基于小波倒谱模型的滤波处理技术及其在超声应力检测中的应用

在超声检测中,应力是通过超声时间延迟来测量的,而超声回波的时间延迟对噪声非常敏感。噪声严重影响应力的测量精度,噪声引起的时间延迟甚至与应力引起的时间延迟处于同一量级。而以往消噪处理都是基于盲信息,没有考虑系统响应特点,消噪效果不好,需一种有效的消噪方法。提出了一种基于倒谱模型新的滤波处理技术,从系统响应的角度,建立超声通道的小波倒谱模型,并通过对钢轨应力测试信号进行滤波处理,试验结果令人满意。     

纳秒级脉冲照射下隐身飞行器的隐身效果分析

为研究冲激雷达的反隐身潜力,首先用时域有限差分方法(FDTD)和解析方法计算了电磁波垂直入射时涂敷窄带雷达吸波材料(RAM)和涂敷等离子体的金属平板的反射率,然后用FDTD仿真了在纳秒级双高斯脉冲照射下某金属缩比隐身飞机模型,及其涂敷窄带RAM及涂敷等离子体的散射特性。结果表明,在低频区外形隐身的隐身效果不明显,RAM和等离子体的吸波效果较差。这证实了发射纳秒级脉冲信号的冲激雷达具有反隐身的潜力。     

Interaction of artificially injected plasma flows with ionospheric plasma

Results of rocket experiments on study of plasma flows (PF) artificially injected by sources separated from vehicles and their effect on medium parameters in ionosphere at altitudes 160:230 km are presented.PF were injected comprising lithium ions with velocities 1,2 x 10⁴ m/sec. and cesium-potassium ions with velocities (1,4–1,5)x10³ m/sec. Mass flow rate in case of lithium PS is 2 mg/sec, and in case of cesium-potassium PS is 0,2 g/sec. During experiments mass-spectrometer measurements of ion medium content in ranges of different ion masses were held, disturbancies of electric fields with frequencies up to 20 kHz and electron flows with energies 0,7keV, 4,6keV and over 40 keV were controlled at distancies from 150m to (500–600)m between plasma source and scientific equipment.     

A solar type U burst in the decimetric range

This paper analyzes a Type U burst at 1.0 – 2.8 GHz which occurred between 12:36:26 – 12:36:32 UT on 1992 August 22, observed by Ond ejov Observatory, Czech Republic. This may be the first example of Type U bursts in the decimetric range, as far as we know. From analysis we came to the following conclusion: (1) The frequency drift rates of the ascending and descending branches are 1.25 and 0.225 GHz/s, respectively, and the velocities of the electron beam are 0.38 c and 0.26 c, respectively; (2) The burst decay of the ascending branch is larger than that of the descending branch; (3) The variations of the maximum frequencies of instantaneous spectra with time appear as from the highest (1.92 GHz) to the lowest (1.0 GHz), then toward higher frequency (1.53 GHz) (this is consistent with that predicted by plasma emission theory); (4) The bandwidths of the ascending branch are about twice that of the descending branch (this may be caused by the larger drift rates of the ascending branch); (5) The temperature of the coronal loop apex is 6.3 × 10⁶ K; (6) The magnetic field at the top of the loop is greater than 9.2 G; (7) This U burst emission is plasma radiation at the second harmonic.     

Effects of prolonged exposure to space flight factors for 175 days on lettuce seeds

We have studied the effects of prolonged (up to 175 days) exposure of $\text{Lactuca sativa}$ seeds to space flight factors, including primary cosmic radiation heavy ions. The data obtained evidence a significant fourfold increase ofs pontaneous mutagenesis in seeds both with regard to the total number of aberrant cells as well as the formation of single cells with multiple aberrations. Comparison of the present experiment with earlier works shows that the frequency of such aberrations increases with the duration of the flight.     

Fluxes of Quasi-trapped Electrons with Energies >0.08 MeV in the Near-Earth Space on Drift Shells <Emphasis Type="Italic">L</Emphasis> < 2

We study the characteristics of fluxes of electrons with energy >80 keV in the near-Earth space regions corresponding to the drift shells L = 1.7, 1.4, and 1.1 observed during the entire period of the GRIF experiment onboard the Spectr module of the Mir orbital station from October 1995 to June 1997. The obtained geographic maps of the distribution of electron fluxes at the height of the station flight (400 km) and, also, the estimates of the spectra indicate that the South-Atlantic Anomaly provides for a mechanism of stable replenishment for shells with L < 1.5. The mechanism of stable replenishment of shells with L < 1.5 may be due to the scattering, in the residual atmosphere, of electrons from the inner radiation belt precipitating into the region of the South-Atlantic Anomaly.     

The waves observed in the ARAKS-East experiment

Experimental results of the Wave measurements over frequency range 0.1–5.0 MHz during the second launch of the ARAKS Experiment (15.02.75) are reported. The differences between the results of the first and the second launches are discussed.     

平板上钝缘舵在超声速绕流中的三维分离特性研究

对于平板上的直立钝缘舵在M_∞=1.79、2.04和2.50的条件下,研究了该平板干扰区中的三维分离特性。着重讨论了钝缘直径、舵面迎角和来流马赫数对主分离线位置和形状的影响。分析了该类三维分离在性态上更强地依赖于无粘流动特性。此外,还对分离区内的二次分离发展过程和形态进行了初步讨论。     

宽带无线接入技术

介绍了两种宽带无线接入技术：本地多点分配业务(LMDS)和自由空间光通信(FSOC)。它们各具特色。前者将新兴的LMDS技术引入无线接入网,而后者是实现无线宽带接入的另一种途径。