长寿命机械连接技术研究应用进展

长寿命机械连接技术是武器装备发展中至关重要的技术之一,是一个国家军事技术能力和科技水平的重要组成部分.综合论述了孔挤压强化技术、干涉连接技术、防腐蚀和抗氧化技术等为代表的先进长寿命机械连接技术的研究和应用现状,对我国开展长寿命机械连接技术的研究具有重要指导意义.     

Location of layered structures in the ionosphere and atmosphere by use of GPS occultation data

A method is introduced to locate the layered structures in the atmosphere and ionosphere based on simultaneous observations of radio wave intensity and phase variations in trans-ionospheric satellite-to-satellite links. The method determines location of a tangent point on the trans-ionospheric ray trajectory where gradient of refractivity is perpendicular to the ray trajectory and influence of a layered structure on radio wave parameters is maximal. An estimate of the location of a layer can be obtained from a combination of the phase and intensity variations. This new technique was applied to measurements provided during FORMOSAT-3 and CHAMP radio occultation (RO) missions. For the considered RO events the location of the inclined plasma layer in the lower ionosphere is found and the electron density distribution is retrieved. The method is checked by measuring the location of the tangent point on the ray trajectory in the neutral gas in the atmosphere. The results showed a fairly good agreement.     

Standing Alfvén waves with m ≫ 1 in a dipole magnetosphere with moving plasma and aurorae

The structure of standing Alfvén waves with large azimuthal wave numbers (m ? 1) is studied in a dipole model of the magnetosphere with rotating plasma. In the direction across magnetic shells the structure of such waves is determined by their dispersion associated with curvature of geomagnetic field lines and corresponds to the travelling wave localized between toroidal and poloidal resonant surfaces. In projection into the ionosphere (along geomagnetic field lines) this structure is similar to the structure of a discrete auroral arc. The azimuthal structure of an auroral arc is similar to azimuthal structure of Alfvén waves with m ∼ 100. Possible interaction mechanisms between the Alfvén waves and energetic electron fluxes forming auroral arcs are discussed.     

Theoretical properties of offset bipolar electric field solitary structures in space plasmas

The bipolar electric field solitary (EFS) structures have been frequently observed in the near Earth plasma regions, such as auroral zone, magnetopause, cusp regions, and magneto-tail. Sometimes these structures are observed as offset bipolar structures. In this paper, the properties of the offset bipolar EFS structures parallel to the magnetic field are studied with an ion fluid model in a cylindrical symmetry by considering electrostatic condition. The model results show that the offset bipolar EFS structures can develop from both ion-acoustic waves and ion cyclotron waves, and propagate along the magnetic field line in the space plasmas if plasma satisfies some conditions. The offset bipolar EFS structures can have both polarities. It will be first negative pulse and then positive pulse if the initial electric field E₀ < 0 or reverse in order if E₀ > 0. The amplitude of the offset bipolar EFS structures first decreases and then increases with the wave propagation velocity. Some results from our model are consistent with the observations.     

Response of the mid-latitude D-region ionosphere to the total solar eclipse of 22 July 2009 studied using VLF signals in South Korean peninsula

In this paper, we analyze VLF signals received at Busan to study the the D-region changes linked with the solar eclipse event of 22 July 2009 for very short (∼390 km) transmitter–receiver great circle path (TRGCP) during local noon time 00:36–03:13 UT (09:36–12:13 KST). The eclipse crossed south of Busan with a maximum obscuration of ∼84%. Observations clearly show a reduction of ∼6.2 dB in the VLF signal strength at the time of maximum solar obscuration (84% at 01:53 UT) as compared to those observed on the control days. Estimated values of change in Wait ionospheric parameters: reflection height (h′) in km and inverse scale height parameter (β) in km⁻¹ from Long Wave Propagation Capability (LWPC) model during the maximum eclipse phase as compared to unperturbed ionosphere are 7 km and 0.055 km⁻¹, respectively. Moreover, the D-region electron density estimated from model computation shows 95% depletion in electron density at the height of ∼71 km. The reflection height is found to increase by ∼7 km in the D-region during the eclipse as compared to those on the control days, implying a depletion in the Lyman-α flux by a factor of ∼7. The present observations are discussed in the light of current understanding on the solar eclipse induced D-region dynamics.     

固体火箭点火超压形成机理与影响因子研究

为研究固体火箭点火超压的形成机理和影响因子,以Ariane 5火箭固体助推器1/35缩比模型为研究对象,〖JP+1〗基于可压缩气体三维Navier-Stokes方程建立固体火箭尾焰流场的数学模型。同时,使用有限速率/涡耗散模型表征尾焰复燃反应,采用有限体积法求解火箭尾焰流场控制方程,得到箭体尾部近场的点火超压幅值与分布情况。与试验数据比较,数值结果较好的反映了点火超压的过程特性。进而,采用该数学模型和求解方法,研究了点火超压的影响因子。计算结果表明,尾焰复燃反应对点火超压的影响较小,与无复燃反应的计算结果比较,点火超压的峰值相对变化幅度不大于1.85%,点火超压的波形与分布特性的变化可以忽略;建压速率越快,点火超压峰值越大,且呈非线性比例关系增长;喷管膨胀比主要影响点火超压的波形,对其峰值影响较小。     

含涂层空心球复合泡沫塑料的黏弹性热应力分析

针对含涂层空心微球的复合泡沫塑料,利用三参数标准线性固体模型和黏-弹性对应原理得到了材料由于温度改变而产生的残余热应力,研究了涂层厚度、体分比和时间等因素对残余热应力的影响。结果表明:随着时间的增加,由温度改变而引起的材料内部的残余热应力将逐渐减小,且涂层厚度和涂层空心微球体分比的减小会使残余热应力增加。此外,沿半径方向热应力在微球内逐渐增加,在涂层和基体中则逐渐减小,在涂层与空心微球的交界处达到最大值。     

液晶显示方法研究管内马赫数4拟似冲击波流动

在一个压力-真空型超声速风洞中, 剪切应力敏感的液晶表面流动显示技术被用来研究方管内马赫数4拟似冲击波的超声速流动.实验是在日本室兰工业大学的超声速风洞中进行.它提供了关于测试表面流动结构的定性信息,诸如湍流边界层分离和再附, 以及边界层流动的维数等.液晶显示结果与纹影实验照片和油膜方法进行比较,证实了它是一种非常有效的表面流动显示工具.     

The Nonlinear Model of the Response of Airglow to Gravity Waves

In this paper, we develope a time-dependent, nonlinear, photochemical-dynamical 2-D model which is composed of 3 models: dynamical gravity wave model, middle atmospheric photochemical model, and airglow layer photochemical model. We use the model to study the effect of the gravity wave propagation on the airglow layer. The comparison between the effects of the different wavelength gravity wave on the airglow emission distributions is made. When the vertical wavelength of the gravity wave is close to or is shorter than the thickness of the airglow layer, the gravity wave can make complex structure of the airglow layer, such as the double and multi-peak structures of the airglow layers. However, the gravity wave that has long vertical wavelength can make large scale perturbation of the airglow emission distribution.     

应力波在变截面杆中传播的数值分析

 利用ＨＯＮＤＯ有限元程序对应力波在变截面杆中的传播进行了分析。根据分析结果提出采用有台阶的锥形调制器取代现有调制器可以解决手提式铆枪过重的问题。有台阶的调制器对应力透射波的放大效果不会有明显变化,但可减轻重量５０％以上。同时利用该程序对应力波在不同几何构形的调制器中的传播进行了对比分析,根据输出波形的质量对应力波调制器的几何尺寸进行了优化设计,提出了锥体的底角和直径范围。