溅射靶对离子推力器的热辐射影响研究

为了研究真空环境设备内溅射靶温度升高后对30 cm离子推力器的热辐射影响,采用有限元分析的方法,首先对真空舱内的离子推力器羽流分布进行了模拟,在获得羽流对溅射靶造成的温度变化后,进一步分析了溅射靶温度升高对离子推力器温度以及栅极热形变位移所造成的影响.仿真结果显示,推力器羽流可采用定向分子流模型进行描述,羽流在真空舱内...     

数值模拟喷焰2.7微米红外辐射特性

以固体火箭发动机尾喷焰的红外探测为主要应用背景,利用反向蒙特卡罗法和有限体积法计算了火箭尾喷焰红外辐射特性,获得了尾喷焰在探测波长为2.7μm下的红外辐射的空间、光谱分布特性,两种方法的计算结果也非常接近,具有重要的理论意义和实际应用背景。     

Investigation on plume interference effect of solid propellant micro-thruster

The three-dimensional numerical simulation of two-phase plume flow of solid propellant micro-thrusters was developed. Then it was used to investigate the plume interference effect by combining the direct simulation Monte Carlo (DSMC) method for multi-component gas flow with the two-way coupling model for two-phase rarefied flow. At different space between the two micro-thrusters and different wall temperature,the plume interference effect was analyzed specifically. The results show that under the plume interference effect the gas is compressed and the flow direction is changed,which resulted in the increasing of gas pressure and temperature; solid phase made no significant effect on the flow parameters of gas phase; with the rising of the space between the two micro-thrusters,the maximum pressure decreased and the maximum temperature increased in the domain under the plume interference effect; the wall temperature could influence the temperature of the gas which is extremely close to the wall,but not the gas pressure.      

轻型飞机纵向静稳定性试验的估算

推导出了在试飞试验前对轻型飞机纵向静稳定性进行估算的公式,分别给出了握杆和松杆状态下静稳定性的估算方法。在此估算的基础上推导出了试飞试验时所要测的驾驶杆位移和杆力等估算式,进而提出了从试验数据到飞机中性点和实际纵向静稳定裕度的分析处理方法。     

一种快速求解Orr-Sommerfeld方程中性稳定性曲线的方法

提出一种快速准确求解 Orr- Som merfeld(O- S)方程的中性曲线和临界雷诺数 Recr的方法。在求解过程中 ,先分析 a0 ,cr0 的范围 ,利用网格自适应自动搜索 a0 ,cr0 ,采用三次样条函数计算并迭代到一定精度从而获得雷诺数 Re与波数 a及波速 cr 的关系曲线 ,克服了通常求解中性曲线时 ,要预估每一点的 a,cr的不足。算例表明 ,本方法计算速度快 ,结果准确 ,花较少的机时就能计算出与谱方法精度相当的临界 Recr。     

对流辐射板抑制涡扇发动机热喷流红外辐射的实验

用对流辐射换热板来降低混合排气涡扇发动机热喷流的红外辐射,并在涡扇发动机热喷流模拟实验台上进行了实验研究.测量了安装对流辐射换热板前后,轴对称喷管的热喷流的温度分布,轴对称喷管和二元喷管的热喷流在3～5 μm波段的红外辐射强度.结果表明:对流辐射换热板可以降低热喷流高温核心区的温度约10%,降低涡扇发动机热喷流的红外辐射强度约20%～30%.      

Performance of GPS-based accelerometry: A simulation experiment

Recent studies have shown that with the availability of high-quality CHAMP and GRACE gravity field models, it is feasible to determine accurate non-gravitational accelerations for low Earth orbiting satellites indirectly from precise GPS satellite-to-satellite observations. Possible applications of this so-called GPS-based accelerometry approach consist of accelerometer calibration and atmospheric density and wind computations. With the growing number of high-quality space-borne GPS receivers, this method could be applied to a large range of satellites. In this paper an extensive simulation study has been carried out, based on real accelerometer data from the GRACE mission, in order to determine the optimal processing strategy and the resulting accuracy of the estimated non-gravitational accelerations. It is shown that the optimal processing strategy consists of a piecewise linear parameterization of the estimated empirical accelerations, together with short 6-h orbit arcs. The GPS-based accelerometry approach makes use of triple-differenced GPS observations and the impact of considering the correlated observation noise was found to be marginal in the presence of other error sources such as GPS ephemeris errors. Using a priori non-gravitational force models improves the recovery of low temporal resolution accelerations, except during huge geomagnetic storms. With this strategy, non-gravitational accelerations can be recovered during high solar activity with an accuracy of better than 10% of the total signal in along-track direction and around 25–40% in cross-track direction, at time resolutions of around 8–20 min. During solar minimum conditions, the relative recovery error will increase to approximately 50% in along-track direction and around 60–70% in cross-track direction, due to the reduced atmospheric drag signal. Unfortunately, GPS-based accelerometry is hardly sensitive in the radial direction.     

三维多组分羽流及其效应的数值模拟

考虑到实际卫星总体布局特点及姿控发动机燃气喷流为多组分的特点,采用差分求解N-S(Navier-Stokes)方程耦合DSMC(Direct Simulation Monte Carlo)方法建立三维多组分羽流场的数值模拟模型,对5 N无水肼单组元姿控发动机喷管产生的燃气羽流场及其效应进行数值模拟,计算得出羽流场的物理参数分布、化学组分分布,得到了羽流对太阳能帆板的羽流气动力和气动热效应.计算结果表明对于太阳能帆板的羽流效应防护应以N2,NH3为主,姿控发动机羽流会对太阳能帆板撞击产生气动力和气动热的影响,在太阳能帆板前沿中点处,存在气动压强峰值和气动热流峰值.计算结果为研究羽流效应提供了参考依据.     

航天器发动机羽流对太阳电池板力及热效应仿真

文章将差分求解N-S方程与DSMC方法相结合,研究了航天器单台发动机连续工作时的真空羽流对航天器太阳电池板的力效应和热效应。通过求解N-S方程,获得发动机喷管的内流场;再以内流场计算结果作为模拟粒子入口边界条件,应用DSMC方法,在并行计算机平台上进行三维羽流场和力及热效应计算,得到航天器单发动机连续工作情况下羽流场对太阳电池板的力效应和热效应。文章以太阳电池板处于斜45°状态为例,对仿真结果进行了分析。     

微波在液体火箭发动机真空羽流中的衰减

为研究液体火箭发动机真空羽流对微波的衰减作用,以某双组元液体火箭发动机为对象,使用热力计算程序对燃烧室内的电子数密度进行了计算,使用冻 结假设和有限化学反应速率假设两种情况对喷管内带电粒子的电离和再结合过程进行了模拟,并对羽流中带电粒子数密度和5~30GHz微波穿过羽流的衰减量进行了估算.研究结果显示:该发动机燃烧室和喷管出口的电子数密度量级分别为 1013~1014cm-3和1010~1011cm-3,K,Na等碱金属为主要电子释放剂,Cl-,OH-等基团为主要电子吸收剂;低频微波在羽流中衰减更严重,5GHz微波的衰减可达4.5dB;微波斜穿羽流的衰减通常大于横穿情况.