影响高超声速进气道起动能力的因素分析

对一系列不同收缩比、不同波系配置的内压缩通道二维流场进行了数值模拟。研究了面积收缩比、飞行高度和来流攻角对高超声速进气道起动性能的影响，提出了进口起动马赫数和来流起动马赫数的概念。研究表明，当进气道收缩比增大时，进气道的进口起动马赫数增大；来流起动马赫数由外压波系强度和进口起动马赫数决定，所以来流攻角变化改变外压波系强度，从而改变来流起动马赫数；随着飞行高度的增加，来流起动马赫数和进口起动马赫数增大，造成这一变化的原因是飞行高度不同，来流雷诺数不同，造成收缩段进口截面附面层厚度不同。     

超燃冲压发动机研究综述

超燃冲压发动机技术是一项新型的、具有广阔发展前景的推进技术。本文对国内外超燃冲压发动机最新研制情况进行了综述，重点论述了该类发动机关键技术研究情况，并对关键技术研究及思路提出了几点建议。     

固体火箭发动机试验模态分析技术研究

将固体火箭发动机划分为144个自由度，采用锤击法，单点激励多点响应（SIMO）对其在4种工况下进行了频率响应的测量，应用了多种方法进行模态参数识别和数据拟合，并对其结果进行比较，获得了发动机在各工况1kHz以内的各阶固有频率、振型和阻尼，并对试验模态分析技术在固体火箭发动机试验中的应用进行了研究。     

一种辅助高超音速进气道起动方法研究

用数值方法研究了楔角形内压缩进气道的起动过程,确定了研究楔角形进气道辅助起动方法是否有效的一般过程。研究了一种辅助进气道起动的方法,即将进气道突然暴露在高速气流之中。结果表明,降低进气道内初始压强,然后进行这种脉冲起动,可大大降低进气道的起动马赫数;发动机流道内初始压强对这种进气道辅助起动方法有重要影响,初始压强高于一定值时,该方法不产生作用。     

异型封闭腔辐射几何学问题

讨论了解决异型封闭腔辐射几何学问题的几种方法:异型封闭腔内,表面间可见性的判断方法;优化异型封闭腔角系数计算的方法;确定异型封闭腔内定向辐射的壁面辐射源的方法.计算了两种结构喷管封闭腔内的角系数,并从角系数的互换性和完整性定理验证了方法的正确性和有效性,为异型封闭腔的辐射计算解决了几何问题.     

The fundamental parameters of the central stars of eight WR ring nebulae

We describe work that has recently been completed on deriving the fundamental parameters of eight WR stars through the photoionization modelling of their surrounding nebulae using non-LTE WR flux distributions. The resulting effective temperatures range from 57 000–71 000 K for the WN4-5 stars and <30 000–42 000 K for the WN6-8 stars. The derived stellar parameters are compared with those obtained from stellar emission line modelling. We find good agreement for the hot early WN stars, indicating that the non-LTE WR flux distributions have essentially the correct shape in the crucial far-UV region. We find lower temperatures for the four cooler late WN stars, particularly for the two WN6 stars. For the nebulae surrounding these stars, we find that the model flux distributions produce too much nebular ionization. We suggest that these discrepancies arise because of the lack of line-blanketing in the WR atmospheres. For the WO1 central star of G2.4+1.4, with strong nebular He II 4686 A emission, we derive a temperature of 105 000 K, somewhat less than previous estimates. The positions of our eight WR stars on the H-R diagram are compared with the evolutionary tracks of Maeder (1990) for solar metallicity. In common with previous workers, we find that our derived luminosities are too low, giving an initial mass range of 25–40 M, below that expected for the majority of WR stars.     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

高超侧压进气道前/后掠的数值分析和比较

侧板构型和唇口位置是影响侧压式进气道性能的关键参数。选取了5个具有一定代表性的状态点对前/后掠进气道模型进行了计算和分析,重点比较了当侧板前/后掠时进气道的流量系数、压升、出口气流均匀度等性能。通过对比分析,发现侧板前掠时进气道的流量系数、压升大于侧板后掠结果,且进气道出口流场更均匀。当马赫数较低时,前/后掠进气道性能差别比较明显:同为50%溢流窗,来流马赫数4时,侧板前掠的进气道流量系数比侧板后掠的情形高出7.7%;而当来流马赫数为8.09时,侧板前掠的进气道流量系数仅高2.6%。     

直升机红外抑制器两种进气方式下的实验研究

利用地面模拟试验件通过实验比较分析了两种进气方式对红外抑制器性能的影响。为了模拟直升机前飞和悬停两种状态,在模型上端开口,分别引入旋翼下洗气流和前端进气,对比分析了这两种状态下模型壁面温度和红外辐射强度的大小。结果表明:引入速度为18 m/s的旋翼下洗气流使得模型壁面内外两侧均受到冷却气膜的保护,从而使壁面温度降低了36%;同时再引入流量为0.2 kg/s的前端进气,可使红外抑制器模型在3~5μm和8~14μm的红外辐射强度分别降低为原来的11%和28%。     

进气道设计中的几个工程计算问题

本文对进气道设计中二维斜激波计算、圆唇口总压恢复系数估算、亚音速临界流量系数估算及最小喉道面积的确定等几个工程计算方法进行了改进,以适应在计算机上计算.计算精度满足设计参数选择的要求.