On the primordial black holes in the earth

Astrophysical limitations do not exclude the possibility of some number of dark matter primordial Black Holes (BH) being seeded in the interiors of the Earth at the epoch of planet condensation in the young Solar System. We show that limitations on the neutrino radiation due to the BH quantum evaporation and accretion growth of BH mass completely forbid the existence of primordial BH of any mass in the Earth.     

Electrochemical cutting of mortise-tenon joint structure by rotary tube electrode with helically distributed jet-flow holes

In aero-engines, mortise-tenon joint structures are often used to connect the blades to the turbine disk. The disadvantages associated with conventional manufacturing techniques mean that a low-cost, high-efficiency, and high-quality nickel-based mortise–tenon joint structure is an urgent requirement in the field of aviation engineering. Electrochemical cutting is a potential machining method for manufacturing these parts, as there is no tool degradation in the cutting process and high-quality s...     

电镀立方氮化硼砂轮在超深小孔磨削中的应用

电镀立方氮化硼砂轮在高精度、低表面粗糙度值的超深小孔磨削中,可大幅提高砂轮轴刚性,从而提高加工质量和生产效率。     

承载紧固孔边应力强度因子

 <正> 1.孔边穿透裂纹应力强度因子 采用宽度修正系数FB(c/W),可得紧固件孔边裂纹的SIF式中f_1(α/R)、钉载作用时的FB(c/W)以及未开裂应力σ_Y(X)。对双向载荷下的宽度修正系数,采用文献的数据最小二乘拟合,得     

气体介质中深小孔电火花加工技术研究

 深小孔加工一直是机械制造领域的难题之一。在分析和研究气体介质中电火花加工技术的基础上，就其在深小孔加工中的应用进行了深入的理论与实验研究。分别用管状圆柱电极和削边电极在通用电火花成形加工机床上成功地加工出直径为2 mm、深径比大于20、锥度小于0.5%的深小孔。研究表明，相对于传统的液中电火花加工，气体介质中电火花加工深小孔具有电极损耗率低、加工过程稳定等特点。而且由于无需庞大的工作液系统，该方法适合于大型零部件上深小孔加工。     

金属橡胶毛坯铺设路径规划

针对金属橡胶毛坯铺设工艺,提出了以背景网格为基础的优化模型,利用遗传算法建立了定位销设计和路径规划的优化方法,为毛坯铺设提供了理论依据.定位销数量由底面背景网格非零网格数确定,定位销排布由遗传算法计算得到.根据定位销优化设计结果,逐层对铺设路径进行规划,优化路径比经验路径所得毛坯更加均匀、密实,铺设层数越多,路径规划的优势越明显,铺设10层时,两毛坯目标函数b的值相差50%;单层路径数对毛坯的铺设质量影响不大;随着螺旋卷铺设长度的增加,不同单层路径数铺设的毛坯接触状态趋于一致.      

基于机器视觉的高精度螺孔定位方法研究

针对手工安装工件、劳动强度大以及效率低等问题,提出了一种基于机器视觉的螺孔定位检测方法.利用CCD摄像机实时采集局部待定位物图像,并对图像进行处理,提取螺孔坐标,然后通过物理坐标关系得到拍摄范围外的螺孔的坐标,最后经过eye-hand手眼标定转换到机器人坐标系下的坐标.该方法解决了受外界条件限制,对目标测量的过程不能一步完成的问题-实现了较大物件的自动、快速、准确定位功能.     

Working Group 3 Report: Coronal Hole Boundaries and Interactions with Adjacent Regions

Summarized below are the discussions of working group 3 on "Coronal hole boundaries and interactions with adjacent regions" which took place at the 7th SOHO workshop in Northeast Harbor, Maine, USA, 28 September to 1 October 1998. A number of recent observational and theoretical results were presented during the discussions to shed light on different aspects of coronal hole boundaries. The working group also included presentations on streamers and coronal holes to emphasis the difference between the plasma properties in these regions, and to serve as guidelines for the definition of the boundaries. Observations, particularly white light observations, show that multiple streamers are present close to the solar limb at all times. At some distance from the sun, typically below 2 R, these streamers merge into a relatively narrow sheet as seen, for example, in LASCO and UVCS images. The presence of multiple current sheets in interplanetary space was also briefly addressed. Coronal hole boundaries were defined as the abrupt transition from the bright appearing plasma sheet to the dark coronal hole regions. Observations in the inner corona seem to indicate a transition of typically 10 to 20 degrees, whereas observations in interplanetary space, carried out from Ulysses, show on one hand an even faster transition of less than 2 degrees which is in agreement with earlier Helios results. On the other hand, these observations also show that the transition happens on different scales, some of which are significantly larger. The slow solar wind is connected to the streamer belt/plasma sheet, even though the discussions were still not conclusive on the point where exactly the slow solar wind originates. Considered the high variability of plasma characteristics in slow wind streams, it seems most likely that several types of coronal regions produce slow solar wind, such as streamer stalks, streamer legs and open field regions between active regions, and maybe even regions just inside of the coronal holes. Observational and theoretical studies presented during the discussions show evidence that each of these regions may indeed contribute to the solar slow wind. This revised version was published online in June 2006 with corrections to the Cover Date.     

狭缝型接受孔对径向预旋系统的影响

为提高径向预旋系统温降减少系统的流动损失,运用数值模拟方法对比分析不同长宽比的狭缝型接受孔及传统直孔型接受孔对预旋系统温降流阻特性的影响。结果表明,随着狭缝长宽比在1~10范围内增加,接受孔有效流通面积增大,喷嘴出口气流流速及系统无量纲质量流量均增大;当旋转雷诺数大于2.6×106时,系统温降随着狭缝长宽比的增加而增加,总压损失随之先增加后趋于稳定。长宽比为6~10的狭缝型接受孔较传统直孔型接受孔有更高的温降及较高的压力损失。当旋转雷诺数等于7.9×106,长宽比为10的狭缝式接受孔较传统直孔接受孔系统温降系数增加36.7%,总压损失系数增加2.2%。     

基于结构参数分析的姊妹孔气膜冷却性能研究

以姊妹孔气膜冷却结构的偏转角度、倾斜角度和吹风比为因素,并以壁面平均气膜冷却效率为评价指标,应用田口方法设计了三因素五水平正交表,并结合数值计算对不同工况下的流场特征和冷却效率分布进行了分析。计算结果表明：高吹风比下姊妹孔冷却效率为常规圆柱孔冷却效率的165%~412.5%,正向10°偏转的姊妹孔冷却效率均大于负向10°偏转的姊妹孔冷却效率。参数化结果表明：吹风比为0.5、偏转角度为10°、倾斜角度为35°的结构表现出最佳冷却效果。