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Investigation of the infrared characteristics of a rocket nozzle is very important for the study of infrared initiating technology. The Narrow-Band Zone model is developed for that purpose. The spectral transmission and absorption factors are introduced, and the equations between radiative heat flux and the temperature of waill surfaces and gas are developed. The radiative heat transfer in one axisymmetric cylindrical enclosure filled with homogeneous radiative participating medium is computed with the Narrow-Band Zone model and compared with those in the reference documents. The comparison shows good agreement. The radiative heat transfer to the nozzle of one rocket engine is also calculated with the Narrow-Band Zone model, and the outgoing radiative energy flux and energy rate integrated in a mid-wave infrared band 2-6 pm, a long-wave infrared band 8-14 pm and the full wave band are analyzed. The following conclusions can be derived: the spectral radiation from the inlet and outlet of the nozzle show apparent spectral discontinuity, which appears greater in the 2.7-2.95 pm than in the neighboring wave band. The spectral outgoing radiative energy flux of nozzle wail is similar to that of gray body, which decreases with wavelength in 2-14 pm. The outgoing radiative energy flux on the nozzle wall is greater in the cylindrical and contracting section of nozzle, but smaller in the divergent section, which is determined by temperature. The nozzle of the rocket engine radiates most energy in the mid-wave surfaces by absorption. The most important feature of gas radiation is the strong selection of the waveband, so the detailed study of the infrared characteristics of nozzle of the rocket engine should be carried out on narrow-band computation. 相似文献
123.
A theoretical model of semi-elliptic surface crack growth based on the low cycle strain damage accumulation near the crack tip along the cracking direction and the Newman–Raju formula is developed. The crack is regarded as a sharp notch with a small curvature radius and the process zone is assumed to be the size of cyclic plastic zone. The modified Hutchinson, Rice and Rosengren(HRR) formulations are used in the presented study. Assuming that the shape of surface crack front is controlled by two critical points: the deepest point and the surface point.The theoretical model is applied to semi-elliptic surface cracked Al 7075-T6 alloy plate under cyclic loading, and five different initial crack shapes are discussed in present study. Good agreement between experimental and theoretical results is obtained. 相似文献
124.
一种折叠弹翼悬挂物的分离轨迹试验技术 总被引:2,自引:0,他引:2
提出了一种新的折叠弹翼悬挂物机弹分离轨迹试验技术,重点解决了在机弹分离过程中折叠弹翼动态展开时悬挂物的气动力获取问题。研究表明,提出的试验技术通过将悬挂物气动力修正方法引入到悬挂物分离安全性研究当中,准确地得到悬挂物的分离特性,解决了折叠弹翼悬挂物分离轨迹风洞试验技术瓶颈,为折叠弹翼悬挂物的投放分离安全性提供一套工程实用的解决方案。 相似文献
125.
介绍一种智能型的精密电阻自动考核筛选装置,解决了考核筛选精密电阻时繁重的重复性劳动,并保证了电阻测量的准确性,该装置还可应用于筛选考核稳压块等具有温度系数的器件。 相似文献
126.
针对大数据排序算法的需求,提出了基于任务驱动的并行排序算法。该算法采用任务驱动、AIO(Asynchronous Input/Output,异步输入/输出)和双缓冲区机制等技术充分利用系统资源;通过构造等价排序键,优化快速排序算法;并在算法实现上,采用多线程处理任务,通过控制线程个数控制并行度。综合利用这些技术,该算法使得大数据的排序性能接近理论极限值,在CPU(Central Processing Unit,中央处理器)资源充裕的情况下,利用异步压缩技术,还可以突破这一极限,最终实现的系统2 000s就可以对超过500Gbyte的磁盘数据做一次完整的排序。在数据库设计中充分利用此思想,将会实现连接和线程的分离,数据库将可以支持更大的连接数,从而提高数据库支持的并发度。 相似文献
127.
Lujing Cai Hong Wang 《IEEE transactions on aerospace and electronic systems》1994,30(4):1009-1020
Among the few known adaptive filtering algorithms which have an embedded (integrated) constant false alarm rate (CFAR) performance feature, the generalized likelihood ratio (GLR) test algorithm has been found to be robust in non-Gaussian clutter. This paper examines the detection performance of the GLR algorithm in nonhomogeneous/nonstationary clutter environments which lead to nonidentical distribution of secondary (training) data. For two common types of nonhomogeneity, i.e., the so-called “signal contamination” and “clutter edge”, the asymptotic detection performance is derived and compared with simulations. These asymptotic results are relatively simple to use and they predict the GLR performance in nonhomogeneous environments quite well. The GLR performance loss due to the nonhomogeneity is also evaluated. It is found that the “generalized angle” between the desired and contaminating signal plays an important role in the study of the effects of signal contamination. It is also found that the performance degradation due to the clutter edge depends largely on the width of the clutter spectrum and target-clutter Doppler separation 相似文献
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129.
A. G. Kosovichev T. L. Duvall Jr. A. C. Birch L. Gizon P. H. Scherrer Junwei Zhao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,29(12):289-1910
Dynamical and thermal variations of the internal structure of the Sun can affect the energy flow and result in variations in irradiance at the surface. Studying variations in the interior is crucial for understanding the mechanisms of the irradiance variations. “Global” helioseismology based on analysis of normal mode frequencies, has helped to reveal radial and latitudinal variations of the solar structure and dynamics associated with the solar cycle in the deep interior. A new technique, - “local-area” helioseismology or heliotomography, offers additional potentially important diagnostics by providing three-dimensional maps of the sound speed and flows in the upper convection zone. These diagnostics are based on inversion of travel times of acoustic waves which propagate between different points on the solar surface through the interior. The most significant variations in the thermodynamic structure found by this method are associated with sunspots and complexes of solar activity. The inversion results provide evidence for areas of higher sound speed beneath sunspot regions located at depths of 4–20 Mm, which may be due to accumulated heat or magnetic field concentrations. However, the physics of these structures is not yet understood. Heliotomography also provides information about large-scale stable longitudinal structures in the solar interior, which can be used in irradiance models. This new diagnostic tool for solar variability is currently under development. It will require both a substantial theoretical and modeling effort and high-resolution data to develop new capabilities for understanding mechanisms of solar variability. 相似文献
130.