Stark broadening of Y III spectral lines

Using a semiclassical approach, we have considered electron-, proton-, and ionized helium-impact line width and shifts for 32 Y III multiplets. Published in Zhurnal Prikladnoi Spektroskopii, Vol. 65, No. 4, pp. 476–481, July–August, 1998.     

Stark broadening of In III, Tb III, and Pb IV spectral lines

Using a semiclassical approach, the authors consider the widths and shifts of spectral lines for twenty In III and two Tl III multiplets initialed by collisions with electrons, protons, and ions of helium at a density of the perturbing particles of 10¹⁷ cm⁻³ and temperatures from 20,000 to 500,000 K. For two Pb IV multiplets, the widths and shifts of spectral lines produced by collisions with electrons, protons, and ions of He III at a density of the perturbing particles of 10¹⁷ cm⁻³ and temperatures from 50,000 to 1,000,000 K are considered similarly. Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 66, No. 6, pp. 753–757, November–December, 1999.     

光场的非傍轴性对光谱移动和光谱开关的影响

利用瑞利衍射积分公式，推导出多色高斯光束被硬边光阑衍射后光谱的解析公式，傍轴近似的光谱公式可作为特例得到.着重研究了束腰宽度与中心波长之比w₀/λ₀和截断参数δ对光谱移动和光谱开关的影响.结果表明，只有当w₀/λ₀和δ满足一定条件时，傍轴近似结果才与非傍轴结果一致.光场的非傍轴性会引起光谱移动不同和产生光谱开关的临界位置变化. 关键词： 非傍轴光场 高斯光束 光谱移动 光谱开关     

极性染料溶液的微微秒动态荧光光谱移位

本文测量了染料分子DCM、甲酚紫、DODCI和DTDCI在极性溶剂中的微微秒时间分辨荧光光谱;作者将动态的光谱移位归结为由于溶质分子激发态与基态偶极矩的显著差异而引起的周围溶剂分子的介电弛豫;并从动态的光谱移位得到的弛豫时间很接近由连续腔体理论模型求得的计算值,表明连续胜体模型用于描述动态的光谱移位现象是适用的.     

Quark-antiquark scattering phase shift and meson spectral function in pion superfluid

We study the quark-antiquark scattering phase shift and meson spectral function in the pion superfluid described by the Nambu-Jona-Lasinio model. Meson mixing in the pion superfluid dramatically changes the full scattering phase shift and significantly broadens the spectral function of some collective modes.     

偏振型干涉成像光谱仪谱线位置定标方法的研究

论述了偏振型干涉成像光谱仪的工作原理, 针对复原光谱谱线位置漂移问题, 提出了原理修正和数据处理两种具有代表性的实验室谱线位置定标方法, 给出了定标结果及对比分析. 原理修正方法从干涉型成像光谱仪的参数选择着手, 分析了产生谱线位置漂移的原因, 针对复原谱线位置随行变化的问题, 给出了修正方案, 使得谱线位置精度明显提高; 对于给定的四组激光器标准波长, 谱线位置均方根误差由定标前的28.3914下降至5.5371, 该方法对干涉型成像光谱仪具有普适性, 且其定标参数对分析仪器指标提供了便利. 数据处理方法弥补了原理修正定标存在的数据量大、短波定标效果弱等弊端, 谱线位置均方根误差下降至0.9178, 该方法实施简单, 对不同的输入波长, 所取不同行的数据用统一的表达式进行修正. 该方法化繁为简、间接定标的思想具有一定的借鉴价值. 该研究为偏振型干涉成像光谱仪的设计、研制、调试和工程化提供了重要的理论依据和实践指导.     

Stark broadening of ar VIII spectral lines

Using the semiclassical perturbation method, we consider, for nine Ar VIII transitions, widths and shifts of spectral lines that are due to collisions with electrons, protons, and ions of He III ut a perturbing particle density of 10¹⁸ cm⁻³ and temperatures between 200,000 and 3,000,000 K. Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 67, No. 3, pp. 286–288, May–June, 2000.     

超短脉冲厄米-高斯光束在湍流大气中的光谱移动和光谱跃变

基于广义惠更斯-菲涅尔原理，推导出了超短脉冲厄米-高斯(H-G)光束在湍流大气中的光谱传输方程，研究了其光谱移动和光谱跃变特性，并给予了合理的物理解释.研究表明，超短脉冲H-G 光束通过湍流大气传输其光谱特性由大气折射率结构常数、厄米多项式阶数、脉冲宽度和观察点位置坐标等因素共同决定.轴上点光谱为蓝移，随着离轴距离的增大，光谱由蓝移变为红移，无光谱移动点的位置坐标与脉冲宽度无关.此外，当湍流增强到一定程度时离轴点还存在光谱跃变现象.自由空间与湍流大气中的光谱跃变行为存在很大的差异，本文对此进行了详细的分析. 关键词： 超短脉冲厄米-高斯(H-G)光束 湍流大气 光谱移动 光谱跃变     

Water vapor line width and shift calculations with accurate vibration-rotation wave functions

Calculations of H₂¹⁶O rotation-vibration line broadening and shifting due to N₂ pressure effects are performed using a semi-empirical approach. The calculations are based on impact theory modified by introducing additional parameters to extend the use of empirical data. These model parameters are determined by fitting the broadening and shifting coefficients to experimental data. The method is further developed by using anharmonic wavefunctions in the estimates of the line profiles. The main feature of the present calculation is the use of a complete set of high-accuracy vibration-rotation dipole transition moments calculated for all possible transitions using wavefunctions determined from variational nuclear motion calculations and an ab initio dipole moment surface. This approach explicitly takes into account all scattering channels induced by collisions. Results of these calculations clearly demonstrate improved agreement between observed and calculated parameters for both the line widths and the line shifts.     

Theoretical analysis of collisional shift and broadening of antiprotonic helium spectral lines

Effect of medium density on shift and broadening of ( ) spectral lines is considered in the framework of binary-collision approximation with an effective ( )–He potential including the long-range attraction and short-range repulsion. Quantum calculations of the scattering phase shifts at reasonable values of the potential parameters allow to explain the main features of the observed density effect on the shape of ( ) spectral lines in low-temperature helium. This revised version was published online in August 2006 with corrections to the Cover Date.     

部分相干啁啾光学相干涡旋晶格在生物组织湍流中的平均光强与光谱位移

本文研究了部分相干啁啾光学相干涡旋晶格在生物组织湍流中的平均光强和光谱位移,详细探讨了单色光场中的光学晶格结构和多色光场中的光谱快速跃迁特性.研究表明:在生物组织湍流中,光束从具有涡旋核的环形结构演变为具有暗区的周期阵列结构,最后呈类高斯图样.尽管晶格常数能调制光束结构,但它不影响光束在生物组织湍流中的光谱跃迁行为.光...     

Measurements of N2-broadening and -shifting parameters of the water vapor spectral lines in the second hexad region

The water vapor line broadening and shifting in the ν₁+ν₂+ν₃ band induced by nitrogen pressure are measured with Bruker IFS 125 HR FTIR spectrometer at the spectral resolution of 0.01 cm⁻¹ for the line with upper states angular momentum up to 11. Line contour parameters are calculated using a semi-empirical approach extended by the use of empirical data to determine some fitting model parameters. We use the complete set of high accuracy vibration-rotation dipole transition moments calculated for all possible transitions using wavefunctions determined from variational nuclear motion calculations and an ab initio dipole moment surface. Calculated values of line contour parameters are in a good agreement with observed parameters.     

Experimental investigation of the line center of Hg intercombination spectral line 253.7 nm perturbed by Kr

The collision broadening and shift of the Hg intercombination spectral line 253.7 nm (6¹S₀–6³P₁) perturbed by Kr has been investigated using a high-resolution scanning Fabry–Perot interferometer. The values of the pressure broadening and shift coefficients β and δ, respectively, for the studied line have been obtained. The obtained coefficients β and δ are compared with their corresponding published experimental values and also those calculated using Lindholm–Foley impact theory.     

Ti类氦Kα线在高温稠密等离子体中的漂移

采用离子球模型,通过自洽求解Dirac方程和Poisson方程,得到类氦Ti离子Kα线系的两条电偶极辐射光谱能量随不同等离子体环境的变化关系.同时分析了束缚电子交换能随等离子体环境的变化规律.结果表明：光谱能量漂移量随等离子体电子密度变化呈现出很好的线性关系.对此,拟合得到Ti类氦Kα线光谱能量漂移量随等离子体环境参数变化的公式,对探索高温高密度等离子体诊断方法具有一定意义. 关键词： 类氦离子 自洽场离子球模型 光谱漂移 等离子体诊断     

Six-bit all-optical quantization using photonic crystal fiber with soliton self-frequency shift and pre-chirp spectral compression techniques

In this paper,we propose an optical quantization scheme for all-optical analog-to-digital conversion that facilitates photonics integration.A segment of 10-m photonic crystal fiber with a high nonlinear coefficient of 62.8 W 1/km is utilized to realize large scale soliton self-frequency shift relevant to the power of the sampled optical signal.Furthermore,a 100-m dispersion-increasing fiber is used as the spectral compression module for further resolution enhancement.Simulation results show that 317-nm maximum wavelength shift is realized with 1550-nm initial wavelength and 6-bit quantization resolution is obtained with a subsequent spectral compression process.     

紫铜等离子体特征谱线及其展宽形成机制

利用波长为1064 nm,最大能量为500 mJ的 Nd:YAG脉冲激光器对紫铜进行冲击,并且改变激光能量,获得一系列等离子体特征谱线,结果表明:本实验条件下,获得铜原子谱线不完整,只有5条明显激发谱线,分别为:CuⅠ 406.33 nm, CuⅠ 458.69 nm, CuⅠ 521.8 nm, CuⅠ 529.25 nm, CuⅠ 578.2 nm。根据跃迁原理,得出激光不能使铜原子完全受到激发;选取CuⅠ 521.8 nm原子光谱与CuⅠ 578.2 nm的原子光谱谱线线型作为分析对象,发现其展宽线型不同,分别为Lorenz线型与Gauss线型。通过对应线型曲线方程分析得出,同一原子光谱不同波段对应形成光谱展宽机制不同。     

紫铜等离子体特征谱线及其展宽形成机制

利用波长为1064 nm,最大能量为500 mJ的 Nd：YAG脉冲激光器对紫铜进行冲击,并且改变激光能量,获得一系列等离子体特征谱线,结果表明：本实验条件下,获得铜原子谱线不完整,只有5条明显激发谱线,分别为：CuⅠ 406.33 nm, CuⅠ 458.69 nm, CuⅠ 521.8 nm, CuⅠ 529.25 nm, CuⅠ 578.2 nm。根据跃迁原理,得出激光不能使铜原子完全受到激发;选取CuⅠ 521.8 nm原子光谱与CuⅠ 578.2 nm的原子光谱谱线线型作为分析对象,发现其展宽线型不同,分别为Lorenz线型与Gauss线型。通过对应线型曲线方程分析得出,同一原子光谱不同波段对应形成光谱展宽机制不同。     

Stark Broadening of Ne II and Ne III Spectral Lines

Using a semiclassical approach, the widths and shifts of the spectral lines of three Ne II and six Ne III multiplets caused by collisions with electrons, protons, and helium ions at a density of perturbing particles of 10¹⁷ cm^–3 and different temperatures have been calculated. The results obtained have been compared with the known experimental and theoretical data.     

Investigation of the mechanism of spectral emission and redshifts of atomic line in laser-induced plasmas

In low-temperature plasmas, the specific emission mechanism and the evolvement of the continuum and isolated lines are quite complex, which are described in detail. The calculations from the Stark-broadening measurement of individual lines show the density to be of the order of magnitude of 10¹⁸ cm⁻³. It is seen that the redshifts of spectral lines detected in this experiment are influenced by the electron density. A possible reason for this is given.