双喷管发动机喷流对飞行器气动特性的影响

从三维薄层近似N S方程出发 ,采用高效ENO差分格式 ,对位于弹体中部两侧的双喷管发动机喷流与马赫数Ma∞ =0 7～ 0 9、攻角α =0°～ 10°飞行条件下弹体绕流形成的干扰流场进行了数值模拟。研究发现与无喷流情况相比较 ,引入喷流使升力和俯仰力矩增加 ,压心后移 ;在飞行攻角一定时 ,马赫数对飞行器气动力特性影响较小 ;有侧风干扰时 ,喷流增强了航向稳定性。对零攻角情况喷管安装和喷管出口不对称带来侧向力和偏航力矩也进行了研究。计算结果与飞行实验观测现象定性一致     

双锋角钻头钻削碳纤维增强树脂基复合材料钻孔缺陷的研究

针对碳纤维复合材料钻孔时易产生撕裂、毛刺等缺陷的特点,采用双锋角钻头为研究对象,从横刃、第一主切削刃和第二主切削刃对孔入、出口缺陷的影响和加工参数对撕裂因子的影响规律等方面分析双锋角钻头钻孔特点,并与普通麻花钻进行对比。结果表明:在相同的加工参数下,双锋角钻头双主切削刃加工特点降低了入、出口钻削轴向力,有效抑制了入、出口撕裂、毛刺等缺陷产生,更适合于钻削碳纤维复合材料。主轴转速增大有利于减小撕裂因子,随着进给速度的增加撕裂因子呈增大的趋势。采用多元线性回归方法建立了试验两种钻头钻孔入、出口的撕裂因子与加工参数之间的回归预测模型。     

A triangle voting algorithm based on double feature constraints for star sensors

A novel autonomous star identification algorithm is presented in this study. In the proposed algorithm, each sensor star constructs multi-triangle with its bright neighbor stars and obtains its candidates by triangle voting process, in which the triangle is considered as the basic voting element. In order to accelerate the speed of this algorithm and reduce the required memory for star database, feature extraction is carried out to reduce the dimension of triangles and each triangle is described by its base and height. During the identification period, the voting scheme based on double feature constraints is proposed to implement triangle voting. This scheme guarantees that only the catalog star satisfying two features can vote for the sensor star, which improves the robustness towards false stars. The simulation and real star image test demonstrate that compared with the other two algorithms, the proposed algorithm is more robust towards position noise, magnitude noise and false stars.     

Magnetospheric Physics in China: 2012–2014

In the past two years, many progresses have been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS and RBSP missions, or by computer simulations. This paper briefly reviews these works based on papers selected from the 126 publications from March 2012 to March 2014. The subjects cover various sub-branches of magnetospheric physics,including geomagnetic storm, magnetospheric substorm and magnetic reconnection.     

大型数控龙门桥式加工中心的研制

针对船舶、航空、轨道交通、核电等行业的大型零件加工需求,研制了大型数控龙门桥式加工中心,3个移动轴行程为3m×5m×0.8m,可实现O.02mm的镗铣加工精度.通过对加工中心若干技术研究集成,使之具备以下重大特点:(1)研究伺服电机解耦控制方法及双驱动同步技术,保证横梁在两侧桥式立柱导轨上的精确同步纵向移动;(2)通过旋转螺母丝杠结构分别独立驱动双主轴头在横梁上的横向移动,实现双主轴独立加工;(3)利用双回转摆动铣头附件及控制系统集成,实现大型零件的五轴数控加工.所研制的加工中心具有工作台承重大、加工效率高、使用方便、自动化程度较高等特点,已成功用于生产.     

CCD信号处理的滤波器设计

介绍了CCD信号处理电路的工作原理,描述了相关双采样对CCD输出信号的处理过程以及处理后的波形。通过对相关双采样的输出与A/D采样时钟的时序关系,确定了A/D变换前的滤波器对相关双采样输出信号的前沿最大影响,然后通过计算确定滤波器的带宽以及相关参数。最后对滤波器进行了初步设计,最后使用Pspice软件对滤波器进行了仿真。     

Progress of Double Star Program 2006—2008

This paper presents the status of two satellites of Double Star Program,and a part of scientific results based on the data of Double Star Program obtained during the period of 2006-2008.Other scientific results in the magnetospheric physics research can be found in "Multi scale physical process in the magnetosphere" of this issue.     

Energy spectrum of proton flux near geomagnetic equator at low altitudes

The results of proton energy (tens keV – several MeV) spectrum measurements near geomagnetic equator (L < 1.15) at low altitudes (<1000 km) are presented. We used data of experiments onboard ACTIVE, SAMPEX, NOAA TIROS-N satellites and SPRUT-VI (MIR station) and cover a time range of about 30 years (including previous measurements). It was found that the kappa-distribution function fits the experimental spectrum with the best correlation coefficient. A comparison of energy spectra of near-equatorial protons and ring-current protons was made. Using the estimation of the life time of near-equatorial protons we explain the difference in spectral indices of radiation belt and near-equatorial proton formation. We conclude that the ring current is the main source of the near-equatorial protons.     

The plasma sheet and boundary layers under northward IMF: A multi-point and multi-instrument perspective

During conditions of northward interplanetary magnetic field (IMF), the near-tail plasma sheet is known to become denser and cooler, and is described as the cold-dense plasma sheet (CDPS). While its source is likely the solar wind, the prominent penetration mechanisms are less clear. The two main candidates are solar wind direct capture via double high-latitude reconnection on the dayside and Kelvin–Helmholtz/diffusive processes at the flank magnetopause. This paper presents a case study on the formation of the CDPS utilizing a wide variety of space- and ground-based observations, but primarily from the Double Star and Polar spacecraft on December 5th, 2004. The pertinent observations can be summarized as follows: TC-1 observes quasi-periodic (∼2 min period) cold-dense boundary layer (compared to a hot-tenuous plasma sheet) signatures interspersed with magnetosheath plasma at the dusk flank magnetopause near the dawn-dusk terminator. Analysis of this region suggests the boundary to be Kelvin–Helmholtz unstable and that plasma transport is ongoing across the boundary. At the same time, IMAGE spacecraft and ground based SuperDARN measurements provide evidence of high-latitude reconnection in both hemispheres. The Polar spacecraft, located in the southern hemisphere afternoon sector, sunward of TC-1, observes a persistent boundary layer with no obvious signature of boundary waves. The plasma is of a similar appearance to that observed by TC-1 inside the boundary layer further down the dusk flank, and by TC-2 in the near-Earth magnetotail. We present comparisons of electron phase space distributions between the spacecraft. Although the dayside boundary layer at Polar is most likely formed via double high-altitude reconnection, and is somewhat comparable to the flank boundary layer at Double Star, some differences argue in favour of additional transport that augment solar wind plasma entry into the tail regions.