临近空间高空气球地基探测能力分析

基于探测系统背景辐射特性及高空气球辐射特性,建立了探测系统辐射接收模型.考虑大气传输、光学系统成像、探测器及其采样对辐射的影响,精确计算了高空气球辐射及背景辐射在探测器焦平面阵列上产生的信号电子数,推导出用于高空气球探测的信噪比.利用Modtran软件仿真计算了自身辐射、镜背景辐射、漫背景辐射亮度,分析了复杂大气条件下的气球辐射特性,及高空气球镜反射率、漫反射率与积分时间对探测系统信噪比的影响.结果表明:采用光谱滤波技术,在晴朗无云天气下,可见光近红外(0.6~2.4)探测器适合高空气球探测;在复杂大气条件下,长波红外(8~12)探测器适合高空气球探测;在积分时间为0.25s,镜反射率为0.32,漫反射率为0.68时,或积分时间为1s,镜反射率0.43,漫反射率0.57时,探测系统对高空气球探测能力最强.     

Orientational anisotropic studies by field rotation technique: near zero-field pulsed EPR experiments of pentacene doped in p-terphenyl

We report a new technique to map the orientational anisotropy of paramagnetic systems without physically changing the crystal orientations in near zero-field (NZF) pulsed EPR experiments. By implementing three sets of orthogonal coils around the sample, we are ble to create a magnetic vector up to 2 mT in any three-dimensional orientation in space. In NZF region, the hyperfine tensor elements are comparable to the electronic Zeeman interaction energy, thus very rich spectral patterns can be obtained by "dialing" in a magnetic field vector without moving the sample. The technique further allows us to examine the site symmetry of organic crystals and powdered solids doped with chromophores which can be photo-excited to the triplet state by laser light. The technique is exemplified in the study of pentacene in p-terphenyl crystals.     

药品近红外光谱通用性定量模型评价参数的选择

为寻找药品近红外通用性定量模型在建立过程中用于确立最优模型的关键评价参数组合,收集整理了目前各种商品化化学计量学软件及文献中的13个常用于评价近红外定量模型的统计学参数,结合人用药品注册技术要求国际协调会对于药品定量分析方法验证基本要求,对92个药品近红外通用性定量分析模型的这些参数进行了计算和分析。通过对各个参数之间相互关系的研究,确定了适合于药品近红外通用性定量分析模型评价的参数组合,并统计出了这些参数的数值范围：用于模型准确性评价的关键参数为交叉验证均方根误差/预测均方根误差、平均相对偏差和相对分析误差;大部分交叉验证均方根误差/预测均方根误差结果在3%以内,其中交叉验证均方根误差在数值上与平均绝对偏差相当,大部分相对分析误差值大于2,而平均相对偏差的数值与所建模型的类型(剂型、样品的包装形式)和待测成分含量的分布有关。模型线性评价关键参数为决定系数;大部分模型的决定系数在80%～100%之间。模型耐用性关键评价参数为预测均方根误差与交叉验证均方根误差的比值,大部分模型该参数在1.5以内。精密度评价关键参数为重复测定结果的标准差;该参数对于规范近红外的操作,以及考核模型能否在不同仪器间传递具有重要的意义,但目前药品近红外通用性定量模型对于分析精密度的关注较少,无法估计出具体数值范围。该研究不仅为药品近红外通用性模型的建立者和使用者提供了评价模型优劣的依据,也为完善药品近红外光谱通用性定量分析模型的参数评价体系提供了基础数据。     

高强高效近红外光源的不同光源强度对玉米杂交种鉴别的影响

以2009年产自海南的农华101玉米种子作为研究对象,基于近红外漫透射光谱法(波长范围908.1~1 677.2 nm),研究了一种高强高效近红外光源在不同光源电压以及光源至光谱仪不同距离两种条件下对玉米杂交种鉴别的影响。对光谱进行一阶导数、矢量归一化的预处理后,使用主成分分析(PCA)和正交线性判别分析(OLDA)提取光谱特征,使用支持向量机(SVM)分别建立种子纯度鉴定模型,统计不同实验条件下的识别率。结果表明,在电压较低或者光源至光谱仪的距离较大的时候,光源强度较低,得到的光谱曲线有较多的毛刺,此时的识别率较低,增大电压或者降低光源至光谱仪的距离时,光谱曲线变得较为平滑,识别率明显升高,说明在一定范围内增大光源强度会提高模型的正确鉴定率。     

Influence of the halo upon angular distributions for elastic scattering and breakup

The angular distributions for elastic scattering and breakup of halo nuclei are analysed using a near-side/far-side decomposition within the framework of the dynamical eikonal approximation. This analysis is performed for ¹¹Be impinging on Pb at 69 MeV/nucleon. These distributions exhibit very similar features. In particular they are both near-side dominated, as expected from Coulomb-dominated reactions. The general shape of these distributions is sensitive mostly to the projectile-target interactions, but is also affected by the extension of the halo. This suggests the elastic scattering not to be affected by a loss of flux towards the breakup channel.     

The absorption spectrum of phosphine (PH3) between 2.8 and 3.7 μm: Line positions, intensities, and assignments

Over 8000 line positions and intensities of phosphine (PH₃) at 3 μm have been measured at 0.0115 cm⁻¹ resolution with the McMath-Pierce Fourier Transform spectrometer at Kitt Peak. The observed line intensities ranged from 4.13 × 10⁻⁶ to 4.69 × 10⁻² cm⁻² atm⁻¹ at 296 K, for line positions between 2724.477 and 3601.652 cm⁻¹. This region spans eight interacting vibrational states: 3ν₂ (2940.8 cm⁻¹), 2ν₂ + ν₄ (3085.6 cm⁻¹), ν₂ + 2ν₄ (3214.9 cm⁻¹), ν₁ + ν₂ (3307.6 cm⁻¹), ν₂ + ν₃ (3310.5 cm⁻¹), 3ν₄ (∼3345 cm⁻¹), ν₁ + ν₄ (3426.9 cm⁻¹), and ν₃ + ν₄ (3432.9 cm⁻¹). Assignments have been determined for all the bands except 3ν₄ (a weak band in a highly congested area) for a total of 4232 transitions. The total integrated intensity for this region is 5.70 cm⁻² atm⁻¹ near 296 K, and assigned lines account for 79% of the observed absorption. The two strongest bands in the region are ν₁ + ν₄ and ν₃ + ν₄ with band strengths at 296 K of 1.61 and 2.01 cm⁻² atm⁻¹, respectively. An empirical database of PH₃ line parameters (positions, intensities, and assignments) is now available. Lower state energies (corresponding to assignments from this study) and line widths from the literature are included; default values are used for unassigned features.     

Self-broadened widths and shifts of CO2: 4750-7000 cm

In the previous paper, we report line strength measurements for 58 bands of ¹²CO₂ between 4550 and 7000 cm⁻¹ [R.A. Toth, L.R. Brown, C.E. Miller, V. Malathy Devi, D. Chris Benner, J. Mol. Spectrosc., this issue, doi:10.1016/j.jms.2006.008.001.]. In the present study, self-broadenedwidth and self-induced pressure shift coefficients are determined in two intervals:

(a) between 4750 and 5400 cm⁻¹for bands of the Fermi triad (20011 ← 00001, 20012 ← 00001, 20013 ← 00001), three corresponding hot bands (21111 ← 01101, 21112 ← 01101, 21113 ← 01101) and the 01121← 00001 combination band;

(b) between 6100 and 7000 cm⁻¹ for the Fermi tetrad (30014 ← 00001, 30013 ← 00001, 30012 ← 00001, 30011 ← 00001), two associated hot bands (31113 ← 01101, 31112 ← 01101), as well as 00031 ← 00001 and its hot band 01131 ← 01101.

Least-squares fits of the experimental width and pressure shift coefficients are modeled using empirical expressions:

     

InGaAsP/InP photodetectors targeting on 1.06 μm wavelength detection

InP-based InGaAsP photodetectors targeting on 1.06 μm wavelength detection have been grown by gas source molecular beam epitaxy and demonstrated. For the detector with 200 μm mesa diameter, the dark current at 10 mV reverse bias and R₀A are 8.89 pA (2.2 × 10⁻⁸ A/cm²) and 3.9 × 10⁵ Ω cm² at room temperature. The responsivity and detectivity of the InGaAsP detector are 0.30 A/W and 1.45 × 10¹² cm Hz^1/2 W⁻¹ at 1.06 μm wavelength. Comparing to the reference In_0.53Ga_0.47As detector, the dark current of this InGaAsP detector is about 570 times lower and the detectivity is more than ten times higher, which agrees well with the theoretical estimation.     

近红外“3R”法双谱自适应去噪

针对近红外透射和吸收双光谱提出一种自适应的去噪方法。同步采集样品的近红外透射谱和吸收谱,在相同分解原则下总体经验模态法分解两组光谱,得到单组分特征模态分量。计算特征模态分量与原透射谱、吸收谱之间相关性,以及两组特征模态分量之间相关性,相关性最小模态分量初判为噪声分量。分析该分量在光谱中点处自相关性,若中点处很大,其他点几乎为零或很小,可以判断该分量为噪声。这种基于模态分量相关性的噪声判别方法称为“3R”法则。剔除噪声分量,重构光谱信号,循环上述分解过程,直到不满足“3R”法则,降噪过程结束。构造理想光谱,叠加噪声,“3R”法降噪效果优于EMD和EEMD低通滤波器,略逊于小波分解。真实光谱实验中,经过上述方法降噪处理过的玉米叶片光谱采用3层BP神经网络建立与叶绿素之间预测模型,“3R”法处理模型具有最大校正相关系数和预测相关系数,最小校正标准差和预测标准差。在四种降噪方法中,“3R”法对光谱谱峰位置和峰高的影响最小。实验表明,“3R”双谱去噪方法无需预设迭代次数,不用考虑分解层数,没有基函数,是自适应的,该方法适合近红外光谱去噪。     

Determining the Zn Content of Cherry in Field Using VNIR Spectroscopy

Visible and near-infrared(VNIR)spectroscopy is an eco-friendly method used for estimating plant nutrient deficiencies.The aim of this study was to investigate the possibility of using VNIR method for estimating Zn content in cherry orchard leaves under field conditions.The study was conducted in 3different locations in Isparta region of Turkey.Fifteen cherry orchards containing normal and Zn deficient plants were chosen,and 60 leaf samples were collected from each location.The reflectance spectra of the leaves were measured with an ASD FieldSpec HandHeld spectroradiometer and a plant probe.The Zn contents of leaf samples were predicted through laboratory analysis.The spectral reflectance measurements were used to estimate the Zn levels using stepwise multiple linear regression analysis method.Prediction models were created using the highest coefficient of determination value.The results show that Zn content of cherry trees can be estimated using the VNIR spectroscopic method(87.5相似文献