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末段突防击水概率是反舰导弹设计和使用人员必须解决的一个问题。文章综合考虑了击水概率影响因素,从掠海飞行导弹背景建模、反舰导弹高度控制系统和弹体纵向运动方程等方面人手,对给定海情下反舰导弹高度输出进行仿真研究,并利用统计试验的方法对击水概率进行计算。仿真结果证实了不同海情下飞行高度对击水概率的影响。 相似文献
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Titanium and its alloys have found very wide application in aerospace due to their excellent characteristics although their processing is still a challenge. Electrochemical machining is an important issue in the fabrication of titanium and titanium alloys. Wire electrochemical machining (WECM) is mainly used for workpiece cutting under the condition of different thickness plates. It has a great advantage over wire electro-discharge machining, which is the absence of heat-affected zone around the cutting area. Moreover, the wire electrode in WECM could be used repetitively because it is not worn out. Thus, much attention has been paid to WECM. The effective way of removing electrolysis products is of importance to WECM. In this paper, the axial electrolyte flushing is presented to WECM for removing electrolysis products and renewing electrolyte. The Taguchi experiment is conducted to optimize the machining parameters, such as wire feedrate, machining voltage, electrolyte concentration, etc. Experimental results show that WECM with axial electrolyte flushing is a promising issue in the fabrication of titanium alloy (TC1). The feasibility of multi-wire electrochemical machining is also demonstrated to improve the machining productivity of WECM. 相似文献
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采用环抛方法对有预埋件和无预埋件的两块碳纤维-微晶复合材料反射镜进行光学加工,之后进行了稳定性实验研究,采用Zygo干涉仪实测了碳纤维-微晶复合材料反射镜面形.稳定实验后,有预埋件反射镜面形P-V值为3.013λ,RMS值为0.669λ;无预埋件反射镜面形P-V值为2.313λ,RMS值为0.276λ(λ=632.8 nm).实验结果证明,有预埋件的碳纤维-微晶复合材料反射镜结构优于无预埋件结构,为碳纤维-微晶复合材料反射镜的工程化提供参考. 相似文献
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Yuxi Li Wei Lu Guangyou Fang Bin Zhou Shaoxiang Shen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):2267-2278
Lunar Regolith Penetrating Array Radar (LRPR) is one main payload of the Lander for Chinese Chang’E-5 (CE-5) mission. It is used to support the drilling and sampling device and to detect lunar regolith thickness and structure of the landing site. LRPR will only work in situ under static status, so the antenna array is employed. Since the antenna array is about 90?cm high from the ground, the layout is irregular, and the metal structure of the lander seriously interferes with LRPR, these factors make it very difficult to reconstruct the image of the drilling area, so the performance verification must be carried out. We propose a set of methods to process LRPR’s data and reconstruct image. The verification experiments demonstrate that these methods are suitable for LRPR, the thickness and structure of the lunar regolith from zero to two meters can be clearly mapped, the vertical resolution is a few centimeters, and the electromagnetic properties of the subsurface can be estimated. Therefore, the performance of LRPR meets the requirements, and LRPR can successfully support drilling and sampling. 相似文献
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张山 《南京航空航天大学学报》2018,13(1):75-86
本文使用基于钻孔测井数据的3类模型,即常速度外推模型、速度梯度模型、双深度参数外推模型,通过对北京地区460个深度超过30m的钻孔剪切波速资料进行分析,详细探究了V_(S30)估算模型在本研究区的适用性。研究结果表明双深度参数外推模型在估算V_(S30)上准确度很高,其不需要大量的数据进行回归分析,且不具有区域独立性,可以为全球包括北京地区场地类别划分提供依据,进而在震害快速评估中用于确定场地影响,是一种值得推广的估算模型。 相似文献
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Xing Meng Hanxian Fang Libin Weng Zhendi Liu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):2118-2125
Through concurrently measurements by Communication/Navigation Outage Forecasting System (C/NOFS), Sanya VHF radar and GPS ionospheric scintillation receiver on 12 March 2010, five plasma bubbles were found and three of them were observed by all those instruments. Two well-developed plumes with strong backscatter echoes were measured by Sanya radar and their corresponding depletions were observed by C/NOFS in Orbit 10317, 10318 and 10319. Broad plasma depletions resulting from merging process were found in orbit of 10318. The occurrence time and geophysical positions of scintillations correlate well with observations implemented by Sanya VHF radar and C/NOFS. Observations from three types of instrument indicate that the spread F irregularities have distinct scale. There were longitudinal differences between Sanya VHF radar and C/NOFS as irregularities measured, and the eastward drift of developed bubbles are responsible for these differences. 相似文献