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排序方式: 共有228条查询结果,搜索用时 31 毫秒
51.
Masanori Matsushita Toshihiro Chujo Jun Matsumoto Osamu Mori Rikio Yokota Hiroyuki Toyota Yasutaka Satou Nobukatsu Okuizumi Hideki Kato Tetsuya Nakamura Yuichi Shibata Tatsuro Nakao Kazuyuki Mori Sanae Fujii Yuki Takao Yuki Kubo Yuya Miyamoto Yuichiro Nada Yudai Kimishima 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(9):2899-2911
This paper reports on the manufacturing and evaluation of a solar power sail membrane prototype for the OKEANOS project. The in-house prototype was built by the Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency. Mechanical and electrical evaluation tests were conducted. The membrane, thin-film solar cells, reflectivity control devices were good condition after the manufacturing and handling. The improvements in the manufacturing process and design were found. The manufacturing process and design were fundamentally established. After the prototype, improvement plans for the manufacturing process and design were tried. We have a prospect of manufacturing the flight model sail and continue to the development. 相似文献
52.
为了更加准确地模拟涡轮叶片表面颗粒物沉积的增长过程和分布状况,研究颗粒物沉积过程中粘附、剥离直至稳定平衡的规律,在经改进的颗粒粘附模型基础上考虑两种剥离形式,利用Fluent的User Defined Function (UDF)功能和网格重构技术,最终实现了熔融石蜡颗粒于带有气膜冷却的平板上沉积动态增长的过程。通过与相同条件下所得实验结果的对比,验证了所用模型的有效性和合理性。随后研究了是否加入剥离模型、气膜冷却吹风比、气膜孔射流角度等因素对沉积效果的影响。计算结果表明,考虑颗粒的剥离效应将减少颗粒物沉积的总量,尤其是在气膜孔后较短区域内;此外,吹风比的增加将使颗粒不易撞击壁面,已粘附的颗粒也更容易剥离从而降低沉积的厚度和质量;射流角度不断增大则使气膜覆盖效果变差,壁面温度升高,颗粒更易达到熔融状态沉积下来。研究发现该数值方法有助于更加精确地仿真沉积增长的过程,证实了吹风比和射流角度对沉积的分布和厚度有很大影响。当射流角度处于35°~40°时,可在一定程度上减少沉积。 相似文献
53.
In the process of composite prepreg tape winding, the compaction force could influence the quality of winding products. According to the analysis and experiments, during the winding process of a rocket motor nozzle aft exit cone with a winding angle, there would be an error between the deposition speed of tape layers and the feeding speed of the compaction roller, which could influence the compaction force. Both a lack of compaction and overcompaction related to the feed-ing of the compaction roller could result in defects of winding nozzles. Thus, a flexible winding sys-tem has been developed for rocket motor nozzle winding. In the system, feeding of the compaction roller could be adjusted in real time to achieve an invariable compaction force. According to exper-iments, the force deformation model of the winding tape is a time-varying system. Thus, a forgetting factor recursive least square based parameter estimation proportional-integral-differential (PID) controller has been developed, which could estimate the time-varying parameter and control the compaction force by adjusting the feeding of the compaction roller during the winding process. According to the experimental results, a winding nozzle with fewer voids and a smooth surface could be wounded by the invariable compaction force in the flexible winding system. 相似文献
54.
Nonlinear uncertainty quantification of the impact of geometric variability on compressor performance using an adjoint method 总被引:3,自引:3,他引:0
Manufactured blades are inevitably different from their design intent, which leads to a deviation of the performance from the intended value. To quantify the associated performance uncertainty, many approaches have been developed. The traditional Monte Carlo method based on a Computational Fluid Dynamics solver(MC-CFD) for a three-dimensional compressor is prohibitively expensive. Existing alternatives to the MC-CFD, such as surrogate models and secondorder derivatives based on the adjoint metho... 相似文献
55.
在再生自适应子集模拟(RASS)法的基础上,提出了一种改进的再生自适应子集模拟(MRASS)法以用于结构系统的可靠性及可靠性灵敏度分析。MRASS法继承了RASS法中马尔可夫链再生、延迟拒绝、自适应马尔可夫过程及分量各自采样等优点,并改进了自适应采样过程。MRASS法通过对产生的样本点的接受率与最佳接受率进行比较,有针对性地寻找合适的建议分布方差,提高了抽样的效率。工程算例的数值结果表明:MRASS法相比于RASS法及传统的子集模拟(SS)法,在处理具有高维随机变量、小失效概率及高度非线性特点的结构系统时,有更好的适应性、稳健性及精度。 相似文献
56.
57.
先进焊接技术在飞机制造中的应用 总被引:1,自引:0,他引:1
通过对国外飞机制造公司焊接技术的应用分析,明确了先进焊接技术——电子束焊、激光焊和搅拌焊技术的应用现状和使用范围,并结合西飞公司的实际情况,提出应该发展电子束焊和激光焊接技术,以弥补未来制造能力的不足;同时应重点关注搅拌摩擦焊接技术的发展动态,掌握国外该技术的应用状况和使用经验。 相似文献
58.
59.
K.S. Cheng D.O. Chernyshov V. Dogiel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
X-ray observations indicate that the Galactic black hole Sgr A∗ is inactive now, however, we suggest that Sgr A∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼1052 erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?105 yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼107 yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process. 相似文献
60.