环向圈连带冠叶片的动态分析

 本文将动态子结构方法中链式加载技术与群论算法相结合,提出环向固连带冠叶片动力特性分析的一种新方法。文中列出了分析步骤与具体公式,并有实例的计算结果。该方方法适用于研究具有带冠叶片的单级转子中,“冠”的整体效应。     

涡流阀几何参数对固体发动机推力调节特性的影响

为了获得涡流阀参数对发动机推力调节性能的影响规律,针对涡流阀的加注方式以及几何结构,利用建立的基于涡流阀方案的固体火箭发动机推力可调实验系统开展了实验研究。通过实验结果的分析,得到了加注环孔径、涡流室高度和直径以及中心进气面积的不同对涡流阀调节性能的影响规律。结果表明:适当降低涡流室的高度、较大的中心进气面积、较大的涡流室直径有利于提高涡流阀的调节性能。因此,可以通过对涡流阀结构的优化设计来提高发动机的推力调节性能。     

粉末高温合金FGH96惯性摩擦焊接头常温力学性能分析

第二代粉末高温合金FGH96是采用损伤容限设计思想研制的新型粉末高温合金,是当前750℃工作条件下满足高推比、高燃效发动机使用要求的涡轮盘、环形件和其他热端部件的理想材料.结合FGH96惯性摩擦焊接头的组织特征和强化相γ′数量分析接头的显微硬度和常温拉伸性能.结果表明,FGH96惯性摩擦焊接头具有良好的常温力学性能.     

计算机辅助公差设计与分析的研究现状及展望

对目前计算机辅助环境下的设计公差和工序公差的设计与分析、尺寸公差和形位公差的确定、公差设计理论以及计算机辅助公差的应用现状等多方面进行了归纳和概括,分析了当前这些技术和理论的不足,并结合当前的实情,展望了计算机辅助公差设计与分析技术的发展趋势.     

SRM 纤维缠绕壳体的蒙特卡罗随机有限元分析

采用蒙特卡罗随机有限元方法，结合复合材料壳体力学、纤维缠绕理论等知识，分析了固体火箭发动机纤维缠绕壳体在燃气内压随机变化作用下的应力响应，绘出应力分布曲线，为固体火箭发动机结构可靠性评估奠定基础。     

一次火箭参数对RBCC引射模态性能的影响

应用经过校验的三维湍流有限体积数值算法，对引射模态下RBCC模型不同一次引射火箭结构和工作参数条件下的多种工作状态进行了模拟。结果发现：提高一次火箭燃烧室工作压强，二次流量增加，系统推力增加，混合效果增强；一次火箭喷管形状直接影响引射掺混效果，但在保证足够一次流量的前提下，方形管道中可以使用锥形一次喷管，不会带来性能上的较大差异；一次火箭喷管数目增加，掺混质量提高；一次喷管扩张半角的改变不会影响二次引入流量，但会影响掺混效果和一次火箭自身推力；一次喷管面积膨胀比的变化，不会影响二次引入流量．但会改变混合效果。     

六喷管超音速引射器性能的理论分析和实验研究

对某一定尺寸的六喷管超音速引射器进行气动性能的实验研究。结果表明：随着主次流压比Ｐ＊ｐ／Ｐ＊ｓ增加，引射系数及修正引射系数下降；当引射系数增加时，混合管动量修正系数Ｋｍ下降，但主喷管流量系数μ变化不大。对上述工况进行理论计算的结果与实验数据符合良好。     

室温贮存对树脂粘度和加压点的影响

讨论了５４０５改性双马来酰亚胺树脂基体在室温下，贮存时间对粘度以及对固化过程中加压点的影响，给出了相应的计算方法。     

Phased array of large reflectors for deep-space communication

In this paper the problem of uplink array calibration for deep-space communication is considered. A phased array of many modest-size reflectors antennas is used to drastically improve the uplink effective isotropic radiated power of a ground station. A radar calibration procedure for the array phase distribution is presented using a number of in-orbit targets. Design of optimal orbit and the number of calibration targets is investigated for providing frequent calibration opportunities needed for compensating array elements phase center movements as the array tracks a spacecraft. Array far-field focusing based on the near-filed in-orbit (low Earth orbit (LEO)) calibration targets is also presented and array gain degradation analysis based on the position error of the array elements and in-orbit targets has been carried out. It is shown that errors in the in-orbit targets positions significantly degrade the far-field array gain while the errors in array elements positions are not very important. Analysis of phase errors caused by thermal noise, system instability, and atmospheric effects show insignificant array gain degradation by these factors     

The Pre-CME Sun

The coronal mass ejection (CME) phenomenon occurs in closed magnetic field regions on the Sun such as active regions, filament regions, transequatorial interconnection regions, and complexes involving a combination of these. This chapter describes the current knowledge on these closed field structures and how they lead to CMEs. After describing the specific magnetic structures observed in the CME source region, we compare the substructures of CMEs to what is observed before eruption. Evolution of the closed magnetic structures in response to various photospheric motions over different time scales (convection, differential rotation, meridional circulation) somehow leads to the eruption. We describe this pre-eruption evolution and attempt to link them to the observed features of CMEs. Small-scale energetic signatures in the form of electron acceleration (signified by nonthermal radio bursts at metric wavelengths) and plasma heating (observed as compact soft X-ray brightening) may be indicative of impending CMEs. We survey these pre-eruptive energy releases using observations taken before and during the eruption of several CMEs. Finally, we discuss how the observations can be converted into useful inputs to numerical models that can describe the CME initiation.