Simulation analysis for effects of bone loss on acceleration tolerance of human lumbar vertebra

The purpose of the present study was to analyze and predict the changes in acceleration tolerance of human vertebra as a result of bone loss caused by long-term space flight. A human L3–L4 vertebra FEM model was constructed, in which the cancellous bone was separated, and surrounding ligaments were also taken into account. The simulation results demonstrated that bone loss has more of an effect on the acceleration tolerance in x-direction. The results serve to aid in the creation of new acceleration tolerance standards, ensuring astronauts return home safely after long-term space flight. This study shows that more attention should be focused on the bone degradation of crew members and to create new protective designs for space capsules in the future.     

On the observability of Mars entry navigation using radiometric measurements

A thorough observability analysis of the Mars entry navigation using radiometric measurements from ground based beacons is performed. This analysis involves the evaluation of the Fisher information matrix which is derived from the maximum likelihood estimation. A series of navigation cases with multiple beacons are investigated, and both range and range-rate measurements are considered. The determinant of Fisher information matrix is used to quantify the observability of navigation system, while the trace of Fisher information matrix is used to determine the lower-bound of estimation errors. For one and two beacon cases, the navigation system is unobservable. However, the eigenvectors of Fisher information matrix give the observable and unobservable component. When three or more beacon measurements are employed, the states of entry vehicle become observable. Some valuable analytic conclusions on the relationship between the geometric configuration of beacons and observability are obtained consequently. Finally, simulation results from two navigation examples indicate that our effort is useful for understanding and assessing the observability of the Mars entry navigation using radiometric measurements.     

一种新型的微机补偿晶体振荡器及开发系统

提出了一种新型的以微处理器为核心的AT切温度补偿晶体振荡器 (MCXO)的设计思想 ,说明了其开发系统的原理 ,给出了最后的实验结果。使用该开发系统得到的这种振荡器可以工作在 - 40℃～ 85℃的环境内 ,频率—温度稳定性≤± 5× 10 - 7。     

基于FPGA的星载步进电机控制电路设计

针对航天设备在轨运行时间长、不易更换的特点,提出了一种力矩宽且范围可调的步进电机控制电路设计。该电路原理样机以Xilinx公司的XC3S400pq-208型FPGA为核心控制芯片,以LMD18200为步进电机驱动芯片。在对电路总体设计进行介绍的基础上,重点阐述了航天过程中步进电机阻力矩增加的问题,以及通过脉冲频率和PWM控制技术调节输出力矩的方法。试验结果表明,力矩可调范围的最大值能够使力矩裕度达到4,匹配步进电机在轨运行过程中的力矩要求。     

编队飞行卫星群构型保持及初始化

导出了基于相对轨道要素的编队飞行卫星群轨道相对运动控制的轨道机动方程；提出了编队飞行卫星群轨道相对运动控制的轨道机动控制策略，利用不同方向的脉冲控制相对运动的轨道参数，包括轨道平面内机动和轨道平面外机动控制。根据相对轨道要素的变轨机动控制，进行编队飞行卫星群构型的初始化。这样的构型初始化可以视作一次特殊的变轨机动控制，很容易实现编队飞行构型的初始化机动。     

半捷联式导引头视线转率提取算法

捷联式光学导引头的探测装置直接固联于弹体上,许多现有的制导信息处理方法都不再适用.对半捷联式导引头进行研究,根据其与常平架式与捷联式导引头不同的配置方式,推导了滚仰式和偏航俯仰式半捷联导引头视线转率提取算法,并分析了影响半捷联导引头视线转率提取精度的主要因素及误差传递关系,通过Simulink仿真验证了算法的正确性.      

高压脉冲电子束的控制及其对焊缝形貌影响

研制出一台150 kV/30 kW高压脉冲电子束焊机,介绍了控制脉冲束流产生的偏压脉冲电源拓扑电路结构及脉冲束流频率、占空比、束流基值、束流峰值的调节控制技术.在0~1 kHz频率范围内,该电源可输出最大幅值200 mA的脉冲电子束束流,且工艺参数调节方便.分别采用脉冲束流与连续束流电子束工艺焊接了1Cr18Ni9Ti奥氏体不锈钢,对不同工艺的焊缝形貌进行了对比分析.与连续束流电子束焊接工艺相比,采用脉冲电子束焊接工艺的焊缝熔深增加,深宽比增大;对于脉冲电子束焊接工艺,占空比给定时,随着束流频率增加,焊接缺陷减少.试验结果表明:脉冲束流频率、占空比是影响焊缝成形的关键工艺参数;脉冲调制方式控制偏压是获得高压脉冲电子束的理想控制技术之一.      

GPS在气象火箭遥测跟踪上的应用

利用GPS全球定位系统、天线云台和宽波瓣天线组成的跟踪系统, 研究了接收位置信息与跟踪之间的时间差, 气象火箭理论弹道误差导致的中断跟踪,气象火箭探空仪分离后至初次定位前的跟踪, 天线云台转到359°位置后反转359°及跟踪过程中跟踪中断后的继续跟踪等关键问题,成功实现了气象火箭探空仪的遥测跟踪. 该跟踪系统在子午工程气象火箭试验中得到较好的应用, 此种跟踪方式相比传统雷达跟踪方式具有体积小、重量轻、操作简单、成本低、机动性强、跟踪可靠性强等诸多优点.     

非接触检测大螺纹件的可行性

针对科研生产中大螺纹件检测费时费力、检测准确度不高的实际情况,提出以激光位移传感器作为非接触扫描测头,配以三坐标架框架及转台等附件,组建非接触检测大螺纹件的检测校准装置的方案。通过扫描螺纹牙型的实际轮廓,计算螺纹的综合参数,并与标准螺纹数据比对,判定螺纹的合格与否。同时,验证了该方法的可行性。     

Variations of ionospheric total electron content before three strong earthquakes in the Qinghai-Tibet region

We investigate the ionospheric total electron content (TEC) anomalies occurred in the Qinghai-Tibet region before three large earthquakes (M > 7.0). The temporal and spatial TEC variations were used to detect the ionospheric possible precursors of these earthquakes. We identified two TEC enhancements in the afternoon local time 9 days and 2–3 days before each earthquake, between which a TEC decrement occurred 3–6 days before earthquakes. These anomalies happened in the area of about 30° in latitude and the maximum is localized equatorward from the epicenters. These TEC anomalies can be found in all three earthquakes regardless the geomagnetic conditions. The features of these anomalies have something in common and may have differences from those caused by geomagnetic storms. Our results suggest that these ionospheric TEC perturbations may be precursors of the large earthquakes.