Optimal station-keeping near Earth–Moon collinear libration points using continuous and impulsive maneuvers

In this study the gravitational perturbations of the Sun and other planets are modeled on the dynamics near the Earth–Moon Lagrange points and optimal continuous and discrete station-keeping maneuvers are found to maintain spacecraft about these points. The most critical perturbation effect near the L₁ and L₂ Lagrange points of the Earth–Moon is the ellipticity of the Moon’s orbit and the Sun’s gravity, respectively. These perturbations deviate the spacecraft from its nominal orbit and have been modeled through a restricted five-body problem (R5BP) formulation compatible with circular restricted three-body problem (CR3BP). The continuous control or impulsive maneuvers can compensate the deviation and keep the spacecraft on the closed orbit about the Lagrange point. The continuous control has been computed using linear quadratic regulator (LQR) and is compared with nonlinear programming (NP). The multiple shooting (MS) has been used for the computation of impulsive maneuvers to keep the trajectory closed and subsequently an optimized MS (OMS) method and multiple impulses optimization (MIO) method have been introduced, which minimize the summation of multiple impulses. In these two methods the spacecraft is allowed to deviate from the nominal orbit; however, the spacecraft trajectory should close itself. In this manner, some closed or nearly closed trajectories around the Earth–Moon Lagrange points are found that need almost zero station-keeping maneuver.     

用于非定常粘性流动计算的无网格算法(英文)

把无网格算法发展用于求解涉及动边界的非定常粘性流动问题。在处理粘性流动的布点问题时,通过在远离物面的区域采用无粘流动计算时所用的各向同性点云,而在物面附近引入各向异性点云,从而在保证物面法线方向布点较密以准确模拟边界层的同时,有效控制了布点总量,减少了计算时间。对于动边界问题,本文在上述方法获得的初始布点的基础上,采用基于扰动衰减规律的点云移动技术,快速得到物面运动到其他位置时流场求解所需点云。在所获得的点云上,采用一种带权系数的二次极小曲面逼近方法来离散Navier-Stokes方程的空间导数,权系数的引入使得流场求解时对各向同性点云和各向异性点云无需分开考虑,而是采用统一的求解方法,从而简化了编程求解。用发展的无网格算法,结合Navier-Stokes方程求解双时间推进方法,并耦合Spalart-Allmaras湍流模型,先成功地模拟出NLR7301翼型后缘摆动诱发的非定常流,并通过与实验比较,验证了本方法.接着进行了NACA0012失速模拟,给出了动态失速过程,展示出用本文方法处理复杂动边界问题的效果。     

一种新的计算非稳态流动的自适应无网格方法

基于带权点填充布点方法,结合指定流场参数梯度的分布,提出了一种新的无网格自适应方法计算非稳态问题。该方法的自适应探测器 E 由节点的权重和参数梯度组成。使用自适应探测器识别出加密或者粗化的区域,形成加密空腔和粗化空腔,然后重新填充布点。新节点的权重由自适应探测器 E 结合该处的梯度大小通过预测-校正迭代算法计算得到。另外,由于参数梯度在激波附近波动范围比较大,所以新节点的权重存在最大值和最小值。首先对预先设置压强梯度的流场区域进行自适应布点,并与传统自适应布点结果进行对比,点云分布图显示所提自适应方法重新生成的点云结构疏密分布更加合理。进一步,将此自适应方法应用于 Riemann 问题和激波碰撞圆柱问题,计算结果表明该方法可以在节点数目较低的情况下显著提高运动激波的分辨率。在激波碰撞圆柱问题中,比较了使用自适应算法和非自适应算法得到相当的结果所使用时间,前者是后者的20.6%,因此该自适应算法在计算效率方面也具有较大的优势。     

多传感器对编队目标无源定位的数据关联技术研究

针对多传感器对编队目标进行测向交叉定位会产生大量虚假点的问题,提出了一种属性方位联合数据关联方法.采用基于支持度的关联算法对传感器探测到的目标属性数据进行初步关联,剔除部分虚假交点.然后利用改进的基准线最小距离法从候选集合中找出目标的真实测量数据关联集合.仿真结果表明,相对传统的方位数据关联方法,该方法不仅可以快速剔除虚假点,而且能够显著提高关联正确率.     

Emission heights of coronal bright points on Fe XII radiance map

The study of coronal bright points (BPs) is important for understanding coronal heating and the origin of the solar wind. Previous studies indicated that coronal BPs have a highly significant tendency to coincide with magnetic neutral lines in the photosphere. Here we further studied the emission heights of the BPs above the photosphere in the bipolar magnetic loops that are apparently associated with them. As BPs are seen in projection against the disk their true emission heights are unknown. The correlation of the BP locations on the Fe XII radiance map from EIT with the magnetic field features (in particular neutral lines) was investigated in detail. The coronal magnetic field was determined by an extrapolation of the photospheric field (derived from 2-D magnetograms obtained from the Kitt Peak observatory) to different altitudes above the disk. It was found that most BPs sit on or near a photospheric neutral line, but that the emission occurs at a height of about 5 Mm. Some BPs, while being seen in projection, still seem to coincide with neutral lines, although their emission takes place at heights of more than 10 Mm. Such coincidences almost disappear for emissions above 20 Mm. We also projected the upper segments of the 3-D magnetic field lines above different heights, respectively, on to the tangent x–y plane, where x is in the east–west and y in the south–north direction. The shape of each BP was compared with the respective field-line segment nearby. This comparison suggests that most coronal BPs are actually located on the top of their associated magnetic loops. Finally, we calculated for each selected BP region the correlation coefficient between the Fe XII intensity enhancement and the horizontal component of the extrapolated magnetic field vector at the same x–y position in planes of different heights, respectively. We found that for almost all the BP regions we studied the correlation coefficient, with increasing height, increases to a maximal value and then decreases again. The height corresponding to this maximum was defined as the correlation height, which for most bright points was found to range below 20 Mm.     

三维散乱点的c~1曲面插值及应用

本文介绍了一种对三维散乱点插值的二次Bernstein-Bezier c~1曲面构造方法。首先,不规则分布的3D数据点{(x_i,y_i,z_i),i=1,2,3,…,N}被投影到X-Y平面上,并按本文提出的能够处理任意区域内不规则分布点的三角化算法,自动形成平面三角形插值网络。然后按照所形成的三角形网络和网络结点处的函数值,分别估计出每一数据点上的一阶导数值。最后本文给出了用二次多项式表示的三角形网络上的Bernstein-Bezier c~1曲面插值公式,并指出了这一曲面插值模型在某些应用领域的广阔前景。     

测井车电缆滚筒的传动系统设计

简要论述了该石油测井车电缆滚筒传动系统的设计要点。测井车的研制成功，满足了先进测井技术的要求，成为各油田替代进口的产品。     

对 k-ω 湍流模型的改进

为了更适合于较复杂几何外形的数值计算，本文提出仅引入１个参数来改进ｋ－ω湍流模型并采用了一种双网格系统的有限体积格式来求解Ｎ－Ｓ方程与改进的的ｋ－ω模型方程。通过平板附面层的计算结果表明了用本文提出的对ｋ－ω湍流模型的改进对控制转捩是有效的。     

采用激光跟踪仪测量飞机外形

利用激光跟踪仪测量空间点坐标的原理，通过“转站”建立飞机坐标系，采集飞机外形坐标点云，处理数据并建立数学模型。     

考虑压气机动静干涉效应的非设计工况性能数值模拟

1引言非定常流动是叶轮机械内部固有的本质属性,而现有的设计体系中不论是在设计或分析时基本上采用定常流动的假设,从而忽略了非定常流动对叶轮机械在气动、结构强度等方面的影响。目前,国内外对非定常流动的研究比较多,但其中采用非定常流动数值模拟方法预估压气机非设计工况