太空中的PM2.5——太阳系尘埃动力学研究进展

对太阳系尘埃动力学所涉及到的基本内容进行概述，包括尘埃的种类、成分、尺寸、密度、形状和生命周期。介绍了近年来在尘埃的来源与生成机制方面的力学过程、主要理论、模型与方法，包括冲击溅射、表面喷射、风化、滑坡、质量脱落、旋转断裂等，阐述了尘埃的充电过程与磁场环境，简要概述了航天任务的尘埃探测结果，介绍了尘埃受力模型、单个尘埃颗粒的运动以及大量尘埃的分布特征、动力学现象及内在规律方面的最新研究结论。最后对太阳系尘埃动力学领域的未来发展趋势进行了展望。     

A novel SETI strategy targeting the solar focal regions of the most nearby stars

Many hypotheses have been raised to explain the famous Fermi paradox. One of them is that self-replicating probes could have explored the whole Galaxy, including our Solar System, and that they are still to be detected. In this scenario, it is proposed here that probes from neighboring stellar systems could use the stars they orbit as gravitational lenses to communicate efficiently with each other. Under this hypothesis, a novel SETI approach would be to monitor the solar focal regions of the most nearby stars to search for communication devices. The envisioned devices are probably not detectable by imagery or stellar occultation, but an intensive multi-spectral monitoring campaign could possibly detect some communication leakages. Another and more direct option would be to message the focal regions of nearby stars in an attempt to initiate a reaction.     

Relaying Selection with Network-coded Cooperative Protocols in Aeronautical Communications

In this article, we exploit the idea of network-coded cooperative protocol in aeronautical communications which combines different source nodes'information at the relay and joint decoding at the destination. Recently, the network coding in cooperative communications has been categorized into two mainstreams, bit-level and signal-level combinations, which are both discussed in the article. And to be exclusively, multiple access relay channel(MARC) is adopted. The mutual information expressions of both above-cited network-coded protocols are deduced, which prove that without proper selected relays to perform network coding, the spatial diversity of the proposed protocol cannot be obtained. This then leads to search for the selection and grouping algorithms. An adjacency matrix is defined to describe the connectivity of the nodes in one radio contact disk, so that, the selection and grouping of algorithm is equivalent to constructing this adjacency matrix to minimize the system outage probability evaluated in term of the mutual information. Besides, a network-coded cooperative protocol requires the acyclic network, of which the construction is to avoid loop-4 in the matrix. The article ends with simulations to demonstrate the viability of the proposed algorithms.     

多辐射器航天器热控流体回路布局的(火积)耗散分析

为了优化多辐射器航天器热控流体回路布局，提高流体回路的散热效率，降低流体回路温度，本文基于(火积)理论，分别对多个辐射器串联和并联的流体回路布局的散热进行了分析。结果表明，排散相同热量时，流体回路的流体与管路壁面之间的温差均匀性越好，流体回路散热过程(火积)耗散越小，系统散热过程越优。进一步，对于2个辐射器的情况，分别对辐射器设置了不同的空间辐射加热热流，对辐射器的流体回路布局方式进行了比较。结果表明，辐射器与流体回路串联时，系统散热性能要优于两者并联，系统的流体温度水平最低，结果与(火积)理论分析的预测完全一致。研究结论对多辐射器的航天器热控流体回路设计具有指导意义。     

A new modeling method of solar energetic proton events for ISO specification

Solar energetic protons degrade performance and reliability of spacecraft systems due to single-event effects, total dose effects and displacement damage in electronics components including solar cells. On designing a solar cell panel, a total fluence of solar energetic protons (SEPs) which cause solar cell damage is needed to estimate power loss of the solar cells over mission life. Nowadays a solar panel area of spacecraft is increasing as spacecraft mission life becomes longer (15–18 years). Thus an accurate SEP model is strongly required for the cost-minimum design from the aerospace industry. The SEP model, JPL-91 proposed by Feynman et al., is currently used widely for solar cell designing. However, it is known that the JPL-91 model predicts higher fluences of protons than values actually experienced in space, especially after 7 years on orbit. In addition, the model is based on several assumptions, and also needs Monte-Carlo simulations for calculating fluences. In this study, we propose a new method for modeling SEPs especially focused on solar cell degradation. The newly-proposed method is empirical, which constructs a model based directly upon proton flux measurement data taken by instruments onboard spacecraft. This method has neither assumptions nor dependence on SEP event selection, both of which are needed in JPL-91. The model fluences derived from this method show lower fluences in longer missions compared to JPL-91. This method has been proposed to ISO (International Organization for Standardization) and has been discussed for a new standard SEP model.     

基于可观测度分析和模型预测的空间自标定方法

光纤陀螺以其优点适合空间飞行器定姿要求,但长期在轨飞行必须对光纤陀螺进行自标定。通常采用高维复杂陀螺模型计算实时性误差,而采用舍去状态量的降维模型影响系统定姿精度。针对这一问题,通过星敏感器观测,对高维陀螺模型进行可观测度分析,提出了一种基于模型预测的降维模型,将可观测度较低的状态作为模型误差进行预测估计,保证了系统精度并大大减小了计算量。半物理仿真结果表明此算法精度略高于高维模型自标定方法,计算量仅为高维模型的1/10,显著提高了系统的实时性。     

VHF地空数据链网关信息处理模式分析

VHF数据链网关信息处理模式直接影响系统的实时性,采用排队论模型详细分析了两种信息处理模式对系统实时性的影响,进行了计算机仿真,通过分析仿真结果,得到了适合的信息处理模式。     

卫星多波束天线赋形波束的最优化计算

主要介绍了卫星多波束天线的基本原理和数学模型 ;说明了卫星多波束天线赋形问题的本质是一个优化问题 ;用两种可行有效的优化方法——最小 p乘法和最小最大法分别对矩形区域和中国本土进行了赋形 ,并在最后分析了两种算法的优缺点     

剩余推进剂排放系统研究

论述中国首枚上面级火箭剩余推进剂排放方案论证 ,排放系统方案选择 ;提出中国专用排放系统方案 ,排放系统设计、研制与试验研究的全过程 ,为解决中国长征型号上面级火箭高空爆炸解体问题提供了技术基础     

IPX实时通信软件的设计与实现

分析了基于IPX(Internetwork Packet eXchange)协议的实时通信编程原理,讨论了针对某网络所开发的实时通信软件IPXSR的设计思想、特点、实现技术和调用方法.目前该软件已经通过了验收和鉴定,在实际系统中得到应用,效果良好.并能够方便地移植到其他的物理网络系统中,具有较大的实用价值.