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41.
本文通过计算机模拟研究,结合气体折射率场的光验知识.考查了将Radon变换迭代法用于光学干涉层析计量含有遮挡物的三维折射率场的重建精度。作为一个应用实例,测量和计算了某一截面的气体温度分布,并与热电偶测量的值进行了比较。  相似文献   
42.
航天材料热物理性能测试技术的发展现状   总被引:1,自引:0,他引:1  
根据航天材料热物理性能测试技术的特点 ,系统介绍了国内航天材料热物理性能测试技术的发展状况和发展趋势 ,并详细介绍了目前我国航天材料热物理性能测试领域中所具备的测试技术和测试装置、航天热物理性能所涉及的研究领域和内容以及目前正在开展的研究工作。  相似文献   
43.
喷管扩张段烧蚀的“台阶效应”计算   总被引:1,自引:0,他引:1       下载免费PDF全文
何国强  何洪庆  毛根旺 《推进技术》1990,11(6):19-22,73
当喉衬和扩张段内衬采用具有不同烧蚀率的材料时,常出现“台阶效应”.本文以气动热化学烧蚀机理为基楚,提出应用适当的对流换热和加剧的化学反应计算对台阶效应区进行修正的方法,使台阶效应区的烧蚀率预示更切合实际工况.  相似文献   
44.
于雪晖  王盾  李周  赵鸿娟 《航空学报》2019,40(5):322507-322507
提出一种面向未来卫星在轨应用的闭环物理高精度时间同步方法。比较了所提方法与其他时间同步方法的区别与优势,建立了远程系统时间同步基本模型与误差传递模型,基于双向测距和时间传递技术分析了高精度钟差获取原理,给出了时钟调整环路的时域频域参数依赖关系。完成了高精度时间同步地面试验系统构建,测试了开环非调钟状态下钟差测量精度误差、闭环调钟状态下时间同步准确度误差以及长时运行情况下的时间同步监测结果。测试结果表明,该方法能够实现优于1 ns量级的时间同步,为高精度时间同步技术研究提供了新的途径。  相似文献   
45.
为提高铯束管跃迁信号强度,在束光学参数设计中,用蒙特卡罗方法模拟计算铯原子通过率和未跃迁比例。通过改变模拟计算中的束光学参数,分析铯原子通过率、未跃迁比例和倍增器首极电流的变化趋势,得到了主要束光学参数的合理取值范围。在铯束管实际装配和试验中使用束光学参数设计结果,有效地增加了倍增器首极电流。  相似文献   
46.
《中国航空学报》2020,33(7):2043-2054
Finite element modeling (FEM), microscopy, X-ray computed tomography (CT) and mechanical property tests were used to study the microstructure, porosity and mechanical properties of an AlSi10Mg alloy produced by selective laser melting (SLM). The simulation of the melt pool and thermal history under different energy densities produced an optimized result with an energy density of 44.5 J·mm−3. The high cooling rate during the SLM process significantly refined the previous α-Al dendrites. The growth direction of the network-like Al-Si eutectic structure at different orientations confirmed the anisotropic nature of the microstructure. Furthermore, the microhardness, tensile testing and fracture analysis results proved that there were no obvious distinctions in the strength between the transverse and longitudinal directions, and that the ductility was anisotropic, possibly due to the shape and distribution of the pores. The pores measured by X-ray CT at different energy densities confirmed that the sphericity of the pores was inversely related to pores volumes. With optimized processing conditions, the porosity of the selective laser melted sample decreased leading to the improved fabricated fuel system component via SLM.  相似文献   
47.
以丁腈橡胶(CTBN)为增韧剂对环氧树脂(F51)进行增韧改性,通过FTIR、TG以及力学性能测试研究了丁腈橡胶对环氧树脂固化反应、热稳定性能和力学性能的影响,并分析了其增韧机理;分别采用燃气流剪切烧蚀试验和电弧风动烧蚀实验考核了低密度烧蚀材料的烧蚀性能。结果表明:经CTBN改性后,两者的分子链产生了一定程度的交联;树脂基体的拉伸、弯曲性能有所下降,但韧性得到了增强;热稳定性大大提高,增韧后的F51树脂在800℃时的残重率由增韧前的23%提高到了54%;低密度烧蚀材料的抗剪切、抗剥蚀能力得到了增强,且碳层的尺寸稳定性也得到了改善,烧蚀性能提高。  相似文献   
48.
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.  相似文献   
49.
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.  相似文献   
50.
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.  相似文献   
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