天基强银河背景下的空间碎片探测试验及分析

本文设计并完成了银河背景下碎片探测试验，数据分析表明，强的银河背景会降低探测器对暗弱碎片的探测能力，但对碎片的天文定位精度影响不大。本文验证了采用基于探测概率的极限探测星等方法表征探测器极限探测能力的合理性，以及基于仿真的方法增加数据完备度的可行性。本文的工作将为后续天基探测器的设计及探测试验的开展提供依据。     

铝颗粒云燃烧研究进展

为探究铝颗粒云燃烧特性,把握其研究进展,并为后续研究工作提供参考,本文首先简述了铝颗粒点火、燃烧过程,总结了铝颗粒燃烧机理;其次,综述了铝颗粒云燃烧的实验、理论和模拟研究进展,从不同维度分析了影响颗粒云火焰速度的关键参数,并提出颗粒云燃烧的研究方向,包括提升颗粒云燃烧实验颗粒分散均匀性与表征精度、降低火焰传播速度等实验结果散差、改善颗粒云燃烧理论预测模型精度及构建实用的颗粒云燃烧模拟CFD模型。     

Observation of a 27-day solar signature in noctilucent cloud altitude

Previous studies have identified solar 27-day signatures in several parameters in the Mesosphere/Lower thermosphere region, including temperature and Noctilucent cloud (NLC) occurrence frequency. In this study we report on a solar 27-day signature in NLC altitude with peak-to-peak variations of about 400?m. We use SCIAMACHY limb-scatter observations from 2002 to 2012 to detect NLCs. The superposed epoch analysis method is applied to extract solar 27-day signatures. A 27-day signature in NLC altitude can be identified in both hemispheres in the SCIAMACHY dataset, but the signature is more pronounced in the northern hemisphere. The solar signature in NLC altitude is found to be in phase with solar activity and temperature for latitudes $?70°$N. We provide a qualitative explanation for the positive correlation between solar activity and NLC altitude based on published model simulations.     

A debris image tracking using optical flow algorithm

This study proposes a motion detection and object tracking technique for GEO debris in a sequence of images. A couple of techniques (called the “stacking method” and “line-identifying technique”) were recently proposed to address the same problem. Although these techniques are effective at detecting the debris position and motion in the image sequences, there are some issues concerned with computational load and assumed debris motion. This study derives a method to estimate motion vectors of objects in image sequence and finally detect the debris locations by using a computer vision technique called an optical flow algorithm. The new method detects these parameters in low computational time in a serial manner, which implies that it has an advantage to track not only linear but also nonlinear motion of GEO debris more easily than the previous methods. The feasibility of the proposed methods is validated using real and synthesized image sequences which contain some typical debris motions.     

基于光场成像的快照式气膜孔三维测量技术

叶片气膜孔的几何参数对其冷却效率具有十分重要的影响,需采取有效手段对加工的气膜孔几何参数进行检测。基于光场成像原理,初步探索了单光场相机快照式三维测量技术在气膜孔检测上的应用。与其他光学测量技术相比,该技术仅通过一次拍摄,即可快速从捕获的单张原始光场图像中计算得到气膜孔的三维点云数据,其数据采集效率很高。实验中对一组标准量块进行了测量,展示了单光场相机应用于工业级精密测量的潜力。对实际叶片上气膜孔几何参数的检测结果初步表明了该技术应用于气膜孔三维测量的可能性。由于单光场相机成像系统的结构简单,易于操作且便于与其他传感器设备集成,可为气膜孔三维测量问题提供一种新的解决方案。     

MLI碎片防护能力增强措施对隔热性能的影响

从原理上、实验测试和理论建模三个角度分析了MLI碎片防护增强措施对ML I隔热性能的影响。研究表明,在一定范围内增加MLI单元数、添加增强性材料、增加反射屏 之间距离的措施均不会明显改变MLI的隔热性能,真空状态下20单元MLI隔离物的接触率约为 40％。由于增强防护性能的措施会影响到MLI的放气性能,应研究改善增强型MLI的放气性 能的措施,并在反射屏与增强性材料之间及增强性材料之间添加间隔材料。
     

Aerosols and clouds in the upper troposphere–lower stratosphere region detected by GOMOS and ACE: Intercomparison and analysis of the years 2004 and 2005

Satellite-based limb occultation measurements are well suited for the detection and mapping of polar stratospheric clouds (PSCs) and cirrus clouds. PSCs are of fundamental importance for the formation of the Antarctic ozone hole that occurs every year since the early 1980s in Southern Hemisphere spring. Despite progress in the observation, modeling and understanding of PSCs in recent years, there are still important questions which remain to be resolved, e.g. PSC microphysics, composition, formation mechanisms and long-term changes in occurrence. In addition, it has recently become clear that cirrus clouds significantly affect the global energy balance and climate, due to their influence on atmospheric thermal structure.     

复杂外形下的无网格算法研究

研究了二维、三维复杂外形下的无网格算法。在一种布置点云方法的基础上,发展一种曲面拟合的重构方式构造流场物理量,并应用于AUSM+_up格式计算欧拉方程的数值通量;计算采用了隐式时间推进,并引入当地时间步长和残值光顺等加速收敛措施。通过对某三段翼型低速流动、M6机翼跨音速流动、某全机跨音速流动进行了数值模拟,表明本文发展的无网格算法能有效地模拟复杂外形的无粘绕流。     

箔条云团的布朗运动扩散模型

假定箔条所在位置处大气运动速度是一个维纳随机过程,同时在忽略箔条的质量时箔条的运动完全反应当地大气的运动,在此基础上建立箔条云团的扩散模型及数值仿真模型. 对扩散模型进行分析得到了箔条云团扩散过程中的数字特征.对数值仿真模型的分析表明必须对大气的运动方差进行时间离散化补偿,进行离散化补偿后箔条云团的数字特征不受模拟时时间步长的影响.模拟结果证明了分析的正确性.