yb3+双包层光纤激光器

用相位掩模法, 在圆形掺Yb3+双包层光纤上制作了Bragg光纤光栅,并用它作为双包层光纤激光器的输出腔镜, 在光栅反射中心波长1055.2 nm位置得到了窄线宽的激光输出, FWHM为0.271 nm, 信噪比约为40 dB.这种结构的双包层光纤激光器, 在双包层增益光纤和后腔镜间没有连接损耗, 减小了双包层光纤激光器体积. 用自行制作的等强度梁对作为输出腔镜的光纤光栅做双向应力调谐, 实现了激光波长无啁啾调谐输出, 调谐范围1051.1~1060.04nm,调谐量达8.9nm, 调谐过程中激光3 dB线宽基本无变化.     

8字形腔波长可调谐锁模脉冲光纤激光器

采用非线性光纤环形镜加脉冲锁模技术及可调谐光纤光栅滤波器,对8字形腔被动锁模掺铒光纤激光器进行了波长可调谐输出的实验研究.在EDFA抽运光功率一定的情况下,通过调节偏振控制器和可调谐光纤光栅滤波器,获得了光谱稳定、重复频率1.1 MHz、输出功率起伏小于0.8 dBm、中心波长在1 548~1 570 nm内连续可调的短脉冲输出.该激光器可实现自启动锁模,且长时间稳定工作无需任何调整.     

小型可调谐单纵模TEA CO2激光器

对在三镜腔中插入法布里-珀罗(F-P)标准具实现单纵模激光输出的方法进行了分析,计算了激光器的输出特性。设计研制了一台单纵模可调谐TEA CO2激光器。采用在三镜腔中插入F-P标准具的方法实现了单纵模激光的调谐输出。当激光器以5 Hz重复频率运转时,得到9P(16)谱线能量大于200 mJ,脉冲宽度约为150 ns。     

1μm波段宽带可调谐锁模光纤激光器

报道了一种工作于1μm波段、正常色散区、基于半导体可饱和吸收镜(SESAM)的被动锁模光纤激光器。激光器以高掺杂Yb光纤为增益物质,结合可调谐滤波器,形成环形腔结构。采用976nm半导体激光器抽运,当抽运功率大于16dBm时,激光器可实现1033～1069nm波长范围内重复频率为25.4MHz的宽带可调谐输出,性能稳定,在调谐范围内均可观测到非常规则的矩形输出光谱。在固定抽运功率下,对调谐范围内输出功率、光谱带宽、时域脉宽进行了实验测量和分析。在波长为1064nm时,用单通道光栅对将谱宽为1.745nm、时域脉宽为34.85ps的脉冲压缩至15.45ps。     

增益开关型Ti~(3+):Al_2O_3对激光器的时间特性研究

本文报道增益开关型Ti~(3+) :Al_2O_3激光器输出脉冲的时间特性;给出激光器在宽带输出及调谐工作状态下,输出脉冲的时间特性曲线.实验中获得最小的脉宽为1.2ns.在一定的实验条件下,脉冲宽度可在5～27.5ns范围内连续变化.在调谐状态下,用一输出耦合镜得到波长可调谐范围为730～850nm.用三块棱镜作调谐器,在中心波长780nm处,最大输出能量为4.7mJ,谱线宽度为0.13nm(FWHM).     

环形腔声光可调谐掺铒光纤激光器调谐范围的研究

介绍了一种基于声光可调谐滤波器(AOTF)的可调谐掺铒光纤激光器。从掺铒光纤放大器的速率方程和传输方程出发,推导出声光可调谐掺铒光纤激光器的输出公式,理论上解释了该环形腔声光可调谐掺铒光纤激光器调谐范围仅决定于掺铒光纤的增益带宽;并在实验中测得该激光器调谐范围为1 526.05 nm到1 560.63 nm,这个区间对应着实验所得掺铒光纤自发辐射谱的增益区间,从而验证了理论推导所得结论。     

A dynamic phase-conjugate mirror based on CdF<Subscript>2</Subscript> crystals with bistable centers

A four-wave phase-conjugate mirror on reflection gratings recorded in a CdF₂ crystal with bistable centers has been studied experimentally. The mirror reflectivity and speed have been measured, and the coefficient of third-order nonlinearity of this medium has been estimated. The quality of the wave reflected from the phase-conjugate mirror has been investigated in model experiments.     

畸变波前相位校正效果分析

 以随机相位屏构造波前畸变相位,运用高通滤波的方法模拟变形镜对光束波前畸变相位的校正作用,模拟分析了畸变波前的相位校正效果,定量分析了校正效果与低频相位畸变和高频相位畸变之间的关系,并进一步讨论了变形镜的校正位置对校正效果的影响。研究结果表明:对于给定单元尺寸的变形镜,随着畸变波前中高频相位畸变所占比例的增大,经校正后的远场光束质量明显降低,校正效果也越来越差。此外,光学变形镜所在位置对校正效果存在明显影响,校正效果随校正位置的变化呈现出起伏变化。     

Investigation of the First Mirror on Tokamak

The study progress of NNSF in 2006 has been presented in this paper. The aim and plan of this item have been described briefly. Three test mirror exposure experiments have been done in this year. The main components of the deposited materials on the first mirror are carbon and iron analyzed by AES. The first mirror is polluted easier during glow discharge and wall processing than omhic discharge.     

Thermal lens compensation by convex deformation of a flat mirror with variable annular force

An optical surface with convex parabolic shape over a large area has been created using a 12.7-mm-diameter annular pusher to deform a flat 25.4-mm-diameter mirror. The deformable mirror assembly has been modeled using finite element analysis software as well as analytical solutions. The measured parabolic surface deformation shows good agreement with those models. Mirror performance was studied using a Shack–Hartman wavefront sensor and the mirror has been applied to compensate thermal lensing in a Nd:YAG rod amplifier. PACS 41.85.Ct; 42.60.Da     

Do magnetic fields prevent mirror particles from entering the galactic disk?

Recently it has been suggested that magnetic fields prevent mirror particles from entering the galactic disk, thereby disfavouring the mirror dark matter explanation of the dark matter direct detection experiments. We show that mirror particle self interactions will typically randomize the directions of heavy mirror particles on length scales much shorter than their gyroradius. This means that heavy mirror particles are free to enter the galactic disk and consequently mirror dark matter remains consistent with all experiments and observations.     

X-ray tomographic image of a deposit on a spherical surface

A method has been developed to obtain two-dimensional X-ray tomographic images of deposit objects located on bent mirror surfaces. A procedure that makes it possible to obtain two-dimensional X-ray image of an object (fingerprint) located on the surface of a spherical mirror has been proposed and experimentally implemented. Mathematical algorithms for reconstructing images have been developed.     

镜面莫尔轮廓法

提出镜面莫尔轮廓法的光路配置方法。提供了镜面所形成条纹的计算公式的推算原理。拍摄了斜镜面、柱形镜面的莫尔轮廓条纹照片,判读结果与本文提供的理论公式的计算结果比较一致。     

基于激光平面镜反射的长度测量仪的理论设计

给出了利用小型激光器和平面镜测量长度的基本原理,测量长度及其不确定度与平面镜转动角之间的关系,并例举了有关理论计算和分析．讨论了设计长度测量仪的注意事项．该长度测量仪可用于大学、中学物理实验教学和一般的长度测量．     

Φ1.2m球面镜支撑的力学分析和试验研究

通过使用有限元软件对大镜面进行模拟计算和分析,可以预先确定加工和装校支撑方法是否符合设计要求,从而有效地减少了设计的盲目性。分析计算了口径为1 2m的球面镜在不同工况下的受力变形。按选择的支撑和检验方式进行了装校试验,实际的球面镜检验结果验证了分析的正确性。     

Dynamical Casimir effect in superradiant light scattering by Bose–Einstein condensate in an optomechanical cavity

We investigate the effects of dynamical Casimir effect in superradiant light scattering by Bose-Einstein condensate in an optomechanical cavity. The system is studied using both classical and quantized mirror motions. The cavity frequency is harmonically modulated in time for both the cases. The main quantity of interest is the number of intracavity scattered photons. The system has been investigated under the weak and strong modulations. It has been observed that the amplitude of the scattered photons is more for the classical mirror motion than the quantized mirror motion. Also, initially, the amplitude of scattered photons is high for lower modulation amplitude than higher modulation amplitude. We also found that the behavior of the plots are similar under strong and weak modulations for the quantized mirror motion.