Application of Contact Graph Routing in Satellite Delay Tolerant Networks

Satellite networks have many inherent advantages over terrestrial networks and have become an important part of the global network infrastructure. Routing aimed at satellite networks has become a hot and challenging research topic. Satellite networks, which are special kind of Delay Tolerant Networks (DTN), can also adopt the routing solutions of DTN. Among the many routing proposals, Contact Graph Routing (CGR) is an excellent candidate, since it is designed particularly for use in highly deterministic space networks. The applicability of CGR in satellite networks is evaluated by utilizing the space oriented DTN gateway model based on OPNET(Optimized Network Engineering Tool). Link failures are solved with neighbor discovery mechanism and route recomputation. Earth observation scenario is used in the simulations to investigate CGR’s performance. The results show that the CGR performances are better in terms of effectively utilizing satellite networks resources to calculate continuous route path and alternative route can be successfully calculated under link failures by utilizing fault tolerance scheme.     

Orbit Design for Twin-spacecraft Space VLBI

Space Very Long Baseline Interferometry (S-VLBI) is an aperture synthesis technique utilizing an array of radio telescopes including ground telescopes and space orbiting telescopes. It can achieve much higher spatial resolution than that from the ground-only VLBI. In this paper, a new concept of twin spacecraft S-VLBI has been proposed, which utilizes the space-space baselines formed by two satellites to obtain larger and uniform uv coverage without atmospheric influence and hence achieve high quality images with higher angular resolution. The orbit selections of the two satellites are investigated. The imaging performance and actual launch conditions are all taken into account in orbit designing of the twin spacecraft S-VLBI. Three schemes of orbit design using traditional elliptical orbits and circular orbits are presented. These design results can be used for different scientific goals. Furthermore, these designing ideas can provide useful references for the future Chinese millimeter-wave S-VLBI mission.     

基于机动力模型的GEO卫星恢复期间定轨

北斗卫星导航系统(BDS)中GEO卫星频繁的轨道机动对高精度、实时不间断的导 航服务需求提出了更高要求, 如何在短弧跟踪条件下提高GEO卫星轨道快速 恢复能力, 是提升导航系统服务精度的关键因素. 针对该问题, 本文提出了基 于机动力模型的动力学定轨方法, 尝试利用高精度的C波段转发式测距数据, 辅 以机动期间的遥测遥控信息建立机动力模型, 联合轨控前后的观测数据进行动 力学长弧定轨. 利用BDS中GEO卫星实测数据进行了定轨试验与分析, 结果表明, 恢复期间需要采用解算机动推力的定轨方法, 联合机动前、机动期间和机 动后4h数据定轨的轨道位置精度在20m量级, 径向精度优于2.5m. 该方 法克服了短弧跟踪条件下动力学法定轨和单点定位中的诸多问题, 提供了解决 GEO卫星机动后轨道快速恢复问题的技术方法.     

FC72-氮气混合气体流动冷凝效率研究

混合气体（可凝蒸气与不可凝气体）相对于纯可凝蒸气,其流动冷凝过程更为复杂,冷凝效率受不可凝气体的浓度及冷凝温度影响.为对空间任务蒸发冷凝实验平台排放的废气FC72进行清理回收,针对所研制的FC72气液分离与收集器,在地面环境下对不同浓度的混合气体在不同冷凝温度下进行了流动冷凝效率实验.结果表明,对于FC72与氮气的混合气体,当冷凝器温度一定时,随着FC72浓度的增加,该气液分离与收集器的冷凝效率提高.在冷凝器温度约为-10℃,FC72浓度高于70%时,流动冷凝效率达到80%以上;当冷凝器温度降低至约-13℃,FC72浓度高于30%时,流动冷凝效率达到70%以上;当冷凝器温度降至约-15℃,FC72浓度高于20%时,流动冷凝速率均达到60%以上.     

标准孔板流量计内部流场的CFD数值模拟

通过在标准孔板流量计中引入CFD数值模拟,为流出系数的获取提供了新途径.对不可压缩流体在不同流量、不同直径比、不同孔板轴向厚度和不同流动介质下的内部流场进行了数值模拟计算,并将计算出的流出系数与根据ISO公式计算出的流出系数进行了分析对比.结果表明,随着结构参数和工作条件的改变,流出系数都会随之发生变化,但ISO公式对孔板厚度的变化不太敏感.CFD数值模拟可以作为标准孔板流量计的辅助设计与标定手段,以进一步提高孔板流量计计量的准确性.     

亚、跨、超声速下空腔流场特性实验研究

在FL-21跨、超声速风洞中对空腔流场特性进行了较为深入的实验研究.空腔的长深比L/D为7、8、9、12、15,试验马赫数M范围为0.6、0.9、1.2、1.5、1.8,试验雷诺数Re为1.23~2.26×107.研究表明:空腔流场特性主要由空腔长深比L/D和来流马赫数所决定,这两个参数的变化均能引起空腔的流场类型发生变化.另外,边界层厚度涠钥涨坏撞康难沽Ψ植家灿凶畔灾挠跋?随着边界层厚度与空腔深度之比?D的减小,空腔的流场类型有向闭式穴流动转变的趋势.     

LEO-LEO掩星事件持续时间及卫星间相对角速度仿真分析

通过对LEO-LEO掩星事件仿真,分析卫星轨道参数对掩星事件持续时间和卫星间相对角速度的影响.结果表明：对掩星事件持续时间影响较大的LEO-LEO卫星轨道参数依次为轨道倾角、升交点赤经、轨道高度,近地点角距对掩星事件持续时间影响不大;LEO-LEO卫星轨道倾角互补时,掩星事件持续时间最短,为98s;两颗LEO卫星轨道倾角之和或者升交点赤经之差在120°-240°范围内,掩星持续时间约100~150s;两颗LEO卫星轨道越高,掩星持续时间越短;掩星发生时,LEO卫星间水平方向相对角速度最大值约为0.14（°）·^-1,俯仰方向相对角速度最大值约为0.078（°）·s^-1.

     

Electrostatic Structure of the Electron Phase-space Holes Generated by the Electron Two-stream Instability with a Finite Width

Space satellite observations in an electron phase-space hole (electron hole) have shown that bipolar structures are discovered at the parallel cut of parallel electric field, while unipolar structures spring from the parallel cut of perpendicular electric field. Particle-in-cell (PIC) simulations have demonstrated that the electron bi-stream instability induces several electron holes during its nonlinear evolution. However, how the unipolar structure of the parallel cut of the perpendicular electric field formed in these electron holes is still an unsolved problem, especially in a strongly magnetized plasma (Ω_e > ω_pe, where Ω_e is defined as electron gyrofrequency and ω_pe is defined as plasma frequency, respectively). In this paper, with two-dimensional (2D) electrostatic PIC simulations, the evolution of the electron two-stream instability with a finite width in strongly magnetized plasma is investigated. Initially, those conditions lead to monochromatic electrostatic waves, and these waves coalesce with each other during their nonlinear evolution. At last, a solitary electrostatic structure is formed. In such an electron hole, a bipolar structure is formed in the parallel cut of parallel electric field, while a unipolar structure presents in the parallel cut of perpendicular electric field.

     

含孔隙的2.5D编织陶瓷基复合材料弹性常数预测

为获取更为全面的编织陶瓷基复合材料弹性常数,支撑材料力学性能研究,提出考虑纤维性能退化和基体孔隙的编织陶瓷基复合材料弹性常数预测方法。围绕25D编织陶瓷基复合材料,通过微焦点断层扫描获取材料孔隙率和孔隙分布,并测量碳化硅纤维单丝经热处理后的高温强度和模量。再结合细观力学有限元法理论,通过Digimat建立含孔隙的25D陶瓷基复合材料代表体单元有限元模型,计算得到材料弹性常数。同时对元件级试验件进行了室温单向拉伸和面内剪切试验,弹性常数计算值和试验值吻合较好,验证了该方法可以用来预测含孔隙的25D编织陶瓷基复合材料的弹性常数,为其力学性能与失效机理分析建立基础。     

老龄结构分析中腐蚀坑与等效裂纹间的量化关系

通过对航空结构的主体材料LY12-CZ进行预腐蚀试验,得到在不同条件下的腐蚀坑尺寸,然后进行疲劳试验并得到试验件寿命,再利用蒙特卡罗(MonteCarlo)方法对Paris公式进行数值积分并求解非线性方程,从而确定了与已知尺寸腐蚀坑有相同寿命所对应的等效表面裂纹的尺寸,最后把等效裂纹和腐蚀坑的尺寸分别代到模拟软件AFGROW内进行寿命预测并和试验疲劳寿命进行了比较。结果发现,把腐蚀坑等效为具有相同寿命的表面裂纹时,等效表面裂纹的尺寸比对应腐蚀的尺寸小19.7%-22.5%。