关于氩等离子体热导率的测量

本文对《空气动力学学报》１９９７年第４期上发表的氩等离子体的热导率的实验研究结果的可靠性做了讨论。提出了一些提高实验数据可靠性的建议。     

He-like Ar xvii triplet observed by RESIK

We present the observations of He-like Ar triplet lines obtained by RESIK spectrometer aboard CORONAS-F. Interpretation of intensity ratios between triplet lines of lower Z elements is known to provide useful diagnostics of plasma conditions within the emitting source. Here, we investigate whether triplet line ratios are useful for interpretation of higher Z element spectra. A high sensitivity, low background and precise absolute calibration of RESIK allow to consider in addition also the continuum contribution. This provides a way to determine the Ar absolute abundance from the observed triplet component ratios. The method is presented and the results are shown for two selected flares. Derived values of Ar absolute abundance for these flares are found to be similar: 2.6 × 10⁻⁶ and 2.9 × 10⁻⁶. They fall in the range between presently accepted Ar photospheric and coronal abundances.     

Propagation of non-linear ion-sound pulses in dusty plasma waveguides

There are a lot of objects in space associated with dusty plasma inclusions. Such inclusions may bear a prolonged shape and behave as waveguides for ion-sound waves. In the case of space plasmas, the dust particles can possess both negative charge, due to electron attachment, and positive one, due to photoionization. In this paper the propagation of linear and non-linear ion-sound wave pulses in the dusty plasma waveguides, possessing positive charge, is studied. It has been demonstrated that non-linear dynamics of baseband pulse propagation in plasma waveguide possesses essentially non-solitonic behavior. Namely, propagation of a long ion-sound pulse leads to an excitation of a shock-like wave but not a stable localized nonlinear pulse. Also, when a Korteveg–de Vries (KdV) soliton is incident onto the dusty plasma waveguide, some part of the soliton energy is captured by the waveguide and transformed into a multi-pulse structure. Additionally, an interaction of dusty plasma inclusions with KdV soliton can lead to the occurrence of transverse instabilities of the soliton and its eventual destruction.     

EXPERIMENTAL STUDY OF FLOW FIELDS IN THE VICINITY OF A FILM COOLING HOLE EXIT

Sofar,filmcoolingisextensivelyadoptedforprotectinghightemperaturepartsingasturbine.Manyresearchworksarefocusedonflow[1~3Jandheattransfer[4'5jinthedownstreamofthecircularhole,buttheflowcharacteristicsattheholeexit,especiallyforflaredholeexit,arenotreportedatpresent.Inordertodesignasuitab1eholeshapeforpracticalcoolingandprovideplentyexperimentaldataforverificationofcomputercodes,adetai1edexperimentalin-vestigationabout3-Dflowfieldsattheexitofasinglecircularandfan-shapedholehasbeencompleted.1Exp…     

有翼高超声速再入飞行器气动设计难点问题

有翼高超声速再入飞行器是近年来的研究热点,气动设计是飞行器设计的关键。为了更清楚地认识有翼高超声速再入飞行器气动设计的难点问题,对有翼高超声速再入飞行器的发展、优势及总体任务剖面进行了介绍,从5个方面详细介绍了该类飞行器气动设计的难点问题,包括多约束复杂面对称气动布局设计、高温真实气体效应对气动特性影响、天地差异与天地换算方法、反作用控制系统(RCS)喷流干扰对气动特性的影响以及气动数据不确定度等,简要阐明了这些难点问题对总体设计的重要性以及初步的解决思路,为有翼高超声速再入飞行器气动设计提供了一些参考。     

PR状态方程在超临界喷射模型中的应用

针对超临界流体物性的特殊性,对超临界喷射数值模拟方法进行研究。基于PR状态方程建立了考虑超临界流体特点的超临界喷射数值模型,并采用该模型对超临界C10H22喷射到超临界N2环境中的喷射进行了数值模拟。对比研究了采用PR状态方程的真实气体模型和理想气体模型得出的密度、温度、质量分数分布以及超临界喷射长度和喷射扩张角的变化规律和差异性,并与试验数据进行了对比。结果表明:2种模型在物性预测上的差异会造成以上喷射特性模拟结果的巨大差异,理想气体模型模拟结果与试验数据误差很大,利用真实气体模型能够得到与试验数据较为吻合的结果。基于PR状态方程的超临界喷射数值模型准确可靠,可为碳氢燃料的超临界喷射现象提供参考。     

热障涂层技术在航空发动机涡轮叶片上的应用

热障涂层是提高航空发动机涡轮叶片工作温度的有效途径之一。根据某型发动机高压涡轮工作叶片、导向器叶片的结构特点和各种涂层制备技术的优缺点,制定了工作叶片和导向叶片表面底层、面层和内腔的涂层制备方案。对工作叶片、导向器叶片材料试样表面涂层的性能开展一系列测试试验。结果表明:涂层性能满足要求,涂层制备方案合理可行;对工作叶片、导向器叶片内表面涂层的厚度,气膜孔径的影响以及质量增加情况进行测量分析,结果均满足设计要求,表明涂层制备工艺合理可行。     

不同类型多级等离子体激励器诱导气流的力学特性研究

等离子体激励器通过产生的等离子加速气流,可以实现对流动的控制。单级等离子体激励器由于受到等离子体放电的物理限制,其控制作用较小;为了提高等离子体流动控制的效果,关于多级等离子体激励器的研究得到发展。采用图像采集和粒子示踪测速系统(PIV),对传统多级等离子体激励器和多级双极性等离子体激励器的放电现象以及气流加速进行研究,并通过流场速度分布计算等离子体激励器对空气产生的推力和吸力。结果表明:随着电压的升高,传统多级等离子体激励器产生的推力和吸力会逐渐减弱;而多级双极性等离子体激励器产生的推力和吸力均呈逐渐增强的趋势。     

Modeling Multifractality of the Solar Wind

The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence. The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios (plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal measure on the weighted baker’s map.     

Shear Flow Instabilities in Low-Beta Space Plasmas

We study instabilities driven by a sheared plasma flow in the low-frequency domain. Two unstable branches are found: the ion-sound mode and the kinetic Alfvén mode. Both instabilities are aperiodic. The ion-sound instability does not depend on the plasma β (gas/magnetic pressure ratio) and has a maximum growth rate of about 0.1 of the velocity gradient dV ₀/dx. On the other hand, the kinetic Alfvén instability is stronger for larger β and dominates the ion-sound instability for β > 0.05. Possible applications for space plasmas are shortly discussed.