虚拟式声显微镜及应用技术研究

本文描述一台虚拟式扫描声显微镜及应用技术研究，它的硬件特别简单，仅由一台带有超高速A/D卡和快脉冲收发卡的PC机和机械扫描系统组成，主要的功能均由软件完成，脉冲收发卡仅包括脉冲产生和高频放大器，A/D卡采用PCI总线，采样率1GSPS，数据传输率100MB/s，系统能采集并实时显示频率达百兆的未检波回波信号，采修订本以的信号经软件处理，可在屏幕上实时显示样品的A、B、C型幅度像或相位像，仪器利用信号处理技术提高信号的信噪比；进行特征提取，识别，该仪器在材料识别，电子、光电子器件和焊接质量检测等方面功能较强，具有广阔的开发应用前景。     

高速光测装置的价值函数

本文提出一个价值函数,作为高速光测装置的评价准则。此函数建立在装置可能获得的信息容量和质量的基础上,例如,数据锐度和装置的多功能性等。     

A new instrument for measuring the viscoelastic properties of dilute polymer solutions

A new oscillating capillary viscometer has been developed and used for measuring viscoelastic flow properties of dilute polymer solutions. These flow properties are determined from measurements of the pressure to volume flow relationships for sinusoidal flow in cylindrical glass capillaries. The theory for this measurement procedure is based upon the known theory for oscillatory flow of a viscoelastic fluid in circular tubes and which is presented with a few supplementations in this paper.The oscillatory flow is generated by a piezoelectric driver which is dipped directly into the aqueous solution. The advantage of this driver is that the excitation voltage for the piston is a direct measure of the motion of the piston. Changes in pressure are measured with a sensitive low-pressure quartz tranducer.The viscometer was tested with aqueous glycerol solutions and a gelatin gel. The viscoelastic flow properties of dilute polymer solutions (gelatin, gelatin/color-coupler, polyacrylamide) were then investigated in the frequency range 5 Hz to 150 Hz at very small volume flow amplitudes. The results presented illustrate the suitability of the method. The results are also evaluated with regard to the stabilizing action of slightly viscoelastic gelatinous coating liquids in the high-speed coating process in the manufacture of photographic materials.     

CHARACTERISTICS OF 30--60 DAY OSCILLATION OF GENERAL CIRCULATION IN NORTHERN HEMISPHERE

Some characteristics of the 30- 60 day oscillation in general circulation are investigatedin this paper. In the tropical atmosphere, besides some results consisting with the knownfacts, we still find that the 30- 60 day atmospheric oscillations are very obvious in theequatorial eastern Pacific, and the zonal scale of the vorticity and divergence for the30- 60 day oscillation in the tropics is much smaller than wavenumber 1. There are the strongest 30- 60 day oscillations at the high latitudes in the Northern Hemi-sphere, but weaker at 20°-40°N latitudes. The 30- 60 day oscillations have an obviousbarotropic structure at mid-high latitudes and their zonal scales are smaller than those in thetropics. The 30- 60 day oscillations at the mid-latitudes propagate westwards and fast in thewintertime. At the high latitudes, 30- 60 day oscillations propagate westwards in the win-tertime but eastwards in the summertime. Meridional propagations of the oscillation arerather different in various regions.     

On the output characteristics of a semiconductor optical amplifier driven by an ultrafast optical time division multiplexing pulse train

A comprehensive theoretical analysis of a semiconductor optical amplifier (SOA) that is subject to an ultrafast optical time division multiplexing pulse stream is presented with the help of a simple but efficient model developed for this purpose. The model combines the necessary set of mathematical equations with the appropriate simplifying assumptions to describe in the time domain gain saturation and recovery for the case of multiple incoming pulses. In this manner, analytical expressions can be obtained for the power and chirp profile of the amplified pulses, essentially extending the work that has been performed for a single pulse only. This allows to identify the critical operational parameters and to investigate and evaluate their effect on these two output characteristics. The derived simulation curves are thoroughly studied to specify the limitations imposed on the SOA small signal gain and carrier lifetime as well as on the full-width at half-maximum (FWHM) and energy of the input pulses and, based on a series of logical arguments, to extract useful rules concerning their selection so as to achieve improved performance with respect to the practical applications of all-optical switching and pulse compression. The obtained results indicate that due to the continuous insertion of pulses, the requirements for the SOA small signal gain and the input pulse energy are stringent than those for the case of isolated pulse amplification. The combination of these two parameters determines also the regime in which the amplifier must be biased to operate in order to ensure distortionless pulse amplification and enhanced chirp for efficient pulse compression and it has been found that low saturation is necessary for the former case whilst heavy saturation for the latter. The scopes of the corresponding requirements for the carrier lifetime and the FWHM are also tight but to a less extent and can be simply satisfied with the available photonics technology. These results are in good agreement with the available experimental data essentially proving the validity and robustness of the model. The model can be thus applied to predict the behavior of more complex all-optical circuits of enhanced functionality in which the SOA is the basic functional device.     

A rail noise prediction model for the Tehran-Karaj commuter train

Rail noise prediction models enable consideration of different scenarios for the optimal management of noise prevention and mitigation. This project is aimed at developing an equation that enables computation of L_A,max for the Tehran-Karaj commuter train, a type of Diesel-Electric Locomotive. The form of the proposed model is derived from equations for predicting L_A,max for a single locomotive pass-by, proposed in the manual prepared by Harris Miller Miller & Hanson Inc. for the US Federal Transit Administration, and in the French rail noise prediction model. The algorithm for predicting L_A,max for the Tehran-Karaj commuter train has been developed on the basis of the 50 measurements from 5 locations at distances of 25 m, 35 m, 45 m, 55 m, and 65 m from the centre of the track and at a height of 1.5 m. In the field measurements, the reference distance and the reference vehicle speed have respectively been set equal to 25 m and 80 km per hour. The reference L_A,max, length and the speed correction coefficients have been estimated from the field measurements and have been found to be 86.2 dB(A), 11.3, and 18.4 respectively. The fitness test (Kolmogorov-Smirnov) and regression analysis indicate satisfactory results.     

非线性掺铒光纤环镜中超短光孤子串的产生及放大

利用数值模拟方法证明了,双频弱连续波的拍频信号在分布增益的非线性掺铒光纤环镜内传输,能产生超短光孤子串.数值计算表明,当输入信号为重复率<20 GHz的拍频弱信号时,可在较短的环镜长度内产生占空比大且高质量的光孤子串.研究同时发现,输入信号的平均功率越大,所需环镜长度越短.与其他方法相比,该方法不仅能克服传统方法所产生的脉冲重复率受限的困难,而且在无需采用特种光纤的情况下,将弱信号转化为超短光孤子串.     

A study of daily variation in cosmic ray intensity during high/low amplitude days

A detailed study has been conducted on the long-term changes in the diurnal, semi-diurnal and tri-diurnal anisotropies of cosmic rays in terms of the high/low amplitude anisotropic wave train events (HAE/LAE) during the period 1981–94 using the neutron monitor data from Deep River Neutron Monitoring Station. In all, 38 HAE and 28 LAE cases have been studied. An inter-comparison of the first three harmonics during these events has been made so as to understand the basic reason for the occurrence of these types of events. It has been observed that the phase of diurnal anisotropy shifts towards earlier hours for HAEs and it shifts towards earlier hour as compared to 18-h direction for LAEs. For semi-diurnal anisotropy, phase remains statistically the same for both HAE and LAE. In the case of tri-diurnal anisotropy, phase is evenly distributed for both types of events. The interplanetary magnetic field (IMF) and solar wind plasma (SWP) parameters during these events are also investigated. It has also been observed that HAE/LAEs are weakly dependent on high-speed solar wind velocity. The two types of solar wind streams (corotating streams and flare-generated streams) produce significant deviations in cosmic ray intensity during HAE/LAE.      

柱形装药水中爆炸气泡的形态演变

 采用高速摄影方法在实验水箱中获得了长径比为3.35~6.75的柱形PETN炸药水中爆炸气泡脉动的图像,进而结合真实的爆轰过程和Rayleigh气泡运动方程,研究了气泡的形态演变规律。研究结果表明,柱形装药在水中爆炸时,形成的初始气泡的形状为非球对称形,这种非对称特征随长径比的增加而增大。气泡表面的运动也表现出明显的非球对称特征,气泡表面在装药径向的膨胀运动呈指数衰减,在装药轴向两端的膨胀运动更接近于分段线性衰减。气泡表面的不对称运动与柱形装药水下爆炸的能量输出结构不均有关,与冲击波的有效能量分布规律是相似的。     

水下高速射弹超空泡运动建模与仿真

建立并简化了水下高速射弹动力学和运动学模型。基于空泡模型假设和空泡截面独立扩张原理,确定了空化数与速度、深度的耦合计算关系;定义了水下射弹尾翼穿刺前的临界空化数;对水下高速射弹弹道特性进行了仿真研究。仿真计算结果表明：水下射弹有效射程受初始入射角影响较大;随着初始入射角的增大,有效射程逐渐减小;提升初速度可以带来有效射程的增大,但增幅效果不显著,在满足预定指标条件下应合理选择初速度;初始攻角对射弹弹道散布影响较大,初始角速度对其影响很小,但较大的初始角速度会带来明显的攻角变化。