超磁致伸缩材料作动器的研制及特性分析

 采用自制的TbDyFe超磁致伸缩材料设计并制作了主动振动控制用超磁致伸缩作动器 ,并对其偏置磁场、激励磁场、静态特性、动态特性和主动控制减振效果进行了测试和分析。研究结果表明 ,作动器工作应变在TbDyFe材料的线性区 ,其总伸缩量可达 70 μm。低频动态特性好 ,谐频影响小。在自适应滤波控制方式下使用该作动器对正弦振动进行主动控制减振 ,减振效果达到 30dB。磁场均匀性对作动器输出特性有明显影响 ,采用Ansys有限元软件精确设计作动器激励磁场 ,可提高超磁致伸缩材料沿轴向磁场均匀性。     

Aerosols on the Giant Planets and Titan

On the giant planets and Titan, like on the terrestrial planets, aerosols play an important part in the physico-chemistry of the upper atmosphere (P ≤ 0.5 bar). Above all, aerosols significantly affect radiative transfer processes, mainly through light scattering, thus influencing the atmospheric energy budget and dynamics. Because there is usually significant coupling between atmospheric circulation and haze production, aerosols may constitute useful tracers of atmospheric dynamics.More generally, since their production is directly linked to some kind of energy deposition, their study may also provide clues to external sources of energy as well as their variability. Finally, aerosols indirectly influence other processes such as cloud formation and disequilibrium chemistry, by acting either as condensation nuclei or as reaction sites for surface chemistry. Here, I present a review of observational and modeling results based on remote sensing data, and also some insights derived from laboratory simulations. Despite our knowledge of the effects of aerosols in outer planetary atmospheres, however, relatively little is understood about the pathways which produce them, either endogenously (as end-products of gas-phase photochemical or shock reactions) or exogenously (as residues of meteroid ablation).     

微磁强计弱磁处理芯片设计与实现

为适应微纳卫星平台的应用需求、实现磁强计的微型化,针对巨磁阻抗(GMI)效应微磁强计的研制需求设计并研制了弱磁信号处理芯片.在分析GMI微磁强计构造的基础上,针对单机(微)小型化提出了弱磁信号处理电路芯片化的方案;结合空间应用特点,设计并实现了基于SOI CMOS工艺的弱磁信号处理芯片.实测结果表明:基于所研制的弱磁信号处理芯片不仅实现了磁强计的微型化、集成化,而且具有良好的弱磁测量性能.     

射流伺服阀用放大型超磁致伸缩执行器建模及分析

为提高射流伺服阀的动态性能,设计了采用桥式微位移放大机构的射流伺服阀用放大型超磁致伸缩执行器(AGMA)。建立了计输入位移损失的放大机构模型以及非线性位移输出理论模型,并采用有限元法对所建放大机构模型进行了对比验证,结果表明:放大机构的输入刚度模型最大误差0.78N/μm,放大倍数模型最大误差0.22,放大倍数受输入位移影响较小。最后,试验研究了AGMA的静动态特性,结果显示:控制电流在-0.5A到0.5A缓慢变化时,AGMA输出位移约为78μm;当控制电流从-0.5A跃变到0.5A时,其峰值位移约为71μm,峰值时间约为0.014s,调节时间小于0.1s;当控制电流幅值为0.5A时,其输出位移幅频宽40Hz,谐振频率约为30Hz。     

Coupled Clouds and Chemistry of the Giant Planets— A Case for Multiprobes

In seeking to understand the formation of the giant planets and the origin of their atmospheres, the heavy element abundance in well-mixed atmosphere is key. However, clouds come in the way. Thus, composition and condensation are intimately intertwined with the mystery of planetary formation and atmospheric origin. Clouds also provide important clues to dynamical processes in the atmosphere. In this chapter we discuss the thermochemical processes that determine the composition, structure, and characteristics of the Jovian clouds. We also discuss the significance of clouds in the big picture of the formation of giant planets and their atmospheres. We recommend multiprobes at all four giant planets in order to break new ground.     

小行星探测科学目标进展与展望

由于较好地保留了太阳系早期形成和演化历史的遗迹,小行星,尤其是近地小行星,已成为国际深空探测领域的研究热点。介绍了小行星的定义、分类和主要探测方式,指出目前小行星探测已进入空间探测的新时代;总结了国际小行星探测的现状,包括已实施和正在实施的小行星探测任务的科学目标、科学载荷配置,以及获取的主要科学数据等;探讨了未来小行星探测的发展趋势和主要科学问题,并对我国未来自主小行星探测任务科学目标的制定进行了展望。     

柔性铰链放大式超磁致伸缩致动器磁弹耦合模型

针对超磁致伸缩致动器(GMA)输出位移有限的问题,采用柔性铰链放大机构放大GMA输出位移,利用材料力学理论、拉格朗日动力学方程和有限元法对柔性铰链放大机构的位移放大倍数、动力学特性进行了分析.结合Jiles-Atherton(J-A)模型和二次畴转模型建立了柔性铰链放大式GMA的磁弹耦合模型,并在软件AMESim&Simulink联合仿真环境中进行了数值仿真.制作了柔性铰链放大式GMA样机,对其进行了动态性能实验,仿真和实验表明:经过放大,柔性铰链放大式GMA输出位移可以达到0.4mm;频带宽超过100Hz;所建立的磁弹耦合模型是有效的.      

超磁致伸缩作动器小回线动态J-A模型

超磁致伸缩作动器（GMA）输入输出之间存在着磁滞非线性关系,当研究其中高频输出特性时,为了降低材料自身迟滞非线性特性的影响,往往选用零点与饱和状态之间线性度较好的不饱和小回线,因此很有必要开展动态不饱和小回线数学模型的研究。首先在综合研究磁致伸缩材料（GMM）和GMA结构动力学特性的基础上结合安培环路定理提出以励磁电流为输入、应变为输出的动态Jiles-Atherton（J-A）模型,然后在引入磁滞回线特性变量的基础上得出J-A模型关键模型参数对其特性的影响规律,根据不饱和小回线仿真与实验波形的偏离特性提出模型参数的修正方法得到不饱和小回线动态J-A模型。最后,在不同频率和不同饱和幅值下通过实验验证该数学模型的正确性。      

Interstellar planetary protection

In the coming decades the detection of Earth-like extrasolar planets, either apparently lifeless or exhibiting spectral signatures of life, will encourage design studies for craft to visit them. These missions will require the elaboration of an interstellar planetary protection protocol. Given a specific dose required to sterilize microorganisms on a spacecraft, a critical mean velocity can be determined below which a craft becomes self-sterilizing. This velocity is calculated to be below velocities previously projected for interstellar missions, suggesting that an active sterilization protocol prior to launch might be required. Given uncertainties in the surface conditions of a destination extrasolar planet, particularly at microscopic scales, the potential for unknown biochemistries and biologies elsewhere, or the possible inoculation of a lifeless planet that is habitable, then both lander and orbiter interstellar missions should be completely free of all viable organisms, necessitating a planetary protection approach applied to orbiters and landers bound for star systems with unknown local conditions for habitability. I discuss the case of existing craft on interstellar trajectories – Pioneer 10, 11 and Voyager 1 and 2.