排序方式: 共有133条查询结果,搜索用时 250 毫秒
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1.构造及其原始数据 滑轨舱门收放机构由中、侧滑轨、三角支架、外伸臂、链条条、链轮、液压马达及减速装置等组成(图1)。一根中滑轨布置在43框前飞机对称平面内与飞机外形的下零纵线相贴合,两根侧滑轨分别布置在43框后机身的两侧,舱门的前端由一个接头铰支在三角支架上,三角支架的前支点与链条相连,舱门的后部和两个外伸臂固接, 相似文献
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近年来,针对弱信号的高灵敏度接收机已逐渐成为国内外的研究热点。加长相干积分时间可以提高信噪比,从而跟踪到更弱的信号。但是,北斗导航接收机跟踪环路并不可以无限加长相干积分时间,相干积分时间的长短和功效还受到卫星导航电文比特跳变的限制。为了消除导航电文比特跳变对相干积分的影响,提出了一种改进的基于最大似然估计的北斗信号位同步方法,完成位同步后再利用先猜后检的方法便可以实现长相干积分。利用软件接收机进行编程设计,仿真结果表明:该长相干积分算法能够稳定可靠地实现对弱信号的跟踪,20ms相干积分环路信噪比约提升12dB,40ms相干积分环路信噪比约提升15dB,80ms相干积分环路信噪比约提升17dB,提高了北斗导航接收机的灵敏度。 相似文献
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基于叶片非接触式动应变重构理论,开展动应变重构不确定性量化方法研究。基于方差合成定理建立重构叶片动应变不确定性量化分析模型;以模拟转子叶片为研究对象,开展旋转叶片叶端定时试验,利用周向傅里叶算法获取不同叶端定时传感器布局下的测点振幅,通过最大熵方法拟合振幅分布概率密度函数,确定叶端定时测振的不确定性参数;结合Kriging代理模型和试验共振频率数据对叶片有限元模型进行修正,获取关键测点位移-应变转换因子,并获取考虑共振转速以及测点位置不确定性的转换因子不确定性参数;获取重构动应变的均值、标准不确定度和包含区间,与应变片测量数据作对比。结果表明,除5号叶片A测点外,测量动应变均位于重构动应变的95%置信度下的包含区间内,且所有叶片的应变片测点动应变重构误差不超过15%。 相似文献
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L. Zampieri C. Germanà C. Barbieri G. Naletto A. Čadež I. Capraro A. Di Paola C. Facchinetti T. Occhipinti D. Ponikvar E. Verroi P. Zoccarato 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We are developing fast photon-counter instruments to study the rapid variability of astrophysical sources by time tagging photon arrival times with unprecedented accuracy, making use of a Rubidium clock and GPS receiver. The first realization of such optical photon-counters, dubbed AquEYE (the Asiago Quantum Eye), was mounted in 2008 at the 182 cm Copernicus Observatory in Asiago. AquEYE observed the Crab pulsar several times and collected data of extraordinary quality that allowed us to perform accurate optical timing of the Crab pulsar and to study the pulse shape stability on a timescale from days to years with an excellent definition. Our results reinforce the evidence for decadal stability of the inclination angle between the spin and magnetic axis of the Crab pulsar. Future realizations of our instrument will make use of the Galileo Global Navigation Satellite System (GNSS) time signal. 相似文献
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实现了一款具有通用性的Turbo码编译码器,对CCSDS(Consultative Committee for Space Data Systems)规范中的信息数据帧长度进行扩展,不仅支持原有的5种帧长,而且能实现16384bit内255bit的任意整数倍帧长的信息序列的编译码.针对标准外的编码参数,分别对不同译码算法(MAP,SW-MAP,log-MAP算法)的译码性能进行了仿真,并与标准参数的译码器进行比较.将算法程序以C++动态链接库的形式实现,编写Python测试程序,产生待仿真码长的随机信号,编译码后计算误码率,绘制出信噪比和误码率的关系曲线图.通过相应的仿真发现,所设计的编译码器具有所需的通用性;同时对不同算法的性能进行了分析比较;研究各项参数对于译码性能的影响,包括信息序列长度、码率、迭代次数等. 相似文献
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《中国航空学报》2020,33(7):1953-1968
The vibration caused blade High Cycle Fatigue (HCF) is seriously affects the safety operation of turbomachinery especially for aero-engine. Thus, it is crucial important to identify the blade vibration parameters and then evaluate the dynamic stress amplitude. Blade Tip Timing (BTT) method is one of the promising method to solve these problems. While, it need a high resolution Once Per Revolution (OPR) signal which is difficult to get for the aero-engine. Here, a Coupled Vibration Analysis (CVA) method for identifying blade vibration parameters by a none OPR BTT is proposed. The method assumes that every real blade has its own vibration performance at a given speed. Whereby, it can take any blade as the reference blade, and the other blades using the reference blade as the OPR for vibration displacement calculating and further parameter identifying. The proposed method is validated by numerical model. Also, experimental studies are carried out on a straight blade and a twisted three dimensional blade test rig as well as a large industrial axial compressor respectively. The results show that the proposed method can accurately identify the blade synchronous vibration parameters and quantitatively evaluate the mistuning in bladed disks, which lays a foundation for the reliability improvement of aero-engine. 相似文献
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对于脉冲星试验01星的两年实测数据,针对蟹状星云脉冲星星历经历了多次更新的特点,提出了更新标准脉冲轮廓进行X射线计时的改进方法。以一系列观测时长为实测数据分组,再采用改进后的方法进行计时分析并与改进前的结果进行对比。通过对比改进前后的计时结果,发现改进方法得到的计时残差的均方根(root mean square, RMS)平均降低了14.2%,定位精度平均提高了14.4%,估计原子钟相对频率偏差的精度平均提高了26.2%,体现了改进方法处理经历多次星历更新的Crab脉冲星观测数据的合理性和优越性。此外,改进方法对脉冲星试验01星两年观测数据的稳定度σz没有量级上的改进,说明改进方法对Crab脉冲星时间稳定度的影响不大。 相似文献