MEMS环形谐振陀螺闭环系统建模、仿真与参数分析

针对一款数字可配置的MEMS环形谐振陀螺,对陀螺表头和信号处理电路进行数学建模,推导陀螺检测系统指标参数与机电特性参数之间数学关系,为可配置ASIC电路提供理论支撑.通过对实测表头数据和理论模型数据进行对比分析,验证了模型的有效性与准确性.     

NASICON固体电解质SO2传感器的特性研究

采用溶胶-凝胶法合成NASICON固体电解质材料,并以其为基体材料制作管式SO2传感器,敏感电极采用Na2SO3-30?SO4或者Na2SO4-30?SO4(摩尔比)复合硫酸盐.SO2浓度在(10～100)×10-6体积分数范围内,两种器件的灵敏度分别为81.1和60.6mV/decade.敏感电极为Na2SO3-30?SO4的元件响应和恢复时间分别为28.2 s和57.7 s;敏感电极为Na2SO4-30?SO4的元件响应和恢复时间分别为39.8 s和67.4 s.     

Bow Shock and Upstream Phenomena at Mars

Mars Global Surveyor is the sixth spacecraft to return measurements of the Martian bow shock. The earlier missions were Mariner 4 (1964), Mars 2 and 3 (1972), Mars 5 (1975) and Phobos 2 (1989) (see reviews by Gringauz, 1981; Slavin and Holzer, 1982; Russell, 1985; Vaisberg, 1992a,b; Zakharov, 1992). Previous investigations of planetary bow shocks have established that their position, shape and jump conditions are functions of the upstream flow parameters and the nature of the solar wind — planet interaction (Spreiter and Stahara, 1980; Slavin et al., 1983; Russell, 1985). At Mars, however, the exact nature of the solar wind interaction was elusive due to the lack of low altitude plasma and magnetic field measurements (e.g., Axford, 1991). In fact our knowledge of the nature of the interaction of Mars with the solar wind was incomplete until the arrival of MGS and the acquisition of close-in magnetic field data (Acuña et al., 1998). As detailed by a series of review papers in this monograph, the Mars Global Surveyor (MGS) mission has now shown that the Mars environment is very complex with strong, highly structured crustal magnetic remnants in the southern hemisphere, while the northern hemisphere experiences the direct impingement of solar wind plasma. This review paper first presents a survey of the observations on the Martian bow shock and the upstream phenomena in the light of results from all the missions to date. It also discusses the kinetic properties of the Martian bow shock compared to the predictions of simulations studies. Then it examines the current status of understanding of these phenomena, including the possible sources of upstream low-frequency waves and the interpretations of localized disturbances in the upstream solar wind around Mars. Finally, it briefly discusses the open issues and questions that require further study.     

非平行边界层C型失稳的非线性演化(英文)

提出用抛物化稳定性方程(PSE)新方法,研究非平行边界层从层流向湍流转捩的C型失稳的演化过程,特别是非线性演化问题。研究了至关重要的初始条件,包括各扰动谐波的初始解、初始站均流变形的模拟、以及通过对线性 PSE 的求解获得 TS波和C型亚谐扰动的初始站值等。发展了高精度的数值方法,满足PSE的关键性正规化条件,实现非线性抛物化稳定性方程的有效求解和稳定推进。算例展示了Blasius边界层的C型失稳的非线性演化过程,与典型实验结果相吻合。     

火箭级间热分离初始阶段流场的数值模拟

针对多级火箭级间热分离这一复杂环境条件下的级间段流场进行了数值研究。计算采用AUSM 有限体积格式,针对相应的流场假设,分别求解了非定常轴对称和非定常三维Faver平均的Navier-Stokes方程。两种计算结果的比较表明,由级间排气口的分布而引起的三维效应主要集中在喷管与火箭外壳所围成的空腔内部,而喷管内部由于流速很高,排气口带来的三维效应对管内上游流动影响很小。计算结果可为级间分离段和发动机热防护的设计提供参考。     

逆序法在日语声调标示中的应用

随着日语声调研究的不断深入,声调标示法系统已成为日语声调教学的有效手段。声调标示法具有一种特殊性,那就是它必须同时具备抽象性和形象性。在探讨正序声调标示法局限性的基础上,提出应该重视逆序声调标示法。其次,针对目前逆序声调标示法还未建立起形象性图形的现状,尝试建立与逆序声调标示法相对应的简洁明快的日语声调模型。     

辅助工程师设计的知识融合设计方法:卫星舱布局设计(英文)

卫星舱布局设计属工程系统设计问题,为用传统计算方法难以解决的问题,该问题具有三重难度:工程复杂性、计算复杂性和达到工程实用难。卫星布局设计师的成功经验表明,它需要依赖设计师的经验和智慧、借鉴先验知识和辅以"计算"进行设计,并实现人机结合。本文的人机结合方法采用在线人知识、在线计算知识和先验知识(如参考布局施工图)的知识融合方法,并在卫星布局CAD、仿真与评价系统平台上实现,发挥人机各自特长。主要研究:(1)设计知识:包括在线人知识、在线计算知识和先验知识的表达;(2)上述3类知识的广义描述模型及其知识融合方法;(3)人的作用。经以简化的国际通信卫星舱布局设计为例的数值实验验证,表明了本文方法的可行性。     

高速飞行器非视距短波通信的可行性验证飞行试验

当高速飞行器处于失稳失控等紧急情况时，现有航天器测控方法可能面临地面站天线无法及时跟踪和对准飞行器的问题，这将导致测控通信链路的中断，无法传输紧急的安控遥控指令。为了在飞行器失稳失控、非视距通信时与地面站维持通信，提出将短波通信应用于高速飞行器测控通信系统的应急通信，并进行非视距短波通信的飞行试验以验证方法的可行性。在试验中，地面站发射7 MHz的短波信号，高速飞行器内部安装的交流磁场计用于接收短波信号，获得了短波的磁场强度与飞行环境的本底噪声。试验结果表明，随着飞行器海拔的增加，磁场强度减小，高速飞行器始终能在非视距和天线不对准的情况下接收到短波信号，证实了短波应用于高速飞行器应急通信的可行性。试验是进一步验证高速飞行器在远距离、超视距以及拒止环境下应急通信的技术基础，同时，也为高速飞行器短波通信系统的研制提供重要的数据支撑。     

基于改进遗传算法的星图畸变校正方法

由于光学成像系统的非线性几何畸变,使得星敏感器所获星图与理想星图有一定的差别,为完成高精度定姿,必须对畸变星图进行校正.首先,介绍了光学系统的畸变原理,并建立了以径向几何畸变为主的星图畸变模型.之后引入改进遗传算法对畸变参数进行了优化:采用引进成长算子的二进制编码,避免了算法陷入伪极值;通过改进适应度函数和适时调整变异...     

Corrosion Properties of Light-weight and High-strength 2195 Al-Li Alloy

The intergranular corrosion and exfoliation corrosion of 2195 Al-Li alloy treated by multi-step heating-rate controlled aging (MSRC) are studied. The corrosion features of 2195 Al-Li alloys which are respectively treated by high-temperature nucleation MSRC (H-M) and low-temperature nucleation MSRC (L-M) are contrasted. And the corrosion mechanism of 2195 Al-Li alloy is also discussed from the viewpoint of microstructure (types, distribution, etc.) of the strengthening phase. The results show that 2195 Al-Li alloy after H-M is more susceptible to intergranular corrosion and exfoliation corrosion than that of alloy after L-M. The degree of intergranular corrosion increases with the increase of predeformation amount and the surface parallel to the rolling direction is more prone to exfoliation corrosion. The main reason of intergranular corrosion and exfoliation corrosion is the for-mation of corrosion galvanic couples among T1 phase, ?θ’ phase and grain boundary precipitate-free zones (PFZ).