Propagation of interplanetary shocks into the Earth’s magnetosphere

This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper.     

侧面安装使用的压力传感器用激波管进行动态特性校准的方法研究

通过理论分析和实验结果指出了用激波管动压校准装置校准压力传感器时被校传感器安装在激波管侧面进行校准存在的问题 ,给出了如何对侧面安装使用的压力传感器用激波管进行动态特性校准的方法。     

独资公司特征分析及有效管理

我国新《公司法》修订后，独资公司的法律地位在立法上得到了认可。作为一种新的公司形态，独资公司对传统的公司法的基本理论构成了直接的挑战。如何在法律上对其进行规制并使之健康发展，成为当前急需探讨的问题。     

Magnetospheric electric field variations caused by storm-time shock fronts

On January 20, 2005 there was an X 7.1 solar flare at 0636 UT with an accompanied halo coronal mass ejection (CME). The resultant interplanetary shock impacted earth ∼36 h later. Near earth, the Advanced Composition Explorer (ACE) spacecraft observed two impulses with a staircase structure in density and pressure. The estimated earth-arrival times of these impulses were 1713 UT and 1845 UT on January 21, 2005. Three MINIature Spectrometer (MINIS) balloons were aloft on January 21st; one in the northern polar stratosphere and two in the southern polar stratosphere. MeV relativistic electron precipitation (REP) observed by all three balloons is coincident (<3 min) with the impulse arrivals and magnetospheric compression observed by both GOES 10 and 12. Balloon electric field data from the southern hemisphere show no signs of the impulse electric field directly reaching the ionosphere. Enhancement of the balloon-observed convection electric field by as much as 40 mV/m in less than 20 min during this time period is consistent with typical substorm growth. Precipitation-induced ionospheric conductivity enhancements are suggested to be (a) the result of both shock arrival and substorm activity and (b) the cause of rapid (<6 min) decreases in the observed electric field (by as much as 40 mV/m). There is poor agreement between peak cross polar cap potential in the northern hemisphere calculated from Super Dual Auroral Radar Network (SuperDARN) echoes and horizontal electric field at the MINIS balloon locations in the southern hemisphere. Possible reasons for this poor agreement include (a) a true lack of north–south conjugacy between measurement sites, (b) an invalid comparison between global (SuperDARN radar) and local (MINIS balloon) measurements and/or (c) radar absorption resulting from precipitation-induced D-region ionosphere density enhancements.     

闭口管内气体非线性振荡研究

采用新型的计算效率较高的ＥＮＯ差分模式,从一维非定常Ｅｕｌｅｒ方程出发,对受扰动气体在闭口管内的传播现象进行了数值模拟。计算发展小扰动情况下,当激振频率接近管内气体的固有频率时会发生非线性振荡,有激波产生;但当扰动较大时,激振频率的影响变得不明显。     

基于MARS的多径干扰抑制方法与实验研究

多径干扰是天线测量中普遍存在的环境干扰,它通常是由待测天线附近的设备对测试信号的反射所引起。针对天线定标中的多径干扰问题,提出采用数字吸波体反射抑制(MARS)技术对天线接收信号进行模式滤波,将信号中的多径干扰分量进行分离并滤除,进而降低测量环境中的多径效应。推导了相关公式,在天线平面近场测量系统中对该技术的效果进行了验证,实验中采用分布于待测天线附近的多个角反射器模拟环境中的反射源。结果表明该方法可以有效降低测量环境中多径效应对测量结果的影响,在待测天线最大辐射方向上的平均增益误差小于0.1dB,提高了天线测量精度。     

带限位台阶的高阻尼橡胶减振器性能试验分析

航天工程中的有害振动可通过高阻尼橡胶减振器进行控制,但核心耗能单元和其他部件之间的连接容易失效。为了改进高阻尼橡胶减振器中阻尼材料和钢板的连接模式,使两者在较大变形下具有较高的机械连接性能,并且避免采用高温高压整体硫化的生产工艺,提出了一种带限位台阶的装配式高阻尼橡胶减振器。该减振器的阻尼材料和钢板之间采用常温胶黏连接模式,且在阻尼材料和钢板的连接边界面上设置了若干个具有一定高度的阶梯状限位台阶。对限位阶梯总高度分别为3 mm、4 mm、5 mm的3种不同装配式高阻尼橡胶减振器进行了不同加载频率和幅值的性能试验。试验结果表明:新型装配式高阻尼橡胶减振器在大变形下具有较强的耗能能力。带限位台阶的减振器和没有限位台阶的减振器相比,最大储能模量提高了22.3%,损耗因子提高了24.9%,且在较大位移幅值工况下,滞回曲线由原本的椭圆形变成类8字型,在保证较高阻尼力的同时使得滞回曲线所包络的面积增大,最大增幅可达588%。该新型减振器无需高温高压整体硫化,可以显著降低生产成本并提高生产效率,具有显著的性能优势和广泛的应用前景。     

Experimental characteristics of oblique shock train upstream propagation

The structure and dynamics of an oblique shock train in a duct model are investigated experimentally in a hypersonic wind tunnel. Measurements of the pressure distribution in front of and across the oblique shock train have been taken and the dynamics of upstream propagation of the oblique shock train have been analyzed from the synchronized schlieren imaging with the dynamic pressure measurements. The formation and propagation of the oblique shock train are ini-tiated by the throttling device at the downstream end of the duct model. Multiple reflected shocks, expansion fans and separated flow bubbles exist in the unthrottled flow, causing three adverse-pressure-gradient phases and three favorable-pressure-gradient phases upstream the oblique shock train. The leading edge of the oblique shock train propagates upstream, and translates to be asym-metric with the increase of backpressure. The upstream propagation rate of the oblique shock train increases rapidly when the leading edge of the oblique shock train encounters the separation bubble near the shock reflection point and the adverse-pressure-gradient phase, while the oblique shock train slow movement when the leading edge of the oblique shock train is in the favorable-pressure-gradient phase for unthrottled flow. The asymmetric flow pattern and oscillatory nature of the oblique shock train are observed throughout the whole upstream propagation process.     

Theoretical investigation of shock stand-off distance for non-equilibrium flows over spheres

We derived a theoretical solution of the shock stand-off distance for a non-equilibrium flow over spheres based on Wen and Hornung’s solution and Olivier’s solution. Compared with previous approaches, the main advantage of the present approach is allowing an analytic solution without involving any semi-empirical parameter for the whole non-equilibrium flow regimes. The effects of some important physical quantities therefore can be fully revealed via the analytic solution. By combining the current solution with Ideal Dissociating Gas (IDG) model, we investigate the effects of free stream kinetic energy and free stream dissociation level (which can be very different between different facilities) on the shock stand-off distance.     

集成BLISCO和iPMA的多学科可靠性设计优化

为解决传统的基于可靠性的多学科设计优化(RBMDO)由于存在优化过程多层嵌套、多学科分析和可靠性分析反复迭代而导致的低效率问题,提出集成两级集成系统协同优化(BLISCO)策略和改进功能测度法(iPMA)的多学科可靠性设计优化方法。首先,基于序列化思想将多学科可靠性设计优化解耦,避免了每次多学科设计优化(MDO)对完整可靠性分析模型的反复调用与迭代。其次,采用高效的更适合复杂工程组织形式的BLISCO策略进行确定性多学科设计优化,摒弃了协同优化的一致性约束和两级集成系统综合法的复杂分析和近似建模问题,提高了计算效率。然后,基于角度更新策略对功能测度法(PMA)进行改进,采用更新角度替代极限状态函数值进行可靠性分析与判别,减少了多学科可靠性分析次数。最后,结合某机型起落架的缓冲器设计实例对所提方法进行验证,结果表明该方法的计算效率较其他方法分别提高了30.93%和19.97%,验证了方法的有效性,且具有工程实用价值。