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71.
72.
近距离DPIV粒子成像分析 总被引:2,自引:0,他引:2
在PIV(Particle Image Velocimetry)近距离拍摄中,通过对在非傍轴成像条件下薄透镜成像公式的推导,求得粒子图像成像点的近似解析解,对粒子图像的成像位置在PIV图像计算中的影响作了讨论;同时也对已知直径粒子进行了试验拍摄,将试验所得的数据与理论推导的结果进行了比较,对在近距离拍摄中光圈对粒子成像的影响给出了定量分析. 相似文献
73.
JSF战机动力装置研制新特点浅析 总被引:1,自引:0,他引:1
美国军方提出以现有发动机型号F119为基础来研制第四代轻型战机JSF,既降低了新机的技术风险,缩短型号研制周期,又可大幅度地节省项目研发资金和降低型号全寿命成本,这一思路值得关注或借鉴。通过对F-35战机基本型发动机F135和备用型F136发动机的最新发展动态分析,阐述了军用飞机动力装置类型从常规的涡喷/涡扇发动机向非常规的变循环发动机转变是一个必然发展趋势;而航空动力研制方法正从”传统设计”向更先进的”预测设计”过渡。 相似文献
74.
<正> 1。引言 局部应力应变法是目前预测结构裂纹起始寿命的一种行之有效的方法。根据局部应力应变法的原理,可以用计算的方法来预测构件裂纹起始寿命。在计算中,从载荷谱得到局部应变谱,可利用有限元法分析结构的局部应力应变响应。当然还可利用半经验公式(如Neuber法等)。在计算中若考虑材料的记忆特性和循环σ-ε曲线,这无疑对真实地反映受载构件的局部应力应变响应是有利的。但要做到这一点,用有限元分析所需的机时相当可观,因为它要对整个寿命期间的载荷历程进行分析计算,至少也要针对一个典型谱分析计算。 计算中材料的循环应力应变曲线一般可采用下式 相似文献
75.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):107-114
This paper presents an novel extreme learning machine (ELM)-based prediction model for the ionospheric propagation factor M(3000)F2 at Darwin station (12.4°S, 131.5°E; −44.5°dip) in Australia. The proposed ELM model is trained with hourly daily values of M(3000)F2 from the period 1998–2014 except 2001 and 2009. The hourly daily values of 2001 (high solar activity) and 2009 (low solar activity) are used for validating the prediction accuracy. The proposed ELM for modeling M(3000)F2 can achieve faster training process and similar testing accuracy compared with backward propagation neural network (BPNN). In addition, the performance of the ELM is verified by comparing the predicted values of M(3000)F2 with observed values and the international reference ionosphere (IRI −2016) model predicted values. Based on the error differences (the root mean square error (RMSE) and the M(3000)F2 percentage improvement values M(3000)F2IMP(%)), the result demonstrates the effectiveness of the ELM model compared with the IRI-2016 model at hourly, daily, monthly, and yearly in high (2001) and low (2009) solar activity years. The ELM also shows good agreement with observations compared with the IRI during disturbed magnetic activity. 相似文献
76.
K.S. Paul H. Haralambous C. Oikonomou A. Paul 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(6):1958-1967
Multi-reflected echoes (MREs) and satellite traces (STs) are referred in literature as ionogram signatures of Travelling Ionospheric Disturbances (TIDs) which is a phenomenon that apparently drives spread F development mainly at nighttime mid-latitude ionosphere. A long-term statistical study has been undertaken to investigate the morphological aspect of these signatures over the lower midlatitude European station of Nicosia, Cyprus (35.19°N, 33.38°E geographic; magnetic dip. 29.38°N) by inspecting all ionograms recorded by the DPS-4D digisonde in the interval 2009–2016. The results underline the systematic manifestation of these TID signatures over Cyprus with a possible (although not quite clear) solar activity dependence and a distinctive seasonal and diurnal occurrence rate with a seasonal peak of STs during summer and of MREs during January to April. Based on the experimental results of the present study, the seasonal occurrence rate of MREs and STs is found to increase by 75% and 56% during high solar activity periods. Satellite traces are well known ionogram signatures of TIDs and mostly correlated to the nighttime spread F formation. The occurrence of mid-latitude spread Fs over European longitude sector normally increases during summer. The occurrences of TIDs are also prominent at this interval of the year over nighttime mid-latitude ionosphere. The presence of MREs as an ionogram signature of TIDs over mid-latitude ionosphere is unique in nature. 相似文献
77.
The ‘scintillations’ observed on signals received in the equatorial region from GPS satellites are due to plasma instabilities
in the F region of the ionosphere, also detected as spread F. These instabilities give rise to depletions of ionisation or
‘bubbles’. The occurrence of these events and their relation to the equatorial electrojet are reviewed. Possibilities of short-term
forecasting are examined with particular attention to problems encountered in modelling the equatorial electrojet.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
78.
文章介绍了IEEE802.3 CRC-32的一种VHDL语言程序实现。对CRC的重要性进行了简要的介绍,重点讨论了CRC的算法分析、CRC-32的VHDL语言程序实现。 相似文献
79.
移相 PWM波是很多开关电源常用的驱动脉冲信号。双向全桥直流变换器(Bidirectional-Full-Bridge DCDC Converter,BDC)在双重移相控制方式下时需要 4组两两互补的移相 PWM波。文章基于 TMS320F2812型 DSP(Digital Signal Processor)分析了 2种生成移相 PWM的方法。为提高双向全桥直流变换器工作的安全性和可靠性,为移相 PWM波设置死区时间。对所提出的方法进行测试后结果良好,对于双向全桥直流变换器闭环控制系统的构建具有重要意义。 相似文献
80.
Effect of the seed perturbation amplitude on the equatorial spread F initiation during solar minimum
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):255-267
The contribution of gravity wave (GW) to the initiation/development of spread F during a solar minimum year was investigated through the comparison of the observed precursory parameters and characteristics of the corresponding equatorial spread F (ESF) events. The ionospheric parameters were recorded at the magnetic equatorial station Sao Luis (2.3°S, 44°W, dip latitude 2°S) during March and October 2010. These data were used to estimate the influence of the relative gravity wave amplitude and the ambient ionospheric condition on the diurnal variation of the spread F initiation. The vertical velocity drift indicated a clear control and defines the threshold for the seasonal variability of the ESF occurrence. However, it was insufficient to solely determine or predict the day to day variation of ESF occurrence. Thus, few days with contrasting ambient ionospheric condition and magnitude of GW amplitude were analysed in order to investigate the role of the different precursory factors in the observed diurnal variation of the plasma irregularity development. The density scale length and gravity wave amplitude were shown to immensely contribute to the linear instability growth rate, especially during the days with a low post-sunset rise. Thus, the experimental observations have demonstrated the strong inter-dependence between the precursory factors and they have also highlighted the probable control of the ESF morphology. 相似文献