余辉等离子体的实验研究

利用调制脉冲产生的余辉等离子体的参数测量表明:等离子体空间电位和电子温度的衰变是重要的,它在余辉等离子体的密度衰变过程研究中必须予以考虑.对容器中余辉等离子体密度径向分布的测量结果与理论预言是一致的.     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

等离子体助燃下超燃支板燃烧室燃烧特性数值研究

为了将支板喷注器与等离子体射流这两种促进超声速燃烧室燃烧的方式结合起来,设计了一种带有等离子体射流喷孔的支板燃烧室,并在超声速来流的条件下,针对燃料喷注总压、燃料喷注位置、等离子体射流介质、等离子体射流总压对燃烧室燃烧性能的影响进行了三维数值模拟。研究发现:增大燃料的喷注总压,燃烧室的燃烧范围明显增大,燃烧效率呈现出先增大后减小的趋势,在燃料喷注总压为2.0MPa时,燃烧效率达到最大值90.4%;不同的燃料喷注位置对燃烧室的燃烧范围影响较小;等离子体射流介质为O2时,燃烧效率最高,燃烧范围最广;提高等离子体射流的喷注总压,能够提升凹腔剪切层高度,有效促进燃烧,但同时也带来了更高的总压损失。     

Spectroscopy peculiarities of thermal plasma of electric arc discharge between electrodes with Zn admixtures

Plasma of the free burning electric arc between Ag–SnO₂–ZnO composite electrodes as well as brass electrodes were investigated. The plasma temperature distributions were obtained by Boltzmann plot method involving Cu I, Ag I or Zn I spectral line emissions. The electron density distributions were obtained from the width and from absolute intensity of spectral lines. The laser absorption spectroscopy was used for measurement of copper atom concentration in plasma. Plasma equilibrium composition was calculated using two independent groups of experimental values (temperature and copper atom concentration, temperature and electron density). It was found that plasma of the free burning electric arc between brass electrodes is in local thermodynamical equilibrium. The experimental verification of the spectroscopic data of Zn I spectral lines was carried out.     

Experimental study on plasma jet deflection and energy extraction with MHD control

This paper presents an integrated research scheme for vector deflection and energy extraction in a gas plasma jet under Magneto-Hydrodynamic (MHD) control. A MHD-controlled thrust-vector test rig was used to conduct the experimental research. A gas plasma was obtained by injecting ionization seeds of Cs₂CO₃ into the combustion chamber via artificially forced ionization. The effects of the gas temperature and ionization seed mass fraction on the plasma jet deflection and energy extraction were experimentally verified under an applied magnetic field. The experimental results were analyzed theoretically. The results showed that the deflection amplitude of the gas plasma jet and the extracted voltage signal intensity increased with increasing gas temperature and the ionization seed mass fraction. The extracted dynamic voltage signals proved that the ionization seeds of Cs₂CO₃ induced gas ionization at 1173 K. The experiment verified that it is feasible to simultaneously achieve jet deflection and extract energy under the action of an external magnetic field.     

等离子鞘套热力学波动对电磁波传播的影响

针对等离子鞘套热力学波动造成电磁波传播特性变化的问题，结合湍流理论、等离子理论和电磁波传播理论，得到了热力学参数波动与介电常数间的关系。计算了不同状态下热力学参数波动引起S和Ka波段电磁波透射和反射系数的变化。结果表明，当电子密度增大，S波段反射系数变化减小、透射系数变化增大；当Ka波段在碰撞频率10MHz时，反射系数变化增大、透射系数变化减小，在碰撞频率1GHz和50GHz时透射系数变化反射系数变化先增后减。不同高度下波动的影响也不同，S波段透射和反射系数变化随高度升高先减后增；Ka波段透射系数变化先减后增、反射系数变化先减后增而后再次减小。因此，应根据实际环境状态获得波动的包络范围，进而针对性开展测控通信系统设计。     

预燃式等离子体射流点火器工作特性实验研究

为解决发动机点火包线小于飞行包线的实际问题,提供等离子体点火技术在航空发动机中的工程应用新思路,论文设计了一种预燃式等离子体射流点火器,实验研究了放电特性和射流特性。结果表明,预燃式等离子体射流点火器与空气等离子体射流点火器相比,在提升射流能量降低电源功率方面有着较大的优势,电流相同时通入甲烷在较大流量时可减小驱动电源功率,总流量为44L/min时,减幅可达14.99%;同时预燃式等离子体射流较空气等离子体射流稳定,且射流长度增加,扩大了点火面积,有利于点火。     

纳秒脉冲表面介质阻挡放电激励改善飞翼力矩特性的实验研究

针对飞翼布局力矩控制问题,采用纳秒脉冲表面介质阻挡放电（NS-DBD）激励,在来流风速30 m/s时,开展飞翼等离子体流动控制风洞试验,研究了不同激励参数和位置对飞翼升阻特性和力矩特性的影响。结果表明,NS-DBD激励能够有效改善飞翼大迎角气动特性。激励频率对飞翼升阻特性影响较大,激励频率为0.2 kHz时,增升效果最好,最大升力系数提高14.5%,失速迎角推迟5°。随着激励频率的增加,增升效果逐渐变差,减阻效果变好。单侧施加激励时,能够实现大迎角下飞翼模型的力矩控制,随着激励频率的增加,滚转力矩的控制效果减小,激励频率为0.2kHz时,平均滚转力矩系数变化为ΔMX=0.005691;偏航力矩的控制效果增大,激励频率为1kHz时,平均偏航力矩系数变化为ΔMY=-0.001571;俯仰力矩的控制效果减小,激励频率为0.2kHz时,平均俯仰力矩系数变化为ΔMZ=-0.002576。在中翼段和内翼段施加激励,破坏了飞翼的俯仰力矩特性,在外翼段和机翼右侧施加激励,能够显著改善飞翼的俯仰力矩特性。流场测量结果表明：等离子体激励对飞翼气动力矩的控制,主要是通过控制流动分离和控制横向流动来实现的。NS-DBD激励为改善飞翼布局稳定性和操纵性提供一种潜在的技术手段。     

射频介质阻挡放电改善NACA 0015翼型气动性能的实验

介质阻挡放电(DBD)均匀稳定、易于敷设,是机翼/翼型等离子体流动控制(PFC)中最常用的激励方式。射频介质阻挡放电激励频率高、放电功率大,且能在流场中产生明显的加热,应用潜力大。采用射频电源驱动DBD激励器产生等离子体,分析放电的体积力、热特性和诱导流场特性,开展了射频介质阻挡放电改善NACA 0015翼型气动性能的实验,研究了占空比、调制频率、载波频率和电源功率等参数对流动控制效果的影响规律。结果表明:射频等离子体激励的体积力效应随激励电压的增大而增加;射频等离子体激励产生的热量在诱导的流场中进行传导,加速流场;当来流速度为20m/s,Re=3.36×10~5时,在翼型前缘施加激励,使翼型临界失速迎角推迟1°,最大升力系数增大6.43%,且在过失速迎角下仍具有流动控制效果,使升力下降变缓;调制频率越大,控制效果越好;存在最佳占空比、载波频率和功率,占空比对流场控制效果的影响最显著,最佳占空比、载波频率和功率分别为20%,460kHz和50W。射频等离子体激励以体积力效应、热效应和诱导壁面射流改善失速流场,使得NACA0015翼型气动性能极大改善,流动分离得到有效控制。     

Modeling of ionospheric scintillation at low-latitude

The presence and movement of plasma density fluctuations in the F-region of the ionosphere are studied by monitoring phase and amplitude of radio waves propagating through the region. In this paper, we have used weak scattering theory and assumed the plasma density fluctuations to behave like phase changing diffraction screen. Appropriate relations for scintillation index S₄, and phase variance δ? are derived and computed for different parameters of the plasma density irregularities of the ionosphere. SROSS-C2 satellite in situ measurements of plasma density fluctuations, which provide direct information about the structure and morphology of irregularities that are responsible for scintillation of radio waves, were used first time to develop a scintillation model for low latitude. It is observed that the scintillation index S₄ and phase variance δ? depends on the strength of the plasma turbulence. Finally, the results obtained from modeling are compared and discussed with the available recent results.