基于特征的雷达信号环境仿真

通过分析装备的试验需求,解析雷达信号环境的特征,提出了具有针对性、适应性、可扩展性和层次化的雷达信号环境仿真策略。对实践应用具有较强的参考性。     

论航天器的综合环境试验

讨论了在航天器研制中综合环境试验的重要性和必要性,简单介绍了航天器研制中的各种综合环境试验,对如何设计和应用综合环境试验提出了一些看法。     

光纤光栅温度传感器研究进展

归纳了以光纤光栅为基础的温度传感器的研究现状,总结了这些温度传感器的基本原理,再现了它们的主要结构,展示了原文提到的实验过程和数据分析结果,并对这些传感器的优点和不足进行了分析,提出了部分改进方案。通过研究发现：光纤光栅温度传感器具有优良的特性,能够在恶劣环境下测量极高的温度,具有广阔的应用前景。     

末端能量管理段迭代校正轨道算法研究

针对航天器进入末端能量管理段接口处时位置和航迹偏角存在大范围摄动的问题，提出一种使用迭代校正法的轨道快速生成算法。该算法可以根据航天器的具体初始状态，自动选择直接进场或者间接进场策略，快速生成可行的参考轨迹。首先通过跟踪轨迹地面投影实现侧向制导；根据末端能量管理段的起始点与终点的高度与速度约束生成参考动压-高度剖面，并跟踪此剖面实现纵向制导。然后采用迭代校正计算快速确定航向校准柱的位置与最终半径两个参数用以调整航程，保证航天器在末端的所有状态满足自动着陆段接口的边界约束。仿真结果校验了该算法可以根据航天器的具体状态快速生成符合约束条件的末端能量管理段飞行轨道，具有很好的鲁棒控制性能。     

基于工作过程的《制冷技术》课程教学设计

根据高等职业教育新的课程理念,对《制冷技术》课程的教学进行了改革。基于对实际工作过程的分析和思考,设计了学习情境,重构了课程内容,以学生为主体组织实施教学,创新了考核方法,有效地提高了教学效果。     

Characterization of the near Earth radiation environment by Liulin type spectrometers

Comprehensive study of the dose, flux and deposited energy spectra shape data obtained by Liulin type spectrometers on spacecraft (five different experiments) and aircraft since 2001 is performed with the aim of understanding how well these parameters can characterize the type of predominant particles and their energy in the near Earth radiation environment. Three different methods for characterisation of the incoming radiation from Liulin spectrometers are described. The results revealed that the most informative one is by the shape of the deposited energy spectra. Spectra generated by Galactic Cosmic Rays (GCR) protons and their secondaries are with linear falling shape in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra inside the South Atlantic Anomaly (SAA) region depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions these spectra are similar to the GCR spectra. Mixed radiation by protons and electrons and/or bremsstrahlung is characterized by spectra with 2 maxima. All type of spectra has a knee close to 6.2 MeV deposited energy, which correspond to the stopping energy of protons in the detector. Dose to flux ratio known also as specific dose is another high information parameter, which is given by experimentally obtained formulae [Heffner, J. Nuclear radiation and safety in space. M. Atomizdat. 115, 1971 (in Russian)] connecting the dose to flux ratio and the incident energy of the particles.     

浅谈银行信贷资产债权维护的配套设置

本文主要从强化商业银行内控、建立信贷资产债权保全机制、营造诚实信用环境三方面论述维护银行信贷资产债权的配套措施。     

全面视角下“法律面前人人平等原则”的探讨

本文以全面视角审视了法律面前人人平等是什么，并就我们为什么需要法律面前人人平等原则，以及如何实现法律面前人人平等等问题进行了探讨。     

Thermo-mechanical design and testing of a microbalance for space applications

This work focuses on the thermo-mechanical design of the microbalance used for the VISTA (Volatile In Situ Thermogravimetry Analyzer) sensor. VISTA has been designed to operate in situ in different space environments (asteroids, Mars, icy satellites). In this paper we focus on its application on Mars, where the expected environmental conditions are the most challenging for the thermo-mechanical design.     

Optimal steering law of refractive sail

The interaction between electromagnetic waves and matter is the working principle of a photon-propelled spacecraft, which extracts momentum from the solar radiation to obtain a propulsive acceleration. An example is offered by solar sails, which use a thin membrane to reflect the impinging photons. The solar radiation momentum may actually be transferred to matter by means of various optical phenomena, such as absorption, emission, or refraction. This paper deals with the novel concept of a refractive sail, through which the Sun’s light is refracted by crossing a film made of polymeric micro-prisms. The main feature of a refractive sail is to give a large transverse component of thrust even when the sail nominal plane is orthogonal to the Sun-spacecraft line. Starting from the recent literature results, this paper proposes a semi-analytical thrust model that estimates the characteristics of the propulsive acceleration vector as a function of the sail attitude angles. Such a mathematical model is then used to analyze a simplified Earth-Mars and Earth-Venus interplanetary transfer within an optimal framework.