考虑星历误差的天文测角/时间延迟量测组合导航方法

基于太阳震荡的时间延迟是一种新型天文导航量测量，可以提供探测器相对反射天体的距离信息，与星光角距量测量结合，可以提高导航性能。然而，星光角距量测模型与时间延迟量测模型均含有火卫一相对火星的位置矢量，火卫一的星历误差将影响导航精度。针对这一问题，提出了一种基于在线估计的天文测角/时间延迟量测组合导航方法，建立了包含火卫一位置及速度的状态模型，利用星光角距及时间延迟量测量同时对火卫一的位置和速度进行在线估计，仿真结果表明，提出的方法可以有效抑制火卫一星历误差对组合导航精度的影响，为探测器提供高精度的自主导航信息。     

An empirical solar radiation pressure model for satellites moving in the orbit-normal mode

We present a family of empirical solar radiation pressure (SRP) models suited for satellites orbiting the Earth in the orbit normal (ON) mode. The proposed ECOM-TB model describes the SRP accelerations in the so-called terminator coordinate system. The choice of the coordinate system and the SRP parametrization is based on theoretical assumptions and on simulation results with a QZS-1-like box-wing model, where the SRP accelerations acting on the solar panels and on the box are assessed separately. The new SRP model takes into account that in ON-mode the incident angle of the solar radiation on the solar panels is not constant like in the yaw-steering (YS) attitude mode. It depends on the elevation angle of the Sun above the satellite’s orbital plane. The resulting SRP vector acts, therefore, not only in the Sun-satellite direction, but has also a component normal to it. Both components are changing as a function of the incident angle. ECOM-TB has been used for precise orbit determination (POD) for QZS-1 and BeiDou2 (BDS2) satellites in medium (MEO) and inclined geosynchronous Earth orbits (IGSO) based on IGS MGEX data from 2014 and 2015. The resulting orbits have been validated with SLR, long-arc orbit fits, orbit misclosures, and by the satellite clock corrections based on the orbits. The validation results confirm that—compared to ECOM2—ECOM-TB significantly (factor 3–4) improves the POD of QZS-1 in ON-mode for orbits with different arc lengths (one, three, and five days). Moderate orbit improvements are achieved for BDS2 MEO satellites—especially if ECOM-TB is supported by pseudo-stochastic pulses (the model is then called ECOM-TBP). For BDS2 IGSOs, ECOM-TB with its 9 SRP parameters appears to be over-parameterized. For use with BDS2 IGSO spacecraft we therefore developed a minimized model version called ECOM-TBMP, which is based on the same axis decomposition as ECOM-TB, but has only 2 SRP parameters and is supported by pseudo-stochastic parameters, as well. This model shows a similar performance as ECOM-TB with short arcs, but an improved performance with (3-day) long-arcs. The new SRP models have been activated in CODE’s IGS MGEX solution in Summer 2018. Like the other ECOM models the ECOM-TB derivatives might be used together with an a priori model.     

高空飞行环境中液体运载火箭底部热环境研究

采用数值模拟和飞行测试验证相结合的方法对液体运载火箭高空对流/辐射耦合换热问题开展系统深入研究。基于燃气多组分输运Navier-Stokes方程、热辐射方程、Realizable k-ε两方程湍流模型，建立了高空含自由流的运载火箭燃气喷流流动模型。辐射模型采用离散坐标法(DOM)，空间离散采用二阶迎风TVD格式，对多个典型飞行高度火箭底部热流进行大型并行计算，将数值结果与试验数据进行广泛对比，验证了计算模型的精度和有效性。数值研究表明，火箭底部辐射热流在刚起飞阶段达到最大值，随着飞行高度上升，辐射热流逐渐降低，火箭底部对流热流表现为先升高后降低的趋势，并在20 km高空达到峰值。本文的预测分析方法对液体运载火箭底部热防护设计具有重要的理论意义和工程应用价值。     

The adjusted optical properties for Galileo/BeiDou-2/QZS-1 satellites and initial results on BeiDou-3e and QZS-2 satellites

Solar Radiation Pressure (SRP) is the dominant non-gravitational perturbation for GNSS (Global Navigation Satellite System) satellites. In the absence of precise surface models, the Empirical CODE Orbit Models (ECOM, ECOM2) are widely used in GNSS satellite orbit determination. Based on previous studies, the use of an a priori box-wing model enhances the ECOM model, especially if the spacecraft is a stretched body satellite. However, so far not all the GNSS system providers have published their metadata. To ensure a precise use of the a priori box-wing model, we estimate the optical parameters of all the Galileo, BeiDou-2, and QZS-1 (Quasi Zenith Satellite System) satellites based on the physical processes from SRP to acceleration. Validation using orbit prediction proves that the adjusted parameters of Galileo and QZS-1 satellites exhibit almost the same performance as the corresponding published and “best guess” values. Whereas, the estimated parameters of BeiDou-2 satellites demonstrate an improvement of more than 60% over the initial “guess” values. The resulting optical parameters of all the satellites are introduced into an a priori box-wing model, which is jointly used with ECOM and ECOM2 model in the orbit determination. Results show that the pure ECOM2 model exhibits better performance than the pure ECOM model for Galileo, BeiDou-2 GEO and QZS-1 orbits. Combined with the a priori box-wing model the ECOM model (ECOM+BW) results in the best Galileo, BeiDou-2 GEO and QZS-1 orbits. The standard deviation (STD) of satellite laser ranging residuals reduce by about 20% and 5% with respect to the pure ECOM2 model for Galileo and BeiDou-2 GEO orbits, while the reductions are about 40% and 60% for QZS-1 orbits in yaw-steering and orbit-normal mode respectively. BeiDou-2 IGSO and MEO satellite orbits do not benefit much from the a priori box-wing model. In summary, we suggest setting up a unified SRP model of ECOM+BW for Galileo, QZS-1, and BeiDou-2 orbits based on the adjusted metadata. In addition, we estimate the optical parameters of BeiDou-3e and QZS-2 satellites using a limited number of tracking stations. Results regarding the unified SRP model indicate the same advantages, the STD of satellite laser ranging residuals reduces by about 30% and 20% for QZS-2 and BeiDou-3e orbits respectively over orbit products without a priori model. The estimation procedure is effective and easy to apply to the new emerging satellites in the future.     

可靠性设计优化的球空间设计法

可靠性设计优化（RBDO）在航空航天等领域已经被广泛应用，具有显著提高可靠性的效果；然而它包含两个迭代循环-总体优化循环和可靠性分析循环，双循环求解方法效率低下甚至难以承受。本文提出一种可以提高可靠性设计优化求解效率的方法-球空间设计法，该方法可以方便地表达搜索区域，最大可能失效点可以从极值点处精确获取；同时，该方法可以将总体优化以及可靠性分析同步进行。本文所提出的球空间法的有效性将通过2个算例进行测试，测试结果表明该方法不仅精度与同类方法持平，求解效率有明显提升，它将会对提高航空航天装备如卫星、火箭、飞行器等产品的可靠性提供更为有效的方法和技术支持。     

空间目标监视雷达信号频率的优选准则

随着在轨微小卫星及空间碎片数量不断增加，为保证在轨卫星的运行安全，需要对微小目标进行有效跟踪探测及稳定编目。雷达作为近地空间目标监视的主用设备，在对厘米级小目标进行探测跟踪时，其工作频率是决定其能否可靠探测关键因素，高频有利于探测小目标，并可获得相对稳定的RCS，但高频信号的波束小、搜索能力较低，实现难度大，也使得成本过高。为适于实际工程应用，需从效费比出发，对频率进行优选。本文从目标RCS的角度提出一种空间目标监视雷达信号频率的优选准则，给出该准则下周长波长比ka的取值范围。为了更加清楚地说明该优选准则的应用，给出了直径5 cm和10 cm的目标在该准则下信号频率的取值范围，并与国外工作做了比较，证明该准则可行。     

基于G-M制冷机的大尺寸冷屏设计方法

介绍了基于Gifford-Mcmahon (G-M)制冷机的大尺寸冷屏的设计方法。该低温冷屏配合真空环境模拟室共同使用，为遥感卫星的星载遥感器等部件的红外定标试验提供20K的低温冷背景。该冷屏采用5台G-M制冷机进行制冷，外形尺寸达到1m×1m，是目前国内同类型冷屏中尺寸最大的。详细介绍了冷屏在容器内的安装布置、冷缩时的补偿等结构设计方法、冷屏的表面温度分布以及降温时间等计算分析。成功解决了大尺寸冷屏在低温环境下的冷缩补偿难题，试验结果表明:冷屏主要测点温度为15K，温度均匀性误差为±1K，达到并超过设计要求。      

MIDACO software performance on interplanetary trajectory benchmarks

A numerical study of the MIDACO optimization software on the well known GTOP benchmark set, published by the European Space Agency (ESA), is presented. The GTOP database provides trajectory models of real-world interplanetary space missions such as Cassini, Messenger or Rosetta. The trajectory models are formulated as constrained nonlinear optimization problems and are known to be difficult to solve.     

飞机封闭腔室减重降噪优化方法

噪声水平是现代飞机封闭腔室设计的重要指标,设计中单纯地对壁板进行加肋处理虽能显著降低噪声但会大大增加结构质量,为此对由封闭腔室构成的结构-声耦合系统进行了减重降噪优化研究。基于结构-声耦合有限元模型,利用有限元软件ACTRAN计算了频谱加载时舱内的声压响应。通过试验对简化处理及数值计算进行了验证,并修正了相关模型参数。为了降低结构质量,以加强肋为边界对舱门壁板进行了分区,通过对各个区域壁板厚度及肋条截面积的优化设计,使系统动刚度分配更趋合理,降低了声辐射能量以及结构-声腔的耦合性,从而实现了在满足噪声约束条件下减轻结构质量的目标。本文的工作对实际工程中由加肋壁板所构成的类似结构的减重降噪设计有着较好的工程指导价值。     

过氧化氢/紫外线/臭氧氧化技术处理肼类污水的应用

采用放大试验规模（处理量1 m³/h）的H₂O₂（过氧化氢）/UV（紫外线）/O₃（臭氧）氧化技术处理肼类推进剂污水，在30.0±1.6 ℃，pH=9.0±0.2的条件下，研究肼类的过氧化氢增强光解臭氧化降解。对比不同氧化技术的协同效应以及对污水降解的影响，重点考察过氧化氢、紫外线、臭氧和初始浓度等工艺参数对降解效果的影响，对氧化技术的应用进行了优化。研究结果表明：该技术可使COD去除率提高27.66%，肼类的降解速率随着过氧化氢投加量、紫外线辐射强度、O₃投加速率和水质地提高而升高，随着初始质量浓度的提高而下降。在最佳工艺下，处理5 000 mg/L质量浓度的废水，处理60 min时，COD去除率分别为98.62%（偏二甲肼）、99.17%（甲基肼）、99.94%（肼）和93.25%（单推-3）。