送粉方式对等离子喷涂NiCrAlY/ Al2 O3涂层介电性能的影响

以内送粉和外送粉两种方式微弧等离子喷涂工艺制备了NiCrAlY/Al_2O_3复合涂层,分析了送粉方式对涂层相组成、微观结构和介电性能的影响。结果表明:与外送粉相比,内送粉方式沉积的涂层具有较高的沉积效率和较低的孔隙率。由于喷涂过程中α-Al_2O_3颗粒完全熔融,内送粉喷涂所得到涂层主要为γ/γ′和γ-Al_2O_3相,并且涂层结构致密,NiCrAlY颗粒分布均匀。介电性能测试表明,以外送粉方式制备的涂层复介电常数实部和虚部几乎不随频率发生变化。而以内送粉方式喷涂的涂层复介电常数实部和虚部随频率的增加而降低,呈现明显的频散现象。     

燃烧室头部激励的等离子体强化燃烧特性实验研究

等离子体助燃是一种新型的强化燃烧技术，近年来受到国内外学者的广泛关注。本文开创性地研制了基于旋转滑动弧等离子体的强化燃烧头部，建立了某型航空发动机三头部燃烧室实验件的等离子体助燃实验平台，验证了该等离子体强化燃烧技术应用于型号发动机燃烧室的可行性。实验研究等离子体助燃在不同余气系数和不同输入电压条件下对平均出口温度、燃烧效率、温度分布系数以及熄火边界的影响。实验结果表明，与正常燃烧相比，施加等离子体助燃后的燃烧效率有明显的提高，在输入电压为U0=240V，余气系数为 α=0.8时，等离子体助燃的燃烧效率提高3.24%。实施等离子体助燃后，燃烧室出口温度分布场分布得到明显的改善，在富油工况α=0.8，出口温度分布系数减少39.8%。等离子体助燃输入电压越高熄火边界扩展程度越明显，相比于正常工况条件下，等离子体助燃U0=240V的熄火边界扩宽了7.34%。     

Ionospheric total electron content response to annular solar eclipse on June 21, 2020

The effects of physical events on the ionosphere structure is an important field of study, especially for navigation and radio communication. The paper presents the spatio-temporal ionospheric TEC response to the recent annular solar eclipse on June 21, 2020, which spans across two continents, Africa and Asia, and 14 countries. This eclipse took place on the same day as the June Solstice. The Global Navigation Satellite System (GNSS) based TEC data of the Global Ionosphere Maps (GIMs), 9 International GNSS Service (IGS) stations and FORMOSAT-7/COSMIC-2 (F7/C2) were utilized to analyze TEC response during the eclipse. The phases of the TEC time series were determined by taking the difference of the observed TEC values on eclipse day from the previous 5-day median TEC values. The results showed clear depletions in the TEC time series on June 21. These decreases were between 1 and 9 TECU (15–60%) depending on the location of IGS stations. The depletions are relatively higher at the stations close to the path of annular eclipse than those farther away. Furthermore, a reduction of about ?10 TECU in the form of an equatorial plasma bubble (EPB) was observed in GIMs at ~20° away from the equator towards northpole, between 08:00–11:00 UT where its maximum phase is located in southeast Japan. Additionally, an overall depletion of ~10% was observed in F7/C2 derived TEC at an altitude of 240 km (hmF2) in all regions affected by the solar eclipse, whereas, significant TEC fluctuations between the altitudes of 100 km ? 140 km were analyzed using the Savitzky-Golay smoothing filter. To prove TEC depletions are not caused by space weather, the variation of the sunspot number (SSN), solar wind (V_SW), disturbance storm-time (Dst), and Kp indices were investigated from 16th to 22nd June. The quiet space weather before and during the solar eclipse proved that the observed depletions in the TEC time series and profiles were caused by the annular solar eclipse.     

Plasma polarization electric field derived from radio sounding of solar wind acceleration region with spacecraft signals

Presented is the analytical approximation of averaged solar wind velocity radial dependence in the solar wind acceleration region at heliolatitudes below 60° under low and moderate solar activity. This empirical approximation is based on the data of radio sounding of the solar corona with radio signals from various spacecraft. Deduced is an equation connecting the solar wind velocity radial dependence and the radial dependence of solar wind plasma polarization electric field intensity. This allows constructing a semi-empirical radial dependence of plasma polarization electric field corresponding to the empirical radial dependence of solar wind velocity. Main properties of the semi-empirical dependence, which is based on radio sounding data, are described.     

Electron density inversed by plasma lines induced by suprathermal electron in the ionospheric modification experiment

Incoherent scatter radar (ISR) is the most powerful ground-based measurement facility to study the ionosphere. The plasma lines are not routinely detected by the incoherent scatter radar due to the low intensity, which falls below the measured spectral noise level of the incoherent scatter radar. The plasma lines are occasionally enhanced by suprathermal electrons through the Landau damping process and detectable to the incoherent scatter radar. In this study, by using the European Incoherent Scatter Association (EISCAT) UHF incoherent scatter radar, the experiment observation presents that the enhanced plasma lines were observed. These plasma lines were considered as manifest of the suprathermal electrons generated by the high-frequency heating wave during the ionospheric modification. The electron density profile is also obtained from the enhanced plasma lines. This study can be a promising technique for obtaining the accurate electron density during ionospheric modification experiment.     

惯性静电约束推力器放电过程数值模拟研究

为了研究惯性静电约束推力器(Inertial Electrostatic Confinement Thruster,IECT)的放电原理和工作机制,采用漂移-扩散流体模拟方法,基于圆柱形惯性静电约束推力器的结构,研究不同栅网线直径、栅网个数、推力器尺寸条件下等离子体放电情况和阴极电压、背景气压对推力器放电的影响。结果表明:在所研究条件下,保证阴极必要的几何透过率的同时,适当增加推力器栅网个数可以提高喷射离子密度,减小羽流发散角;随着阴极电压和背景气压的增大,推力器喷射的等离子体密度增大。但是,压强继续增大会达到临界值,等离子体被约束在推力器内部无法喷出,即喷射模式无法运行,故阴极电压与背景气压对IECT均有较大影响。     

类X-37B升力体再入飞行通信特性中断研究

针对再入非平衡等离子流场的数值仿真方法及等离子体鞘套对不同波段电磁波传输特性的预测开展研究。首先，利用某工程钝头体飞行器再入实测通信飞行测量数据，初步校验数值仿真等离子体特性和通信特性方法的正确性；其次，在典型弹道下针对升力体再入飞行器开展等离子体鞘套数值仿真，分别给出S波段、Ka波段与K波段电磁波衰减特性，研究指出结合当前国内中继星体制情况采用高频段电磁波Ka波段或K波段中继通信方式是解决通信黑障的技术途径之一；最后，研究了电磁波数衰减受传播方向角和攻角的影响规律。研究结果可为发展解决我国再入飞行器通信黑障的设计方案提供参考。     

电弧喷射器流场模拟中电场计算的多重网格法

在建立电弧喷射器内等离子体流场电场计算模型以及基本算法基础上,研究了采用多重网格对收敛速度的改进效果。数值计算证实了此方法的有效性尤其对流场电场耦合计算是有利的。     

小口径电热化学超高速发射实验研究

在小口径发射装置上进行了以液体发射药为化学工质的电热化学发射实验研究,采用不同的装药结构及装药量改进内弹道性能, 可使弹丸获得超高速。对电能释放与化学能释放过程的合理匹配表明, 等离子体能够增强液体药的燃烧并影响压力变化曲线。通过等离子体射流与液体药装填方式的控制, 如采用环状装药结构, 可以增进等离子体与发射药的相互作用, 提高内弹道性能     

太阳纯电子事件和质子-电子事件的电子能谱的机制

本文计算、分析了太阳耀斑加速电子在日冕中传输时激发的等离子体尾场的效应,认为耀斑电子的高能成份激发的尾场,能够加速低能耀斑电子,低能耀斑电子的能量增值可达几十keV至上百keV,这种尾场加速将软化约100keV以下的能量范围内(探测阈之上)的耀斑电子能谱。结合考虑尾场效应,本文提出了太阳耀斑加速电子从加速区到形成电子事件之间的能谱演化模式,说明了太阳纯电子事件的双幂律电子能谱和太阳质子-电子事件的单幂律电子能谱的形成,认为两类事件的电子能谱差异为耀斑电子日冕传输中不同程度的尾场效应所致,前者尾场效应弱,电子能谱呈双幂律,后者尾场效应较强,电子能谱为单幂律谱。