The use of Gaussian equations of motions of a satellite for local gravity anomaly recovery

The orbital elements of a low Earth orbiting satellite and their velocities can be used for local determination of gravity anomaly. The important issue is to find direct relations among the anomalies and these parameters. Here, a primary theoretical study is presented for this purpose. The Gaussian equations of motion of a satellite are used to develop integral formulas for recovering the gravity anomalies. The behaviour of kernels of the integrals are investigated for a two-month simulated orbit similar to that of the Gravity field and steady-state ocean circulation explorer (GOCE) mission over Fennoscandia. Numerical investigations show that the integral formulas have neither isotropic nor well-behaved kernels. In such a case, gravity anomaly recovery is not successful due to large spatial truncation error of the integral formulas. Reformulation of the problem by combining the orbital elements and their velocities leads to an integral with a well-behaved kernel which is suitable for our purpose. Also based on these combinations some general relations among the orbital elements and their velocities are obtained which can be used for validation of orbital parameters and their velocities.     

国有企业资产重组中职工带资分流的法律研究

如何做好主辅分离，既加强主业企业的竞争优势，又妥善安置好分流职工，是国有企业资产重组中的一个重要课题。采取职工带资分流的方式，是解决这一难题的一个有效途径。鉴于我国目前在此方面的相关立法并不健全，我国应进一步完善相关立法。     

Dynamics of a spacecraft and normalization around Lagrangian points in the Neptune–Triton system

The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L₂, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method.     

多任务在轨服务模块化智能航天器技术研究

首先介绍了在轨服务技术的分类及国内外近期研究进展,结合各国已开展项目的验证情况,分析了在轨服务模式、适应多任务在轨服务航天器的发展思路。为适应卫星发射和在轨服务的任务需要,提出了多任务服务航天器的方案设想,以期降低在轨服务操作的难度,提升在轨服务系统执行多任务的能力。最后初步分析了用于演示验证任务的服务航天器总体参数及任务规划。     

“任务驱动”下的计算机专业课程教学实践与探索

本文总结了“任务驱动”在教学中的应用，提出了“任务”设计要全方位立体化进行考虑；评价要全方位多样化。指出了“任务驱动”必须与多种教学法优化组合，才能发挥其最大教学效率。     

现代远程教育的媒体素材构建方法

本文阐述了媒体素材的采集及处理方法 ,对现代远程教育工程建设可提供有效的帮助     

浅析运输类飞机经济舱头排旅客座椅头部损伤判据的影响因素

介绍了头部损伤判据HIC的概念、适航要求及影响运输类飞机客舱头排旅客座椅HIC的相关参数;叙述了旅客座椅头排距、头部撞击壁板的刚度、安全带织带伸长率、乘坐摩擦系数等参数的影响和重要程度;对如何设计符合HIC要求的经济舱头排旅客座椅和壁板提出了建议。     

判断力权值的确定方法及AHP中群组判断矩阵的形成

在ＡＨＰ模型中，请一组专家对某一属性进行评价，根据专家的判断能力，给出判断力权值，再通过适当的数学处理方法，可得最优判断矩阵，这是ＡＨＰ中构造判断矩阵的一种新方法。     

跨声速风洞斜孔壁非线性流动试验

为分析跨声速风洞斜孔壁近壁区域的流动特性，评估气流偏角-压力系数的非线性关联，在0.6 m跨超声速风洞中开展了基于七孔探针的流动特性测量试验。通过气流偏角和压力系数分布分析了斜孔壁流动的差阻特性，以及马赫数、模型升力对斜孔壁流动的影响，最后基于试验结果发展了计算斜孔壁特性参数的微分法，并与经验方法结果进行对比。结果表明，斜孔壁流动呈现出明显的差阻性和非线性，在负压差范围内，近壁流动仍以出流为主；高亚声速时，空风洞模型区孔壁流动特性趋于实壁；安装模型后，随着升力的增大，升力面对应的孔壁区域流动向入流发展，孔壁流动特性趋于开口边界。     

Characterization of the cataloged Fengyun-1C fragments and their long-term effect on the LEO environment

The intentional breakup of Fengyun-1C on 11 January 2007 created the most severe orbital debris cloud in history. The altitude where the event occurred was probably the worst location for a major breakup in the low Earth orbit (LEO) region, since it was already highly populated with operational satellites and debris generated from previous breakups. The addition of so many fragments not only poses a realistic threat to operational satellites in the region, but also increases the instability (i.e., collision cascade effect) of the debris population there.