离散光谱分辨率对喷流红外特性FVM计算的影响

建立了辐射传递方程(RTE)的有限元体积法(FVM)计算模型,研究了离散光谱分辨率对FVM计算精度的影响,提出了离散光谱分辨率无关解的概念,并编制了相应的FORTRAN源程序,结合大气飞行发动机标准算例进行了一系列计算和比较.结果表明;在给定的红外光谱域中,随着离散光谱的分辨率的提高,计算出的方向光谱辐射强度渐渐趋向于同一个值.在航空发动机喷流2～5μm红外光谱区间中,当划分150个以上等间隔光谱微元后,FVM可以保证达到离散光谱分辨率无关解.      

利用红外技术进行层板冷却特性实验研究

为了研究层板冷却特性,应用远红外热像测温技术,对一个真实尺寸的层板结构进行了实验.层板的气膜孔、绕流柱及冲击孔直径分别为0.,0.8,0.8 mm,内腔高及总板厚分别为0.8,2.6 mm,孔柱数比为1:4:1.为了准确测量表面温度,采用了高精度热电偶校正法,建立修正关系;为了描述层板综合冷却效率,采用热像数字信号运算法,直接进行数据处理.实验在高温亚声速风洞中进行,实验结果展示了冷却介质注射量对层板冷却特性的影响,证明远红外热像技术用来研究层板冷却特性是一种有效的方法.      

空间红外遥感器定标机构故障应急退出装置

针对空间红外遥感器定标机构故障模式,首次设计了一种基于记忆合金的应急退出装置,以解决因电机或控制电路故障而导致的整个成像系统失效问题。该应急退出装置通过对记忆合金棒进行加热,使其受热收缩,从而驱动齿轮传动系统脱离啮合状态,完成机构复位运动。为验证该应急退出装置的功能和性能,利用研制产品进行了真空、大气环境等多种状态下的应急退出试验。结果表明:在大气和真空环境中,该装置能实现多种状态下的可靠退出功能;在28 V额定直流工作电压下,应急退出总时间可达145～152 s。该机构具有实现简便、可靠性高、退出速度快等优点,在空间机构的故障应急方面具有较大的工程应用潜力。     

玫瑰扫描光学系统头罩气动热建模与仿真

在导弹高速飞行过程中，光学头罩的温度受气动热效应作用而急剧升高，会产生严重的气动热辐射效应。为研究头罩气动热对玫瑰扫描光学系统的影响，建立了基于CFD流体仿真软件的头罩温度场模型。在仿真软件对光学系统结构进行三维建模后，通过光学软件对头罩热辐射对探测器的影响进行了仿真和计算。仿真结果表明：玫瑰扫描光学系统对头罩的温度梯度较为敏感，当头罩温度非均匀分布时，探测器会接收到气动热辐射干扰信号，对弱小目标的正常探测和提取产生干扰，气动热辐射效应不容忽视。     

Triton, Pluto, Centaurs, and Trans-Neptunian Bodies

The diverse populations of icy bodies of the outer Solar System (OSS) give critical information on the composition and structure of the solar nebula and the early phases of planet formation. The two principal repositories of icy bodies are the Kuiper belt or disk, and the Oort Cloud, both of which are the source regions of the comets. Nearly 1000 individual Kuiper belt objects have been discovered; their dynamical distribution is a clue to the early outward migration and gravitational scattering power of Neptune. Pluto is perhaps the largest Kuiper belt object. Pluto is distinguished by its large satellite, a variable atmosphere, and a surface composed of several ices and probable organic solid materials that give it color. Triton is probably a former member of the Kuiper belt population, suggested by its retrograde orbit as a satellite of Neptune. Like Pluto, Triton has a variable atmosphere, compositionally diverse icy surface, and an organic atmospheric haze. Centaur objects appear to come from the Kuiper belt and occupy temporary orbits in the planetary zone; the compositional similarity of one well studied Centaur (5145 Pholus) to comets is notable. New discoveries continue apace, as observational surveys reveal new objects and refined observing techniques yield more physical information about specific bodies.     

Pre-Main Sequence Stars Seen by ISO

Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive the questions which should be answered by the forthcoming FIR instrumentation. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

The Cool Interstellar Medium

Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the interstellar medium, where T _gas≲ 500 K, n _H∼ 100–10⁵ cm⁻³ and the electron density is a few 10⁻⁴. JEL codes: D24, L60, 047 Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

卫星真空热试验中红外加热笼的创新设计

针对某型号卫星加热笼设计中的一些特殊问题,设计了一些特殊的处理方法,包括加热带双面涂黑漆的方法,加热笼结构设计中的一些特殊处理,以及支架控温装置等的设计。试验证明,这些方法在卫星真空热试验过程中取得了好的效果,可以为今后加热笼的设计开阔思路,有利于更好地完成试验任务。     

Thermo-mechanical properties of RTM-made carbon fibre/polyimide composite attaching collar under transient heating

This study focuses on the thermo-mechanical properties of Carbon Fibre/Polyimide Composite (CFPC) attaching collars under transient heating. The CFPC attaching collars were fabricated by a high-temperature resin transfer moulding process, and their thermo-mechanical properties under the conditions of simultaneous transient heating and bending load were investigated. The results show that the attaching collar tends to fail at 118% of the limit load. The failure mode includes the fracture of the connecting screws, local extrusion damage of the hole edges, and slight ablation damage at the outer plies. And there is no observable residual deformation in the composite attaching collar. Furthermore, considering that the material properties vary with temperature, a progressive damage model based on the sequential thermo-mechanical coupling method was established to study the failure mechanism of the attaching collar. Finally, the damage factor of the CFPC was calculated to assess the safety status of the attaching collar. The results show that the primary damage modes of the composite attaching collar are intralaminar failure, which mainly occurs at the heat insulation layer and the hole edges, and these slightly affect the structural bearing capacity. A good correlation between the experiment and FEA is obtained. The test methods and analysis models proposed contribute to the safety assessment of composite structures under transient heating.     

进气加温模拟装置对涡扇发动机进气流场稳定性影响试验

为分析新设计的进气加温模拟装置对涡扇发动机进气流场稳定性的影响,对试验设备、测试方案、进气流场的稳定性评 估方法和试验方案进行设计研究。通过开展气源供气温度、供气流量和发动机状态多因素匹配工况下涡扇发动机与进气加温模 拟装置的联合试验,确定发动机进口气流稳定性指标的最高值。对不同试验工况数据进行计算分析,结果表明：进气加温模拟的 稳压进气道对发动机进口压力场影响较小,发动机状态稳定时进口温度场只有1个高温区,T 1 升高以及发动机状态提高,温度场及 压力场不稳定性增大,多工况下发动机温场周向不均匀度最大为0.6907%,压力场周向畸变指数最大为0.0187%。进气加温模拟 装置条件下,发动机压力场和温度场稳定性情况满足发动机试验要求,可为后续开展发动机进气加温试验提供参考。