反舰导弹平面机动突防策略的优化设计

研究了遗传算法在反舰导弹综合突防策略的优化设计方面的应用.反舰导弹的综合突防包括若干个相互承接的环节,首先将反舰导弹的综合突防概率优化问题分解为各个环节突防的条件概率的优化问题,复杂事件得到简化.反舰导弹为了提高突防概率必须做机动,每个环节对应的机动参数取值在一定范围内变化,每个环节的突防概率受到对应的这组参数的影响.选用遗传算法对突防参数进行优化设计.用遗传算法对反舰导弹各个突防环节进行优化设计,找出使每个突防环节突防概率最大的一组参数,进而得到综合突防最优机动参数组合,使反舰导弹的综合突防概率最大.     

The use of an electric field in increasing the resistance of plants to the action of unfavorable space flight factors.

The key role in increasing the resistance of plants to unfavorable space flight factors is assigned to biomembranes of root cells. It is these biomembranes in which numerous biochemical and biophysical processes determining the adaptive capacity of plant organisms occur. In the initial period of exposure to unfavorable space flight factors the adaptation reactions of the plant organism undoubtedly increase its resistance. But the intensification of removal of H+ ions through the plasmalemma with an increase of the external influence sharply raises the quantity of cations leaving the cell, which leads to the accumulation of a considerable quantity of intracellular negative charges. These charges together with negative charges built in the membrane force protons to concentrate on the external surface of the membrane. Since protons have a very strong electric field, they form such a charge of which the electric field is about from several to hundreds of V/cm. The concentration of positive charges of protons entails the formation of a double electric field which extremely impedes the diffusion of other ions. Thus, a proton barrier is formed. Its length can be very considerable due to which the whole process of transmembrane energy and mass-transfer is disturbed. The proton barrier is easily destroyed by a weak electric field created in the root zone. In experiments on electrostimulation of different plants under space flight conditions at the orbital station MIR the absorption of nutrient elements by the root system increased to the optimal level, the ratio of physiologically active substances in the rhizosphere was normalized, the content of chlorophyll, carotin, and ascorbic acid in leaves corresponded to the ground-based control. Understanding of the mechanism of formation of a proton barrier on the plasmalemma of root cells as a result of the response of plants to the negative action of external factors (microgravity) is of great importance. It allows the possibility of life support of the vegetable kingdom in extreme conditions to be estimated in a new way.     

铲挖式表层月壤采样器设计与试验

针对月球表层土壤的采样任务,设计了一种搭载于机械臂末端的采样器。基于离散元手段,利用Scott真实月壤微型三轴压缩试验数据,完成仿真散体颗粒特性参数匹配,开展了采样器铲取、挖取采样过程的仿真分析,获得作业过程采样器的动力学特性。此外,开发了采样器性能测试系统,针对不同模拟月壤对象进行了采样试验,测试获得了采样器采样能力随深度及月壤硬度的变化情况,得到采样器操作参数的可行区域。采样器能够实现铲取、挖取和封装容器转移多重任务,研究工作为中国未来的月面采样任务提供方案借鉴和技术支撑。     

载人运输飞船流体回路方案研究

流体回路是载人运输飞船热控分系统的重要组成部分,结合飞船所采取的其他热控措施,流体回路必须满足各种可能出现的热工况要求,同时尽量少占用飞船的资源。在进行分析和比较的基础上,确定流体回路的方案和系统配置,结合对接目标的热设计,重点解决与目标停靠期间的热控问题。文中介绍了载人运输飞船流体回路的主要设计要求及考虑重点,在能量平衡分析的基础上设计了两种流体回路方案,并进行了热分析计算和性能比较,对流体工质的选择也提出了建议。     

磁尾等离子体团型结构的数值模拟

考虑横越磁尾不同区域的数密度与离子温度的分布特点,取宁静磁尾温度、密度呈同样形态的非均匀分布,作为模拟计算的初态,对初始By为不同分布的3个算例作模拟计算．数值结果展示了3类磁结构的演化特征．考察磁尾中性片一个给定点的磁场变化,做出3个算例典型事件的磁场矢端图．它们从另一个侧面展示了磁尾通量绳型等离子体团、具有复杂闭合磁力线位形类似于“闭合环”的等离子体团,以及二维“磁岛”型等离子体团的特点．观测表明,多数磁尾等离子体团为具有强核心场的通量绳结构．通过跟踪一个通量绳型等离子体团的发展,作出等离子体团各方向速度与磁场强度随x演化的曲线．其中,vx与磁场强度|B|在近尾至中尾的计算值与Geotail卫星资料统计分析结果大致相符．此外,与Jin等取初始温度为均匀分布的计算结果相比,本文给出的通量绳型等离子体团,其内温度较高、密度较低,与资料分析结果的偏离也随之减小．     

VHF/UHF波段发射机互调抑制比测试方法研究

建立了发射机射频电路简化模型,并利用该模型和非线性多项式模型,研究了发射机互调(IM)发射电平与射频前端滤波器插入损耗、干扰信号功率和频率偏差之间的关系,对当前发射机互调抑制比的定义进行了修正;分析了传统发射机互调抑制比测试方法的局限性,设计了一种新型的发射机互调测试链路配置,分析了测试链路关键物理参数间的关联关系,建立了测试数据处理模型,该方法扩宽了测试带宽和功率范围,降低了对测试器件的要求。对实际电台的测试结果表明,本文提出的理论分析结论和发射机互调抑制比测试方法正确有效。     

System Design for the Event Horizon Imaging Experiment Using the PECMEO Concept

The concept for space interferometry from Polar or Equatorial Circular Medium Earth Orbits (the PECMEO concept) is a promising way to acquire the image of the “shadow” of the event horizon of Sagittarius A* with an angular resolution of circa 5 microarcseconds. The concept is intended to decrease the size of the main reflector of the instrument to about 3 m using a precise orbit reconstruction based on Global Navigation Satellite System (GNSS) navigation, inter-satellite range and range-rate measurements, and data from the Attitude and Orbit Determination System (AODS). The paper provides the current progress on the definition of the subsystems required for the concept on the basis of simulations, radio regulations, and available technology. The paper proposes the requirement for the localization of the phase centre of the main reflector. The paper provides information about the visibility of GNSS satellites and the needed accuracies of the AODS. The paper proposes the frequency plan for the instrument and its Inter-Satellite Links (ISLs). The concepts for measurement of range and range rate using ISLs (as well as for the data exchange at these ISLs) are presented. The block diagram of the interferometer is described and its sensitivity is estimated. The link budget for both ISLs is given as well as their critical components. The calculated measurement quality factors are given. The paper shows the expected performance of the sub-systems of the interferometer. The requirements for the localization of the main reflectors and the information about the availability of the GNSS satellites are based on the simulations results. The frequency plan is obtained according to the PECMEO concept and taking into account the radio regulations. The existing technology defines the accuracies of the AODS as well as the link budgets and the measurement accuracies for both ISLs and the sensitivity of the instrument. The paper provides input information for the development of the orbit reconstruction filter and the whole PECMEO system.      

基于有限元3-RPS并联机床轻量化优化设计

为了减轻3-RPS并联机床质量,提高其刚度,分别对静平台与支链进行了结构改进.采用连接单元模拟机床中运动副,对并联机床静刚度进行有限元分析.通过分析结果获得静平台的刚度薄弱环节、支链的变形及其对机床变形的影响规律.在静平台刚度薄弱处增加抵抗变形的筋板,并通过减小其框架尺寸的方式优化静平台结构.采用悬臂梁模型分析支链的变形,以支链质量和变形乘积最小对支链进行尺寸优化.改进后的并联机床质量显著减轻,机床变形明显减小.优化结果能够提高机床动态响应性能以及机床精度.     

Adaptation of the bottomside electron density profile of the IRI model to data of topside radiosounding

A method is proposed for reconstructing the electron density profiles N(h) of the IRI model from ionograms of topside satellite sounding of the ionosphere. An ionograms feature is the presence of traces of signal reflection from the Earth's surface. The profile reconstruction is carried out in two stages. At the first stage, the N(h) –profile is calculated from the lower boundary of the ionosphere to the satellite height (total profile) by the method presented in this paper using the ionogram. In this case, the monotonic profile of the topside ionosphere is calculated by the classical method. The profile of the inner ionosphere is represented by analytical functions, the parameters of which are calculated by optimization methods using traces of signal reflection, both from the topside ionosphere and from the Earth. At the second stage, the profile calculated from the ionogram is used to obtain the key parameters: the height of the maximum hmF2 of the F2 layer, the critical frequency foF2, the values of B0 and B1, which determine the profile shape in the F region in the IRI model. The input of key parameters, time of observation, and coordinates of sounding into the IRI model allows obtaining the IRI-profile corrected to real experimental conditions. The results of using the data of the ISIS-2 satellite show that the profiles calculated from the ionograms and the IRI profiles corrected from them are close to each other in the inner ionosphere and can differ significantly in the topside ionosphere. This indicates the possibility of obtaining a profile in the inner ionosphere close to the real distribution, which can significantly expand the information database useful for the IRTAM (IRI Realmax Assimilative Modeling) model. The calculated profiles can be used independently for local ionospheric research.     

星载光学敏感器受天体干扰的可能性分析

各种用途的星载光学敏感器均可能受到日、月、地等天体进入敏感区所形成的干扰.对光轴固定于星体的星敏感器,以及光轴在空间中保持方位不变的天文望远镜两类星载光学敏感器,根据敏感锥面和天体锥面之间的空间位置关系,导出了天体干扰的发生条件,给出了预测干扰发生时间的实用计算公式.      

小行星防御动能撞击效果评估

以动能撞击防御潜在威胁小行星概念为背景,采用物质点法(Material Point Method,MPM)模拟了铝弹高速撞击S型小行星的过程,将撞击结果导入引力N体–离散元动力学模型中,对其后续演化过程进行仿真,并分析了撞击后碎片对地球的威胁指数。结果显示小行星在高速撞击的作用下部分破碎,大量碎片以与撞击方向相反的速度向外喷射,从而提升了小行星的撞击偏移效果。研究采用了两种不同结构的小行星模型:完整结构(monolithic structure)的小行星在遭受撞击后会喷射出比原小行星小得多的碎片,而碎石堆结构(rubble-pile structure)的小行星在撞击作用下可分裂成大小和速度分布较为均匀的碎片。威胁指数的分析表明动能撞击方式确实有效减小了小行星的威胁程度,撞击后的最大剩余碎片可被成功偏移至安全轨道,但仍有部分碎片会与地球相撞。与完整结构相比,针对碎石堆结构小行星的撞击防御的总体效果更好,次生灾害主要为大质量碎片的撞击。研究方法可用于未来开展防御小行星的动能撞击任务的撞击条件选择和撞击结果预估。     

挤压油膜阻尼器失效的判据

 挤压油膜阻尼器(简称SFD)设计不当,会导致功能失效.对弹支-挤压油膜阻尼器来说,失效有2种形式:一是过不了临界,即转子系统的振幅随转速的上升而一直增大;二是出现双稳态特性.2帧失效判据图已经作出:一是双稳态区域图,只要轴承参数和质量偏心率数组不选在双稳态区域内,便不致产生双稳态特性;二是减振失效边界图,只要前述数据组不在失效边界的一侧,便不致产生过不了临界的现象.经实验证明,上述结论从正反2个方面看都是正确的.实验也进一步确认了挤压油膜阻尼器优越的减振功能.     

气泡雾化喷嘴的试验研究

进行了组不同结构形式的气泡雾化喷嘴的试验研究，初步试验结果表明：这种新型喷嘴对液体介质粘度不敏感，在小气液比条件下获得了很好的雾化效果，雾化性能明显优于从国外引进的某些空气雾化喷嘴，该成果已于１９９３年２月７日被授予中华人民共和国实用型专利。     

类X-20高超声速飞行器反馈线性化控制研究

通过对类X-20高超声速飞行器的气动系数与高度、马赫数、攻角、侧滑角和舵偏角的关系进行分析,对各项气动系数进行了简化和拟合,并将舵偏增量视作控制输入,在此基础上建立了类X-20飞行器仿射非线性形式的控制模型,证明了它是可以输入输出精确线性化的,从而可以设计反馈线性化控制器.最后在存在大气密度、气动力矩系数和转动惯量不确定性情形下,针对原动力学模型进行闭环仿真研究,原动力学模型考虑地球旋转,气动数据直接从类X-20飞行器的气动数据表插值得到.仿真结果表明,所设计的控制律可以实现控制目标,具有较强鲁棒性.     

Design of a formation of solar pumped lasers for asteroid deflection

This paper presents the design of a multi-spacecraft system for the deflection of asteroids. Each spacecraft is equipped with a fibre laser and a solar concentrator. The laser induces the sublimation of a portion of the surface of the asteroid, and the resultant jet of gas and debris thrusts the asteroid off its natural course. The main idea is to have a formation of spacecraft flying in the proximity of the asteroid with all the spacecraft beaming to the same location to achieve the required deflection thrust. The paper presents the design of the formation orbits and the multi-objective optimisation of the formation in order to minimise the total mass in space and maximise the deflection of the asteroid. The paper demonstrates how significant deflections can be obtained with relatively small sized, easy-to-control spacecraft.     

Kinetic characteristics of the theoretical ecosystems with different extent of openness.

In this paper, the influence of the extent of openness of ecosystem that is defined by the dilution rate, which characterizes the extent of flowage of the pond, on the intensity of the biotic circulation in ecosystems with different regulation types, number of trophic links and extent of closing has been investigated. We considered open systems, we took into account the return of the limiting substances, such as nitrogen and phosphorous, into the cycle by degradation of detritus and products of vital functions of consumers. It was shown by the numerical calculations that the increase of the dilution rate in without recycle ecosystems leads to increase of the net primary production up to the maximum value corresponding to the two-link trophic chain (biogenic substance and producer) and then, to gradually decrease. The residual concentration of biogenic limiting substances monotone increases. Net primary production and residual concentration of biogenic limiting substances in systems with recycle with even number of links behaves similarly to that in without recycle ecosystems. In the systems with recycle with the odd number of links that values lies on the stable level. We showed that in wide range of the dilution rate the recycling of the ecosystem can highly increase the net primary production and reduce residual concentration of biogenic limiting substances. The influence of the dilution rate on numbers of links that may exist in the system was analyzed.     

载人航天器的再入制导控制与仿真计算

研究了弹道一升力式载人航天器的再入制导规律和各种再入误差源对其落点的影响。主要包括以下内容：再入纵向制导和侧向制导规律的确定;分析各种单项误差对落点的影响;用ＭｏｎｔｅＣａｒｌｏ方法模拟各种再入误差源及其对落点偏差的综合影响。通过大量的模拟计算,掌据各种再入误差对落点偏差的影响,提出再入误差应具有的指标要求,并得到一些有益的结论。计算结果表明,确定的制导规律可以达到满意的落点控制效果。     

曲面幕墙清洁机器人攀爬技术

针对国家大剧院超椭球外表面的清洗问题,设计了一种新型自攀爬机器人.机器人具有全方位运动能力,相对于擦洗运动而言,攀爬运动是影响机器人作业安全性的主要因素.分析了攀爬运动的运动学模型,利用拉格朗日方法对该状态下的动力学问题进行了研究,并针对攀爬运动的特殊性,对机器人前后俯仰支撑控制问题进行分析,结合建筑物表面特点并依靠仿真,得到机器人作业过程中俯仰机构受力分布曲线,为机器人攀爬支撑力的切换提供了理论依据.      

Modeling and identification of an electro-mechanical system: The LISA grabbing positioning and release mechanism case

In the frame of space missions, mechanisms often constitute critical systems whose functionality and performance need to be tested on ground before the mission launch. The LISA scientific space mission will detect gravitational waves by measuring the relative displacement of pairs of free-floating test masses set into geodesic motion onboard of three spacecrafts. Inside each satellite, the injection of the test masses from the caged configuration into the geodesic trajectory will be performed by the grabbing positioning and release mechanism. To provide a successful injection, the test masses must be dynamically released with a minimal residual velocity against adhesion with the holding device. A parameter that determines the test mass residual velocity is the quickness of the retraction of the holding device. The need arises then to characterize the dynamic response of the release mechanism in order to predict its behaviour in the in-flight conditions. Once a validated model of the mechanism is available, the compliance of the system to the tight requirement on the maximum allowed residual velocity of the test mass may be verified. Starting from an electro-mechanical model of the mechanism dynamics, this paper presents the results of the experimental identification of its relevant parameters.     

Dust hazard near Halley Comet in case of the VEGA project

The motion of dust particles near Halley Comet is studied and the probability of dust impacts with the spacecraft in case of the VEGA (Venus-Halley)- project is determined. The formation of a crater due to a particle impact with the dust shield is considered and the necessity for using a dual-sheet bumper shield is substantiated. The thickness of a front sheet that plays a role of the particle evaporator is estimated theoretically. The numerical experiment is carried out that simulates the dynamics of collision and evaporation of a particle. Three factors causing perforations of the rear sheet are discussed, i.e. dust penetrated through holes in the front sheet, gas jets and spall fragments of the front-sheet. The consideration of these factors makes it possible to estimate basic parameters of the dual-sheet bumper shield. Flexural vibrations of the front sheet under action of the reverse gaseous jet from the rear sheet are discussed that can affect essentially the shield strength. The perturbing effect of the dust and gas fluxes on the spacecraft is studied.