P-ε-N曲线拟合法

给出一种描述P－ε－N曲线的方法──三参数幂函数拟合法。该方法可以使P－ε－N曲线试验数据在双对数函数坐标系lgN-lg（ε-ε0）中最大限度地呈现线性关系，因而具有较小的均方差，而且解反映出P－ε－N曲线的变化趋势。对于应变-寿命关系也具有可逆性，因而可以方便地进行应变疲劳可靠性计算。     

近室温磁制冷工质选择的热力学准则

对近年来在制冷界研究相当活跃的磁制冷的工质，尤其是近室温磁制冷的工质－铁磁材料，在外加磁场中的热力学特性进行了分析、讨论，并在此基础上总结了选取近室温磁制冷工质的理论依据和原则，使实际中的选择工作有了针对性，减少了盲目性。     

航天器宽带随机振动响应分析

简要概述了航天器宽带随机振动试验和分析的必要性以及国内外预示技术的发展与现状；然后以某卫星为例，利用有限元方法和统计能量分析（SEA）对整星的宽带随机振动学环境进行了预示，经过与试验结果的对比，验证了上述方法的可行性。     

ACTIVE VIBRATION CONTROL OF A CANTILEVER BEAM USING PIEZOELECTRIC SENSORS AND ACTUATORS

讨论了利用压电片作为传感器和驱动器对悬臂梁进行主动振动控制问题，针对模态频率差距较大的系统，提出了分组建模和控制的方法。使用滤波器消除观测溢出。文中还讨论了传感器／驱动器配置问题。实验结果验证了所述方法的有效性。     

Event-triggered adaptive fuzzy attitude takeover control of spacecraft

The problem of attitude takeover control of spacecraft by using cellular satellites with limited communication, actuator faults and input saturation is investigated. In order to lighten the communication burden of cellular satellites, an event-triggered control strategy is adopted. The filtered attitude information needs to be transmitted only when the defined measurement error reaches the event-triggered threshold in this strategy. Then, to deal with the unknown inertia matrix, actuator faults, external disturbances and the errors caused by event-triggered scheme, fuzzy logic systems is introduced to estimate the uncertainties directly. Combining fuzzy logic control strategy and the event-triggered method, the first event-triggered adaptive fuzzy control law is developed. Then, torque saturation of cellular satellites is further considered in the second control law, where the upper bound of the uncertainties is estimated by fuzzy logic systems. The resulting closed-loop systems under the two control laws are guaranteed to be bounded. Finally, the effectiveness of two proposed control laws is verified by the numerical simulations.     

An engineering model of Titan surface winds for Dragonfly landed operations

Winds near the ground on Titan for the Dragonfly landing site (near Selk crater, 10°N) for the mid-2030s (Titan late southern summer, L_s ~ 310°) are estimated for mission design purposes. Prevailing winds due to the global circulation are typically 0.5 m/s, and do not exceed 1 m/s. Local terrain-induced flows such as slope winds appear to be similarly capped at 1 m/s. At various landing sites and times, these two contributions will vectorially combine to yield steady winds (for part of a Titan day, Tsol) of up to 2.0 m/s, but typically less – the slope wind component will be small in the mid-morning. In early afternoon, as on Earth and Mars, solar-driven convection in the planetary boundary layer will cause wind fluctuations of the order of 0.1 m/s, varying with a typical timescale of ~1000 s. Occasionally this convection organizes into coherent ‘dust devil’ vortices: detectable vortices with speeds of 1 m/s are predicted about once per Titan day. We have introduced the convective velocity scale combined with the advection time of PBL cells as a metric to derive the frequency of occurrence of gusts associated with convective vortices (‘dust devils’). Maximum possible vortex winds on Titan of 2.8 m/s may be expected only once per 40 Tsols, and define the maximum wind (4.8 m/s at 10 m height) that Dragonfly must tolerate without damage. The applicability of different wind combinations, scaled to the height of relevant Dragonfly components above the ground (e.g. the maximum corresponds to 3.9 m/s at 1.3 m height) by a logarithmic wind profile, to Dragonfly design and operations are discussed.     

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。     

结构吸波材料多层阻抗渐变设计及应用

对多层阻抗渐变的吸波结构设计思想进行了分析,介绍了多层阻抗渐变思想在吸波层板和泡沫两类结构吸波材料设计上的应用。理论计算与试验验证结果均表明,采用多层阻抗渐变设计能够使吸波层板和泡沫的吸波带宽向低频拓展,同时显著提高吸波泡沫的吸收强度。具有三个阻抗渐变吸收层的4 mm厚吸波层板在5~18 GHz频段反射率小于-10 d B;具有六个阻抗渐变吸收层的22 mm厚吸波泡沫在2~18 GHz频段反射率小于-10 d B,其中在6~18 GHz频段反射率小于-20 d B,8~12 GHz频段反射率小于-30 d B。多层阻抗渐变设计是提高结构吸波材料吸波性能的有效手段。     

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.