风扇转子叶片周向积叠的三维气动优化设计

为了研究优化环境对优化结果的影响,利用商业软件NUMECA对某风扇第一级转子叶片进行了气动优化设计,并对比研究了第一级转子单排叶片的优化及其在整级环境中的优化结果。研究发现．单叶排优化后．虽然能提高整级风扇的效率,但是由于匹配的原因,整级风扇在整个流量范围内总压比都比优化前的有所减小;在级环境中优化后,该级风扇的效率和稳定工作范围都扩大了,且保证了级压比不变,其优化效果比单叶排的优化效果好。     

机载电子设备在海洋环境中的腐蚀分析

为了分析清楚机载电子设备部件在海洋气候环境中发生腐蚀现象的原因。对发生腐蚀的壳体、螺钉和连接器进行取样,对样品的正面及切片的横截面利用扫描电子显微镜、X射线能谱仪、X射线光电子能谱仪和红外线光谱分析仪等技术手段进行分析。通过分析表明电子设备不仅遭受盐雾环境腐蚀,而且还有浸渍海水的现象。针对机载电子设备腐蚀分析的结果,结合工程设计经验,从机载电子设备结构设计、防护工艺两方面提出了具体的改进方法来避免或减少腐蚀现象的发生。     

高超声速钝锥模型及其尾迹红外辐射实验研究

介绍了利用InSb红外辐射计在弹道靶上测量底部直径为10mm、半锥角和头部半径分别为9°、2.2mm(模型A),8°、0.6mm(模型B)的两种非烧蚀钝锥模型及其尾迹的红外辐射.模型速度大于6km/s,飞行环境压力约4.8kPa,红外辐射测量波段为1~3μm、3~5μm.结果表明:非烧蚀钝锥模型头身部红外辐射远大于尾迹红外辐射,在相同飞行速度和环境压力条件下,模型A产生的红外辐射比模型B产生的红外辐射强.     

导弹蒙皮红外辐射特性的数值计算与分析

采用逆向蒙特卡罗(RMC)计算方法,在给定的飞行状态下分别计算出亚声速与超声速导弹蒙皮辐射源在不同方位角的2～μm、8～14 μm波段红外光谱辐射强度及强度场分布.结果表明:对亚声速导弹,相对于8～14 μm,其2～μm的辐射可忽略不计;对超声速导弹,相对于2～μm,其8～14 μm的辐射只有0%左右,但其绝对值较大而不可忽略不计.导弹的红外辐射在0°～90°探测位置内增加,在90°～180°内减小.大气对低空亚声速导弹辐射衰减作用强,对高空超声速导弹辐射衰减作用弱.超声速导弹的最大辐射强度是亚声速的18倍.      

诱发卫星深层充电的高能电子环境模式研究

文章介绍了与卫星介质深层充电相关的辐射带高能电子环境的主要特征和规律,建立了相应的高能电子环境模式及软件,并运用该模式针对某飞行器的深层充放电危险性进行了分析和评估。结果表明该模式相对于AE8模式更好地反映了高能电子环境的动态特征,与欧空局建立的FLUMIC模式符合较好。该模式与深层充电分析模型相结合,可用于对航天器的充放电异常进行在轨诊断,以及在工程上针对深层充电进行防护设计。     

航天材料对质子辐射防护性能的模拟研究

随着航天材料技术的飞速发展,先进复合材料(ACM)在航天器上的应用价值越来越大。文章从辐射防护角度对航天材料的防护性能作出评价。利用SRIM程序,先模拟各单元素材料的辐射防护性能,再结合实际模拟多种材料的辐射防护效果,对比分析先进复合材料在航天器质子辐射防护上的优势。     

多机并联火箭羽流流场及其底部热环境分析

针对某多机并联火箭羽流流场结构复杂、底部热环境极为恶劣,有可能导致发动机结构部件失效的问题,通过数值仿真对其飞行过程不同高度下的羽流流场及热环境进行研究,并与热环境实测结果进行了对比分析。计算结果表明:火箭低空飞行时,各发动机羽流互不干扰,随着飞行高度不断增加,羽流逐渐扩张并开始相互干扰,最后在箭体底部出现明显回流,最大热流在起飞时刻,与飞行实测值基本一致。出现回流之前,箭体底部主要受辐射热影响,随着回流出现,对流热流随之增大,但也远小于起飞时刻的热流峰值。计算得到的多机并联火箭羽流流场及其热环境分布对发动机舱外结构热防护优化设计具有一定的指导意义。     

Nonlinear aeroelastic analysis of the folding fin with freeplay under thermal environment

The nonlinear aeroelastic behavior of a folding fin in supersonic flow is investigated in this paper. The finite element model of the fin is established and the deployable hinges are represented by three torsion springs with the freeplay nonlinearity. The aerodynamic grid point is assumed to be at the center of each aerodynamic box for simplicity. The aerodynamic governing equation is given by using the infinite plate spline method and the modified linear piston theory. An improved fixed-interface modal synthesis method, which can reduce the rigid connections at the interface, is developed to save the problem size and computation time. The uniform temperature field is applied to create the thermal environment. For the linear flutter analyses, the flutter speed increases first and then decreases with the rise of the hinge stiffness due to the change of the flutter coupling mechanism. For the nonlinear analyses, a larger freeplay angle results in a higher vibration divergent speed. Two different types of limit cycle oscillations and a multiperiodic motion are observed in the wide range of airspeed under the linear flutter boundary. The linear flutter speed shows a slight descend in the thermal environment, but the effect of the temperature on the vibration divergent speed is different under different hinge stiffnesses when there exists freeplay.     

配置点谱方法求解非均匀介质内辐射传热问题

发动机内的燃气等高温介质随着组分和浓度的变化，会引起折射率在空间上的非均匀分布，从而导致辐射能束沿着曲线传播，其相应的辐射传热过程也更为复杂。为了避免射线追踪方法的复杂计算、提高计算效率，本文提出了配置点谱方法求解二维非均匀介质内辐射传热问题。在求解过程中，角向采用离散坐标法处理，空间采用配置点谱方法处理。通过将三种非均匀介质内辐射传热问题的配置点谱方法结果与文献结果进行对比分析，发现配置点谱方法可以在较少的节点数下，获得准确、有效地计算结果。并且，采用配置点谱方法求解三种算例的计算时间均消耗较少，均在20分钟以内。这将为进一步开展发动机复杂结构内高温燃气辐射快速仿真提供基础。     

Observations of the local interstellar medium with the Extreme Ultraviolet Explorer

Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm^–3 while the H II density ranges between 0.0 and 0.14 cm^–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm^–3 K, a factor of 2 to 3 above previous estimates.