机载火控雷达在中远距空战中的抗干扰方法

根据机载火控雷达的性能特点,针对中远距空战面临的电子干扰环境,首先分析和探讨了机载火控雷达的抗干扰技术措施,给出了抗噪声干扰、距离欺骗干扰、速度欺骗干扰、角度欺骗干扰和消极干扰的一些具体方法。然后,从战术使用的角度探讨了机载火控雷达的抗干扰方法,提出了机载火控雷达与欺骗干扰协同、编队协同以及电子防护的战术抗干扰措施。     

蜂窝结构吸波材料的斜入射电磁吸波特性研究

为分析蜂窝结构吸波材料在电磁波斜入射条件下的反射特性,首先基于长波长近似条件下的强扰动理论,得到蜂窝结构吸波材料的等效电磁参数;再利用各向异性分层介质条件下的横向场传播的本征波解,推导出蜂窝结构吸波材料对斜入射电磁波的反射系数公式;进而得到蜂窝结构吸波材料的反射率随入射角的变化关系。反射率的计算结果表明：在特定入射角情况下,对于不同的蜂窝高度,吸收剂存在最优厚度,可使其反射率最小。研究结果对蜂窝结构吸波材料的优化设计具有一定意义。     

某小型无人机中长波辐射特性测量及辐射强度反演

随着“自杀式”无人机集群的饱和式攻击在战场上发挥巨大威力,如何有效拦截是各国近年来研究的重要方向,而红外探测是最热门也是最高效的探测拦截手段之一。为此,开展某典型无人机目标中长波红外探测试验,获取典型某无人机目标辐射特性数据,完成中长波红外辐射强度反演。同时,考虑环境变化对红外探测的影响,为使用红外探测手段完成无人机目标拦截提供实测效果演示。本文研究结果可作为论证中长波对无人机目标探测差异的依据,以支撑探测体制的选择。     

Spatial variation of the supersonic thermal plasma flow downstream of the termination shock

In this paper we start from the most recently observed fact that the solar wind plasma after passage over the termination shock is still supersonic with a Mach number of about 2. To explain this unexpected phenomenon and to predict the evolution of properties of the downstream plasma flow we here consider a two-fluid proton plasma with pick-up protons as a separate suprathermal, second proton fluid. We then formulate a self-consistent system of hydrodynamical conservation equations coupling the two fluids by dynamical and thermodynamical coupling terms and taking into account the effects of newly incorporated protons due to charge exchange with the H-atoms in the heliosheath. This then allows us to predict that in the most probable case the solar wind protons will become subsonic over a distance of about 30 AU downstream of the shock. As we can also show, it may, however, happen that the plasma mixture later again reconverts to a supersonic signature and has to undergo a second shock before meeting the heliopause.     

Report on the Kiso cometary dust trail survey

Cometary dust trails were first observed by IRAS; they are widely known to be the origins of meteoric showers. A new window has been opened for the study of dust trails, using ground-based observations. We succeeded in obtaining direct images of the 22P/Kopff dust trail with the Kiso 1.05-m Schmidt telescope. Following this initial success, we have continued to perform a dust trail survey at Kiso. As a result of this survey, we have detected dust trails along the orbit of six periodic comets, between February 2002 and March 2004. The optical depth of these dust trails are 10⁻⁹ to 10⁻⁸, which is consistent with IRAS measurements. In this paper, we describe the observations and data reduction procedures, and report the brief result obtained between February 2002 and March 2004.     

Possible physical properties of the flow in the vicinity of the heliopause

An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath.     

导体与非导体介质翼型的缩比模型RCS数值计算分析

应用二维电磁散射有限元算法理论考虑了几组导体和非导体介质翼型的缩比计算模型,计算出缩比模型的RCS并与1:1模型进行对比.结果显示,导体翼型的缩比模型RCS计算结果与推及的二维导体外形缩比模型测量定律完全符合;非导体翼型的缩比模型在等效阻抗增大时,按缩比测量定律计算的RCS与1:1模型间的相对误差越来越大,但在等效阻抗小于0.5时缩比定律是有效的.     

论新闻报料

新闻报料具有扩大新闻源、丰富新闻内容、增强新闻地方化色彩、强化媒体舆论监督作用等积极作用,但也弱化了新闻的真实性原则、媒体社会功能与社会责任感,应从建立科学规范的报料核实体制,加强通讯员队伍与新闻线人的建设与培养,加强对媒体及媒体市场的管理等方面来规范新闻报料。     

基于背景纹影技术的随机介质折射率场测量

针对光线通过复杂流场时产生的光传输效应问题,提出了基于背景纹影技术的复杂折射率场测量方法,给出了根据粒子图像偏移量求解折射率场分布的计算方法和推导过程,并对该方法的分辨率与灵敏度进行了理论分析。在此基础上,对火焰上方折射率场的分布进行了实验测量,利用粒子图像测量(PIV)技术对实验图像进行处理。结果表明:实验测量得到的空气折射率最大值为100029,最小值为100009,测量有效值小于00001。表明该方法具有较高的测量精度,能够有效实现复杂折射率场的实时精确测量。      

基体特性对HTPB推进剂力学性能的影响

按工程生产工艺要求,制得hydroxyl terminated polybutadiene (HTPB)固化胶片,通过控制试验环境温度（-50、-35、-20、0、20、35℃）,得到了基于Prony级数形式的具有不同松弛特性的复合基体材料的松弛行为描述,为细观模型的建立提供了必要参数。随后基于分子动力学方法,结合具有内聚本构的黏接单元,建立了推进剂的细观计算模型。为验证所建数值模型的准确性,对固体推进剂在常温条件下进行宏观松弛力学试验,将仿真结果与试验数值的对比,试验结果与仿真结果相差在20%范围之内。最后对具有不同随机分布及不同基体松弛特性的推进剂细观模型进行有限元计算,结果表明:颗粒随机性不影响推进剂的宏观力学行为,而基体松弛特性显著影响固体推进剂的宏观力学性能,基体松弛特性获取环境温度与推进剂的宏观初始模量、延伸率以及强度均呈指数型关系。