谐振式陀螺全角模式误差来源与接口技术

全角模式是谐振式陀螺的新型接口技术，具有直接测量角度、动态范围大的优点，但其对陀螺元器件对称性要求极高的缺点限制了它的实际应用。首先，从谐振式陀螺全角模式的原理出发，讨论了各种不理想因素对全角模式运行造成的问题。然后，从器件设计和控制系统两方面出发，讨论了可行的技术路线。最后，通过数值仿真的方法证明了理论分析的正确性，并给出了谐振式陀螺的选型和控制系统的建议。     

The impact of different background errors in the assimilation of satellite radiances and in-situ observational data using WRFDA for three rainfall events over Iran

Satellite radiances and in-situ observations are assimilated through Weather Research and Forecasting Data Assimilation (WRFDA) system into Advanced Research WRF (ARW) model over Iran and its neighboring area. Domain specific background error based on x and y components of wind speed (UV) control variables is calculated for WRFDA system and some sensitivity experiments are carried out to compare the impact of global background error and the domain specific background errors, both on the precipitation and 2-m temperature forecasts over Iran. Three precipitation events that occurred over the country during January, September and October 2014 are simulated in three different experiments and the results for precipitation and 2-m temperature are verified against the verifying surface observations. Results show that using domain specific background error improves 2-m temperature and 24-h accumulated precipitation forecasts consistently, while global background error may even degrade the forecasts compared to the experiments without data assimilation. The improvement in 2-m temperature is more evident during the first forecast hours and decreases significantly as the forecast length increases.     

ITRS/GCRS transformation: Uncertainty propagation analysis and short-term modelling of IAU 2006/2000A developments

A study of the uncertainty propagation in ITRS/GCRS transformation is presented in this work. General law of propagation of variances is applied to the ITRS/GCRS transformation matrix, deriving the analytical expressions to compute GCRS position uncertainty. This evaluation is based on EOP uncertainties provided by IERS long-term series and formal uncertainties of ITRS-compatible coordinates. Numerical results for the period 1998–2016 are shown and discussed for ITRS positions in different altitudes and latitudes, providing graphical and numerical insights of the mapping of EOP uncertainties to transformed coordinates.Eventually, an analysis of short-term evolution of the Celestial Intermediate Pole coordinates in the GCRS provided by the IAU2006/2000A precession-nutation model is carried out, in order to assess the feasibility to potentially broadcast these parameters in GNSS navigation message. This approach would facilitate the dissemination of terrestrial-celestial transformation parameters for real time users, given that polar motion and UT1-UTC are already foreseen in GPS interface specification. The results presented in this work confirm the feasibility of this idea.     

Exploration life support technology challenges for the Crew Exploration Vehicle and future human missions

As NASA implements the U.S. Space Exploration Policy, life support systems must be provided for an expanding sequence of exploration missions. NASA has implemented effective life support for Apollo, the Space Shuttle, and the International Space Station (ISS) and continues to develop advanced systems. This paper provides an overview of life support requirements, previously implemented systems, and new technologies being developed by the Exploration Life Support Project for the Orion Crew Exploration Vehicle (CEV) and Lunar Outpost and future Mars missions. The two contrasting practical approaches to providing space life support are (1) open loop direct supply of atmosphere, water, and food, and (2) physicochemical regeneration of air and water with direct supply of food. Open loop direct supply of air and water is cost effective for short missions, but recycling oxygen and water saves costly launch mass on longer missions. Because of the short CEV mission durations, the CEV life support system will be open loop as in Apollo and Space Shuttle. New life support technologies for CEV that address identified shortcomings of existing systems are discussed. Because both ISS and Lunar Outpost have a planned 10-year operational life, the Lunar Outpost life support system should be regenerative like that for ISS and it could utilize technologies similar to ISS. The Lunar Outpost life support system, however, should be extensively redesigned to reduce mass, power, and volume, to improve reliability and incorporate lessons learned, and to take advantage of technology advances over the last 20 years. The Lunar Outpost design could also take advantage of partial gravity and lunar resources.     

基于协议变换的图像采集系统设计

介绍了一个基于高速协议变换的实时图像采集系统,该系统实现了从IEEE1394协议到千兆以太网协议的实时变换,将基于IEEE 1394协议的数字相机发出的图像数据转发到以太网上.系统设计使用了SOPC(System On a Programmable Chip)技术,通过Avalon总线将Nios Ⅱ处理器,千兆网MAC核和自定义的1394芯片接口逻辑等IP组件连接在一起形成主要的硬件电路,结合系统软件设计实现了对高速图像数据的实时转发.系统达到了较好的性能,同时具有集成度高,结构简单和扩展性好的特点,展示了利用SOPC技术解决此类问题的优势.     

目标跟踪多智能体一致控制

研究了二阶多智能体系统跟踪一致问题。针对相对速度信息未知的网络,分析了有时滞和无时滞情况下网络的稳定性,给出了系统能够实现跟踪一致的条件。最后,通过仿真表明所提协议比现有协议性能更好。     

连续短线段空间圆弧转接与插补

针对连续短线段高速加工控制需求,研究了利用空间圆弧转接实现高速插补的方法。建立了圆弧转接数学模型,研究了转接的几何约束和运动约束、转接参数计算、空间圆弧插补等相关理论与算法,并详细分析了算法的使用范围、效率制约因素和计算量等工程实现相关问题。仿真和加工实验表明:该转接算法能显著提高加工效率,减小振动,改善工件表面质量。作为空间圆弧转接算法基础的空间圆弧插补算法对空间任意平面内圆弧插补具有实用价值。本文所有算法已经在自主研发的数控平台上进行了验证,应用效果良好。     

Ⅱ型PIO反馈与前馈抑制系统对比

 当舵机速率限制饱和时会产生附加时延,恶化飞行品质,触发Ⅱ型驾驶员诱发振荡（PIO）。运用描述函数法研究速率限制反馈（RLF）和死区增稳（DASA）Ⅱ型PIO抑制系统的开环相位补偿能力,提出RLF抑制系统的参数优化选择方法,分析了DASA抑制系统中死区和滤波器参数对相位补偿能力的影响。研究了两型抑制系统对正弦与偏差输入信号的开环响应特点。建立了含速率限制器的人机系统数学模型,基于描述函数法探究了Ⅱ型PIO的产生机理,推导了抑制Ⅱ型PIO发生的公式,应用连续信号相位补偿法抑制Ⅱ型PIO的发生。对阶跃、离散和正弦3种易于诱发PIO现象的跟踪任务进行数值仿真,对比了两种抑制系统的Ⅱ型PIO抑制能力。结果表明,反馈型RLF抑制系统对Ⅱ型PIO的抑制能力强于前馈型DASA抑制系统,有效降低了Ⅱ型PIO发生的可能性。     

科氏质量流量计全数字闭环系统的设计与实现

科氏质量流量计(CMF,Coriolis Mass Flowmeter)全数字闭环系统,采用现场可编程门阵列(FPGA,Field Programmable Gate Array)和现代数字信号处理方法对CMF传感器进行稳定精确的闭环控制,实时性和精度较高.以高速并行器件FPGA为运算和控制核心,在相位控制中引入FIFO(First In First Out)组件,通过控制FIFO的读、写请求信号来改变时间差,实现对拾振和激励信号的相位差准确、稳定的控制;采用不连续和连续幅值控制相结合的非线性幅值控制方法,快速、准确地设定幅值,适应性强,实现对拾振信号幅值的良好控制,并控制拾振信号以稳定的幅值输出,提高CMF的测量精度和稳定性.实流标定对比实验结果表明:CMF数字闭环在零点稳定性、动态响应特性和重复性方面都优于模拟闭环,并在一定程度上提高了CMF的测量精度.      

基于我国VLBI网航天器定位归算仿真分析

结合我国VLBI观测网现状,通过仿真计算分析了观测时延噪声与系统差、预报轨道偏差和测距误差等对航天器定位归算的影响。结果表明,仅利用VLBI跟踪时附加飞行器地心距约束有利于压制定位点的弥散。 3站 VLBI跟踪的定位解是有偏估计,4站跟踪时要求所加约束的误差应与预报轨道偏差相当,若过大将起不到压制定位点弥散的良好效果,若过小则会在定位结果中引入系统偏差。时延与测距的观测噪声主要引起定位点序列的弥散。若观测量存在系统差则将引起定位结果的系统性偏差,而且定位点序列会发生渐近线性趋势跳变。同时,这也可以作为观测量是否存在系统差的判据。另外,若某时刻前后VLBI跟踪站存在3、4站变更,定位点序列有时发生趋势变化。分析结论对于我国后续探月和萤火计划等工程实践具有借鉴意义。