Ion-acoustic waves in unmagnetized collisionless weakly relativistic plasma of warm-ion and isothermal-electron using time-fractional KdV equation

Collisionless unmagnetized plasma consisting of a mixture of warm ion-fluid and isothermal-electron is considered, assuming that the ion flow velocity has a weak relativistic effect. The reductive perturbation method has been employed to derive the Korteweg–de Vries (KdV) equation for small – but finite-amplitude electrostatic ion-acoustic waves in this plasma. The semi-inverse method and Agrawal’s method lead to the Euler–Lagrange equation that leads to the time fractional KdV equation. The variational-iteration method given by He is used to solve the derived time fractional KdV equation. The calculations show that the fractional order may play the same rule of higher order dissipation in KdV equation to modulate the soliton wave amplitude in the plasma system. The results of the present investigation may be applicable to some plasma environments, such as space-plasmas, laser-plasma interaction, plasma sheet boundary layer of the earth’s magnetosphere, solar atmosphere and interplanetary space.     

刚弹耦合动力学初值问题拟变分原理及其应用

刚弹耦合动力学在国防和民用经济建设中有着广阔的应用前景,但目前还没有完全成熟的理论研究成果。鉴于此,针对刚弹耦合特性,建立初值问题拟变分原理;应用变分方法,推导拟变分原理的拟驻值条件,即得到刚弹耦合动力学的控制方程;给出刚弹耦合动力学初值问题拟变分原理应用的2个算例,1个是应用控制方程求得自由梁的奇数阶振型的解析解,1个是应用变分直接方法 Ritz方法求得自由梁的偶数阶振型的解析解。研究表明,刚弹耦合动力学初值问题拟变分原理为建立有限元计算模型提供了依据。     

高动态环境下舰载子惯导系统分段对准方法

本文在分析惯导系统现有对准方法的基础上,对于拥有高度动态性能的广泛一类的受控运动体提出了一种顺序对准方法和算法,分析了所提出方法可达到的精度和为达到所指出精度所需要的时间。     

Wolf–Rayet optically thick winds with Alfvén waves

The Wolf–Rayet (WR) stars are hot luminous objects which are suffering an extreme mass loss via a continuous stellar wind. The high values of mass loss rates and high terminal velocities of the WR stellar winds constitute a challenge to the theories of radiation driven winds. Several authors incorporated magnetic forces to the line driven mechanism in order to explain these characteristics of the wind. Observations indicate that the WR stellar winds may reach, at the photosphere, velocities of the order of the terminal values, which means that an important part of the wind acceleration occurs at the optically thick region. The aim of this study is to analyze a model in which the wind in a WR star begins to be accelerated in the optically thick part of the wind. We used as initial conditions stellar parameters taken from the literature and solved the energy, mass and momentum equations. We demonstrate that the acceleration only by radiative forces is prevented by the general behavior of the opacities. Combining radiative forces plus a flux of Alfvén waves, we found in the simulations a fast drop in the wind density profile which strongly reduces the extension of the optically thick region and the wind becomes optically thin too close its base. The understanding how the WR wind initiate is still an open issue.     

初始扰动对于气液界面Rayleigh-Taylor不稳定性发展的影响

利用果冻实验技术研究几种不同初始扰动的气液界面Rayleigh-Taylor不稳定性发展过程。通过对不同波长和振幅的实验结果进行对比发现：波长是影响界面扰动发展的主要因素,并且在不同阶段影响的模式不同。在线性阶段,波长较短的扰动发展较快;在非线性阶段,则是波长较长的扰动发展较快。     

提高固定几何二元进气道低马赫数性能的仿真研究

分别以常规低、高马赫数来流设计的固定几何二元混压式进气道为例,采用数值模拟手段,探究了一种改进的外压缩波系配置方案。采用来流马赫数由低到高,外压缩激波依次封口的设计方法,提高了固定几何二元进气道的低马赫数性能。相比常规配波设计的进气道,来流马赫数2.15条件下的流量系数提高了0.07;来流马赫数2.15和2.4条件下,总压恢复提高近0.015。初步研究证明这种设计理念是合理的,该设计方案有待于进一步发展和实验验证。     

超声电喷推进机理研究

超声电喷推进是一种新型的电推进技术,主要用于解决胶体推力器等电推力器发射点集成困难、发射点数密度低的问题。通过将超声振动产生的大量微细驻波作为发射源,超声电喷推进将从根本上提高发射点的数目和密度,形成较大的推力密度。文章对超声电喷推进的发射机理进行了研究,得到相应的理论发射模型。通过对发射表面上微细驻波的形成过程、带电液滴的分离过程进行理论分析,建立了静电场条件下微细驻波波峰临界状态的平衡方程,推导出微细驻波波峰局部半径以及发射液滴尺寸的理论解,并提出了发射电流、比冲和推力的估算方程。在此基础上,分析了极间电场强度、超声振动频率、超声振动功率、推进剂性能黏度、推进剂表面张力系数和电导率对超声电喷推进性能的影响规律,并进行了试验验证。     

机翼用铝合金材料原始疲劳质量对比

当前航空工业的发展对于超高强铝合金材料的需求十分迫切,实现该材料的国产化并达到良好的质量效果至关重要。为了对中国航空工业中常用的7XXX新型铝合金材料的原始疲劳质量（IFQ）进行评估,选取裂纹萌生时间（TTCI）和当量初始缺陷尺寸（EIFS）作为对比参量,分别对中国飞机机翼用7XXX紧固孔试件和俄系BXXX紧固孔试件开展了低、中、高3种应力水平下的疲劳试验,通过对比分析得到了两种试件在不同应力水平下的TTCI趋于一致,最大仅相差3.71%;得到了每个试件的EIFS,应用疲劳统计学方法验证了两种试件材料各自的EIFS值无显著性差异;提出了一种不同超越概率下的结构细节当量初始缺陷模型,直接有效地对飞机结构细节的质量风险进行了评估;建立并对比分析了两种试件结构细节的通用EIFS分布,结果均小于中国军用手册规定的0.125 mm,且在超越概率为5%时,7XXX材料的通用EIFS值要小于BXXX材料的通用EIFS值。     

非均匀来流下等压力梯度曲面压缩系统的试验研究

根据激波和膨胀波理论,设计了Ma=5.3等压力梯度曲面压缩系统。在Ma=3.85和Ma=5.3的小高超风洞完成均匀来流试验,并利用风洞壁面自然发展的附面层进行非均匀来流等压力梯度曲面压缩系统性能试验。试验发现:均匀来流下,试验模型壁面压力均按照等压力梯度规律分布,但来流马赫数Ma=5.3时出口流场均匀性较差;非均匀来流下,大量的附面层吸入不仅影响壁面压力不再呈等压力梯度分布,而且对出口流场均匀性影响也极大。      

A stationary bow shock model for plasmas: The spherical blunt obstacle problem

We present an analytic model of a stationary bow shock which describes the interaction between a supermagnetosonic ambient wind and an obstacle with spherical-like frontal shape. We develop expressions for the bow shock’s geometry and the physical properties of the plasma sheath as functions of the upstream conditions. The solution is limited to magnetic fields parallel to the upstream velocity. The model allows to use any value of the upstream alfvenic and sonic Mach numbers and the polytropic index (γ$\gamma$), pointing out the influence of γ$\gamma$ for the magnetosheath compression and the bow shock shape. When both Mach numbers are small, the upstream magnetic field intensity affects also the bow shock shape. We compare our results with other models finding important consistencies. We also compare our results with in-situ data, we fund a reasonable qualitative agreement; however, it seems that our model underestimates the magnetosheath size.