A Prediction Method for△f0F2min of a Single Station From Interplanetary Parameters Based on Statistical Study

Using 86 CME-interplanetary shock events,the correlation between the peak values of （a） the solar wind parameters(B_z,E_y,P_dyn) and the geomagnetic indices（SYM-H,ASY-H,Kp）, （b） the coupling functions（Borovsky,Akasofu,Newell） and the geomagnetic indices,（c） the solar wind parameters/coupling functions/geomagnetic indices and the ionospheric parameter(Δf₀F_2min), are investigated.The statistical results show that in group（a）,B_{z min} and SYM-H_min have the best correlation,that in group（b）,the best correlation is between the peak values of Akasofu function (A_min) and SYM-H_min,and that in group（c）,the best correlation is between K_pmax andΔf₀F_2min. Based on the statistical results,a method for predicting f₀F₂ of a single station is attempted to be set up.The input is modified B_{z min} and the outputs are SYM-H_min andΔf₀F_2min.Then 25 CME-IPS events that caused geomagnetic storms in 1998 and 2009 are used to check the prediction method. The results show that our method can be used to predict SYM-H_min andΔf₀F_2min.     

Admission Control of VL in AFDX Under HRT Constraints

Avionics full duplex switched ethernet(AFDX) is a switched interconnection technology developed to provide reliable data exchange with strong data transmission time guarantees in internal communication of the spacecraft or aircraft.Virtual link(VL) is an important concept of AFDX to meet quality of service(QoS) requirements in terms of end-to-end message deadlines.A VL admission control algorithm in AFDX network under hard real-time(HRT) constraints is studied.Based on the scheduling prin-ciple of AFDX prot...     

暂冲式风洞大开角扩散段性能的实验研究

布置有多层孔板（丝网）的大开角扩散段通过参数的优化设计,可有效缩短暂冲式风洞启动时间,均匀进入稳定段的气流速度,并降低阀后噪声和气流脉动。针对某大型暂冲式风洞大开角扩散段设计关键技术开展专题研究,设计并进行了不同扩散段扩开角角度和中心体分流锥型式的组合实验,从压力损失、出口截面速度分布和降噪特性三个方面进行了对比分析。试验结果表明：试验件45°扩开角＋65°平底锥的压力损失相对最小,而增加导流尾锥的中心分流锥由于底部难以形成稳态的分离涡使得其压力损失明显偏大,其它试验件组合的压力损失值则相接近;各试验件出口截面的速压分布均呈现以中轴线对称分布的双驼峰趋势,且孔板的开孔率偏高时出口剖面速度分布相对更平滑;试验马赫数下的大开角段对气流噪声的消声量约为12～14dB,对频率在2kHz以上的气流噪声具有相对较强的消声能力,同时气流经过设置有多层孔板的大开角扩散段后,气流波动幅值明显降低,气流脉动得到有效地抑制。     

基于神经网络的多卫星姿态协同控制预测模型

摘要： 针对多卫星近距离对空间目标监测中的姿态协同控制问题，研究基于神经网络的智能控制模型.首先设计了面向任意姿态控制方法的神经网络自适应控制模型，该模型不改变卫星姿态控制方法本身，而是接收由理想控制模型生成的理想控制量，理想控制量经过神经网络后直接生成适用于卫星的控制量.根据神经网络对控制系统的系统级状态预测，基于一致性控制协议，设计了多卫星姿态协同控制模型.采用等效姿态角，通过数值仿真，分别验证了预测控制方法、输出状态预测、协同控制的方法正确性和有效性.     

鲁棒设计及其可靠性(英文)

讨论了鲁棒设计与可靠性工程的基本关系。可靠性分为失效和性能衰减两种情况。本文仔细论证了鲁棒设计的三种方法：系统设计、参数设计和误差设计。它们均可在不同层面上对产品可靠性进行改进，故将可靠性方法与鲁棒设计方法相结合使用后，可以提高产品的质量和可靠性。     

具有气体动力和物理化学非均匀性的超声速物体绕流(英文)

本文研究的问题是超声速气流流过物体时产生的气体动力和物理化学非均匀性及其对物体空气动力特性的影响。就有关流动非均匀性对温度剖面和密度的效应作了详细探讨，还仔细描述了激波与热层相互干扰时以及在激光辐射脉冲的作用下先行激波生成的情况。值得指出的是超声速气流中加入激光辐射能可能改变流动结构，在局部能量释放区域后面呈现的较高和较低压力，有助于控制飞行中物体的运动。可采取某些措施以改进飞行品质。     

壁面带微结构管道内Cassie状态稳定性的实验研究

保持液体在微结构表面处于Cassie状态,是流动减阻的关键。首先利用MicroPTV分别测量了带微结构侧壁处于Cassie和Wenzel状态下的流场速度,表明Cassie状态下近壁速度提高至光滑表面的1.6倍,而Wenzel状态下近壁速度将减小。通过精细控制微管道的驱动压强,观察了液体在近壁由Cassie向Wenzel状态的转变,并测出C/W转变的临界压强值Δpcr约10.9kPa,与Laplace理论预测值10.15kPa基本相符。考虑到Cassie状态失稳也会发生在液体进样过程中,实验还观察了微结构角点对液体进样的＂锚定＂作用,并初步分析了液体进样中自由液面在微结构表面保持Cassie状态的条件。     

Application of ADER Scheme in MHD Simulation

The Arbitrary accuracy Derivatives Riemann problem method(ADER) scheme is a new high order numerical scheme based on the concept of finite volume integration,and it is very easy to be extended up to any order of space and time accuracy by using a Taylor time expansion at the cell interface position.So far the approach has been applied successfully to flow mechanics problems.Our objective here is to carry out the extension of multidimensional ADER schemes to multidimensional MHD systems of conservation laws by calculating several MHD problems in one and two dimensions: (ⅰ) Brio-Wu shock tube problem,(ⅱ) Dai-Woodward shock tube problem,(ⅲ) Orszag-Tang MHD vortex problem.The numerical results prove that the ADER scheme possesses the ability to solve MHD problem,remains high order accuracy both in space and time,keeps precise in capturing the shock.Meanwhile,the compared tests show that the ADER scheme can restrain the oscillation and obtain the high order non-oscillatory result.     

Recent Development and Preliminary Results of Chinese Meridian Project

The Meridian Project is a ground-based network program to monitor solar-terrestrial space environment, which consists of a chain of 15 ground-based observatories located roughly along 120°E longitude and 30°N latitude. The Meridian project started in 2008, and its construction was completed by 2011. The integration and test phase of the Meridian Project conducted in 2011 demonstrated its observation capabilities as expected. The project will be in full operation in 2012. This report gives an overview of the recent development and preliminary results of the Meridian Project since 2010.      

Effect of the Interplanetary Electric Field on the Magnetopause From Global MHD Simulations

The north-south component B_z of the Interplanetary Magnetic Field (IMF) and solar wind dynamic pressure P_d are generally treated as the two main factors in the solar wind that determine the geometry of the magnetosphere. By using the 3D global MHD simulations, we investigate the effect of the Interplanetary Electric Field (IEF) on the size and shape of magnetopause quantitatively. Our numerical experiments confirm that the geometry of the magnetopause are mainly determined by P_dB_z, as expected. However, the dawn-dusk IEFs have great impact on the magnetopause erosion because of the magnetic reconnection, thus affecting the size and shape of the magnetopause. Higher solar wind speed with the same B_z will lead to bigger dawn-dusk IEFs, which means the higher reconnection rate, and then results in more magnetic flux removal from the dayside. Consequently, the dayside magnetopause moves inward and flank magnetopause moves outward.