离解反应速率常数中的方位因素

以碰撞理论为基础探讨了结构方位因素对离解反应速率常数的影响,建立了计及方位特征的离解反应模型,计算对比了热平衡假设下空气中几个典型的离解反应的Arrhenius图.结果表明,在所选实例中,除了反应N₂+N和O₂+O外,考虑方位因素后确实能够更好地理论估算出反应速率常数.对上述例外文中做了一定的讨论.     

光学材料带电粒子辐照效应等效模拟试验方法研究

文章研究了空间带电粒子对光学材料辐照效应的等效模拟试验方法.在辐照试验研究基础上,针对光学材料分析了空间带电粒子辐照试验中辐照源选择、能谱效应,综合与顺次辐照效应和加速试验等几个关键问题,并根据空间带电粒子对光学材料的损伤特点,提出了模拟材料内部吸收荆量分布的等效试验方法.     

贴地飞行时旋翼空气动力学实验研究

 本文对贴地飞行时的旋翼进行了流场显示和桨盘处下洗速度测量的实验研究。揭示并研究了环流和地面涡现象及其对旋翼平面下洗速度分布的影响,指出了旋翼贴地飞行时拉力、力矩等剧烈变化的原因。     

某运输机全机构型雷诺数效应阻力修正研究

采用CFD方法分析了雷诺数效应对某运输机全机构型阻力的影响。基于对某运输机的翼/身/架/舱组合体绕流进行的计算分析,归纳总结出了一种适应于复杂构型的低雷诺数到高雷诺数的阻力修正方法。通过验证可知,该修正方法修正效果良好,为工程中的阻力预测提供了一种简洁有效的方法。     

高焓流动重要基础问题研究进展

本文报道了我们在爆轰驱动高焓激波风洞中开展的测试工作的进展.试验气流有两种典型的状态.分别对应流动速度5km/s与4km/s.这里主要说明在气动热、气动力、红外辐射、电离特性、化学组分等物理量测量方法上,我们所做的努力以及所得到部分典型的结果.     

光电耦合器位移损伤效应研究

文章针对光电耦合器在空间辐射应用中的位移损伤效应,选取了一种典型的光电耦合器4N25进行了1MeV高能电子辐照试验,获得了辐照后器件电流传输比参数（CTR）的退化与电子注量的关系:在试验注量范围（1.3×1012 ~1.5×1013 cm-2）内,nCTR与电子通量成反比。通过位移损伤对器件及材料作用过程的分析,探讨了光电耦合器位移损伤效应作用机理。     

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.