基于精确星光大气折射观测模型的轨道摄动研究

基于星光折射间接敏感地平自主导航方法,改进了现有的大气密度模型和固定高度(25km)的观测模型,建立了自适应连续高度(20km～50km)的星光折射观测模型,并在此观测模型的基础上深入分析研究了影响导航精度的各种轨道摄动力,包括地球形状各阶摄动力、不同高度的大气阻力摄动力、太阳光辐射压力等.提出一种精简的大气模式--静止变标高球面大气,解决了由于高层大气密度的求解复杂,使大气阻力摄动模型不精确的问题,由此取得了较好的导航定位精度.利用UKF和EKF两种不同非线性算法,对考虑各种摄动力后的导航定位精度进行全面的计算机仿真实验,并就仿真结果进行了误差分析,同时研究了各种有关参数对导航精度的影响.     

S781白漆在空间辐照环境下物性变化分析

文章研究S781白漆分别在紫外、质子和紫外+质子+电子综合辐照环境下太阳吸收率(αs)的退化情况,并利用X射线光电子能谱（XPS）和扫描电子显微镜（SEM）对样品表面的成分和形貌进行了分析。结果表明:S781白漆的αs受紫外辐照影响较小,但是在质子和综合辐照条件下退化明显。紫外辐照会对S781的硅树脂粘合剂产生裂解作用,质子辐照下样品表面会有污染形成,电子辐照会对深层的硅树脂性质产生影响。     

卫星无线传能系统主动电场屏蔽效能分析

针对无线传能系统宽频段电场辐射屏蔽的需求,建立了采用主动屏蔽方式的无线传能系统屏蔽效能分析电路模型。推导出主动屏蔽激励源可由无线传能系统电压激励源控制。给出了空间点位置和面位置屏蔽效能计算公式,通过对激励电压源进行傅里叶变换后提取关注频段电压分量可实现对宽频段屏蔽效能的分析。通过仿真分析证明了方法的有效性,屏蔽效能与空间位置有关,同时受限于传输效率的约束。通过调节压控电压源的压控系数可以在传输效率损失相对较小的情况下实现关注位置电场辐射的有效屏蔽。最后通过实验验证了无线传能系统主动屏蔽方式屏蔽效能分析方法的正确性和工程可应用性。     

氧化锌色素在真空紫外辐照下降解机理的研究

研究氧化锌色素在真空紫外辐照下的降解机理,目的是为设计在宽间环境下稳定的氧化锌热涂层提供理论依据。仔细研究了自由电子在氧化锌中的吸收特性及真空紫外辐照对氧化锌电导的贡献,认为真空紫外辐照引起氧化锌色素表面化学吸附氧的解析,同时在氧化锌色素表面产生大量的氧空位,氧空位提供了导带中的自由电子,自由电子在导带内跃迁吸收近红外光子引起氧化锌色素光学性能的退化。     

聚合物基PTC材料稳定性的研究

提高导电复合材料的PTC(Positive Temperature Coefficient)强度和稳定室温电阻的重现性,是研究和使用聚合物基PTC材料所追求的目标.PTC材料经过在开关温度及其以上的较宽温度范围内重复热循环后,室温电阻升高,PTC强度降低.研究了辐射交联和在不同气氛中长时间热老化对聚合物基PTC复合材料的室温电阻、PTC强度、结晶度和开关温度等性能的影响.结果表明:辐射交联和氮气氛保护均有利于提高PTC材料的电性能稳定性,室温电阻和PTC强度的变化率相对较小.     

黑体辐射反问题的正则化Lanczos方法

黑体辐射反问题就是利用测量的黑体辐射能量谱确定黑体的区域温度分布.本文将该问题离散化为欠定线性不适定问题,提出求解欠定线性不适定问题的正则化Lanczos方法.该方法基于Lanczos双对角化过程,用一系列小型线性方程组逼近原不适定问题,应用截断SVD正则化方法使迭代稳定化,并用L-曲线确定相应的正则化参数.数值结果说明了新方法的有效性,并说明了在观测数据出现误差的情况下新方法也能有效地重构区域温度分布.     

再入飞行器目标特性建模研究

再入目标的光辐射和电磁散射特性有重要应用,例如目标的探测、识别和指示技术.飞行器高超声速再入过程中,由于与周围大气强烈相互作用,不仅形成复杂结构再入流场,飞行器表面和流场中还伴随发生复杂化学物理过程,对目标特性产生严重影响.在对再入流场及伴随发生的化学物理过程研究分析的基础上, 建立再入目标特性理论模型框架,建立再入飞行器目标特性的基本计算方法,编制了相应计算程序,对典型再入飞行器的红外辐射和电磁散射特性进行了数值模拟.与相应实验结果的比较表明,流场电子数密度、高温气体辐射、等离子体尾迹的RCS等与实验结果一致.     

超高速碰撞可见光谱辐射强度测量技术

针对航天器防护技术及超高速碰撞物理现象研究需要,为超高速碰撞靶研制了超高速碰撞光谱辐射强度测量系统.笔者对该系统的设计和应用该系统对半无限靶碰撞可见光谱辐射强度测量结果进行了介绍.结果表面:所研制的可见光谱辐射强度测量系统满足超高速碰撞可见光谱辐射强度测量要求,并具有成本低、使用方便和易于扩展功能等特点.     

Spacecraft formation and orbit control using differential attitude-dependent solar radiation pressure

This paper introduces a linear model for spacecraft formation dynamics subject to attitude-dependent solar radiation pressure (SRP) disturbance, with the SRP model accounting for both absorption and specular/diffuse reflection. Spacecraft attitude is represented in modified Rodriguez parameters (MRPs), which also parameterize the orientation of individual facets for a spacecraft with fixed geometry. Compared to earlier work, this model incorporates analytic approximation of the SRP-perturbed chief orbit behavior in a manner enabling its use in applications with infrequent guidance updates. Control examples are shown for single-plate representations of hypothetical spacecraft with generally realistic optical parameters. The results demonstrate the validity of the model and the feasibility of SRP-based formation and rendezvous control in orbits around small bodies and in high orbits around the Earth such as the GEO belt.     

Models for estimating daily photosynthetically active radiation in oceanic and mediterranean climates and their improvement by site adaptation techniques

In this work Photosynthetically Active Radiation (PAR) in oceanic and mediterranean climates is modeled. Twenty-two different models have been developed and tested: eleven Multilinear Regression (MR) models and eleven Artificial Neuron Network (ANN) models, using combinations of variables such as Global Horizontal Irradiance (GHI), Global Extraterrestrial Irradiance (G₀), Temperature (T) and Relative Humidity (RH). Data provided by Satellite Application Facility on Climate Monitoring (CM SAF) are used to develop and train the models, while the models have been validated using field data from four stations located in Spain, covering the different study climates.According to the results, zones with different climate conditions need different models, both for the case of MR and ANN. The results show the need of including the GHI in all models in order to obtain accurate estimates; in fact, the presence of more variables only improves slightly the results in mediterranean climate, while in oceanic climate no improvement is observed.On the other hand, comparing MR and ANN models, ANN models did not show better results than those of MR models in no one of the cases studied. Regarding the climate, both types of models are clearly better for the mediterranean case than for the oceanic one. In order to improve the performance of the model for oceanic climate a correction based on the site adaptation technique was carried out. The good results obtained by this technique fully justify its use.The best proposed models provide better performance than other models which are restricted to certain locations. Besides, the clustering technique based on the PAR variable, used in this work, allows obtaining useful models for a whole region. Finally, another advantage of this methodology is that there is no need of ground measurements for its development, except for the site adaptation technique.