进气温度畸变对某发动机稳定性影响的研究

本文采用有效的畸变传递模型，就进气温度畸变对某发动机稳定性和性能的影响进行了较深入的数值研究．详细地分析了温度畸变对发动机稳定性和性能的影响，探讨了温度畸变在发动机系统中的传递和分布情况。结果表明：对于发动机进口空间温度畸变，发动机稳定裕度损失更多地取决于畸变强度而非周向范围：向对于与时间相关的温度畸变，发动机进口温升率比周向范围的影响更为显著。     

WALL INTERFERENCE CORRECTIONS FORHIGH-LIFT EXPERIMENT

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湍流型动态畸变下涡喷发动机稳定性分析

对湍流型动态畸变进气流场进行了分析和描述，给出了随机涡在压气机进口所产生的总压脉动的通用分布曲线，并统计地分析和预测了该总压脉动引起的最可能最大失速裕度损失。数值分析表明在考虑压气机对非定常流响应方面，最为关心的压气机最大失速裕度损失值是脉动压力的均方根值、功率谱密度、压气机进口转子弦长和转速的函数。     

What do Cosmogenic Isotopes Tell us About Past Solar Forcing of Climate?

In paleoclimate studies, cosmogenic isotopes are frequently used as proxy indicators of past variations in solar irradiance on centennial and millennial timescales. These isotopes are spallation products of galactic cosmic rays (GCRs) impacting Earth's atmosphere, which are deposited and stored in terrestrial reservoirs such as ice sheets, ocean sediments and tree trunks. On timescales shorter than the variations in the geomagnetic field, they are modulated by the heliosphere and thus they are, strictly speaking, an index of heliospheric variability rather than one of solar variability. Strong evidence of climate variations associated with the production (as opposed to the deposition) of these isotopes is emerging. This raises a vital question: do cosmic rays have a direct influence on climate or are they a good proxy indicator for another factor that does (such as the total or spectral solar irradiance)? The former possibility raises further questions about the possible growth of air ions generated by cosmic rays into cloud condensation nuclei and/or the modulation of the global thunderstorm electric circuit. The latter possibility requires new understanding about the required relationship between the heliospheric magnetic fields that scatter cosmic rays and the photospheric magnetic fields which modulate solar irradiance.     

进气压力畸变对某三级风扇流场的影响

介绍了在某三级风扇上进行的固定式插板畸变试验，并详细分析了进气压力畸变对进、出口稳态压力和温度的影响。同时，采用频域和幅值域分析方法对脉动压力进行了分析，给出了脉动压力功率谱密度、幅值概率密度和自相关、互相关分析。     

氢燃料双模态冲压模型发动机M6的试验研究

笔者研究了一个有突扩台阶的氢燃料高超声速冲压发动机模型的气体动力学特性和推力特性。氢气从位于燃烧室突扩台阶后的支板逆来流喷注,测量了氢气燃烧状态下模型发动机壁面的压力分布和推力收益数据。实验结果表明,在氢气的当量油气比为0.35～0.8的范围,在本模型流道构型条件下,氢气自燃,并随当量油气比的增加,燃烧室内压力增加,获得的推力收益增大,最大推力收益达到500N。实验在CARDC的脉冲燃烧风洞中进行,实验马赫数为6,总温1850K,总压5.5MPa。     

炮风洞中进行高温喷流底部热流、压力测量试验

本文介绍了在北京空气动力研究所炮风洞 M 数为6、7、8的气流中进行具有高温喷流的模型底部热流和压力测量试验的有关试验技术。试验结果表明底部对流热流和压力测量值随外流 M 数增大而减小,他们都大于无外流时的测值。辐射热流不受外流影响。     

确定风洞模型压力中心的变距测力试验

本文提出了采用变换模型相对天平校准中心位置来测得同一状态下的不同俯仰力矩值,再通过数学处理或作图获得小攻角下的精确压力中心位置的试验方法。某型号用本方法试验得到了令人满意的结果。     

超声速流中激波/湍流附面层干扰数值模拟

采用修正的B／L湍流模型以及多块结构化网格求解了二维N-S方程。分别对超声速流和高超声速流中的激波／湍流附面层干扰进行了数值研究。本文首先研究了进口马赫数为2．96的超声速流。计算结果准确预测了入射斜激波在平直壁面引起湍流附面层分离的流动特征：分离点的反射激波、分离包引起的膨胀扇以及再附点的反射激波。计算的壁面压力分布与实验值吻合较好，计算的分离区长度与实验值比较有一定误差。本文还对进口马赫数为9．22的高超声速流中压缩角引起的激波／湍流附面层干扰进行了数值研究。计算结果与实验结果吻合较好。     

The characteristics of sharp (small-scale) boundaries of solar wind plasma and magnetic field structures

We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed.