航空发动机滑油泵高空性分析

从流体力学角度,对滑油泵的高空性进行了系统的理论分析:阐述了其产生原理,推导了各种影响因素之间的关系式,得出了如下结论:泵前总阻力系数、滑油密度、油泵设计流量越小,入口管径越大,越有利于保持泵的高空性;而对于转子泵,内齿轮1齿扫过的面积越小,内齿轮齿数越少,内齿轮转速越低,转子宽度越小,越有利于保持高空性;对于齿轮泵,模数和齿数越少,转速越低,转子宽度越小,越有利于保持高空性。反之,则不能保持高空性。     

长航时无人机飞行器管理计算机设计研究

高高空长航时无人驾驶飞机对其任务可靠性和安全性提出了极高的要求,而飞行器管理计算机是保证飞机安全和任务执行的核心部件.飞行器管理计算机采用合适的冗余配置可以有效地提高可靠性和安全性.探讨了一种基于三模冗余(TMR)结构的相似余度容错计算机,描述了计算机的硬件组成以及为满足可靠性要求所采取的任务调度和余度管理算法.在计算机综合化小型化以及调试测试方法方面所进行的创新使计算机具有良好的测试性和维修性并能够适应未来航空电子发展的需求.     

空间交会寻的最优轨道机动

研究了交会寻的阶段的燃料优化问题。在经典Ｃ－Ｗ方法基础上,导出了考虑第一次脉冲位置的双脉冲寻的燃料优化方法。当寻的时间给定时,优化变量为第一次脉冲启动的时刻;当寻的时间不定时,优化变量为第一次脉冲启动的时刻和寻的时间。仿真结果表明,考虑和不考虑第一次脉冲位置,燃料消耗差别悬殊。对于地面站较少、要求寻的时间比较长的情况,该方法有重要意义。     

近距离空间交会动力学

首先研究两个飞行器在近距离相对运动的动力学方程,包括简易（线性化）和精确模型;其次推导出一个工程实用在轨道平面内保持点轨迹椭圆方程;最后讨论保持点的动力学特性和轨道摄动对保持点的影响。     

停车转弯掉高度问题的探讨

首先从分析停车转弯的基本运动入手,根据停车转可能出现的各种情况,重点讨论了停车转弯高度损失的问题,然后较详细地分析了各种转弯情况引起高度损失,最后,以Ｈ６飞机为例进行计算和分析,结果表明,在迫降处置中,可作较大坡度的转弯,以减少高度的损失,为实际飞行提供了最优的操纵手段。     

Artificial equilibrium points and bi-impulsive maneuvers to observe 243 Ida

In the restricted three-body problem, the traditional Lagrange points L₁ and L₂ are the only equilibrium points near the asteroid 243 Ida. The thrust generated by a solar sail over a spacecraft enables the existence of new artificial equilibrium points, which depend on the position of the spacecraft with respect to the asteroid and the attitude of the solar sail. Such equilibrium points generate new spots to observe the body from above or below the plane of motion. Such points are very good observational locations due to their stationary condition. This work provides a preliminary analysis to observe Ida through the use of artificial equilibrium points as spots combined with transfer maneuvers between them. Such combination can be used to observe the asteroid from more different points of view in comparison to fixed ones. The analyses are made for a spacecraft equipped with a solar sail and capable of performing bi-impulsive maneuvers. The solar radiation pressure is used both to maintain the equilibrium condition and to reduce the costs of the transfers and/or to create transfers with longer duration. This is a new aspect of the present research, because it combines the continuous thrust with initial and final small impulses, which are feasible for most of the spacecraft, because the magnitudes of the impulses are very low. These combined maneuvers may reduce the transfer times of the maneuvers in most of the cases, compared with the maneuvers based only on continuous thrust. Several options involved in these transfers are shown, like to minimize the fuel spent ($\mathrm{\Delta }\mathit{v}$) as a function of the transfer time or to extend the duration of the travel between the points. Extended transfer times can be useful when observations are required during the transfers.     

低高度内辐射带高能质子空间分布位形的研究

利用国际地磁参考场模式(IGRF模式)分析了1970-2000年低高度南大西洋负磁异常区位形的漂移与变化，给出了几个高度异常区中心位置磁场强度的变化和位置的变化。利用带电粒子的运动学方程，简要分析了低高度辐射带高能粒子的运动，得出在低高度，磁场是决定辐射带高能粒子空间强度与分布的决定性因素．低高度辐射带空间分布位形的变化特征应该与低高度南大西洋负磁异常区的变化特征基本一致．低高度南大西洋负磁异常区的特征可以作为低高度辐射带空间分布位形的一个初步判据。     

空间机动目标的跟踪和定位

轨道机动控制过程中，推力加速度的不确定性是机动目标运动的主项摄动。通过对推力加速度和机动目标运动建模，在地心惯性系建立了增广系统状态动力学模型，在地平测量坐标系建立了离散量测模型，同时讨论了机动目标增广状态非线性动力学模型的线性化问题。给出了扩展卡尔曼滤波实时估计增广状态向量的算法，仿真分析证明所述算法稳定、收敛，对机动目标具有较高的定位精度。     

简析B757飞机RA故障的关联影响及维护建议

RA系统测量飞机到地面的真实高度。本文介绍了B757飞机RA系统的工作情况,对因RA系统故障引起其他飞机系统工作异常的典型现象进行了分析,介绍了排除故障过程,最后总结了在RA系统实际维护中需要注意的方面,并给出了维护建议。     

Effects of space weather on the ionosphere and LEO satellites’ orbital trajectory in equatorial,low and middle latitude

We study the effects of space weather on the ionosphere and low Earth orbit (LEO) satellites’ orbital trajectory in equatorial, low- and mid-latitude (EQL, LLT and MLT) regions during (and around) the notable storms of October/November, 2003. We briefly review space weather effects on the thermosphere and ionosphere to demonstrate that such effects are also latitude-dependent and well established. Following the review we simulate the trend in variation of satellite’s orbital radius (r), mean height (h) and orbit decay rate (ODR) during 15 October–14 November 2003 in EQL, LLT and MLT. Nominal atmospheric drag on LEO satellite is usually enhanced by space weather or solar-induced variations in thermospheric temperature and density profile. To separate nominal orbit decay from solar-induced accelerated orbit decay, we compute $r\text{,}h$ and ODR in three regimes viz. (i) excluding solar indices (or effect), where $r=r_0\text{,}h=h_0$ and $\mathit{ODR}={\mathit{ODR}}_0$ (ii) with mean value of solar indices for the interval, where $r=r_m\text{,}h=h_m$ and $\mathit{ODR}={\mathit{ODR}}_m$ and (iii) with actual daily values of solar indices for the interval ($r\text{,}h$ and ODR). For a typical LEO satellite at h?=?450?km, we show that the total decay in r during the period is about 4.20?km, 3.90?km and 3.20?km in EQL, LLT and MLT respectively; the respective nominal decay ($r_0$) is 0.40?km, 0.34?km and 0.22?km, while solar-induced orbital decay ($r_m$) is about 3.80?km, 3.55?km and 2.95?km. h also varied in like manner. The respective nominal ${\mathit{ODR}}_0$ is about 13.5?m/day, 11.2?m/day and 7.2?m/day, while solar-induced ${\mathit{ODR}}_m$ is about 124.3?m/day, 116.9?m/day and 97.3?m/day. We also show that severe geomagnetic storms can increase ODR by up to 117% (from daily mean value). However, the extent of space weather effects on LEO Satellite’s trajectory significantly depends on the ballistic co-efficient and orbit of the satellite, and phase of solar cycles, intensity and duration of driving (or influencing) solar event.