MHD waves in coronal flux tubes

The basic MHD waves of a coronal flux loop are investigated for the rectangular box model of a plasma with oblique magnetic field and line-tied at the ends. The waves found are completely different from those in a periodic box, representative for tokamaks. They consist of a mixture of Alfvén components with a ballooning factor, favouring minimal field line bending, and fast components without such a factor. Pure Alfvén modes are only found as singular limiting cases of cluster spectra of Alfvén-fast waves, where the fast components are localised in a photospheric boundary layer which is dictated by the requirements of line-tying. This justifies the assumption of continuous spectra in coronal loops, required for the mechanism of resonant Alfvén wave heating. The waves consist of large amplitude Alfvén components in the corona and fast components with a small but rapidly varying amplitude in the boundary layer, so that they appear to have the right signature for effective transfer of energy from the photosphere to the corona.     

高速转动壳体行波振动实验研究

本文对轴对称薄壁壳结构的振动特性进行了试验研究。对一圆柱薄壳在静止状态和高速旋转状态下进行了模态试验。试验结果验证了轴对称薄壁壳在转动状态下,由于科氏力的影响,同一模态在转动坐标系中,存在不同频率的前后行波。为理论计算和发生在航空发动机中转动薄壁件振动设计,提供了可靠的试验依据。     

飞船返回舱俯仰振荡的动态稳定性研究

本文研究了以平衡攻角为中心作单自由度俯仰振荡的飞船返回舱 ,其动态稳定形态随来流M∞ 的变化。设θ(t)是由平衡攻角起算的俯仰振荡角 ,Cm 是作用在飞船返回舱上的气动俯仰力矩系数 ,Cμ(θ, θ)· θ是机械阻尼力矩 (自由飞行时为零 ,实验时要计入其影响 ) ,文中给出飞船返回舱在平衡攻角处的俯仰振荡动态稳定性判据 ,并证明λ =λ(M∞) = Cm θ0+Cμ(0 ,0 ) 1 - Cm ¨θ0 是决定动稳定形态的重要参数。如果随M∞ 的变化 ,λ(M∞)由λ<0经过λ =0变化到λ>0 ,则飞船返回舱将由稳定的点吸引子形态 (即稳定在平衡攻角状态 )演化为周期吸引子形态 (即作周期振荡 )。对应于λ(M∞) =0的马赫数就是飞船返回舱的俯仰运动出现Hopf分叉的临界马赫数Mcr 。本文首先分析了飞船返回舱所受动态气动俯仰力矩的依赖状态变量 ,然后应用非线性动力学理论对飞船返回舱的俯仰运动进行了定性理论分析 ;最后耦合求解俯仰振荡方程和非定常Navier Stokes方程 ,数值模拟了飞船返回舱俯仰振荡随来流马赫数变化的Hopf分叉过程 ,验证了分析结论     

一种改进的MUSCL格式

给出了一种改进的二阶精度的ＭＵＳＣＬ格式，并用来求解Ｅｕｌｅｒ方程，改进后的ＭＵＳＣＬ格式在线化插值步中，用Ｖａｎ Ｌｅｅｒ的插值斜率对特片变量进行插值，并对与熵波、剪切波对应的特片变量使用了小耗散的插值斜率，在迎风步采用Ｒｏｅ的近似黎曼解求得迎风通量。比较一维和二维的计算结果均可以看出，改进后的ＭＵＳＣＬ格式在消除数值振荡的同时，明显提高了流场间断的分辨率。     

钛合金导管内径滚压连接数值模拟与试验研究

利用有限元方法,对钛合金导管内径滚压连接成形进行数值模拟,通过对导管、管套卸载前后的回弹分析,以及材料流动规律分析,掌握内径滚压连接成形机理;通过试验研究,获得导管材料和管套结构对滚压连接成形的影响规律;并通过耐压试验对不同材料导管连接件的密封性能进行了验证.     

环形射流喷口位置对激波聚焦起爆的影响分析

为了研究环形射流喷口位置对激波聚焦起爆爆震的影响,以氢气和空气混合物为例,对不同环形射流喷口位置条件下的激波聚焦起爆过程进行了数值模拟。结果表明,随着喷口距凹壁面距离L增大,直接聚焦起爆和凹壁面反射起爆所需的临界入射压力逐渐增大,相应的聚焦时刻会滞后,形成焦点的位置距凹壁面越远。     

高超声速风洞多体干扰与分离试验技术

在FL-31风洞中进行了某高超声速飞行器的多体干扰与分离试验技术研究,成功建立了多体干扰与分离试验技术。试验模型是某典型构型的可重复使用航天飞行器,由助推器以及再入体两部分组成。利用风洞上下投放机构实现两模型间的相对运动,采用两台天平对模型的气动力进行测量,同时利用纹影仪记录模型分离过程中的激波干扰情况。结果表明：试验系统设计合理,能准确模拟物体间分离过程,并能精确测量多体干扰的气动力特性,激波干扰清晰可见。     

行星际空间质子引起介质深层充电的GEANT4模拟研究

高通量的空间质子是导致行星际航天器深层充电的主要原因,基于辐射诱导电导率模 型（RIC）和粒子输运模拟工具GEANT4对介质材料在质子辐照条件下的深层充电问题进行了 预估。利用GEANT4-RIC充电计算方法,首先计算出10MeV质子在Kapton和Teflon中的注量和 剂量沉积曲线,进而根据电流连续性方程、泊松方程和电荷俘获方程组成的辐射诱导电导率 模型（RIC）求解出介质内电荷和电场分布,与介质击穿电场阈值对比作为其是否发生放电 的依据。模拟结果证实了对10MeV质子,在质子注量为3×10 12 ／cm 2时Kapton会发 生放电,而Teflon则不会发生放电的一般性试验结论。验证了GEANT4-RIC方法用于行星际航 天器介质材料质子充放电评价的可行性,为此类问题的解决奠定了基础。
     

Hydrodynamic instabilities and transverse waves in propagation mechanism of gaseous detonations

The present study examines the role of transverse waves and hydrodynamic instabilities mainly, Richtmyer–Meshkov instability (RMI) and Kelvin–Helmholtz instability (KHI) in detonation structure using two-dimensional high-resolution numerical simulations of Euler equations. To compare the numerical results with those of experiments, Navier–Stokes simulations are also performed by utilizing the effect of diffusion in highly irregular detonations. Results for both moderate and low activation energy mixtures reveal that upon collision of two triple points a pair of forward and backward facing jets is formed. As the jets spread, they undergo Richtmyer–Meshkov instability. The drastic growth of the forward jet found to have profound role in re-acceleration of the detonation wave at the end of a detonation cell cycle. For irregular detonations, the transverse waves found to have substantial role in propagation mechanism of such detonations. In regular detonations, the lead shock ignites all the gases passing through it, hence, the transverse waves and hydrodynamic instabilities do not play crucial role in propagation mechanism of such regular detonations. In comparison with previous numerical simulations present simulation using single-step kinetics shows a distinct keystone-shaped region at the end of the detonation cell.     

Longitudinal distribution of thermospheric densities and ionization rates in the upper atmosphere of Mars at mid-latitude using MGS ACC data

The Accelerometer Experiment (ACC) onboard Mars Global Surveyor (MGS) measured 1600 density profiles in the upper atmosphere of Mars during aerobraking. These measurements reveal large-scale and small-scale structure in the thermosphere of Mars. Here, the measurements of mass density for 115 orbits (#P0670–P0789) from November 1 to 30, 1998, under spring equinox and medium solar activity conditions (average F_10.7 ∼ 137) during phase 2 of the aerobraking in the thermosphere of Mars at different altitudes and longitudes are presented for northern mid-latitude (17–42°N) in the dayside atmosphere using ACC onboard MGS. From these mass densities, the neutral densities of different gases are derived from their mixing ratios. Using these neutral densities, the longitudinal distribution of photoionization rates and photoelectron impact ionization rates are calculated at wavelength range 1–102.57 nm due to EUV and soft X-ray radiation under photochemical controlled region using Analytical Yield Spectrum approach (AYS). These conditions are appropriate for MGS Phase 2 aerobraking period from which the accelerometer data is used. Under the photochemical equilibrium condition, the electron density near the peak varies as the square root of the total peak ionization rate. Using this fact, an attempt is being made to estimate the mean primary and secondary peak electron density by averaging the longitudinal variations of total peak ionization rates in the northern mid-latitude (17–42°N) ionosphere of Mars, as there is no radio science measurement at this latitude region by MGS.