波音737NG飞机大气数据探头自动加温功能测试的替代方法研究

根据波音AMM手册要求,在更换波音737NG飞机上的大气数据系统传感器后,需通过试车测试其自动加温功能。本文研究了波音737NG飞机大气数据系统探头自动加温的工作原理,并提出避免试车的解决方案。     

Geometric calibration of Colour and Stereo Surface Imaging System of ESA’s Trace Gas Orbiter

There are many geometric calibration methods for “standard” cameras. These methods, however, cannot be used for the calibration of telescopes with large focal lengths and complex off-axis optics. Moreover, specialized calibration methods for the telescopes are scarce in literature. We describe the calibration method that we developed for the Colour and Stereo Surface Imaging System (CaSSIS) telescope, on board of the ExoMars Trace Gas Orbiter (TGO). Although our method is described in the context of CaSSIS, with camera-specific experiments, it is general and can be applied to other telescopes. We further encourage re-use of the proposed method by making our calibration code and data available on-line.     

Spectroscopy peculiarities of thermal plasma of electric arc discharge between electrodes with Zn admixtures

Plasma of the free burning electric arc between Ag–SnO₂–ZnO composite electrodes as well as brass electrodes were investigated. The plasma temperature distributions were obtained by Boltzmann plot method involving Cu I, Ag I or Zn I spectral line emissions. The electron density distributions were obtained from the width and from absolute intensity of spectral lines. The laser absorption spectroscopy was used for measurement of copper atom concentration in plasma. Plasma equilibrium composition was calculated using two independent groups of experimental values (temperature and copper atom concentration, temperature and electron density). It was found that plasma of the free burning electric arc between brass electrodes is in local thermodynamical equilibrium. The experimental verification of the spectroscopic data of Zn I spectral lines was carried out.     

A concept mission for the Stellar Population and Evolution with Cubesats (SPEC)

Binary or multiple stellar systems, constituting almost a third of the content of the Milky Way, represent a high priority astronomical target due to their repercussions on the stellar dynamical and evolutionary parameters. Moreover the spectral study of such class of stars allows to better constrain the evolutionary theories of the Galactic stellar populations. By resolving the members of stellar systems through photometric observations we are able to perform more detailed measurements to infer their mass. In this paper we investigate the feasibility of a cubesat based mission including an optical payload to directly optically discriminate the members of a selected sample of binary systems. The scientific targets, consisting 11?M class dwarf stars binary systems, have been extracted from the already studied Riaz catalogue. These subset has been selected considering the star distance, the members angular separation, and the distance from the Galactic plane (due to limit the background and foreground contamination). The satellite concept is based on a 6 unit Cubesat embedding some commercial off the shelf components and an ad hoc designed optical payload occupying almost 4 units. The optical configuration has been chosen in order to fit the angular resolution requirements, as derived from the target characteristics. Moreover, according to the optical analysis and the computed field of view some requirements on the attitude control system have been inferred and fulfilled by the component selection. The paper is organized as in the following: a brief scientific introduction is made; consequently the project is described with particular attention to the optical design and the standard sub-systems; finally the conclusions are drawn and the future perspectives are investigated.     

助推-滑行式燃料最优真空飞行轨迹的设计方法

建立了飞行器助推-滑行式燃料最优真空飞行轨迹的最优控制模型,给出了一种更为简单、直观的内点约束条件和横截条件的推导方法,讨论了高效且更为稳定的数值计算方法,提出了两种应用模式,通过与连续推力式和脉冲式飞行方案的比较,说明这种设计方法在节省燃料方面具有优势.     

基于幂函数模型的民机结构腐蚀扩展寿命评定方法研究

基于飞机结构腐蚀清除后测量获取的腐蚀深度,提出了飞机结构腐蚀扩展寿命的幂函数动态预测模型以及模型参数定义方法,确定了腐蚀条件下的飞机结构腐蚀扩展寿命评定指标,建立了基于运营状态下飞机结构腐蚀信息更新的民用飞机结构腐蚀扩展寿命评定方法。     

热压罐和RTM成型的C型框弯曲试验研究

通过热压罐和RTM成型工艺的复合材料C型框弯曲试验,研究了两种工艺方法对其承载能力及破坏模式的影响.试验结果表明:热压罐成型的隔框承载能力比RTM成型工艺高27.5％,且其分散性小;两种工艺的破坏位置一致,但RTM成型的隔框在平直段与弯曲段过渡截面处外壁先发生分层,而热压罐成型在该处外壁至破坏前才出现分层损伤.该结论可以为该型结构的工程应用提供有价值的参考.     

基于格子Boltzmann方法表面形貌对微通道对流换热的影响

为推动微通道冷却技术在航空发动机中的应用,进一步提高航空发动机性能,本文通过扫描电子显微镜、粗糙度扫描仪等多方式扫描得到实际加工物体表面形貌,结合分形理论进行处理,得到真实、光滑、分形插值、康托尔集四类圆形截面管模型,管径100μm~400μm;采用格子Boltzmann方法进行数值模拟,首先通过与文献中实验结果的对比,验证了此方法的正确性,然后对空气在这四类圆形截面微通道中的对流换热特性进行了数值模拟,计算雷诺数Re范围80~640;结果发现：表面形貌是微通道中对流换热不可忽略的因素,相对粗糙度越大越有利于换热,真实扫描管的换热性能要比相同条件下光滑管高2.22%;分形理论可用于微通道表面形貌的构建,在相同迭代次数下,分形插值模型与真实扫描形貌换热性能相差0.03%,而康托尔集模型与真实扫描形貌换热性能相差1.88%,分形插值模型较康托尔集模型更能真实地反映实际形貌;微通道中,随着雷诺数的增加Nu将不再是常数,而是有增加的趋势。     

燃气轮机间冷器结构改进试验研究

为了分析间冷器翅片高度、翅片厚度、隔板厚度等结构参数对换热性能的影响,根据船用间冷循环燃气轮机长期工作在海洋环境的性能要求及结构特点,初步设计了机上间冷器,并对其进行了试验验证。根据前期验证结果,对间冷器结构进行了迭代改进。结果表明:在一定范围内,翅片高度增加导致换热效率降低和总压恢复系数增大;翅片厚度增加,导致换热效率提高和总压恢复系数减小;隔板厚度增加导致换热效率降低。     

磁流体湍流中的结构和能量传输

磁流体湍流中存在多种相干结构,包括电流和涡旋结构。文章主要对近几年有关磁流体湍流相干结构及其相关的能量传输的一些工作进行了介绍。不同于中性流体湍流中的管状结构,磁流体中的相干结构多呈现为片状,强电流片附近也存在强涡片结构。磁流体湍流中的能量级串使能量跨尺度从大尺度传递至小尺度;与中性流体湍流能量传输主要集中在相近尺度上不同,磁流体湍流除了动能传输,还有磁能传输,以及动能与磁能之间的跨尺度互相转换。研究表明,磁流体湍流中的能量传输及耗散具有强间歇性,集中在较小区域范围,且与相干结构存在关联。在存在背景磁场的情况下,磁流体湍流中的相干结构在背景磁场方向上被拉长,而同样方向上的能量传输受到抑制。在高马赫数的情况下,激波的产生会使能量传输明显增强,同时带来很强的间歇性,结构函数标度律远远偏离线性标度关系,并且随着阶数的增加,标度指数会达到饱和值。