不同土壤种植下四种柴胡种质药材中常量及微量元素含量的比较研究

采用ICP-AES/ICP-MS技术对7种土壤种植下的4种柴胡种质药材中21种常量及微量元素含量进行了分析测定。综合考虑种质和土壤对柴胡药材中常量和微量元素含量的影响,K,Ca,Mg,Na 4种常量元素含量受种质影响较大,Fe,Cu,Ni,Ti,Cr,V,Zr,Se,Sn,Cs,Cd,Hg,Pb等13种微量元素含量则受土壤影响较大;4种柴胡种质中,以甘肃种质的柴胡药材中常量和微量元素含量较高,中柴1号柴胡药材中常量和微量元素含量较低;在7种土壤种植下,以在北京市延庆县永宁镇盛世营村山地土壤上种植的柴胡药材中常量及微量元素含量较低,而在北京市怀柔区喇嘛沟门乡东岔村土壤上种植的柴胡药材中常量及微量元素含量较高。这些研究结果为了解各自药材中药效成分的含量及其疗效差异起着重要作用,也为选择种质和土壤及栽培出高产优质的柴胡提供重要依据。     

注射用针剂药物的拉曼散射光谱研究

本文从药品鉴别的角度出发,首先论述了拉曼光谱分析技术并测试了九种针剂药品的拉曼光谱,通过分析讨论相关药品的拉曼光谱得出了几点结论:(1)某些药品的拉曼峰较多,特征峰值较强,频移范围比较广,例如:氟尿嘧啶,依托泊苷,异烟肼,克林霉素磷酸酯。(2)某些药品拉曼峰较弱,或是没有明显的特征峰,例如:硫酸阿米卡星,甲氧苄啶,利巴韦林,葡萄糖依诺沙星,硫酸庆大霉素。(3)在分析频率及其相对强度时发现,在某一频率下正对的峰高和面积较大,则其相对强度较大,例如:氟尿嘧啶,异烟肼,硫酸阿米卡星,甲氧苄啶,葡萄糖依诺沙星。虽然得到的结论还不能满足对药品的品质鉴定,但通过拉曼光谱分析技术在药品鉴别中的应用,给出了一些药品的拉曼特征谱,为药品的鉴别提供了参考依据。可以说利用光谱分析技术对药品进行鉴别是完全可行的。     

天然杂质对黄铁矿的电子结构及催化活性的影响

采用密度泛函理论和平面波赝势方法对含天然杂质黄铁矿的电子结构和光学性质进行了计算,并讨论了二十种天然杂质:钴、镍、砷、硒、碲、铜、金、银、钼、锌、铊、锡、钌、钯、铂、汞、镉、铋、铅和锑,对黄铁矿催化活性的影响.结果表明在过渡金属杂质中,杂质能级主要由它们的d轨道产生,而在主族金属及非金属杂质中,杂质能级主要由它们的s或p轨道产生.含铜、钼、砷、金、银或镍的黄铁矿对氧的还原的电催化能力增强.除锌、钼、钌、砷、锑、硒和碲外,其余杂质能增强黄铁矿表面俘获电子的能力,使光生电子和空穴复合的概率减小.光学性质计算表 关键词： 天然黄铁矿 杂质 电子结构 光学性质     

Electromagnetic volume scattering in the half-space: a moment-method analysis without Sommerfeld integrals or their approximations

Traditionally, in moment-method analyses of electromagnetic scattering, the elements of the impedance matrix are calculated as convolutions of the basis elements with the appropriate dyadic Green's function. However, for scattering in the half-space, the vertical and azimuthal copolar terms of the Green's function require evaluation of Sommerfeld integrals which are computationally burdensome. In this paper, it is shown that, in populating the impedance matrix for the half-space problem, evaluation of Sommerfeld integrals is, in fact, not necessary. For monochromatic excitation, the plane-wave expansion of the scattered field constitutes a Fourier transform, in the horizontal plane, of a vector spectral function. This vector function results from the convolution, in the vertical dimension, of the respective angular spectra of the Green's function and the equivalent current. On application of the moment method, through the Weyl identity, the impedance-matrix elements corresponding to the singular terms of the Green's function are convolutions in the horizontal plane of spherical potentials, and Fourier transforms of scalar spectral functions. These scalar functions are derived from the basis elements and, with a judicious choice of basis, they are well behaved and of compact support, and consequently their Fourier transforms can be computed as FFTs.     

基于计算机辅助的医学图像测量与控制方法研究

医学图像常规检查中,需要对目标图像进行测量以获取相关数据。测量主要集中在对距离,面积,角度以及周长等数据的获取。由于医学检测的严谨性,数据准确,方法简便是必不可少的要求。随着计算机技术的发展,其在医学中的应用也得到了广泛的推崇。计算机辅助的医学图像测量不但替代了传统的手工测量方式,也极大地提高了测量的精度与效率。分析医学图像测量算法,针对如何确定目标区域的问题设计了颜色填充的方法,可有效区分出目标区域图像。为了提高该算法的效率,进一步提出了其改进算法,降低了算法执行次数,提高了系统性能。     

Chaos and chaotic transients in an aeroelastic system

Chaotic motions of a two dimensional airfoil with coupled structural nonlinearities, both in pitch as well as plunge degrees of freedom, are investigated via a numerical integration method. The original system of coupled integro-differential equations governing the motion of the present aeroelastic model is transformed into a simple system of six ordinary differential equations (ODEs), rather than the previously frequently used eight ODEs. Complex dynamical behaviors are revealed and identified through the means of bifurcation diagrams, the phase portraits, the amplitude spectra and the Poincare maps. Besides, a more quantitative method, namely that of observing the evolution of the largest Lyapunov exponent (LLE) is also applied to diagnose the motions. Two peculiar phenomena, namely, long (perhaps super-persistent) chaotic transients, and fluctuating Lyapunov exponents, are observed; in the two such cases the LLE method fails to work. In addition, the effects of various system parameters, namely, the position of the elastic axis, the frequency ratio, the airfoil/air mass ratio, the viscous damping ratios, and the location of the center of mass, on the response of the aeroelastic system, are investigated.     

Phenomenon of gravitational repulsion in the general theory of relativity

Einstein's generalization of Newton's theory of gravitation in the general theory of relativity led not only to small quantitative differences between gravitational effects in the relativistic theory and the Newtonian theory, but also to essentially new phenomena and effects peculiar to the relativistic theory and absent in the Newtonian theory. This difference is so large that the gravitational interaction in Einstein's theory even altered the attraction-only property, characteristic of Newton's theory, the law of universal gravitation, and became both attractive and repulsive. It is notable that the nature of the repulsion in gravitational interaction already appears in the simplest case of a spherically symmetric isolated body. Einstein's equations admit for a spherical body a solution whose physical interpretation uniquely indicates the repulsive nature of a gravitational field inside the body, if the number of particles that make up the body is sufficiently large. The structure of such a body, density distribution of the number of particles, mass, and pressure, is determined in the equilibrium state by the pressure of the substance, the gravitational attraction of peripheral layers toward the center, and the gravitational repulsion of inner layers of matter away from the center. As a result of the gravitational repulsion of matter away from the center inside the body there appears a cavity, free of the matter making up the body and its electromagnetic radiation. If the body is cold, then the volume of the world tube of the cavity can differ from zero. In the opposite case, the world tube of the cavity reduces to the world line of the center, which is inaccessible to particles of matter and to electromagnetic radiation. Gravitational repulsion, on the other hand, is a result of the existence of a field singularity at the center of the body, whose world line is time-like.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 4, pp. 61–67, April, 1981.     

嵌入式Linux根文件系统的构建与分析

Linux系统移植主要包括bootloader的移植、内核移植、根文件系统的移植等三大部分。在基于Linux的嵌入式系统的构建过程中,根文件系统是不可缺少的重要组成部分。重点对利用busybox构建根文件系统的过程进行了详细的讲解,包括busybox的配置过程,根文件系统的构建过程,Web服务器BOA的构建过程,网络视频服务器MJPG-streamer的构建过程,NFS挂载根文件系统的测试过程,以及三种文件系统Cramfs、JFFS2及Ramdisk的制作过程,将几种不同的文件系统的性能进行了对比分析。实验表明制作完成的三种文件系统能够正常使用,并且运行稳定。     

混合载气高场不对称波形离子迁移谱中He‐N2 比例对挥发性有机物混叠峰分离的影响研究

载气混合是提高高场不对称波形离子迁移谱（FAIMS）离子分离能力的一个重要方法,在生物大分子质谱研究领域已得到广泛应用,但缺乏在环境小分子领域的研究。选取挥发性有机物（VOCs）中芳香烃、醇、烷烃、酸、酮类中的五种物质（邻二甲苯、异丁醇、正己烷、乙酸、丙酮）为研究对象,研究了混合气体中He-N₂比例对VOCs中单体-二聚体离子混叠峰峰位置、分离度及总离子通过率的影响。实验结果表明,随着FAIMS载气中He比例的增加,5种VOCs中单体及二聚体离子峰峰位置发生偏移,且单体峰与二聚体峰偏移程度不同,单体峰偏移量先增加后减少,而二聚体峰峰位置偏移量逐渐增加;随着FAIMS载气中He比例的增加,五种VOCs离子混叠峰的分离度逐渐增加并趋于饱和,邻二甲苯、异丁醇、正己烷、乙酸、丙酮5种样品的混叠峰分离度达到饱和时对应He比例分别是：20%,30%,10%,40%和20%;随着FAIMS载气中He比例的增加,邻二甲苯、异丁醇、正己烷、丙酮的离子信号强度无明显变化,乙酸的离子信号强度下降明显。该研究为提高FAIMS对环境小分子的分离能力提供了一种可行的方法。同时,也验证了高电场下布朗定律在小分子离子应用上的有效性。     

Structure-preserving algorithms for the Duffing equation

In this paper, the dissipative and the forced terms of the Duffing equation are considered as the perturbations of nonlinear Hamiltonian equations and the perturbational effect is indicated by parameter ε. Firstly, based on the gradient- Hamiltonian decomposition theory of vector fields, by using splitting methods, this paper constructs structure-preserving algorithms （SPAs） for the Duffing equation. Then, according to the Liouville formula, it proves that the Jacobian matrix determinants of the SPAs are equal to that of the exact flow of the Duffing equation. However, considering the explicit Runge Kutta methods, this paper finds that there is an error term of order p＋l for the Jacobian matrix determinants. The volume evolution law of a given region in phase space is discussed for different algorithms, respectively. As a result, the sum of Lyapunov exponents is exactly invariable for the SPAs proposed in this paper. Finally, through numerical experiments, relative norm errors and absolute energy errors of phase trajectories of the SPAs and the Heun method （a second-order Runge-Kutta method） are compared. Computational results illustrate that the SPAs are evidently better than the Heun method when e is small or equal to zero.     

颗粒度对不同煤种可见光-近红外光谱的影响

煤炭是我国最主要的能源,在开采、运输、洗选加工、精煤储运等过程中都需要及时了解煤的成分、含量以及混矸程度,以便掌握和监控煤炭质量。目前,基于可见光-近红外反射光谱的煤炭原位测试技术已经成为一个研究热点。颗粒度是影响光谱特征的重要因素,开展颗粒度对不同煤种反射光谱特征的影响研究,对于深刻认识煤的光谱特征,进而提高煤光谱识别精度具有重要意义。为此,选取我国主要煤炭富集区（包括内蒙古乌海、新疆哈密、山西阳泉）的褐煤、烟煤、无烟煤为研究对象,利用SVC HR-1024光谱仪对不同颗粒度煤样的可见光-近红外光谱进行测试,分析了颗粒度对煤样光谱反射率的影响规律,以及颗粒度对于不同煤种光谱影响的差异。在此基础上,对实验现象背后的物理机理进行了分析讨论。研究表明,变质程度不同的煤反射光谱特征基本相似,即在可见光波段反射率较低且随波长增加出现缓慢下降趋势,在近红外波段快速上升。当煤样颗粒度>0.10 mm时,颗粒度大小对光谱特征的影响较小,煤样反射光谱特征随颗粒度变化规律不明显;当颗粒度<0.10 mm时,颗粒度对煤样的光谱影响增大,且影响主要体现在近红外波段的反射率光谱曲线的斜率大小,颗粒度越小,光谱反射率曲线斜率越大。0.10 mm颗粒度可作为颗粒度对煤的光谱特征影响的敏感界限。不同煤种可见光-近红外光谱曲线受颗粒度的影响程度不同,褐煤的影响最大,烟煤次之,无烟煤影响最小。实验表明,利用反射光谱进行煤质分析和煤种识别时需要考虑颗粒度的影响,同时,选择颗粒度小于0.10 mm的粉末状样品效果要好于大颗粒或块状样品。     

Effect of spraying power on the microstructure and mechanical properties of supersonic plasma-sprayed Ni-based alloy coatings

The aim of this paper was to investigate the microstructure and mechanical properties of the supersonic plasma-sprayed Ni-Cr-B-Si-C coatings prepared at different spraying powers. The microstructure, phase composition, porosity, Young's modulus, micro-hardness, and residual stresses of the coatings were investigated and determined. The variations of the porosity, Young's modulus and micro-hardness of the coatings were evaluated by using statistical method. Results showed that the variations of porosity, Young's modulus and micro-hardness of the coatings followed the Weibull distributions. With increasing the porosity, the micro-hardness and Young's modulus of the coating decreased. The mean value of the Young's modulus of the coating calculated from Weibull plot was almost proportional to the square root of the micro-hardness of the coating. With increasing the power, Young's modulus of the coating increased, which, in turn, resulted in the increment of the residual stress at the coating surface.     

Laser absorption and fluorescence diagnostics of a plasma

Diagnostics of a near-surface laser plasma, the plasma of a strong-current pulse gaseous discharge in inert gases, nitrogen, and carbon dioxide under conditions of intense evaporation of the wall of the discharge chamber, the plasma of a discharge with a hollow cathode, and the active medium of an excimer laser was conducted by methods of intracavity laser spectroscopy and laser-induced fluorescence. The dynamic fields and absolute concentrations of atoms, ions, molecules and electrons, the plasma temperature, and the velocities of flows of particles were measured. The quantitative determination of the density of particles in the erosion laser flame prior to breakdown and the phenomena associated with the formation of molecules in the laser plasma received primary consideration. To whom correspondence should be addressd. Instite of Molecular and Atomic Physics of the Academy of Sciences of Belarus, 70, F. Skorina Ave., Minsk, 220072, Belarus. Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 64, No. 3, pp. 281–290, May–June, 1997.     

星光掩星探测技术的轨道模拟结果分析

星光掩星技术是利用恒星光谱进行地球及其他行星大气痕量成分密度、温度、气溶胶等测量的有效手段。该探测原理主要是根据不同的大气成分在恒星光谱的不同位置上表现出不同的吸收特征,具体表现在:紫外波段可进行臭氧、氧气、氢气等的测量,可见光谱段可探测二氧化氮、三氧化氮、氧气等,红外可探测水蒸气、气溶胶、甲烷、二氧化碳、氧气等。星光掩星的实现过程为:当LEO卫星和恒星分别位于地球的两侧时,恒星发射的光经过地球大气的吸收、散射等作用,被另一侧的LEO所接收,即构成掩星观测。根据光谱流量得到恒星的视星等范围,给出恒星在天球坐标系中的分布和不同的光谱型,以及利用各光谱型可探测的大气成分,再利用恒星和LEO卫星在地固坐标系中的相对位置,进行恒星-LEO星光掩星轨道观测模拟,基本流程为:首先读取LEO卫星的轨道位置以及目标恒星的位置,设置24 h的模拟时间,其次判断是否处于掩星状态,当掩星开始时,计算并输出掩星发生的经纬度、速度等,直至模拟时间结束。其中涉及恒星从天球坐标系转换到地固系的过程, LEO卫星轨道、掩星切点经纬度等的计算。根据模拟流程,计算并分析掩星事件的日观测量、全球分布、持续时间以及漂移速度等,得到以下结果:(1)目标恒星在全天区都有一定数量的分布且具有不同的光谱型,可进行臭氧、二氧化氮等成分的探测;(2)在对星光掩星进行24 h的轨道模拟过程中,日观测量为5 563次,其中包括2 737次上升掩星, 2 826次下降掩星;(3)从全球分布来看,掩星事件主要分布在低纬度,两极最少,其他纬度数量相当,且经度方向分布均匀;(4)根据方位角的分布,正常掩星占比为78.25%,持续时间平均为1.5 min,切点水平漂移在18~600 km;(5)21.75%的侧面掩星事件,其较正常掩星来说,持续时间长,切点的水平漂移速度大,方位角变化也大。该结果为卫星轨道设计和探测载荷设计提供理论指导。     

基于单片机的直流电动机的信号采集系统设计

装甲车辆起动过程中,直流电动机部分容易发生故障,传统的电机诊断方法都是定期制定维修计划,这种检修方式容易造成维修不足、维修过量以及盲目维修的问题,为了深入分析电动机故障发生时的参数信息的变化,构建一套能够采集电机运行参数的系统,对采集电枢电流和振动信号进行时频域分析,能够反映故障发生的特点;该系统以STM32103C8T6为主控芯片,设计了电流、振动信号采集电路,信号调理电路,对A/D转换模块、数据存储模块进行了编程实现,能够对直流电动机的电枢电流和振动信号进行实时采集,并将数据保存到上位机中进行后续的调用处理;通过测量对比直流电动机起动过程轴承部位发生不同故障时的电流和振动信号,利用MATLAB仿真实现时域内的信号显示,并在MATLAB平台中,编程实现了振动信号的时频域分析;仿真结果表明,该采集系统能够准确测量信号,具有成本低,体积小,精度高等优点,能够为故障特征提取提供较好的数据基础。     

低轨四星时差定位技术研究

文章重点分析影响低轨四星时差定位系统精度的主要因素;首先,从四星时差定位的基本原理出发,对四星时差定位的模型和几何精度因子进行了详细的推导,并通过仿真分析了四星构型、时差测量精度、卫星位置误差、基线长度、星座投影面积等对四星时差定位系统精度的影响;通过比较可知,在相同参数条件下,采用Y形构形,减小时差测量误差、提高卫星定位精度、增加基线长度,增大星座投影面积均等均能够提高该系统的定位精度;在低轨四星定位系统应用场景中,四星构型、卫星绝对位置测量精度、基线长度以及星座投影面积对四星时差定位系统精度影响较大,时差测量精度和卫星相对位置测量精度对四星时差定位系统精度影响较小;而在实际任务中应权衡各因素的效费比,来保证定位精度。     

空间调制微型傅里叶变换红外光谱仪研究

针对目前环境、医疗、空间、气象、军事及安全等领域对傅里叶变换红外光谱仪微小型化、轻量化及固态化的迫切需求,提出并研究了一种以MOEMS多级微反射镜为核心器件的空间调制微型傅里叶变换红外光谱仪。在理论研究方面,建立了空间调制微型傅里叶变换红外光谱仪的物理模型,探究了该系统的光场分割与空间采样的光学原理;分析了多级微反射镜的衍射效应,提出了一种通过补边抑制衍射噪声抑制方法;进行了多级微反射镜采样误差的分析,并提出了基于最小二乘拟合的修正算法;通过对光源空间相干性、准直系统像差以及入射光场均匀性的分析,确定了光学系统的总体设计指标;通过对多级微反射镜基片加工精度、分束器材料色散特性和膜层透射效率等的计算分析,确定了干涉系统的设计方法与技术参数。在核心技术方面,提出了两个多级微反射镜的3种制作方法,分析了制作误差的来源及对系统性能的影响。通过工艺设计及实验条件探索,分别采用电铸法、真空镀膜法以及斜面倾角叠片法制作了两个多级微反射镜。在系统设计方面,进行了红外准直与缩束系统的光学设计,对整体光机系统进行了建模仿真,分析了杂散光噪声的来源。在图谱处理方面,利用过零采样方式,通过图像分割算法,获取了干涉图采样序列;通过对干涉图序列的插值、补零、延拓与卷积方法,完成了光谱相位误差的校正;通过离散傅里叶变换解调,实现了由干涉图像到信号光谱的数据反演。最后研究了系统光机整体的集成组装技术,并对原理样机进行了实验测试。本文研制的空间调制微型傅里叶变换红外光谱仪的特点在于:取消了动镜驱动机构与采样控制机构,具有微小型与轻量化的特点;干涉图的采样由多级微反射镜完成,其空间采样的方式增加了系统的稳定性与可靠性,实时采样的特点增加了系统的快速性与有效性;多级微反射镜阵列采用MOEMS工艺技术制作,增加了系统的采样精度。该光谱仪系统的结构及制作方法具有自主知识产权,并具有广阔的应用前景。     

样品的激光诱导击穿光谱及谱线的自吸收现象

以脉冲Nd∶AG激光器的二倍频输出为激发源,获得了一种家庭用煤的激光诱导击穿光谱(laser induced breakdown spectrum,LIBS)。通过对谱线的归属,发现该煤种除包含文献报道的C,Si,Mg,Fe,Al,Ca,Ti,Na,K元素外,还包含Cd,Co,Hf,Ir,Li,Mn,Ni,Rb,Sr,V,W,Zn,Zr等微量元素,谱图中没有出现对应H和O元素的谱线,把该现象归因于H和O原子的跃迁概率较小,而灵敏谱线对应跃迁的上能级能量较大。同时发现随激光脉冲能量的增加,等离子体发射谱线的强度增大,增加到一定程度,K原子766.493和769.921 nm谱线会出现自吸收现象,自吸收的程度随激光能量的增加而增强,出现明显的双峰结构,把自吸收现象归因于原子大的跃迁概率及激光强度增加引起等离子体中粒子数密度的增大。     

掺杂浓度及掺杂层厚度对Si均匀掺杂的GaAs量子阱中电子态结构的影响

本文通过自洽地求解薛定鄂方程及泊松方程计算了在温度T=0, 有效质量近似下, Si均匀掺杂的GaAs/AlGaAs量子阱系统的电子态结构. 研究了掺杂浓度及掺杂层厚度对子带能量, 本征包络函数, 自洽势, 电子密度分布, 及费米能量的影响. 发现在给定掺杂浓度下, 子带能量随掺杂层厚度的增加单调递减, 自洽势的势阱变宽变浅, 电子密度分布变宽, 峰值变低; 在给定掺杂层厚度下, 随掺杂浓度的增加子带能量及费米能级单调递增, 自洽势阱变深变陡变窄, 电子密度分布的峰值变高, 集中在中心. 关键词： 掺杂 量子阱 电子结构 半导体GaAs     

The ulysses space mission

Summary We describe briefly the collaborative ESA-NASA Ulysses mission which will provide, for the first time in the history of the Solar-System exploration,in situ observations of the heliosphere over a broad range of heliographic latitudes. Launched on October 6, 1990, Ulysses has been injected in a high-inclination orbit by means of a gravity-assisted manoeuvre at the time of his encounter with Jupiter, in February 1992. On-board instrumentation will obtain data on the solar wind, the heliospheric magnetic field, radio, X-and γ-bursts plasma waves and interplanetary and interstellar gas and dust. Italy participates to the mission with an experiment, led by Professor Bruno Bertotti, of the University of Pavia, aimed at detecting gravitational waves, and with an interdisciplinary investigation, led by Professor Giancarlo Noci, of the University of Florence, where scientists from the University of Florence, the Arcetri Astrophysical Observatory, the Institute for the Physics of the Interplanetary Space of Frascati and the Observatory of Trieste will use data from different experiments to study the dependence of mass loss, ion composition and turbulence of the solar wind on heliographic latitude. Paper presented at the V Cosmic Physics National Conference, S. Miniato, November 27–30, 1990.