基于概率网格Hough变换的多雷达航迹起始算法

 针对常规Hough变换(THT)航迹起始算法采用二元积累的弊端,提出了一种按测量点迹分布概率进行积累的多雷达航迹起始算法。首先把观测空间划分为统一大小的网格,然后根据雷达测量精度计算出观测数据落在每个网格内的概率,进而得到每个网格存在目标的概率,最后的Hough积累采用网格概率进行加权。与常规Hough变换法相比,新算法起始的航迹具有更高的精度和更好的鲁棒性,适合于不同精度雷达的联合航迹起始。仿真结果验证了算法的有效性。     

分支阻抗调配器调配电纳值的计算

在传输线的匹配计算中,需要用到大量的复变量.复数的运算过程极其复杂,所以传统的求解方法是借助于Smith圆图,用图解的方法得到近似解.用Smith圆图法求解的过程也很复杂,容易出错.为此介绍了一种利用MathCAD软件求解分支调配器调配电纳值的方法.与用Smith圆图求解相比,该方法物理概念清楚,求解过程简单,结果精确.     

Solar modulation of galactic cosmic radiation

In this review an attempt is made to present an integrated view of the solar modulation process that cause time variation of cosmic ray particles. After briefly surveying the relevant large and small scale properties of the interplanetary magnetic fields and plasma, the motion of cosmic ray particles in the disordered interplanetary magnetic fields is discussed. The experimentally observed long term variations of different species of cosmic ray particles are summarised and compared with the theoretical predictions from the diffusion-convection model. The effect of the energy losses due to decelaration in the expanding solar wind are clearly brought out. The radial density gradient, the modulation parameter and their long term variation are discussed to understand the dynamics of the modulating region. The cosmic ray anisotropy measurements at different energies are summarised. At high energies (E 1 GeV), the average diurnal anisotropy is shown to be energy independent and along the 18.00 h direction consistent with their undergoing partial corotation with the sun. The average semi-diurnal anisotropy seems to vary with energy as E ⁺¹ and incident from a direction perpendicular to the interplanetary field line, consistent with the semi-diurnal component being produced by latitudinal gradients. Both the diurnal and semi-diurnal components are shown to be practically time invariant. On a day to day basis, however, the anisotropy characteristics such as the exponent of variation, the amplitude and the phase show very high variability which are interpreted in terms of convection and variable field aligned diffusion due to the redistribution of the galactic cosmic ray density following transient changes in the interplanetary medium. The anisotropy observation at low energies (E 100 MeV) are, however, not explained by the theory.The rigidity dependence and the anisotropies during short term variations such as Forbush decreases are discussed in terms of the proposed field models for the interplanetary field structure and are compared with the observed rigidity dependence of long term variations. The data pertaining to the 27 day corotating Forbush decreases and their association with enhanced diurnal variation are also presented. The relationship between the energetic storm particle events which are caused by the acceleration of particles in the shock fronts and the Forbush decreases which are caused by the exclusion of galactic particles by the enhanced field structure in the same fronts are clearly brought out. Thus the recurrent increases at low energies and recurrent decreases at high energies may both be caused by the field structure in the shock front. In conclusion, the properties of the very short period fluctuations (18–25 cph) are summarised.     

跨音速压气机叶栅流动有粘-无粘相互作用的迭代计算

 本文利用较为先进的附面层内法向速度分布等半经验相关式,发展了一种适用于大逆压梯度的附面层积分方法。将激波近似地用大逆压梯度代替,对湍流附面层进行了快速计算,再将求得的附面层参数与无粘主流计算通过建立适当的数学模型结合起来,反复迭代后将计算结果与实验数据及无粘计算的结果比较,可以看出有粘-无粘迭代对无粘计算结果有明显改进。     

Water Vapor Imagery: A New Observation for Weather Analysis

Water vapor imagery is now available routinely from weather satellites for use in meteorological operations. Research during the past 5 years has provided insight concerning the physical interpretation of this data under varying atmospheric moisture and temperature distributions. Investigations have also identified new applications for use in operational weather analysis and forecasting. The water vapor patterns and the changes of these patterns with time, relate to upper tropospheric flow, the jet stream, tropopause breaks, the intensification of thunderstorms, and tropical storm motion. Animated hourly water vapor imagery will become available next year for use by National Weather Service (NWS) field forecasters. It will provide them with a new diagnostic tool for short range forecasts.     

A decade of remote sensing in India — Some salient results

Remote sensing activities in India over the past decade are briefly described in the paper; some important application areas are explained. Some results are highlighted. Activities in India for building remote sensing spacecraft, sensors and ground segment are summarised. Some facilities in India for remote sensing applications including low cost interpretative equipment developed are described. The paper also outlines the Indian Remote Sensing Satellite (IRS) series, the first of which is presently under development for launch in 1986 and the National Natural Resources Management System (NNRMS) under evolution.     

化学镀Ni-Fe-P-B合金的稳定剂醋酸铅研究

用失重腐蚀、电化学和热处理方法,研究了稳定剂醋酸铅对化学镀Ni-Fe-P-B合金的孔隙率、失重腐蚀速率、腐蚀电流密度和硬度等影响。结果表明:当醋酸铅浓度为1.0 mg/L时,Ni-Fe-P-B合金镀层的腐蚀电流密度最小(1.259 mA/cm2),孔隙率最低(0.33个/cm2),失重腐蚀速率最小。经200~600℃热处理后,合金耐蚀性有不同程度的下降,当CPb(Ac)2=1.0 mg/L时,耐蚀性下降程度最小。然而合金硬度和耐磨性提高了(200~400℃),当CPb(Ac)2=1.0 mg/L,400℃热处理后,合金硬度高达939 HV,是镀态的2倍。     

Bispectral analysis of atmospheric radar signals

The bispectral analysis techniques have been applied on signals received from the back-scattered signals by the MST radar. The results of this analysis are compared with that of the conventional power spectral analysis using the Fast Fourier Transform (FFT) technique. Our results showed that there is a significant advantage in using the bispectral technique over the conventional FFT technique. This study focuses on the importance of bispectral analysis in applications to atmospheric signals.     

Comments on “Discrete-time observability and estimabilityanalysis for bearings-only target motion analysis”

Discusses the extensive mathematical analysis carried out by the authors of the original paper [see ibid., vol. 33, no. 1, p. 178-201, 1997] and submits the following points. The authors used pseudo measurements for recasting the observability problem into a linear framework. They treated the bearings-only passive target tracking system as a deterministic system. It is already established that for deterministic systems, the pseudo measurements are linear functions of the states of the system, though the coefficient matrix is a nonlinear function of the original measurements, By using the pseudo measurements in a linear observer, global stability can be shown. However, if the pseudo measurement observer, for which the analysis is mostly carried out by the authors, is used in a noisy environment as a pseudo measurement filter (PMF), biased estimates are arrived at. Hence, though the approach of authors is quite direct and provides insights about the algebraic structure of the BOT problem, as pseudo measurements are used throughout the analysis is not of much use to the TMA community, as the nonlinear measurement equation along with measurement noise are required to be considered in the BOT problem to obtain unbiased results