某型发动机进口压力畸变实验研究与分析

发动机进口流场畸变是影响发动机稳定性的一个很关键的降稳因子,而进口压力场周向分布不均匀对燃气涡轮发动机的稳定工作范围有很大影响.通过对某型涡喷发动机进行进口压力畸变模拟实验,探讨了发动机进口流场压力畸变的实验程序和方法,通过对实验数据的分析和处理,确定了该型发动机的稳定性对进气压力畸变的敏感程度.     

基于传热与压力损失的气-水换热器耦合设计

针对换热器设计中如何合理兼顾传热效率和压力损失的难题,以矩形流通截面的燃气-水列管式换热器为对象,从理论上分析了设计参数之间的内在联系,揭示了换热面积与燃气流通面积、横向管间距、换热管直径之间的匹配关系,建立了基于压力损失和传热计算的耦合设计方法。这种方法已成功应用于某大型燃气冷却器的设计,也可供其它换热器设计时参考。     

高背压等离子点火器及其液体燃料点火特性实验研究

航天应用的液体火箭发动机及燃烧型加热器燃烧室室压高、燃料流量大、温度低、有重复启动需求,实现安全可靠点火的难度较大.针对这些需求,研究了一种采用高背压设计的电弧等离子体点火器.实验研究了Ar,N2气体工质在高进气压力下的伏安特性,发现N2在宽压力范围内适用于点火.发射光谱分析表明,在高达数MPa的进气压力下,Ar,N2...     

脉动压力测量技术在火箭发动机试验中的应用

为研究和探索火箭发动机地面试验推力室脉动压力测量方法和数据分析技术,介绍了火箭发动机试验中脉动压力测量系统的组成和参数的测量方法;分析了引压导管的动态特性及其对脉动压力参数测量的影响;采用齐平安装的方式,按照所述方法建立脉动压力参数测量系统;结合推力室多个振动测点的数据,分别采用快速傅里叶变换(FFT)和小波包分解两种...     

不同边界层厚度下高马赫数进气道自起动过程研究

为了探寻入口边界层厚度变化对高马赫数进气道自起动性能的影响,对简化的二元高马赫数进气道的加速自起动过程进行数值仿真研究,分析了边界层厚度对自起动过程中流场波系结构变化和自起动性能的影响机制,获得了不同边界层厚度下的进气道自起动性能及主分离包高度的变化规律。结果表明:随着边界层相对厚度从0.05增加至0.3,进气道的自起动马赫数一开始保持不变,然后快速增大;相同主流条件下,不起动流场跨越主分离包无量纲压升和主分离包高度随边界层相对厚度的增大均变小;边界层动量损失厚度和跨越主分离包无量纲压升对进气道起动性能影响重大。     

飞行器级间段跨声速脉动压力特性试验

通过脉动压力风洞试验测量，对比分析了跨声速（马赫数介于0.75~1.2）不同锥角和锥长大小的级间段对锥柱外形飞行器局部脉动压力的影响规律。结果表明，肩部脉动压力主要由以低频为主导的激波振荡所致，能量集中在100 Hz左右的窄带区间，且表现为随着马赫数增加，脉动压力系数峰值先增大后减小，并随着肩部激波的后移而不断向后推移。此外，通过对比分析5种不同锥角模型（10°、12.7°、15.3°、20°、25°）的脉动压力系数最大值发现，随着锥角的增加，脉动压力表现出当锥角小于15°时先平缓增加，随着锥角增大脉动压力系数增加幅度进一步加大的趋势。对比分析不同锥长模型的结果发现，锥长对局部脉动压力的最大峰值几乎没有影响，影响的只是脉动压力在肩部作用区域的大小以及峰值出现的马赫数范围，且表现为锥柱级间段越长其作用范围越大，对应于峰值的马赫数区间越宽。     

Multi-wavelength coordinated observations of ionospheric irregularity structures from an anomaly crest location during unusual solar minimum of the 24th cycle

The present paper reports coordinated ionospheric irregularity measurements at optical as well as GPS wavelengths. Optical measurements were obtained from Tiny Ionospheric Photometer (TIP) sensors installed onboard the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites. GPS radio signals were obtained from a dual frequency GPS receiver operational at Calcutta (22.58°N, 88.38°E geographic; geomagnetic dip: 32.96°; 13.00°N, 161.63°E geomagnetic) under the SCIntillation Network Decision Aid (SCINDA) program. Calcutta is located near the northern crest of Equatorial Ionization Anomaly (EIA) in the Indian longitude sector. The observations were conducted during the unusually low and prolonged solar minima period of 2008–2010. During this period, four cases of post-sunset GPS scintillation were observed from Calcutta. Among those cases, simultaneous fluctuations in GPS Carrier-to-Noise ratios (C/N_o) and measured radiances from TIP over a common ionospheric volume were observed only on February 2, 2008 and September 25, 2008. Fluctuations observed in measured radiances (maximum 0.95 Rayleigh) from TIP due to ionospheric irregularities were found to correspond well with C/N₀ fluctuations on the GPS links observed from Calcutta, such effects being noted even during late evening hours of 21:00–22:00 LT from locations around 40° magnetic dip. These measurements indicate the existence of electron density irregularities of scale sizes varying over several decades from 135.6 nm to 300–400 m well beyond the northern crest of the EIA in the Indian longitude sector during late evening hours even in the unusually low solar activity conditions.     

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。     

Solar flares,CMEs and solar energetic particle events during solar cycle 24

We present here a study of Solar Energetic Particle Events (SEPs) associated with solar flares during 2010–2014 in solar cycle 24. We have selected the flare events (≥GOES M-class), which produced SEPs. The SEPs are classified into three categories i.e. weak (proton intensity?≤?1?pfu), minor (1?pfu?<?proton intensity?<?10?pfu) and major (proton intensity?≥?10?pfu). We used the GOES data for the SEP events which have intensity greater than one pfu and SOHO/ERNE data for the SEP event less than one pfu intensity. In addition to the flare and SEP properties, we have also discussed different properties of associated CMEs.