大型飞机整体壁板喷丸成形延展变形分析

针对基于喷丸成形的大型飞机机翼整体壁板延展变形问题,从影响整体壁板喷丸延展变形的因素出发,通过对整体壁板喷丸成形展向应变的理论计算和实测延展数据对比,得出整体壁板喷丸成形加工环节的延展变形规律。     

变循环发动机对战斗机任务性能影响计算研究

为了研究战斗机任务性能模型的可行性,以战斗机为研究对象,假设其安装变循环发动机,以F-22战斗机机内燃油和带副油箱的任务性能为标准结果,考虑全部的飞行过程,对所建立的模型进行可行性验证。结果表明:计算得到的F-22战斗机内燃油和带副油箱任务性能与文献中的标准结果十分接近,误差分别为0.76%和0.24%;假设的变循环发动机使得加速及超声速飞行等涡喷模式的耗油率降低20%,亚声速巡航航段涡扇模式的耗油率降低25%,变循环发动机能够使战斗机的转场航程增加27.2%,亚声速截击任务剖面的作战半径增加29.1%。本算法具有一定的准确性,可信度较高。     

超高压比民用发动机部件技术水平初步研究

提高总增压比是下一代民用发动机的重要发展趋势之一,有必要对于这一特征的涡扇发动机进行循环参数的研究。利用已有基于Gasturb平台开发的0维变比热部件级性能计算模型,在发动机安装尺寸给定的前提下,总增压比由40提高至60,分析比较不同构型的直驱风扇方案与齿轮传动方案对部件效率,冷却水平对循环参数优选过程的影响。结果表明:为实现更低耗油率,采用更高设计循环增压比,需要部件效率平均提高1%,冷却水平提高20%,此时性能均优于现有的大涵道比涡扇发动机GTF-11。因此,若技术水平未能达到预期目标,则需匹配合适的增压比才能达到更低的耗油率。     

美国自适应发动机研究的进展与启示

为借鉴和参考美国自适应循环发动机的研究与研制经验,综述了美国变循环发动机演变至自适应发动机的3个发展阶段,重点介绍了其在多用途经济可承受的先进涡轮发动机(VAATE)研究计划下的自适应通用发动机技术(ADVENT)分计划、自适应发动机技术验证(AETD)分计划、自适应发动机过渡(AETP)分计划和空中优势自适应推进技术(ADAPT)分计划的开发与验证情况。分析总结出美国自适应发动机具有以下特点:技术先进且应用前景广泛,代表未来发展方向;变循环与自适应循环技术均不成熟,还需深入验证;技术研究采用竞争策略实施。     

预测飞机稳定尾旋的解析法和图像法

尾旋是飞机的极限飞行状态,此一状态极易造成机毁人亡。由于尾旋试飞有极大的风险性,所以在试飞前要进行足够的安全论证,包括理论分析和风洞试验,一般采用两者相结合的方式进行。介绍了解析法和图像法两类方法来研究飞机的稳定尾旋。     

一种基于余数周期的 PRI精确估计算法

针对传统脉冲重复间隔（PRI）分选算法在估计PRI方面存在的不足,提出了一种对PRI周期信号的周期进行精确估计的算法。该算法首先从待分选脉冲序列中提取出属于一部雷达的脉冲样本,然后利用同余方程的余数周期性质对该雷达脉冲序列的PRI进行精确的估计。相对于传统的PRI估计算法,该算法有效地消除了TOA量化误差对PRI估计造成的影响,可以精确地估计出雷达脉冲序列的准确 PRI数值,从而能够更好地满足信号分选算法的处理需求。理论推导及仿真实验均表明了该算法的有效性。     

舵机滚珠丝杠在内部热源作用下响应特性

舵机滚珠丝杠在运行过程中由于摩擦作用和电机运行产生的内部热源会导致其结构温度上升和变形,是影响滚珠丝杠副运行精度的因素之一。本文基于有限元理论建立舵机滚珠丝杠副模型,并通过在ANSYS Workbench中插入命令流的方式实现了在滚珠丝杠上施加移动摩擦热载荷,获得了滚珠丝杠副在内部热源作用下的温度、变形和应力响应特性。结果表明:滚珠丝杠轴向热流密度呈双峰趋势,且其高温区域主要集中在螺母行程范围内的中间区域;随着转速的增加,滚珠丝杠各处温度及其波动幅度加大;丝杠最大热应力位于与轴承配合的轴肩最外侧处。     

双太阳翼GEO卫星在轨角动量管控方法

地球同步轨道(GEO)卫星在轨的主要环境干扰力矩为太阳光压力矩和重力梯度力矩,干扰力矩的累积效应表现为飞轮转速的变化,需要通过外力矩进行角动量卸载避免飞轮饱和。由于GEO磁场极弱,卫星无法使用磁力矩卸载,只能通过喷气卸载,而喷气将对卫星轨道产生影响,因此需要尽可能延长卸载周期。针对配置双对称太阳电池阵GEO卫星的角动量管控需求,首先建立卫星在惯性空间中角动量积累模型,并映射到卫星本体系中,得到本体系中的角动量变化规律。通过飞轮在轨转速遥测数据,精确辨识获取环境干扰力矩特征参数,获得真实可靠的干扰模型。以角动量卸载周期最长为原则,基于在轨环境干扰模型制定角动量管控策略,并准确预估下次角动量卸载时间。经在轨数据处理与分析表明:提出的角动量管控策略,可有效将飞轮的角动量卸载周期提升为原来的2倍,有效提升卫星在轨应用效能,具有实际工程意义。     

Investigation on surface roughness,residual stress and fatigue property of milling in-situ TiB2/7050Al metal matrix composites

For higher efficiency and precision manufacturing, more and more attentions are focused on the surface roughness and residual stress of machined parts to obtain a good fatigue life. At present, the in-situ TiB₂/7050Al metal matrix composites are widely researched due to its attractive properties such as low density, good wear resistance and improved strength. It is of great significance to investigate the machined surface roughness, residual stress and fatigue life for higher efficiency and precision manufacturing of this new kind material. In this study, the surface roughness including two-dimensional and three-dimensional roughness, residual stress and fatigue life of milling in-situ TiB₂/7050Al metal matrix composites were analyzed. It was found from comparative investigation that the three-dimensional surface roughness would be more appropriate to represent the machined surface profile of milling particle reinforced metal matrix composites. The cutting temperature played a great role on the residual stress. However, the effect of increasing cutting force could slow down the transformation from compressive stress to tensile stress under 270 °C. An exponential relationship between three-dimensional roughness and fatigue life was established and the main fracture mechanism was brittle fracture with observation of obvious shellfish veins, river pattern veins and wave shaped veins in fracture surface.     

Time-dependent cosmic ray modulation

Time-dependent cosmic ray modulation is calculated over multiple solar cycles using our well established two-dimensional time-dependent modulation model. Results are compared to Voyager 1, Ulysses and IMP cosmic ray observations to establish compatibility. A time-dependence in the diffusion and drift coefficients, implicitly contained in recent expressions derived by , ,  and , is incorporated into the cosmic ray modulation model. This results in calculations which are compatible with spacecraft observations on a global scale over consecutive solar cycles. This approach compares well to the successful compound approach of Ferreira and Potgieter (2004). For both these approaches the magnetic field magnitude, variance of the field and current sheet tilt angle values observed at Earth are transported time-dependently into the outer heliosphere. However, when results are compared to observations for extreme solar maximum, the computed step-like modulation is not as pronounced as observed. This indicates that some additional merging of these structures into more pronounced modulation barriers along the way is needed.