低空逃逸小RCS目标PD雷达探测技术C

雷达面临的挑战之一是来自于对低空逃逸微弱目标的探测。现代军事逐渐向低空领域扩展,超低空逃逸技术也在日益发展,促使对低空逃逸微弱目标检测技术研究的地位日益提升。雷达对低空微弱目标进行下视探测时,目标的低空和超低空飞行致使雷达接收的回波功率变弱,被淹没在强烈的背景杂波中。与传统脉冲多普勒PD（Pulse-Doppler）雷达不同,合成宽带脉冲多普勒雷达可以同时实现距离和速度的二维高分辨,并且具备良好的相参性和抗干扰性能。针对低空飞行目标的特点进行定性定量分析,对探测所遇到的杂波环境进行仿真验证,提供了一种基于合成宽带脉冲多普勒雷达低空逃逸小雷达截面积RCS目标的探测方法,并对参数设计进行优化分析,降低漏探概率。     

低副瓣有源相控阵天线测试方法研究

利用平面近场测试系统的口面场全息反演功能,摸索出一种低副瓣有源相控阵天线的优化测试方法。实测天线副瓣电平低于-30dB,达到设计指标要求,证明了方法的有效性和适用性,为更快更好完成有源相控阵天线的研制提供了技术手段。     

一种低轨双星雷达信号无模糊频差估计算法

针对低轨双星组合接收低脉冲重复频率(LPRF)雷达信号的频差(DFO)估计存在模糊的问题,提出一种基于时差差分的频差无模糊高精度估计算法,该算法通过对高精度的时差测量值进行中心差分获得无模糊的频差估值。仿真结果表明,新算法能对PRF低至300 Hz的雷达信号进行无模糊的频差估计,估计精度在信噪比高于15 dB时逼近克拉美劳下界,可有效扩大低轨双星时/频差定位系统对LPRF信号的适用范围。     

中国运载火箭技术发展

中国航天运输系统建设起步于20世纪60年代,经过近50年的发展,取得了举世瞩目的成就,建设了布局合理、覆盖全面的空间运输系统体系,能够将不同有效载荷发射到低、中、高不同轨道。国际合作方面,在搭载发射、商业卫星发射服务和在轨交付3个方面也取得了一定成绩。对中国航天运输系统发展成就进行了总结,对航天运输系统未来发展特别是人工智能技术应用进行了展望。     

首颗自主地月转移微卫星“龙江二号”

本文对世界首颗独立完成地月转移、近月制动、环月飞行的微卫星“龙江二号”进行了介绍。首先阐述了龙江二号的任务目标和总体方案;然后重点分析了轨道设计与控制、复杂电磁干扰的标定与抑制、宽视场三维基线干涉测量等关键技术难点;接着回顾了任务的实施过程;最后详细介绍了低频射电探测仪、沙特光学相机和VHF/UHF通信模块与学生微型CMOS相机等有效载荷,并展示了上述载荷获取的初步成果。     

Effects of in-track maneuver on Sun illumination conditions of near-circular low Earth orbits

By developing approximate analytical models considering the J₂ perturbation, the effects of an in-track maneuver on the orbital Sun illumination conditions of near-circular low Earth orbits are analyzed. First, two approximate models for the variations in orbital sunshine angles are developed, one for variations at a given time and the other for variations at a given argument of latitude. Next, two approximate models for variations in orbital arc in Earth shadow are developed, one considers the small eccentricity and the other uses the zero eccentricity. Finally, the developed approximate models are applied to analyzing the Sun illumination conditions of a typical in-track maneuver mission on a near-circular low Earth orbit. From the results obtained, three major conclusions can be drawn. First, the variations in orbital sunshine angles at a given time may reach tens of degrees when the drifting time reaches hundreds of orbital periods, and the approximate model for that situation cannot effectively approach the numerical results. Second, the variations in orbital sunshine angles for any given argument of latitude are only a couple of degrees even when the drifting time reaches 500 orbital periods, and the approximation model developed can effectively approach the numerical results. Third, for variations in orbital arc in Earth shadow, the approximate model considering the small eccentricity has simple expressions and can effectively approach the numerical results; in contrast, the approximate model using the zero eccentricity has relatively worse precision.     

A theoretical model of semi-elliptic surface crack growth

A theoretical model of semi-elliptic surface crack growth based on the low cycle strain damage accumulation near the crack tip along the cracking direction and the Newman–Raju formula is developed. The crack is regarded as a sharp notch with a small curvature radius and the process zone is assumed to be the size of cyclic plastic zone. The modified Hutchinson, Rice and Rosengren(HRR) formulations are used in the presented study. Assuming that the shape of surface crack front is controlled by two critical points: the deepest point and the surface point.The theoretical model is applied to semi-elliptic surface cracked Al 7075-T6 alloy plate under cyclic loading, and five different initial crack shapes are discussed in present study. Good agreement between experimental and theoretical results is obtained.     

轻质隔热纳米孔结构耐烧蚀酚醛材料

在一定温度下,通过改性剂组分与热固性钡酚醛树脂之间热共聚反应,制备了改性酚醛树脂。采
用模压工艺制备出具有目标尺寸和形状的改性酚醛树脂固化物,对该样品分别进行了400 和700℃的炭化处
理,得到了相应的酚醛炭化样品,并测试其密度、失重率、收缩率等特征参数。研究改性剂用量对碳化物特征参
数和性能的影响,如密度、失重率形貌、比表面积、隔热性能、压缩强度等。SEM 研究表明,700℃炭化后样品形
成了“珊瑚状”碳结构,形成了30 ~150 nm 纳米孔。比表面积测试(BET)结果表明其比表面积可达464 m2 / g。
隔热性能与力学性能的测试结果表明,相对于未改性酚醛树脂碳化物,改性酚醛碳化物的热导率降低了
45． 57%,并且保持了较好的压缩强度。     

One-to-one relationship between low latitude whistlers and conjugate source lightning discharges and their propagation characteristics

One-to-one relation with its causative lightning discharges and propagation features of night-time whistlers recorded at low-latitude station, Allahabad (geomag. lat. 16.05°N, L = 1.08), India, from continuous observations made during 1–7 April, 2011 have been studied. The whistler observations were made using the Automatic Whistler Detector (AWD) system and AWESOME VLF receiver. The causative lightning strikes of whistlers were checked in data provided by World-Wide Lightning Location Network (WWLLN). A total of 32 whistlers were observed out of which 23 were correlated with their causative lightnings in and around the conjugate location (geom. lat. 9.87°S) of Allahabad. A multi-flash whistler is also observed on 1 April with dispersions 15.3, 17.5 and 13.6 s^1/2. About 70% (23 out of 32) whistlers were correlated with the WWLLN detected causative lightnings in the conjugate region which supports the ducted mode of propagation at low latitude. The multi-flash and short whistlers also propagated most likely in the ducted mode to this station.     

Evolution of binaries with chemically peculiar primaries

The chemically peculiar (CP) stars are classified into subgroups based on the type of peculiarities. A significant fraction of these are known to be binaries. The faster evolution of the massive component leads to a white dwarf or a neutron star. Further evolution of the binary is analysed taking into consideration, the orbital parameters, effect of magnetic field, spectroscopic peculiarities and finally the statistics of CP binaries and Low Mass X-ray Binaries (LMXB).

The possible consequences of the evolution to lead to the formation of Magnetic Cataclysmic Variables (MCV) and LMXB are discussed.