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1.
雷电空间电磁场一直是电磁领域研究的热门,成熟的算法例如有限时域差分法(FDTD),传输线矩阵法(TLM)以及频域的矩量法(MoM)在计算雷电问题方面都有广泛的应用。由于计算流体力学(CFD)中的Euler方程与电磁学中的Maxwell方程有着相同的守恒形式,而且采用间断伽辽金方法(DG)已经在流场问题上得到广泛的尝试,因此引入了基于计算流体力学的DG方法来离散时域Maxwell方程,并采用网格分区并行技术加速计算,使用基于DG的圆球雷达散射截面积(RCS)算例进行测试,数值结果一致表明DG算法在求解电磁场问题上的可行性,之后通过计算一段近场雷电通道的电场分布并与解析解、某算法仿真解对比,数据基本吻合,说明该方法适合于雷电电磁场的计算。 相似文献
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《中国航空学报》2021,34(5):617-627
In this paper, a progressive approach to predict the multiple shot peening process parameters for complex integral panel is proposed. Firstly, the invariable parameters in the forming process including shot size, mass flow, peening distance and peening angle are determined according to the empirical and machine type. Then, the optimal value of air pressure for the whole shot peening is selected by the experimental data. Finally, the feeding speed for every shot peening path is predicted by regression equation. The integral panel part with thickness from 2 mm to 5 mm and curvature radius from 3200 mm to 16000 mm is taken as a research object, and four experiments are conducted. In order to design specimens for acquiring the forming data, one experiment is conducted to compare the curvature radius of the plate and stringer-structural specimens, which were peened along the middle of the two stringers. The most striking finding of this experiment is that the outer shape error range is below 3.9%, so the plate specimens can be used in predicting feeding speed of the integral panel. The second experiment is performed and results show that when the coverage reaches the limit of 80%, the minimum feeding speed is 50 mm/s. By this feeding speed, the forming curvature radius of the specimens with different thickness from the third experiment is measured and compared with the research object, and the optimal air pressure is 0.15 MPa. Then, the plate specimens with thickness from 2 mm to 5 mm are peened in the fourth experiment, and the measured curvature radius data are used to calculate the feeding speed of different shot peening path by regressive analysis method. The algorithm is validated by forming a test part and the average deviation is 0.496 mm. It is shown that the approach can realize the forming of the integral panel precisely. 相似文献
3.
Ayodeji Ashidi Joseph Ojo Adekunle Adediji Oludare Ajewole 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(5):1612-1622
Existing amplitude scintillation prediction models often perform less satisfactorily when deployed outside the regions where they were formulated. This necessitates the need to evaluate the performance of scintillation models developed in one region using data data from other regions while documenting their relative errors. Due to its variation with elevation angle, frequency, other link parameters and meteorological factors, we employed three years (January 2016 to December 2018) of concurrently measured satellite radio beacons and tropospheric weather parameters to develop a location-based amplitude scintillation prediction model over the Earth-space path of Akure (7.17oN, 5.18oE), South-western Nigeria. The satellite beacon measurement used Tektronix Y400 NetTek Analyzer at 1 s integration time while meteorological parameters, namely; temperature, pressure and relative humidity were measured using Davis Vantage Vue weather station at 1 min integration time. Comparative study of the model’s performance with nine (9) existing scintillation prediction models indicates that the best and worst performing models, in terms of root mean square error (RMSE), are the Statistical Temperature and Refractivity (STN) and direct physical and statistical prediction (DPSP) models with values 11.48 and 51.03 respectively. Also, worst month analysis indicates that April, with respective enhancement and fade values of 0.88 and 0.90 dB for 0.01% exceedance, is the overall worst calendar month for amplitude scintillation. 相似文献
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Mingying Huo Giovanni Mengali Alessandro A. Quarta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(10):2617-2627
Propellantless continuous-thrust propulsion systems, such as electric solar wind sails, may be successfully used for new space missions, especially those requiring high-energy orbit transfers. When the mass-to-thrust ratio is sufficiently large, the spacecraft trajectory is characterized by long flight times with a number of revolutions around the Sun. The corresponding mission analysis, especially when addressed within an optimal context, requires a significant amount of simulation effort. Analytical trajectories are therefore useful aids in a preliminary phase of mission design, even though exact solution are very difficult to obtain. The aim of this paper is to present an accurate, analytical, approximation of the spacecraft trajectory generated by an electric solar wind sail with a constant pitch angle, using the latest mathematical model of the thrust vector. Assuming a heliocentric circular parking orbit and a two-dimensional scenario, the simulation results show that the proposed equations are able to accurately describe the actual spacecraft trajectory for a long time interval when the propulsive acceleration magnitude is sufficiently small. 相似文献
6.
对一起因电池设计缺陷引发装备战训失利的故障进行分析,重点对电池工作机理和设计缺陷展开解析,明确故障定位,并对国内外装备弹上不同体系电池的优缺点进行比较,旨在为产品维护保障、国产化科研等工作提供参考。 相似文献
7.
本文提出了一种基于虚拟页地址映射的NAND Flash管理算法.该算法通过定义坏块表、对应表等结构,以及设计的坏块替换策略和虚拟页地址到实际物理页地址的转换算法,实现上层软件采用虚拟地址对NAND Flash的无坏块连续页地址访问.该算法是一种高效的地址映射算法,能高效地对数据进行索引,占用SRAM空间较少,使系统达到高性能,并使得闪存使用的更加稳定持久. 相似文献
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进行自由空间的光通信或空间对抗,需要在卫星间实现精确的跟踪与瞄准。因为地面测控站的设置非常有限,指令与数据注入的范围受到很多限制,所以要求这种跟瞄在很多时候是无主控制状态下完成的。提出了一种利用在地面测控站的范围内向星上数管中心注入目标卫星、本体卫星的轨道参数,其它时间依靠自主导航飞行和GPS修正的方法,结合本体星的姿态测量、振动测量实现卫星瞄准指向的方位角与俯仰角的精确控制的方法,提高了在地面站无法注入指令与数据时卫星的捕获概率。通过仿真,将计算结果与卫星仿真工具软件STK的数据进行比较,结果一致。最后在嵌入式DSP平台上实现了这一策略。 相似文献