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基于对螺旋钻头的输出月壤阻力、驱动力矩及月壤失效区的分析,建立了钻头的力学模型,该模型综合考虑切削具内外侧面与月壤之间的压力及摩擦力,考虑月壤侧向失效面的面载荷对钻头切削具周向力矩、总功耗及月壤失效距离的影响,数值仿真与试验结果校验了模型的正确性。在数值仿真过程中采用深层月壤本构关系的Mohr-Coulomb模型,使仿真更加符合月壤内摩擦角大于22°的真实情况。利用该模型分析并获得了钻头结构参数对切削具功耗和失效距离的影响规律,以钻头功耗最小为优化目标,用遗传算法对钻头结构参数进行了优化,优化结果降低了钻探过程中的烧钻风险。可为钻取式自动采样机构的钻头设计提供理论依据。 相似文献
54.
Svetlana Karimova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Despite spiral eddies were first seen on the sea surface more than 40 years ago, there is still a lot of uncertainty concerning these eddies. The present paper is aimed to provide the comprehensive results on the occurrence and statistics of small-scale eddies in the three inner seas (the Baltic, Black and Caspian) using satellite synthetic aperture radar (SAR) images. The dataset used includes over 2000 medium resolution Envisat ASAR and ERS-2 SAR images obtained in 2009–2010 in the different parts of the seas mentioned. As a result of the analysis performed ∼14,000 vortical structures were detected. 71% of them were visualized due to surfactant films (“black” eddies), while 29% due to wave/current interactions (“white” eddies). Practically all the eddies detected were cyclonically rotating. Their diameter was within 1–20 km. Characteristic size of the “black” eddies in all the basins was discovered to be less than that of the “white” eddies. Characteristic eddy size for the Baltic, Black and Caspian seas proved to be strictly proportional to the values of the baroclinic Rossby radius of deformation typical for these basins. The “black” eddies did not demonstrate a significant connection with the basin- and meso-scale surface circulation of the seas. Most of the “white” eddies detected were attributed to the zones with the most intense drift currents, i.e. those along the western boundaries and (in the Baltic Sea only) in the elongated parts of the basin. 相似文献
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高压、高速、高温化使得齿轮泵固有困油问题愈发严重,传统卸荷槽结构已难以满足高性能燃油泵设计要求。为此本文提出一种基于运动法的新型卸荷槽结构设计方法,通过构建困油模型并从整泵全局角度分析齿轮参数对困油各项性能的影响规律,以确定齿轮参数并为卸荷槽设计提供约束条件;其次基于齿轮运动规律和卸荷槽设计原则进行了某型燃油齿轮泵卸荷槽的设计,并进行了多个工况下新型卸荷槽和传统卸荷槽困油特性仿真对比;最后试制了样机并通过试验验证了卸荷槽设计的有效性。研究结果表明：所设计的卸荷槽与传统矩形卸荷槽相比,同工况下最大困油压力降低63.4 MPa,流量脉动率减小33.5%,空化区域更小,工作性能更优,能够显著缓解困油带来的不利影响。采用该结构卸荷槽的齿轮泵具有高的容积效率和长时抗汽蚀能力。 相似文献
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王跃 《民用飞机设计与研究》2012,(1):56-60
针对现代民用飞机设计特点,尤其是某些新技术的应用和飞机系列化发展的需求,在充分吸收和借鉴传统飞机概念设计阶段起落架设计方法的基础上,从工程应用角度出发,总结并提出一套现代民用飞机概念设计阶段起落架接地点设计流程及方法。同时,按照设计流程将影响起落架接地点设计的限制因素划分为适航安全、性能、结构、空间布置、运营等影响因素,明晰各限制因素对设计产生的影响。 相似文献
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I. Büsching M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The discovery of direct evidences for the acceleration of high energetic particles at the shell supernova remnant RXJ1713.7-3946 underlined the need to calculate the cosmic ray (CR) distribution in the Galaxy on a spatial grid fine enough to resolve the changes in the CR density due to these kind of objects. It was shown before by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005] that the discrete nature (both in space and time) of super novae (SN) as sources of Galactic CR leads to CR spectra changing in space and time, resulting in a range of possible CR spectra at a given location in the Galaxy. As the most frequent SN types Ib and II are found within spiral arms, one can expect a significant difference of the range of possible spectra in and outside spiral arms. We investigate the variability of the local interstellar CR proton spectrum during the motion of the Sun in and out of spiral arms in its journey around the Galactic center. Using the code described by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005], the proton CR density in the Galaxy is calculated with high spatial and temporal resolution (75 pc in galactocentric radius r and azimuth φ at the position of the Sun and 20 pc in z (perpendicular to the galactic plane), with a time step of 1 kyr), assuming stochastically distributed point sources with a probability distribution that resembles the spiral structure of our Galaxy. We find the averaged CR flux outside the spiral arm to be about 50% of that inside a spiral arm. We further find spatial and temporal variations of the CR flux inside spiral arms. 相似文献
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本文概要的介绍了一种新型器件——非对称式带状线模式馈电网络的基本原理,主要技术指标及其相位关系等。该器件体积小、重量轻、结构紧凑、性能稳定、用于按模式馈电的场合既方便又可靠。 相似文献
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针对2219合金TIG补焊接头X射线底片亮线影像,开展2219合金不同坡口面角TIG补焊接头组织及性能研究。通过X射线、扫描电镜及能谱仪分析接头底片亮线影像位置对应的微观形貌及成分,并通过拉伸试验评价补焊接头力学性能。结果显示:在0～20°随坡口面角α值的增大,X射线底片上亮线影像的黑度逐渐降低;Cu含量较高的α(Al)+θ非平衡共晶组织对X射线的散射与吸收作用较强,是X射线底片亮线影像的成因;坡口面角α角侧受电磁搅拌作用弱于β角侧,其固-液界面前沿的边界层宽度大于β角侧,且温度梯度及边界层内的成分过冷度均大于β角侧,促进了α角侧枝晶的生长。当β角为20°时,在0°～20°随着α角度值增大,接头的抗拉强度与延伸率逐渐增大,20°时获得了优良的室温力学性能。X射线底片上存在亮线影像的补焊接头力学性能满足型号使用要求,亮线影像结构可不按焊接缺陷处理。 相似文献