机翼重量分配方法在轻型飞机中的应用

针对目前飞机初始设计阶段的机翼重量估算公式变量较多,条件限制因素较复杂的情况,提出了一种按照机翼重量分配来估算重量的方法。把机翼重量分配到：承弯结构、承剪结构、分布气动载荷结构、起落架影响结构、前后缘结构、襟副翼机构,燃油影响结构、以及其它附属结构。此方法已经在大型飞机的机翼重量估算上取得了良好的效果。通过与一系列常用机翼重量估算公式的对比分析,并且利用已知的10种轻型飞机完成了算例,结果证明此方法有很强的适应性。     

Coupled Stress-Electricity Model for Electromagnetic Emission Induced by Concrete Fracture

Electromagnetic emission induced during concrete fracturing is of great significance to health monitoring of concrete structures.A coupled stress-electricity model is established by analyzing the interaction between stress and electricity during concrete fracturing.And based on this model,the electromagnetic radiation parameters are calculated.The theoretical calculation is well coincident with experimental results.This work provides theoretical support for concrete testing system.     

急冷锅炉炉管结构优选分析

针对急冷锅炉采用ANSYS软件对急冷锅炉换热单元结构进行数值模拟,得到热负荷均匀情况下各炉管流量分配规律。根据辅助连接管的直径及位置提出6种结构方案,研究其流量分配规律,获得了最优结构。采用数值模拟研究得出最优结构入口联箱和扁圆管的速度场、压力场分布规律均较原结构均匀,从而验证这一结论的正确性。     

离子与霍尔电推进性能和质量的工程数据模型

为了提供航天工程任务设计时优选离子或霍尔电推进的通用对比分析方法,基于工程数据建立了包括推力器、电源处理单元、推力器选择单元、控制单元、推进剂气瓶、调压单元、流率单元、推力器支架、电缆、管路等产品的电推进的性能和质量经验模型。在此基础上通过推导建立了电推进系统干质量通用模型,模型变量参数包括推力器功率、推力器数量和推进...     

小型磁偏转质谱计性能实验研究

自主研发了小型磁偏转质谱计,并对其质量范围、分辨本领、灵敏度和最小可检分压力四个主要性能指标进行了实验测试和比对。结果表明,该质谱计的质量范围为（1~143）amu,相对N₂的分辨本领为1400,灵敏度为4.2×10^-5 A/Pa,最小可检分压力为9.5×10^-7 Pa。该测试和比对结果为磁偏转质谱计进一步的优化设计和性能提高奠定了重要基础。     

谐波信号的通用频谱校正算法在回转机械监测中的应用

分析了常规FFT谱由于能量泄漏和栅栏效应,不能获得简谐振动信号精确幅值、频率和相位的原因。针对现有校正频谱方法的不足,提出了基于黄金分割的通用频谱校正算法。经仿真实例验证,该方法具有计算量小、校正精度高、适应面广的特性。经过回转机械启动实例分析,该方法能得到准确的临界转速、升速曲线和幅频响应曲线,为回转机械的瞬态行为分析提供了新的手段。     

旋转热源传热特性的理论研究

研究了旋转热源的热传导问题，并将其简化为一维、旋转的周期性脉冲热源传热问题。类似于流体流动，一组新的由旋转角速度ω、热物性参数和几何尺寸组合而成的无量纲拟贝克数Pe1，Pe2．毕奥数Bi被导出。结果表明．它们对传热过程起决定性作用。尤为重要的是，数值仿真对每周转的温度分布给出了微观的“精细”结构和宏观的“粗糙”结构，两的差别取决于上述无量纲数的不同组合，显示了上述几个无量纲准则数的相对关系对传热特性的影响。     

装有多孔介质的封闭腔体中热驱动换热的数值研究

以涡轮叶片超级冷却技术为研究背景,用数值计算的方法,模拟了离心力场下装有多孔介质的封闭腔体中的热驱动换热现象。计算结果表明,在封闭腔体中加入大孔隙率多孔介质后确实能起到强化换热的效果,采用的固体介质的导热性越好,封闭腔体中流体的热驱动能力越强,换热效果越好。而且采用导热性比较好的固体介质时,在大孔隙率范围内,随着孔隙率的减少,封闭腔体中流体的热驱动能力和换热均得到增强。     

Space storm measurements of the July 2005 solar extreme events from the low corona to the Earth

The Athens Neutron Monitor Data Processing (ANMODAP) Center recorded an unusual Forbush decrease with a sharp enhancement of cosmic ray intensity right after the main phase of the Forbush decrease on 16 July 2005, followed by a second decrease within less than 12 h. This exceptional event is neither a ground level enhancement nor a geomagnetic effect in cosmic rays. It rather appears as the effect of a special structure of interplanetary disturbances originating from a group of coronal mass ejections (CMEs) in the 13–14 July 2005 period. The initiation of the CMEs was accompanied by type IV radio bursts and intense solar flares (SFs) on the west solar limb (AR 786); this group of energetic phenomena appears under the label of Solar Extreme Events of July 2005. We study the characteristics of these events using combined data from Earth (the ARTEMIS IV radioheliograph, the Athens Neutron Monitor (ANMODAP)), space (WIND/WAVES) and data archives. We propose an interpretation of the unusual Forbush profile in terms of a magnetic structure and a succession of interplanetary shocks interacting with the magnetosphere.     

Modelling and observations of photospheric magnetic helicity

Mounting observational evidence of the emergence of twisted magnetic flux tubes through the photosphere have now been published. Such flux tubes, formed by the solar dynamo and transported through the convection zone, eventually reach the solar atmosphere. Their accumulation in the solar corona leads to flares and coronal mass ejections. Since reconnections occur during the evolution of the flux tubes, the concepts of twist and magnetic stress become inappropriate. Magnetic helicity, as a well preserved quantity, in particular in plasma with high magnetic Reynolds number, is a more suitable physical quantity to use, even if reconnection is involved.