Separation and determination of inorganic cations in beverages by capillary electrophoresis with indirect UV detection

A rapid, simple and reliable capillary electrophoresis method for the separation and quantitation of inorganic cations with indirect UV detection at 214 nm was developed. The electrolyte was: 12 mM imidazole as background absorbance provider; 5 mM malic acid and 1.0 mM 18-crown-6 ether as complexing agents; and 20% D₂O (v/v) to improve ion mobility. The pH was 4.25. The applied voltage was 22 kV at 22°C. Nine ions were completely separated and determined with correlation coefficients of 0.9979-0.9992. The relative standard deviations (RSD) were less than 0.5% for migration time and less than 5.2% for peak area (n=8). The detection limits (S/N=3) were from 0.08 mg L⁻¹ (for Na⁺) to 0.51 mg L⁻¹ (for Cu²⁺). To assess the reliability atomic absorption (AA) was also used to determine the same samples. Satisfactory results were obtained for real samples of jasmine tea drink and coconut milk.      

对位取代酚钾与10′10′-二烃基-9,9′-联二吖啶盐电荷转移光谱的研究

10,10′-二烃基-9, 9′-联二吖啶盐有很强的荧光, 在光学材料^[1]和重金属离子的分析^[2]中有重要的应用价值。     

大孔径静态干涉成象光谱仪中的横向剪切干涉仪

介绍大孔径静态干涉成象光谱仪的光学原理,分析基于Sagnac型横向剪切分束器的干涉系统设计方案,推导了理论和实际的光程差公式,讨论了几种具体的结构形式,总结了各自的优缺点。     

转镜式高灵敏度干涉光谱成像仪ROSI

转镜式高灵敏度干涉光谱成像仪(ROSI) 是一种新型傅里叶变换光谱成像仪,采用了基于Sagnac横向剪切干涉仪的精密转镜扫描机构,通过旋转Sagnac干涉仪的一个反射面,得到被探测目标的空间与光谱信息.ROSI具有共光路、无狭缝、实时性好等特点,因此具有较高的系统稳定性和探测灵敏度并可凝视成像.通过与现有的多种高灵敏度干涉光谱成像仪的比较,表明ROSI克服了现有技术中存在的主要缺陷.     

Prospective study on observations of γ-ray sources in the Galaxy using the HADAR experiment

The High Altitude Detection of Astronomical Radiation (HADAR) experiment is a refracting terrestrial telescope array based on the atmospheric Cherenkov imaging technique. It focuses the Cherenkov light emitted by extensive air showers through a large aperture water-lens system for observing very-high-energy γ-rays and cosmic rays. With the advantages of a large field-of-view (FOV) and low energy threshold, the HADAR experiment operates in a large-scale sky scanning mode to observe galactic sources. This study presents the prospects of using the HADAR experiment for the sky survey of TeV γ-ray sources from TeVCat and provids a one-year survey of statistical significance. Results from the simulation show that a total of 23 galactic point sources, including five supernova remnant sources and superbubbles, four pulsar wind nebula sources, and 14 unidentified sources, were detected in the HADAR FOV with a significance greater than 5 standard deviations (σ). The statistical significance for the Crab Nebula during one year of operation reached 346.0 σ and the one-year integral sensitivity of HADAR above 1 TeV was ~1.3%–2.4% of the flux from the Crab Nebula.     

探测器横纹误差对大孔径静态干涉成像光谱仪影响的建模与修正

大孔径静态干涉成像光谱技术在航天遥感应用中,由于探测器横纹误差影响,使获得的干涉数据无法反演光谱数据,需要对横纹误差进行修正。通过对干涉成像机理的分析,给出探测器横纹误差影响下的干涉成像模型,提出横纹误差影响下干涉数据修正方法。最后利用仪器获取的数据,对提出的修正方法进行验证,由处理结果可以看出,本文所提的修正方法可以很好的修正横纹误差对光谱的影响,提高反演光谱的精度。     

Non-monotone projection gradient method for non-negative matrix factorization

Since Non-negative Matrix Factorization (NMF) was first proposed over a decade ago, it has attracted much attention, particularly when applied to numerous data analysis problems. Most of the existing algorithms for NMF are based on multiplicative iterative and alternating least squares algorithms. However, algorithms based on the optimization method are few, especially in the case where two variables are derived at the same time. In this paper, we propose a non-monotone projection gradient method for NMF and establish the convergence results of our algorithm. Experimental results show that our algorithm converges to better solutions than popular multiplicative update-based algorithms.     

基于多光谱遥感成像链模型的系统信噪比分析

信噪比(SNR)是评价多光谱遥感成像性能的重要指标,在设计多光谱遥感成像仪的最初阶段应进行分析,从而确定各分系统相关参数。多光谱遥感系统的成像链模型综合考虑辐射源、地物光谱反射、大气辐射传输、光学系统成像、分光元件特性、探测器光谱响应和相机噪声等各个环节,可用于进行成像过程端对端的完整分析。以基于滤光片阵列的多光谱遥感系统为例,采用MODTRAN软件进行大气辐射传输计算,对不同太阳天顶角下,不同目标地物计算像面的照度,根据电荷耦合器件探测器的噪声模型,计算出不同工作条件下多光谱遥感系统的SNR。通过对SNR的分析,可给出该类型多光谱遥感系统获得最佳性能的工作条件,并能够结合使用要求进行光学系统参数的优化选择。     

基于高速转镜的高分辨率干涉光谱仪非线性理论研究

介绍一种基于高速转镜的高分辨率光谱仪的原理,讨论了光程差的非线性与转镜转角θ、折射率n的关系,给出光程差的一般公式,并讨论了一般空间光线的光程差,及系统非线性变化规律.计算得到了使非线性最小的理想的材料折射率值,并通过计算机仿真,进行了验证.     

Mo(Ⅵ)-5-溴水杨基荧光酮-CTMAB显色反应的研究及应用

研究了新的三元配合物体系Ｍｏ（Ⅵ）－溴水杨基荧光酮－ＣＴＭＡＢ显色反应的条件,最大吸收波长λｍａｘ在５２８ｎｍ,试剂λｍａｘ在４６８ｎｍ,对比度为６０ｎｍ,ε５２８＝１．４７＊１０＾５Ｌ．ｍｏｌ＾－１．ｃｍ＾－１。该体系选择性好,方法简便、快速,用于测定水样中微量钼,结果满意。