摄动对编队飞行星座相对构型的影响分析

在近圆轨道编队飞行的假设条件下，根据动力学关系推导出了环绕卫星相对参考卫星的运动学简化模型，并以此简化模型为基础，分别研究了大气阻力摄动、日月引力摄动、太阳光压摄动和地球扁率摄动对编队飞行星座的构型影响，着重分析了地球扁率摄动周期项和长期项对构型的影响，并以此对编队轨道设计提出建议。     

姿控发动机内流场及高空羽流流场的DSMC一体化数值模拟

通过引入“平衡抽样方法”有效解决了DSMC求解近连续流区所遇到的碰撞顶计算效率问题;对于过渡流及自由分子流区,构造了适合于DSM仿真的分子碰撞传能模型并配置了一种光滑过渡以减少误差的权函数。在此基础上首次实现了对姿控发动机喷管内流场及包括倒流区在内的高空弱流流场的DSMC方法一体化数值模拟。     

飞机纵向起飞着陆动态特性仿真研究

以刚体系动力学理论为依据,结合飞机起飞着陆运动学特征,建立了起落架-机身组合刚体6自由度全量飞机方程。文内建立的阶跃跟踪驾驶员时域数学模型,有助于评价起飞着落阶段人-机系统的飞行品质。根据该系统的数学模型编制了FORTRAN软件,并对起飞着陆动态特性作出了综合的全面的定量分析。     

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。     

Longitudinal distribution of thermospheric densities and ionization rates in the upper atmosphere of Mars at mid-latitude using MGS ACC data

The Accelerometer Experiment (ACC) onboard Mars Global Surveyor (MGS) measured 1600 density profiles in the upper atmosphere of Mars during aerobraking. These measurements reveal large-scale and small-scale structure in the thermosphere of Mars. Here, the measurements of mass density for 115 orbits (#P0670–P0789) from November 1 to 30, 1998, under spring equinox and medium solar activity conditions (average F_10.7 ∼ 137) during phase 2 of the aerobraking in the thermosphere of Mars at different altitudes and longitudes are presented for northern mid-latitude (17–42°N) in the dayside atmosphere using ACC onboard MGS. From these mass densities, the neutral densities of different gases are derived from their mixing ratios. Using these neutral densities, the longitudinal distribution of photoionization rates and photoelectron impact ionization rates are calculated at wavelength range 1–102.57 nm due to EUV and soft X-ray radiation under photochemical controlled region using Analytical Yield Spectrum approach (AYS). These conditions are appropriate for MGS Phase 2 aerobraking period from which the accelerometer data is used. Under the photochemical equilibrium condition, the electron density near the peak varies as the square root of the total peak ionization rate. Using this fact, an attempt is being made to estimate the mean primary and secondary peak electron density by averaging the longitudinal variations of total peak ionization rates in the northern mid-latitude (17–42°N) ionosphere of Mars, as there is no radio science measurement at this latitude region by MGS.     

燃油降温系统的设计和研制

简要介绍了高空台燃油降温系统的用途、设计方案、设计技术要求、工作原理、主要设备和调试结果。     

某型涡扇发动机燃油调节器改进及高空适应性分析

某小型涡扇发动机开展增大推力、提高使用高度的适应性改型工作.针对以往对原发动机燃油调节器部分所作的分析较少,使得改型工作缺乏必要的理论支持问题.主要分析了发动机燃油调节器的工作原理,建立系统稳态和加减速控制数学模型,并在此基础上对其高空适应性进行分析,最后提出相应的改进分析方法和具体措施.      

长时高空气球的研制发展

综述了美国长时观察用的高空气球的发展,并详细介绍了目前正在研制的超长时气球(ULDB)。     

航空供氧装备生理研究回顾与展望

重点回顾了我国 70年代以来航空供氧装备防护生理学的研究与发展。将我国航空供氧装备生理研究归结为 :高空高总压供氧防护高空低总压供氧简化装备防护和机载分子筛制氧防护生理研究三大部分。提出未来发展几点看法。     

Single event upset investigations on the “Flying Laptop” satellite mission

The radiation effects in electronic parts are called single-event effects, which are deemed to be critical for space missions. This paper presents the Single Event Upsets that were observed in an onboard memory device of the Low Earth Orbit “Flying Laptop” satellite mission during its in-orbit operation. The Single Event Upsets were carefully mapped on the satellite orbital space itself and their root causes were investigated together with their rates of occurrence. Subsequently, the events were traced to show several root cause sources such as (i) trapped energetic protons leaking to low altitudes within the South Atlantic Anomaly, (ii) Solar Energetic Particles emitted by an impulsive event on 10 September 2017, and (iii) Galactic Cosmic Rays. A profound analysis was carried out on the observed flight data, and its corresponding results are actually in agreement with the standard energetic particle models. The presented results provide another important insight on the Single Event Upsets for future Low Earth Orbit satellite missions.