壁压法在低速闭口回流式风洞中的应用

本文介绍了由Hackett提出的一种估算大攻角洞壁干扰修正的壁压信息法。并利用四个几何相似、尺寸不同的平板机翼和翼-身组合体模型在南航NH-2风洞中进行了试验。试验和计算结果表明,该方法使用方便,修正结果准确可靠。但必须指出,对于试验段下游带有平衡缝的闭口回流风洞,洞壁测压数据需经适当的修正才能获得满意的结果。     

高压不稳定环境中的燃料液滴蒸发

对燃料液滴在高压不稳定环境中的蒸发进行了研究，着重讨论了气相介质压力振荡对液滴蒸发特性的影响，计算了Ｃ１２Ｈ２６液滴在Ｎ２介质中蒸发时的蒸发速率、滴温和无因次滴径随时间的变化。结果表明：（１）蒸发速率、滴温发生相同频率的振荡，相位滞后分别为π和π／２；（２）压力振荡使蒸发速率平均值增大，液滴生存时间减少；（３）在不定常加热阶段压力振荡影响很小。     

有质量喷注和边界移动圆柱形流管中的声稳定性

本文利用Ｖａｎ Ｍｏｏｒｈｅｎ提出的平均处理法，从理论上分析了一维流管通道随时间变化和燃烧边界运动对燃烧室线性声稳定性的作用。得出结论是，空腔的瞬态扩大和边界运动平衡掉了一部分声能。     

WALL INTERFERENCE CORRECTIONS FORHIGH-LIFT EXPERIMENT

ＷＡＬＬＩＮＴＥＲＦＥＲＥＮＣＥＣＯＲＲＥＣＴＩＯＮＳＦＯＲＨＩＧＨ－ＬＩＦＴＥＸＰＥＲＩＭＥＮＴＺｈａｎｇＷｅｎｈｕａ（Ｆａｃｕｌｔｙ６０３ｏｆＮａｎｊｉｎｇＵｎｉｖｅｒｓｉｔｙｏｆＡｅｒｏｎａｕｔｉｃｓａｎｄＡｓｔｒｏｎａｕｔｉｃｓ，Ｎａｎｊｉｎ...     

Dissipation of magnetic fields in active galactic nuclei

A model for the emission processes causing rapid variability (less than one day) in active galactic nuclei is developed. Relativistic electron beams escape from reconnection sheets in coronae of accretion disks and excite plasma turbulence with a typical frequency , which depends on the electron number densityn (see also the contribution by R. van Oss). The finite lengths of different beams emerging from different reconnection sheets allows that the waves arecoherently scattered to frequencies ²_pe. For Lorentz factors 10³ and densities typical for disk coronaen10⁶ cm ^–3 (derived from iron line observations) one easily reaches the optical, frequency range. The time scale of the variability is then caused by the relaxation of the electron beams. Likewise, this model explains the very rapid variability in the X-ray (less than 10 minutes) by changing the parameters slightly. According to this scenario the higher the variable frequency is, the closer to the central black hole it should originate.     

Langmuir Turbulence and Solar Radio Bursts

Langmuir waves and turbulence resulting from an electron beam-plasma instability play a fundamental role in the generation of solar radio bursts. We report recent theoretical advances in nonlinear dynamics of Langmuir waves. First, starting from the generalized Zakharov equations, we study the parametric excitation of solar radio bursts at the fundamental plasma frequency driven by a pair of oppositely propagating Langmuir waves with different wave amplitudes. Next, we briefly discuss the emergence of chaos in the Zakharov equations. We point out that chaos can lead to turbulence in the source regions of solar radio emissions. This revised version was published online in August 2006 with corrections to the Cover Date.     

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。     

High-Frequency Radio Signatures of Solar Eruptive Flares

Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures of eruptive solar flares and thus used for the prediction of heliospheric effects. This revised version was published online in August 2006 with corrections to the Cover Date.     

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。