航天器近地空间环境效应综述

空间环境是影响航天器飞行的重要因素之一。文章在总结近地空间环境含义的基础上,按形成因素对近地空间环境进行分类,并详细分析了辐射环境、摄动环境、磁场环境、等离子体环境、微流星体和冷黑环境及其对近地空间航天器的效应。     

基于常规多普勒滤波器组结构的合成宽带距离像性能分析

为了消除散布效应对宽带信号的不利影响,可以利用多个窄带信号合成宽带信号;同时,通过在子带内处理相干脉冲串,可进行杂波抑制、目标速度估计和区分不同速度的目标。然而,在子带内分别使用常规多普勒滤波器组,会引进多普勒散布效应所造成的输出失配误差,从而造成合成距离像的失真。分析了多普勒散布效应与子带常规多普勒滤波器组输出失配之间的关系,推导了运动目标通过滤波器组后所成高分辨距离像的距离走动公式,给出了适合子带常规多普勒滤波器组的目标速度临界值。仿真实验验证了以上结论。     

Effects of a hot jet on detonation initiation and propagation in supersonic combustible mixtures

The effects of a hot jet on detonation initiation and propagation in supersonic combustible mixtures has been studied with two-dimensional numerical simulations with the open-source program AMROC that uses a block-structured adaptive mesh refinement method. Results indicate that the hot jet could ignite the detonation effectively in supersonic combustible mixtures like a pneumatic ramp. After the realization of the detonation initiation, the hot jet can still play an important role on the detonation propagation during its continuous ejection. For a hot jet with certain diameter, it can result in an overdriven detonation with almost constant overdrive degree. After the shutdown of the hot jet, the stable CJ detonation combustion was realized finally in the supersonic combustible mixtures. With the re-ejection of the hot jet, the failed detonation could be reinitiated quickly. Through the control of the re-ejection of the hot jet, it plays a key role not only in the initiation process, but also in the subsequent continuous detonation combustion period.     

Mapping orbits around the asteroid 2001SN263

The present paper has the goal of mapping orbits, with respect to the perturbations, for a spacecraft traveling around the asteroid 2001SN₂₆₃. This asteroid is a triple system, which center of mass is in an elliptic orbit around the Sun. The perturbations considered in the present model are the ones due to the oblateness of the central body, the gravity field of the two satellite bodies (Beta and Gamma), the Sun, the Moon, the asteroids Vesta, Pallas and Ceres and all the planets of the Solar System. This mapping is important, because it shows the relative importance of each force for a given orbit for the spacecraft, helping to make a decision about which forces need to be included in the model for a given accuracy and nominal orbit. Another important application of this type of mapping is to find orbits that are less perturbed, since it is expected that those orbits have good potential to require a smaller number of station-keeping maneuvers. Simulations under different conditions are made to find those orbits. The main reason to study those trajectories is that, currently, there are several institutions in Brazil studying the possibility to make a mission to send a spacecraft to this asteroid (the so-called ASTER mission), because there are many important scientific studies that can be performed in that system. The results showed that Gamma is the main perturbing body, followed by Beta (10 times smaller) and the group Sun–Mars-oblateness of Alpha, with perturbations 1000 times weaker than the effects of Gamma. The other bodies have perturbations 10⁷ times smaller. The results also showed that circular and polar orbits are less perturbed, when compared to elliptical and equatorial orbits. Regarding the semi-major axis, an internal orbit is the best choice, followed by a larger external orbit. The inclination of the orbit plays an important role, and there are values for the inclination where the perturbations show minimum and maximum values, so it is important to make a good decision on those values.     

测试有效性对软件可靠性验证测试量的影响

针对传统软件可靠性验证测试方法均不考虑软件测试性可能会对验证测试用例数量产生影响的现状,提出一种引入测试有效性对软件可靠性验证测试最小量进行改进的方法.分析了软件测试性的定义及其对软件可靠性测试集合的影响,提出软件测试有效性的概念.比较了考虑测试有效性前后软件可靠性验证测试集合在数量上的差异,证明经典统计方法和无先验知识的Bayesian统计推断方法确定的均为假定测试有效性为零情况下的保守估计.提出结合测试有效性的验证测试量的量化表示模型和验证测试方案的改进方法,基于统计故障注入的原理,提出测试有效性的定量评估方法,最后通过示例给出定量评估过程和方法.      

电磁多尺度和非线性效应分析

微观尺度上的结构和电接触特性对于宏观尺度上的电磁特性具有重要的影响.针对多尺度结构的非线性无源互调(PIM)无法用频域方法直接计算的问题,提出了基于Floquet理论的全波方法,对具有周期性微观结构的多尺度电大尺寸问题进行计算,从而准确地计算其电特性.此外,将产生非线性的金属结的等效电路模型引入到全波分析方法中,通过全波方法与等效电路方法相结合的方式来分析多尺度结构的无源互调问题.数值计算结果表明该方法可以有效地评估微观结构对于宏观结构电性能的影响,并解决了时域方法求解电大尺寸微波部件产生的计算累积误差较大这一难题.      

基于不相干平面波叠加以模拟混响声场的航天器低频声固耦合分析

文章针对航天器在混响声场中的随机振动问题,提出一种通过多个不相干的平面波线性叠加以模拟混响声场的实现方法,给出了每个平面波的具体参数并从理论上证明其满足理想混响声场假设。在此基础上利用有限元-边界元耦合方法对整星低频声固耦合问题进行分析,并用混响室噪声试验响应数据进行了验证。研究结果表明:该方法理论推导正确,为航天器低频声固耦合分析及声振力学环境预示提供了一种新的有效手段。     

真空与磁场热处理改善FeCo合金的软磁性能

针对发电机中转子用FeCo合金(国产牌号1J22)进行了组织结构与磁性能的研究.通过对该合金进行真空处理以及磁场热处理,研究了组织结构对软磁性能的影响规律;研究了附加磁场强度以及热处理温度对磁场处理效果的影响,并结合该合金的磁致伸缩伸缩系数的变化规律,分析了磁场热处理效果的微观机制.当合金组织为轧制态时,磁场热处理效果不明显;在合金的再结晶温度以上进行磁场热处理时,获得了显著的磁场热处理效果,矫顽力下降至72A/m(0~9Oe)以下.     

改性双基推进剂拉压不对称力学性能研究

针对改性双基推进剂在不同载荷条件下表现出不同力学响应的现象,对其进行了恒应变率拉伸和压缩试验及蠕变拉伸和压缩试验,获得了4组应变率下拉压应力-应变曲线和3组温度下拉压蠕变-时间曲线,使用应力和应变拉压不对称因子反映了拉伸和压缩曲线的不对称程度。结果表明,改性双基推进剂具有明显的拉压不对称力学性能,且该性能受到应变率和温度的影响。分析了改性双基推进剂具有拉压不对称性的内在成因,认为材料初始缺陷的扩展、材料分子链移动空间的变化、基体材料与填充颗粒材料力学性能的不同是导致改性双基推进剂具有拉压不对称力学性能的内在原因。     

亚声速大迎角模型试验洞壁干扰修正方法研究

通过测量洞壁附近的压力分布来模拟透气壁试验段的洞壁边界条件,采用数值求解Euler方程的方法模拟模型在风洞中的绕流场,然后将洞壁边界条件用远场边界条件替换,用同样方法计算出模型在自由流中的绕流场,从而计算出洞壁干扰对模型的绕流场和气动力的影响。针对大迎角模型的洞壁干扰问题的特殊性,采用重叠网格技术,对飞机大迎角标模和SB-03模型进行了亚声速大迎角的洞壁干扰计算与修正。