STOCHASTIC NEURAL NETWORK AND ITS APPLICATION TO MULTI－MANEUVERING TARGET TRACKING

ＳＴＯＣＨＡＳＴＩＣＮＥＵＲＡＬＮＥＴＷＯＲＫＡＮＤＩＴＳＡＰＰＬＩＣＡＴＩＯＮＴＯＭＵＬＴＩ－ＭＡＮＥＵＶＥＲＩＮＧＴＡＲＧＥＴＴＲＡＣＫＩＮＧＪｉｎｇＺｈｏｎｇｌｉａｎｇ；ＤａｉＧｕａｎｚｈｏｎｇ；ＴｏｎｇＭｉｎｇａｎ；ＺｈｏｕＨｏｎｇｒｅｎ（Ｄ...     

高超声速冲压发动机技术

介绍高超声速冲压发动机的结构要素,指出各要素的性能和研究方法,以及该发动机目前研究的概况与成果。探讨作为高超声速飞行器推进系统设计的可行性。     

The Theory of Gamma-Ray Bursts

This chapter gives a brief review on the theory of gamma-ray bursts (GRBs), including the models of multi-messengers (e.g., prompt multiwavelength electromagnetic emissions, high-energy neutrinos, ultra-high-energy cosmic rays, and gravitational waves) and central engines (in particular, mergers of binary neutron stars for short GRBs). For detailed reviews, please see (Piran in Phys. Rep. 314:575, 1999; Rev. Mod. Phys. 76:1143, 2004; Mészáros in Annu. Rev. Astron. Astrophys. 40:137, 2002; Rep. Prog. Phys. 69:2259, 2006; Zhang and Mészáros in Int. J. Mod. Phys. A 19:2385, 2004; Zhang in Chin. J. Astron. Astrophys. 7:1, 2007; Nakar in Phys. Rep. 442:166, 2007; Kumar and Zhang in Phys. Rep. 561:1, 2015).     

俯仰振荡翼型跨音速粘性绕流的数值计算

以ＬＵ－ＴＶＤ混合格式求解二维非定常湍流Ｎ－Ｓ方程,计算了绕１／４弦点振荡的翼型跨音速粘性绕流解,与实验结果吻合较好。通过取不同ＣＦＬ数计算表明：在能得到非定常稳态解的情况下,取小ＣＦＬ数更能真实地反映非定常时间历程,具有更高的可信度     

基于神经网络的机动目标信息融合与并行自适应跟踪

基于“当前”统计模型和 BP神经网络 ,提出一种新的机动目标神经网络信息融合与并行自适应跟踪算法 ( NIFPAT)。该算法采用双滤波器并行结构 ,利用全状态反馈 ,通过 BP网络调整系统方差以适应目标的运动变化 ,具有对目标各种运动状态的良好自适应跟踪能力     

关于图的边分划的一种算法

为在一个道路交通网内确定建立清障站的合理个数和站址的选择,本文提供了一种简明算法。     

声纳多目标跟踪

本文导出了极坐标下边扫描边跟踪(TWS)数据处理的的跟踪滤波方程,可以获得稳定和渐近无偏的估计。在某声纳站TWS系统的计算机仿真中,采用了点迹与航迹相关的最优配对算法,结果是满意的。     

求解大型对称特征值问题的块Chebyshev-Lanczos方法

本文提出了计算大型对称矩阵若干个最大或最小特征对的块Chebyshev迭代法,讨论了块Chebyshev迭代法对块Lanczos方法的应用,给出了块Chebyshev-Lanczos方法。计算实践表明块Chebyshev-Laaczos方法比块Lanczos方法和Chebyshev-Lanczos方法都优越。     

回注蒸汽型燃气轮机数控系统的仿真研究

按部件建立了数控系统的数学模型。再与回注蒸汽型燃气轮机数学模型闭合,进行了系统的仿真研究。据此优选参数,并分析了不同工况和回注蒸汽对系统动态性能的影响。     

Origin of coronal and interplanetary shock and particle acceleration of a flare/CME event

By using radio data from ground-based telescopes (from 270 MHz to 25 MHz), and from the Radio and Plasma Wave experiment (WAVES) on board the WIND spacecraft (1–14 MHz and several kHz-11 MHz), as well as FY -2 satellite data, the origin of coronal and interplanetary shock and particle acceleration of the 14 July 2000 flare/CME event (the Bastille day event) have been studied. Main conclusions are as follows: (1) We investigate the causal relationship between metric type 11 bursts observed by the digital IZMIRAN radio spectrograph and type II radio emissions in the frequency range from 1–14 MHz and several kHz-11 MHz observed by the WAVES/WIND. The analysis indicate that the fast CME is the origin of both coronal and interplanetary shocks. (2)According to the time profiles of Hard X-ray, and energetic particles (include proton, ³He, and ⁴He) from FY-2 satellite, it is obvious that the Bastille day event is the event, in which both impulsive and gradual phenomena occur. The energetic particles accelerated not only in flare but also in CME.