Analysis on Potential Conflict Frequency of Intersected Air Routes in Terminal Airspace Design

In order to obtain accurate conflict risks in terminal airspace design, the concept and calculation model of potential conflict frequency for intersected routes are proposed. Conflict frequency is represented by the product of horizontal conflict frequency and vertical conflict probability. The horizontal conflict frequency is derived from the probability density distribution of conflicts in a period of time. Based on the recorded radar trajectory data, the concept and model of ROUTE distance are proposed, and the probability density function of aircraft height at a specified ROUTE distance is deduced by kernel density estimation. Furthermore, vertical conflict probability and its horizontal distribution are achieved. Examples of three intersected arrival and departure route design schemes are studied. Compared with scheme 1, the conflict frequency values of the other two improved schemes decrease to 53 % and 24%, respectively. The results show that the model can quantify potential conflict frequency of intersec ted routes.     

无需辅助数据的分布式目标自适应检测器

在非高斯背景和没有辅助数据的条件下,研究了高分辨率雷达分布式目标的自适应检测问题.首先采用有序检测理论和协方差矩阵的迭代估计方法粗略估计散射点集合,进一步利用迭代估计方法获得协方差矩阵的近似最大似然估计,提出了无需辅助数据的自适应检测器(ADWSD).ADWSD在非高斯背景下具有近似恒虚警率特性,且检测性能远好于修正的...     

STUDIES ON MAGNETIC ABRASIVE MACHINING

磁性磨料磁力研磨是近年发展起来的一种高效率、高质量的抛光方法，能够加工复杂外形工件和各种内壁、内腔表面，具有加工装置易于控制、工作环境清洁、加工成本低等优点，具有广阔的应用前景。本文设计、制造了加工装置并进行了一系列的试验，在研磨过程各主要参数对研磨的影响作了研究。试验结果表明，研磨初期加工效率较高，但随着研磨时间的延长，研磨效率降低，研磨质量提高不多；工件转速越高，研磨效率越高，而对研磨质量则没有影响；研磨存在最佳的加工间隙与电流强度值，在此条件下，研磨效率高，研磨质量也较好。本文最后对加工机理作了理论分析，认为磁极的设计与制造研磨能力好、磁性强的磁性磨料是非常重要的。     

近距鸭翼高度对鸭翼－前掠翼布局纵向气动特性影响的实验研究

前掠翼布局由于其潜在的优越性,在未来战斗机的研究设计中将占有日益重要的地位.本文通过风洞测力实验,研究了近距鸭翼相对于前掠主机翼的高度对布局纵向气动性能的影响.实验结果表明:随着主机翼前掠角的增大,近距鸭翼布置高度逐渐增加可获得较好的气动特性.     

基于星座恢复法降低PAPR的性能分析

提出了一种新的降低峰均功率比(Peak-to-average ratio,PAPR)的方法——星座恢复法.在发送端采用软件削波限幅的方法来降低系统的峰均比,其系统结构简单、且可根据系统的要求灵活地改变PAPR值;在接收端根据调制信号的星座特性恢复出被限幅数据的实际值,从而减小了信号的畸变,提高了系统的误码性能.为了使星座恢复法更具实用性,对其算法进行了简化,从而大大地减少了系统的运算量.理论分析和仿真结果表明:与选择性映射法(Selective mapping,SLM)相比,基于星座恢复法的正交频分复用(Orthogonal frequency division multiplexing,OFDM)系统,其误码性能得到了明显的改善,算法较简单,且无需额外信道来传送附加信息.     

燃气的基准表及图制定

本文在阐述基准的热力学概念基础上,提出了燃气基准的计算方法,应用CHAPPELL推荐的有关燃气热力性质表达式,导出计算燃气基准的公式,通过微机计算,将结果整理成燃气基准的有关表、图。     

Ionospheric electron density over Resolute Bay according to E-CHAIM model and RISR radar measurements

In this study, predictions of the E-CHAIM ionospheric model are compared with measurements by the incoherent scatter radars RISR at Resolute Bay, Canada, in the northern polar cap. Reasonable coverage was available for all seasons except winter for which no conclusions were drawn. It is shown that ratios of the model-to measured electron densities are close to unity in the central part of the F layer, around its peak. This is particularly evident for summer daytime. Distributions of the ratios are wider for other seasons indicating larger number of cases when the model underestimates or overestimates. E-CHAIM underestimates the electron density at ionospheric topside and bottomside by ～ 10–20 %. At the bottomside, the underestimations are strongest in summer and equinoctial nighttime. At the topside, the underestimations are strongest in autumn nighttime. Model overestimations are noticeable in the middle part of the F layer during dawn hours in autumn. Overall, the model tends to not predict highest-observed peak electron densities and the largest-observed heights of the peak.     

大展弦比飞翼作战飞机横航向飞行品质特性

基于MIL-STD-1797A飞行品质规范,开展了针对大展弦比飞翼作战飞机滚转轴和偏航轴飞行品质特性的研究.随着控制系统对系统动态特性调节作用的日益增强,由飞机构型所引起的动态响应特性差异已变得越来越小,飞翼飞机的闭环滚转模态、螺旋模态、滚转-螺旋耦合振荡、荷兰滚模态、驾驶员座位处的侧向加速度等均可达到较好的飞行品质,但稳态配平特性主要受构型的影响,不能完全满足飞行品质的要求;分析了大展弦比飞翼作战飞机在快速滚转、侧风起降和非对称推力情形下的对滚转轴和偏航轴操纵效能的要求,由于气动构型和操纵面配置等差异,大展弦比飞翼作战飞机在完成某些飞行任务时对操纵效能的需求与常规构型的飞机存在着较大差异.     

吹风比和曲率对旋转曲面气膜冷却效率影响

采用数值模拟方法,对旋转状态下曲率表面的气膜冷却进行研究.通过不同的曲率半径和吹风比,得到了冷却效率的分布情况,从而获得吹风比和曲率两因素对气膜冷却效率的影响规律.研究结果表明:低吹风比下,冷却效率较好;高吹风比下,气膜容易脱离壁面;凸表面的冷却效率随着曲率半径的增加而逐渐减小;而凹表面的冷却效率随着曲率半径的增加而逐渐增大;凸表面上曲率的影响作用随着旋转数的增加而逐渐弱化;而凹表面上曲率的作用随着旋转数的增大而逐渐增强.     

Study of maximum electron density NmF2 at Karachi and Islamabad during solar minimum (1996) and solar maximum (2000) and its comparison with IRI

The monthly hourly medians of maximum electron density, N_mF₂, at two Pakistani ionospheric stations, Karachi and Islamabad, have been determined for solar minimum (1996) and solar maximum (2000) and compared with IRI predictions using the URSI coefficients. At night and pre-noon period the N_mF₂ values at both stations are almost equal during the 2 years. However, at post-noon the values at Karachi are considerably larger than those at Islamabad due to the equatorial or geomagnetic anomaly. Karachi (geomag. coord. 16.44°N, 139.08°E) lies near the region of the equatorial anomaly (+20 and −20 geomagnetic latitude), so most of the N_mF₂ values at Karachi are larger than those at Islamabad (geomag. coord. 24.46°N, 145.67°E). The maximum monthly values of N_mF₂ show a semi-annual variation at Karachi and Islamabad both during 1996 and 2000 as predicted by IRI.