基于激波风洞的超声速磁流体动力技术实验系统

开展磁流体(MHD)动力技术实验研究,实验系统必须满足两项基本的条件:一是超声速或高超声速气流;二是气流必须是导电流体.基于此,介绍了基于激波风洞的超声速磁流体动力技术实验系统的基本组成、设计思想和调试情况.设计了马赫数Ma=2的超声速喷管及实验段;采用氦气驱动氩气,在平衡接触面运行方式下得到高温气体,通过在低压段注入...     

整体叶盘通道电解加工电极多维运动轨迹优化

为了提高整体叶盘通道余量分布的均匀性,提出了电极运动轨迹优化方法.分析了电解加工间隙对电极运动轨迹的影响,优化了工具电极在叶顶及叶根圆柱面上的运动轨迹,并基于轨迹线上采样点作拟合垂线段中点的样条曲线获得新的轨迹线.为了验证优化后轨迹的合理性,进行了叶盘通道电解加工对比试验.试验表明,与优化前的轨迹相比,采用优化后的轨迹...     

The Dawn Mission to Vesta and Ceres

A review of present understanding of the dissipation region in magnetic reconnection is presented. The review focuses on results of the thermal inertia-based dissipation mechanism but alternative mechanisms are mentioned as well. For the former process, a combination of analytical theory and numerical modeling is presented. Furthermore, a new relation between the electric field expressions for anti-parallel and guide field reconnection is developed.     

ARTEMIS Science Objectives

NASA??s two spacecraft ARTEMIS mission will address both heliospheric and planetary research questions, first while in orbit about the Earth with the Moon and subsequently while in orbit about the Moon. Heliospheric topics include the structure of the Earth??s magnetotail; reconnection, particle acceleration, and turbulence in the Earth??s magnetosphere, at the bow shock, and in the solar wind; and the formation and structure of the lunar wake. Planetary topics include the lunar exosphere and its relationship to the composition of the lunar surface, the effects of electric fields on dust in the exosphere, internal structure of the Moon, and the lunar crustal magnetic field. This paper describes the expected contributions of ARTEMIS to these baseline scientific objectives.     

不锈钢表面氧化对RP一3航空煤油热氧化结焦的影响

利用有限元方法对航空发动机外部管路模态进行了计算,得到了管路的固有频率及模态振型;通过计算,分析了安装不同数量、位置的卡箍对管路固有频率的影响,以此为依据进行了管路调频,避免了管路共振的发生。     

The Lunar Radar Sounder (LRS) Onboard the KAGUYA (SELENE) Spacecraft

The Lunar Radar Sounder (LRS) onboard the KAGUYA (SELENE) spacecraft has successfully performed radar sounder observations of the lunar subsurface structures and passive observations of natural radio and plasma waves from the lunar orbit. After the transfer of the spacecraft into the final lunar orbit and antenna deployment, the operation of LRS started on October 29, 2007. Through the operation until June 10, 2009, 2363 hours worth of radar sounder data and 8961 hours worth of natural radio and plasma wave data have been obtained. It was revealed through radar sounder observations that there are distinct reflectors at a depth of several hundred meters in the nearside maria, which are inferred to be buried regolith layers covered by a basalt layer with a thickness of several hundred meters. Radar sounder data were obtained not only in the nearside maria but also in other regions such as the farside highland region and polar region. LRS also performed passive observations of natural plasma waves associated with interaction processes between the solar wind plasma and the moon, and the natural waves from the Earth, the sun, and Jupiter. Natural radio waves such as auroral kilometric radiation (AKR) with interference patterns caused by the lunar surface reflections, and Jovian hectometric (HOM) emissions were detected. Intense electrostatic plasma waves around 20 kHz were almost always observed at local electron plasma frequency in the solar wind, and the electron density profile, including the lunar wake boundary, was derived along the spacecraft trajectory. Broadband noises below several kHz were frequently observed in the dayside and wake boundary of the moon and it was found that a portion of them consist of bipolar pulses. The datasets obtained by LRS will make contributions for studies on the lunar geology and physical processes of natural radio and plasma wave generation and propagation.     

追踪椭圆轨道目标Hill制导及其误差分析

针对椭圆轨道目标的飞行器近距离交会问题,研究了追踪任意椭圆轨道目标的Hill制导方法.从状态转移矩阵出发推导出追踪椭圆轨道目标的Hill制导表达式,然后推导出连续常值推力作用下系统状态的解析表达式,在此基础上分析了Hill制导过程中线性化误差和J2摄动误差,通过误差项进行补偿,并给出了Hill制导改进算法.仿真分析表明椭圆轨道Hill制导是可行的,且其改进算法能进一步提高制导精度.     

基于MIMO圆阵雷达的二维DOA估计新算法

基于对均匀圆阵导向矢量的分析,将四元均匀圆阵作为多输入多输出(MIMO)雷达的发射阵,通过构造相应的二阶统计量并对其进行联合对角化获得了目标方位角和俯仰角的闭式解,以实现存在角度兼并时目标的二维到达方向(DOA)的估计,并保持原DOA矩阵方法无需二维谱峰搜索和参数配对等优点。仿真结果证明算法正确、可行。     

卫星姿轨控系统故障推演系统设计架构

研究了目前的卫星姿态轨道控制系统,针对其故障预测、诊断及对策提出了一套故障推演系统设计方案.该方案由故障动态注入系统、动态模拟系统、数据归档显示处理系统组成,完成了对在轨卫星的电性接口一致性仿真,通过计算仿真遥测数据与真实遥测数据的相关量获得异常指标,得出可能出现的故障模式;通过软故障、硬故障和真实部件故障注入方式复现...     

Performance measure for Markovian switching systems using best-fitting Gaussian distributions

This paper considers the theoretical posterior Cramer-Rao lower bound (PCRLB) for the case of tracking a manoeuvring target with Markovian switching dynamics. In a recent article [2] it was proposed to calculate the PCRLB conditional on the manoeuvre sequence and then determine the bound as a weighted average, giving an unconditional PCRLB. However, we demonstrate that this approach can produce an overly optimistic lower bound, because the sequence of manoeuvres is implicitly assumed known. Motivated by this, we develop a general approach and derive a closed-form estimate of the PCRLB in the case of Markovian switching systems. The basis of the approach is to, at each time step, replace the multi-modal prior target probability density function (pdf) with a best-fitting Gaussian (BFG) approximation. We present a recursive formula for calculating the mean and covariance of this Gaussian distribution, and demonstrate how the covariance increases as a result of the potential manoeuvres. We are then able to calculate the PCRLB for this BFG model using an existing Riccati-like recursion. Because of the BFG approximation, we are no longer guaranteed a bound and so we refer to our estimate as an "error performance measure" rather than a bound. The presented approach is applied both to filtering and smoothing cases. The simulation results indicate a very close agreement between the proposed performance measure and the error performance of an interacting multiple model estimator.