弱光波前传感器质心计算的新方法

 研究了Shack Hartmann波前传感器质心计算的新方法,即最小二乘高斯拟合方法。分析了Shack-Hartmann波前传感器采用一阶矩质心计算位置方法对光斑强度的敏感性,与最小二乘高斯拟合方法进行了比较,并对Shack Hartmann波前传感器的子孔径波前斜率探测的正确性进行了分析。最后的计算结果表明最小二乘高斯拟合法计算子孔径光斑的质心位置可以减小质心探测的误差。     

介质中双缺陷电荷对碳纳米管场效应晶体管量子输运特性的影响

用非平衡格林函数理论和紧束缚模型近似计算长沟道弹道输运p型碳纳米管场效应管中电流强度.研究当场效应管介质（SiO₂）中存在两个带电缺陷时，载流子散射所引起的电流强度减小和栅极阈值电压偏移量与缺陷位置的关系.介质中两个缺陷所带电荷Q₁=Q₂=+e（-e为电子电荷），都靠近源极或者都靠近漏极，或者一个电荷靠近源极另一个电荷靠近漏极.在工作状态下，所引起的电流强度相对减小比介质中只存在单个正电荷Q=+e且靠近源极（或漏极）时所引起的电流强度相对减小大得多.如果两个正电荷都在沟道中央附近，随着两个电荷的轴向距离减小，栅极阈值电压偏移的绝对值明显增加.栅极阈值电压偏移可达到-0.35 V.     

掺铒光纤中方波信号高次谐波的快慢光特性

光纤中方波信号的慢光技术在全光通信和光纤传感等领域具有重要的应用前景. 提出了谐波相对延时量的度量方法, 分别采用速率方程和相干布居振荡理论, 对掺铒光纤中方波信号的基波和高次谐波的快慢光特性进行了研究. 在无抽运光输入情况下, 改变入射光功率, 入射探测光的基波最大相对延时量能达到20%, 且存在实现最大相对延时量的入射光功率为8 mW; 在有抽运光输入的情况下, 改变信号光增益, 入射探测光的基波相对超前量同样能达到-20%, 且随着信号光增益的增大而增加. N次谐波(N=1, 3, 5, 7, …)在频率f/N(f为基波信号最大延时量对应的调制频率)处有最大相对延时量, 且它们的最大延时量相同, 频率处于相干布居振荡引起的光谱烧孔带宽内.     

基于优化探测窗口的光斑质心探测方法

哈特曼-夏克波前传感器进行波前探测时，用子孔径光斑强度的一阶矩来计算光斑质心位置，子孔径窗口作为探测窗口，但探测时子孔径窗口内噪声对一阶矩有很大的影响，会使质心探测精度产生很大的误差。因此在计算质心位置时探测窗口的选取对探测精度有重要影响，必须选取合适的探测窗口来提高光斑质心探测精度。为此，在传统算法的基础上提出优化探测窗口的方法来提高质心探测精度,仿真和实验结果表明新方法提高了质心探测的精度，未经处理的高噪声恢复波前的波前残差峰谷值是2.851 4λ，均方根值是0.606 3λ，优化探测窗口后波前残差的峰谷值是1.636 2 λ，均方根值是0.367 1 λ，重构误差减小了40％。证明了算法的可行性和稳定性。     

用于白天自适应光学的波前探测方法分析

提出了两种视场偏移哈特曼波前传感器，用于探测白天条件下强背景中目标信号的波前信息.给出了哈特曼波前传感器子孔径中焦面上天光背景非均匀性分布特征的实验结果，详细分析了基于分光棱镜的双焦面视场偏移哈特曼波前传感器的探测误差，并通过基于倾斜镜的单焦面视场偏移哈特曼波前传感器实验给出了波前测量的结果，证明视场偏移哈特曼波前传感器能够精确、稳定的测量白天条件下目标信号的畸变波前信息，同时给出了其在白天条件下探测能力的估算结果及其受限因素，估算结果表明云南天文台的自适应光学系统在10 W/m²·sr天光背景条件下应用视场偏移哈特曼波前传感器能对5等星(可视星等值)目标进行准确的波前探测. 关键词： 自适应光学 波前传感器 白天工作 误差分析     

基于优化探测窗口的光斑质心探测方法

 哈特曼-夏克波前传感器进行波前探测时，用子孔径光斑强度的一阶矩来计算光斑质心位置，子孔径窗口作为探测窗口，但探测时子孔径窗口内噪声对一阶矩有很大的影响，会使质心探测精度产生很大的误差。因此在计算质心位置时探测窗口的选取对探测精度有重要影响，必须选取合适的探测窗口来提高光斑质心探测精度。为此，在传统算法的基础上提出优化探测窗口的方法来提高质心探测精度,仿真和实验结果表明新方法提高了质心探测的精度，未经处理的高噪声恢复波前的波前残差峰谷值是2.851 4λ，均方根值是0.606 3λ，优化探测窗口后波前残差的峰谷值是1.636 2 λ，均方根值是0.367 1 λ，重构误差减小了40％。证明了算法的可行性和稳定性。     

两种M~2因子实验测量方法的比较

为了从实验上分析和验证H-S传感器测量M2因子方法,对使用双曲线拟合法测量M2因子和H-S传感器测量M2因子做了详细的实验研究,且对实验结果、实验误差进行了比较与分析。研究表明:当H-S波前传感器透镜组足够多,重构误差较小,选取合适的泽尼克多项式阶数时,H-S波前传感器一次测量法得到的光束的M2因子与传统方法测得的M2因子值基本相当。与双曲线拟合法相比,H-S传感器法适用范围小,但是当满足测量条件时,H-S传感器法更便捷。     

电子倍增CCD的电荷倍增特性研究

建立了电子倍增CCD的载流子倍增寄存器的电荷倍增模型,分析了电子倍增CCD的结构特征和载流子倍增寄存器的工作原理及其电荷倍增特性.利用Z域分析方法得到载流子倍增寄存器的电荷倍增传递函数及其幅频响应.计算表明,提高载流子倍增寄存器的电荷倍增系数可以提高电子倍增CCD的幅频响应.同时,用增益起伏因子来分析载流子倍增寄存器的增益起伏特性,得到了电荷倍增率,寄存器级数与增益起伏因子的数值关系.在寄存器级数N=400条件下,当电荷倍增系数α≤0.15时,增益起伏因子随电荷倍增系数增大而增大;而当α≥0.15时,增益起伏因子随电荷倍增系数的增大而减小.通过典型的电子倍增CCD相机的实验验证了建立的模型.     

LiF插层对有机发光二极管磁场效应的调控

制备了有LiF插层的有机发光二极管,以八羟基喹啉铝（Alq₃）作为电子传输层,N, N′-二苯基-N, N′-二(1-萘基)-1,1′-联苯-4,4′-二胺（NPB）作为空穴传输层.通过改变Alq₃与NPB间LiF插层的厚度,研究了不同温度下器件的光电特性及电致发光的磁场效应.测量结果表明:LiF插层可以影响器件内部载流子的输运和激发态的形成.较厚的插层阻碍了空穴的传输,使器件的电流效率变低.但实验中发现, 关键词： LiF插层结构 磁场效应 三重态激子     

实际大气湍流下弱光信标Shack-Hartmann波前传感器的波前斜率探测误差

 深入分析了Shack-Hartmann 波前传感器（S-H WFS）在实际大气湍流条件下弱光信标波前斜率的探测误差,导出了定量分析的数学模型。分析结果表明,当S-H WFS用于弱光信标（光子受限）湍流波前斜率的探测时,除了信标光起伏和探测器噪声外,大气强度闪烁、天空背景光等因素会增加探测误差,并且随着探测信标与天空背景光的对比度的下降,质心探测误差会随着孔径到达角起伏的增加而增加。     

用H-S波前传感器测量穿过超声速流场的激光像差特性

 用Hartmann-Shack(H-S)波前传感器可以准确测量穿过超声速流场的激光波面及其变化过程,进一步计算可以获得光束质心漂移、远场分布等数据。给出了H-S方法测量穿过超声速流场激光波面的原理,采用模式法进行了波前重构,计算了在几种流场条件下的激光波面像差特性PV值,RMS值和Zernike像差系数、Strehl比和环围能量曲线等。结果表明,H-S法可以很好地反映流场建立、稳定和结束过程中Zernike像差的变化。比较无流场和给定参数的超声速流场,激光穿越后产生的最明显的像差变化为离焦和低阶像散的增大。在相同流场参数下,无模型时光束质量好于有模型时光束质量。     

Performance analysis of field-of-view shifted Shack–Hartmann wavefront sensor based on splitter

We report on a field-of-view shifted Shack–Hartmann wavefront sensor based on a splitter designed to measure the wavefront information of object light with strong background. The analysis results indicate that increasing the ratio of the signal beam intensity to the incoming beam intensity and reducing the sampling frequency of CCD₂ (detecting the pure background light) can properly enhance the SNR (signal-to-noise ratio) of the object light. A special noise removing algorithm was presented to enhance the centroid measuring accuracy, and it was proved to be effective against the residual noises caused by the differences between the two beam paths. The experimental results indicate that the field-of-view shifted Shack–Hartmann wavefront sensor based on a splitter can exactly measure the wavefront information from the object with strong background. PACS 42.68.Bz; 47.50.Ef; 42.30.Wb     

夏克-哈特曼波前传感器的波前相位探测误差

对夏克－哈特曼（Ｓｈａｃｋ－Ｈａｒｔｍａｎｎ）波前传感器的相位探测误差进行了分析,并分析了它的政论相位探测极限,分析结果表明,夏克－哈特曼波前传感器的相位探测精度与探测器的噪声水平,探测目标的亮度有关,还与被探测对象的特性、孔径波前分割有关。给出了它们的关系表达式。     

Electron spin resonance study of oxygen-17 enriched N,N-dimethyl-4-nitroaniline radical anion

N,N-Dimethyl-d₆-4-nitroaniline enriched to approximately 11 atom. per cent in oxygen-17 has been prepared and the oxygen-17 isotropic hyperfine interaction in the corresponding radical anion has been examined. In dry dimethylformamide solution we find a _O = -8·85 ± 0·02 and a _N = 11·39 ± 0·10 gauss, while in moist acetonitrile solution a _O = -8·82 ± 0·07 and a _N = 12·23 ± 0·11 gauss. These results substantiate the recent suggestion that the isotropic oxygen-17 splittings in π-radicals may be described by a single parameter equation analogous to McConnell's relation for aromatic proton splittings, i.e. a _O = Q _OρO ^π, where Q _O = -41 ± 3 gauss.     

Accuracy analysis of centroid calculated by a modified center detection algorithm for Shack-Hartmann wavefront sensor

The accuracy of the Shack-Hartmann wavefront sensor for measuring the wavefront distortion is mainly dependent upon the measuring accuracy of the centroid of each spot. A modified center detection algorithm, which uses some power from the photon events of each pixel instead of photon events themselves, is analyzed theoretically and the computer simulations are given. The results show that photon noise error and sampling error increases as the power value goes up; and to some powers, the readout noise and background noise error decrease. An experiment is described through which the optimum power can be obtained.     

The N-mode squeezed state with enhanced squeezing

It is known that exp [iλ (Q1P1i/2)] is a unitary single-mode squeezing operator,where Q1,P1 are the coordinate and momentum operators,respectively.In this paper we employ Dirac’s coordinate representation to prove that the exponential operator S n ≡ exp [iλ sum((QiPi+1+Qi+1Pi))) from i=1 to n ],(Qn+1=Q1,Pn+1=P1),is an n-mode squeezing operator which enhances the standard squeezing.By virtue of the technique of integration within an ordered product of operators we derive S n ’s normally ordered expansion and obtain new n-mode squeezed vacuum states,its Wigner function is calculated by using the Weyl ordering invariance under similar transformations.     

Temperature Effects on the Performance of On-Chip Spiral Inductors Used in RF(MM)ICs

Based on the measured S-parameters and proposed circuit model for on-chip spiral inductors, the overall effects of temperature rise on the inductor performance are examined in this paper. For circular spiral inductors on silicon substrates, it is shown that when the temperature increases from 25°C to 85°C, the peak values of Q-factor (Q _max) of these inductors, corresponding to the turn number N = 3 to 7, decrease about 8.8% to 19%, respectively. The metal trace and silicon substrate resistances both increase linearly with temperature, while the capacitance of silicon substrate has a negative temperature coefficient. For a square spiral inductor on GaAs substrate, its Q _max decreases about 37.2% as temperature increases from 25°C to 185°C. The corresponding frequency f _max tends to shift from 9.44GHz to 7.73GHz, and it is reduced about 18.1%.     

Numerical study of centroid detection accuracy for Shack-Hartmann wavefront sensor

It is crucial for the wavefront sensor to reduce the influence of noise and enhance the detection accuracy of the centroid, which is also an important step for improving the performances of adaptive optics. In this paper, based on the theoretical analysis and by utilizing the Monte-Carlo simulation (MCS) technology, the results obtained by using the centroid algorithms have been compared in detail for the case, in which centroid of the signal is not at the center of the detection area and it also has a relatively large area. It is shown that the size of the signal spot and its centroid position have considerable influences on the centroid detection accuracy. The numerical results agree well with the theoretical predictions and the optimized parameters for each algorithm have been found. The study will be helpful for further optimizing the optical system and improving the centroid measurement accuracy of the wavefront sensor.     

两种自适应光学系统中哈特曼波前传感器与变形镜的对准误差

利用直接波前斜率法和变形镜的电压一面形响应特性，研究了常规自适应光学系统和共光路／共模块(CP／CM)自适应光学系统中哈特曼波前传感器与变形镜的对准误差。常规自适应光学系统中，可以用重新测量变形镜的影响函数以减小对准误差的影响，虽并不能消除其影响，但系统都会有很大的调整容差；共光路／共模块自适应光学系统中采用不同的双哈特曼数据处理方法，哈特曼波前传感器与变形镜的对准精度对系统校正能力影响是不同的，采用加修正因子斜率融合法和电压融合法由于在数据融合时考虑了两台哈特曼传感器与变形镜对准的差异，所以对准误差的影响与在常规自适应光学中相同，系统都会有很大的调整容差，而采用直接斜率融合法的共光路／共模块系统由于是建立在两台哈特曼传感器完全一致的假设基础上，所以对对准精度的要求是很高的。分析过程中给出了相应的数值计算结果。