非结构化网格生成中背景网格对源的响应

背景网格对源的响应方法对非结构网格的生成具有重要意义,如果背景网格参数能恰当地反映出源的变化,则所生成的非结构网格就能满足网格设计的要求。将背景网格的三角形单元分为7个子域,根据源在单元中的位置对网格进行局部加密或变形,使每一个源点都与一个背景网格结点相对应,再通过求解热传导方程,使背景网格参数分布光滑,基本反映网格设计的要求,从而提高了非结构化网格的生成质量。     

基于特征空间变换的运载火箭Pogo模型降阶方法

针对运载火箭Pogo状态空间模型存在维数高和奇异性的问题,开展了 Pogo模型的降阶方法研究.基于特征空间变换理论,导出了一般形式的Pogo状态空间模型的解耦形式.该形式与推进系统和结构系统的模态频率相对应,从而通过模态截断或保留感兴趣的模态实现有效的模型降阶.同时,还给出了降阶方法的实数运算公式.在两种不同型号推进系...     

强海杂波背景下目标检测方法综述

高频地波雷达被广泛应用于海面目标的检测,而由于海杂波的分布散射具有很强的动态特性,通常情况下成为了海面目标检测的主要干扰成分。因此,在强海杂波背景下进行目标检测的关键在于如何有效抑制海杂波。从循环对消、子空间分解、模型预测以及分形特征这几方面对海杂波抑制技术进行综述、分析和总结,为后续对海面目标检测提供参考。     

The infra-red background generated by pregalactic stars and their remnants

We examine whether the IR background reported by Matsumoto (1983) could have been generated by stars or black holes in the pregalactic era, z=10100.     

颤振主动抑制中的非线性问题

本文采用谐波平衡法,定量地解释了机翼颤振主动抑制风洞试验中出现的极限环现象。提出了比较精确的计及极限环基阶谐波与三阶谐波的分析计算方法。指出在采用液压舵机的情况下,伺服阀的不灵敏区是出现极限环现象的一个主要原因。     

关键参数对二冲程煤油发动机爆震的影响

针对二冲程汽油发动机改用航空煤油后的爆震抑制和性能恢复进行了研究,利用GT-Power软件建立发动机的一维仿真模型并对煤油发动机的爆震进行了预测和优化。仿真结果表明:推迟点火时刻、远低于和远大于理论空燃比的混合气对爆震都有一定的抑制作用,试验结果验证了仿真结果的正确性。提出并采用协同推迟点火和增加喷油的控制策略进行试验研究。试验结果表明:在低转速大负荷工况下,爆震可被有效抑制,节气门全开时功率恢复在90%以上。发动机转速为5 500 r/min时,功率恢复能达到原机的95.7%。      

随机二相码调相PD引信的距离旁瓣抑制

随机二相码调相ＰＤ（脉冲多普勒）引信，是一种较为新颖的噪声调制引信体制。因距离旁瓣的存在会使该体制引信产生概率性的距离模糊，首先分析了其独特的距离旁瓣特性，然后分析了相关器组法进行距离旁瓣抑制的机理和性能，并提出了以限制码的最大游程加惯性积累电路来抑制的方法。分析表明，两者都能对距离旁瓣进行有效的抑制，而后者更适合于引信电路的特点。     

3D Imaging of the OH mesospheric emissive layer

A new and original stereo imaging method is introduced to measure the altitude of the OH nightglow layer and provide a 3D perspective map of the altitude of the layer centroid. Near-IR photographs of the OH layer are taken at two sites separated by a 645 km distance. Each photograph is processed in order to provide a satellite view of the layer. When superposed, the two views present a common diamond-shaped area. Pairs of matched points that correspond to a physical emissive point in the common area are identified in calculating a normalized cross-correlation coefficient (NCC). This method is suitable for obtaining 3D representations in the case of low-contrast objects. An observational campaign was conducted in July 2006 in Peru. The images were taken simultaneously at Cerro Cosmos (12°09′08.2″ S, 75°33′49.3″ W, altitude 4630 m) close to Huancayo and Cerro Verde Tellolo (16°33′17.6″ S, 71°39′59.4″ W, altitude 2272 m) close to Arequipa. 3D maps of the layer surface were retrieved and compared with pseudo-relief intensity maps of the same region. The mean altitude of the emission barycenter is located at 86.3 km on July 26. Comparable relief wavy features appear in the 3D and intensity maps. It is shown that the vertical amplitude of the wave system varies as exp (Δz/2H) within the altitude range Δz = 83.5–88.0 km, H being the scale height. The oscillatory kinetic energy at the altitude of the OH layer is comprised between 3 × 10⁻⁴ and 5.4 × 10⁻⁴ J/m³, which is 2–3 times smaller than the values derived from partial radio wave at 52°N latitude.     

Primordial black holes and Holeums as progenitors of Galactic diffuse gamma-ray background

Diffuse Galactic gamma-ray flux resulting from the evaporation of primordial black holes has been the subject of intensive research work during the last few decades. Theoretical work addressing this issue started in the 1970s whereas data started pouring in only in the 1990s. We discuss in this paper a model of the potential contribution to the Galactic gamma-ray flux of primordial black holes in binary systems and extend the argument to include stable gravitational bound states called Holeums. The model has a predictive power and can be tested by looking for gamma-ray excess in the vicinity of violent events occurring in the Galaxy such as supernova explosions.     

基于增量学习的高光谱图像目标检测

高光谱图像目标检测是高光谱图像分析中的重要研究内容之一。本文从经典有效的约束能量最小化算法出发,提出了一种基于增量学习的高光谱目标检测方法。当获得新的样本时,不需要重新计算所有样本的自相关矩阵即可对检测器模型进行更新,减轻了星上有限计算资源的负担。实验结果表明:本文提出的目标检测算法在压制背景光谱的同时可以更好地适应目标光谱,提高了算法的检测性能。