颈动脉内血流动力学特征受向前加速度影响的数值模拟

人们在日常或某些特殊条件下常会面临方向和大小发生迅速变化的加速度环境,已有研究发现加速度环境会影响心血管系统生理、病理特征。利用计算机模拟方法详细研究了向前加速度环境下人体颈动脉内的血流动力学参数变化规律。结果表明:加速度会对颈动脉内压力、压力梯度、壁面剪切应力等与血管生理、病理现象密切相关的血流动力学参数产生显著影响。研究结果为加速度环境下颈动脉生理、病理研究提供了一定的理论依据,也为航空航天领域加速度环境下人员防护提供参考。      

大功率无电极高密度等离子体电磁推进概述

无电极高密度等离子体电磁推进技术已成为未来深空探测、载人航天和货运、太阳能电站以及航天器在轨服务与维护等空间任务中极具竞争力的核心推进技术之一。在梳理不同无电极等离子体电磁加速机制基础上,开展大功率无电极高密度等离子体电磁推进技术性能对比,给出新概念无电极场反构型电磁推进技术向未来超大功率拓展的优势和发展潜力,同步分析了该技术亟需解决的关键基础问题,旨在为中国新概念场反构型电磁推进技术的研发提供理论基础。     

小卫星非常规动力学分析与控制

针对小卫星研制中出现的一些非常规动力学问题进行研究,并提出解决办法。针对小卫星组件最大冲击谱量级超出常规冲击试验规范谱的分析与验证困难,通过研究提出了能够分析评估组件高量级冲击的方法。针对小卫星随机振动下强度设计方法还存在较大误差,分析了系统模态质量比与模态频率在一定频段的影响规律,认为忽略模态质量耦合会带来误差,提出了考虑模态质量耦合的准静态载荷计算方法。最后,针对小卫星整星开展了减振研究,分析了正弦和随机减振效果,对于对称安装减振系统,提出了减振系统的主频率计算公式。     

高垂直度和低沉积的MEMS陀螺梳齿结构释放工艺

梳齿型微机电系统（MEMS）陀螺的释放要求结构具有垂直度高、释放过程沉积聚合物少的特点,通过优化深硅刻蚀的工艺参数,包括钝化气体八氟环丁烷（C4F8）的流量、衬底温度、刻蚀气体六氟化硫（SF6）的流量和钝化气体C4F8的压力,实现了结构垂直度为90.0°、支撑层表面沉积物厚度为87.1nm的梳齿结构释放工艺。深硅刻蚀工艺的优化为高性能MEMS陀螺的加工提供了基础。     

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.     

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.     

面向空间天线的TWF复合材料性能研究

利用碳纤维三向编织物（triaxial woven fabric，TWF）作为增强材料，与柔性基体材料硅橡胶复合，制成兼具一定柔性和刚性的复合材料壳膜结构，用于卫星天线反射器，是一种新型的高精度可展开天线实现方案。采用复合材料细观方法，对碳纤维增强硅橡胶TWF复合材料进行了力学性能的研究。首先由纤维和基体的材料特性得到均质纤维束的材料特性；接下来考虑纤维束交织情况（起伏波动）建立由纤维束组成的单胞实体有限元模型；然后对单胞实体有限元模型进行均匀化分析，施加周期性边界条件，最终得到等效的均质材料特性；为满足天线反射器高性能需求，分析了碳纤维种类、纤维体积分数对单胞等效性能的影响规律。对该材料力学性能的研究，可以为其未来应用于大型高精度可展开天线反射器提供一定的理论依据。     

Application of a modified generalized sail model on a solar sail with wrinkles

In this paper, we present an analysis of effect of wrinkles on the solar sail performance. We describe different analytical, semi-analytical and numerical approaches to the calculation of general large-scale curvature of a solar sail as well as parameters of so-called wrinkled domains, and introduce the impact of such wrinkles on the thrust and torque of the solar sail. Finally, we present a model of an optically-orthotropic surface for such non-ideal sail, providing a connection with the Generalized Sail Model, and other solar sail thrust models.     

大型客机低速构型高雷诺数风洞腹撑支架干扰数值模拟

风洞到飞行相关性修正是获取现代大型客机低速气动特性的重要手段，通常采用增压提高风洞试验雷诺数，而支架干扰修正是该修正体系的一个关键环节。采用数值模拟研究了增压风洞腹撑的支架干扰，并分析了腹撑对飞机各部件的干扰及其对风洞流场的影响。通过数值模拟与风洞试验对比，表明升力系数相差0.006，阻力系数最大相差0.001 2，俯仰力矩系数最大相差0.01，验证了CFD数值模拟方法的可靠性。CFD计算结果表明：腹撑使得全机升力增加、阻力减小，俯仰力矩增加；腹撑对升力影响的主要部件是机翼，腹撑使得风洞中心以上动压增加，提升上翼面流速，从而增加了机翼的升力；与传统认识不同的是腹撑对阻力影响为负，且主要影响部件为缝翼，原因为缝翼下偏使得法矢分量向前从而减小了阻力；腹撑对俯仰力矩影响的主要部件是机身及平尾。研究结果揭示了腹撑对飞机气动特性影响的量级、主要影响部件及其流场变化，可为支架干扰数据修正及支架优化设计提供参考。所得结论可更好用于支架干扰试验的开展及风洞到飞行数据的修正，具有一定的工程实用性。     

航空发动机全飞行包线稳态划分方法研究

航空发动机在鲁棒控制器设计过程中存在飞行包线区域难以系统划分的问题,为此,提出基于推力耗油率特性和基于动压耗油率特性的航空发动机飞行包线划分法。根据某型涡扇发动机在全包线范围内稳态工作时的推力、耗油率及动压特性,结合大气条件的客观规律,通过两种划分方法将飞行包线划分为65 个区域,用每个区域对应标称点的参数代替其周围小偏差区域和边界点参数。通过对该发动机全包线内各区域标称点与边界点参数的对比,证明两种方法均对全飞行包线划分有效,可为后续航空发动机控制器设计提供理论基础。