Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

Numerical Simulation of Impact Loading on Solid Propellant Within an Orthotropic Shell

The strain–stress state of the solid propellant rocket engines (SPREs) is simulated under impact. The effect of orientation of elastic and strength properties of orthotropic organoplastic shell material on the strain–stress state of the solid propellant is investigated. Normal and oblique impact of single steel cylinder projectiles, both simultaneous and at different times of multiple, converging steel spheric particles with SPRE are investigated in this study. The investigation is conducted numerically. The numerical modeling was carried out in a three-dimensional formulation by the method of finite elements for the continuous approach of the mechanics of a deformable solid. The destruction of the anisotropic material is described by the tensor-polynomial criterion of the fourth degree, which takes into account the influence of hydrostatic pressure.     

具有衬里的纤维缠绕压力容器分析

给出了具有衬里的纤维缠绕压力容器纤维厚度的设计计算方法。当容器的结构一定时，给出了确定爆破压强的方法。     

声重波激发的赤道Spread—F的拓扑特性研究

本文对声重波激发的Spread-F扰动的非线性制约方程的拓扑特性进行了定性讨论和数值计算．研究了Spread-F的混沌特征及参数范围．结果表明声重波在不同条件时对Spread-F的激发作用有本质的不同．     

太阳风质子束流的演化

太阳神飞船观测表明，太阳风高速流中质子束分量相对于核分量的密度随日心距离增加而增加．提出解释这一观测现象的机理并给出二维数值模拟结果．由于阿尔芬波速随日心距离增加而减少，第二支左旋波将与更多的质子共振，把部分原来属于核分布的质子拉到束分布中来．用数值模拟方程方法求解回旋波共振导致的准线性扩散方程，数值结果与观测结果相符合．     

扩张管和燃料部分填充对PDE效能的影响

采用基于有限速率基元化学反应模型的网格自适应有限体积方法,数值模拟以脉冲爆轰发动机为背景的爆轰波通过扩张喷管的流场,研究了喷管形状及喷管充气状况对脉冲爆轰发动机推进性能的影响。结果表明,氢-氧混合物产生爆轰波的等截面爆轰管冲量在某一比例合适的部分填充时达到最大,而对较大扩张角的喷管来说,其冲量一般随喷管内可燃气体填充比例的增加而增加,比冲通常随可燃气体填充比例的减少而增加;合适的喷管和燃料填充系数能使比冲显著提高。     

边界层流动的非平行稳定性研究

采用极为有效的抛物化稳定性方程（PSE）方法研究边界民支的非平行稳定性。并利用抛物线坐标变换、有限远延拓边界条件、及流向和法向全差分的数值方法，对不同频率的二维Tollmien-Schichting波的非平行稳定尾进行了计算和分析，计算结果与Orr-Sommerfeld方程（OES）的解以及谱配置方法的PSE结果作了详细的比较，得到了满意的结果。     

自吸气脉冲爆震发动机超声速进气道气动性能的数值研究

采用有限体积法计算了某轴对称超声速进气道,在不同幅度和频率的出口扰动压强下的进气道内结尾正激波的运动情况,得出了进气道内结尾正激波运动特性和扰动压强的频率和幅度的关系。在计算中,本文采用了多块结构化网格,控制体积的界面无粘通量采用三阶迎风格式插值获得,同时采用了minmod通量限制器,以确保在激波处的解的物理特性;扩散通量采用二阶中心差分格式插值获得。定常计算采用当地时间步法,非定常计算采用双时间步法。离散的代数方程采用交替方向迭代法求解。     

基元化学反应一维爆轰波的数值模拟

应用基元化学反应模型对一维氢氧混合气体爆轰波进行数值模拟。采用一端高温高压点火起爆的方式,模拟爆轰波的传播。对一维爆轰波的结构、传播特征以及各个化学组分的变化趋势进行了研究。通过将模拟的结果同国内外的研究结果进行对比,发现了一些规律,为多维爆轰波的数值模拟和脉冲爆轰发动机的研究奠定一定的基础。