Ultrasound assisted solidification process of ternary Cu–Sn–Sb alloy

It is well-known that the application of ultrasound during liquid to solid transitions for alloys can refine the solidification microstructure and thus improves the mechanical properties. How-ever, most published work focuses on single phase dendritic growth, whereas little has been con-ducted on the multiphase alloys with complicated phase transformations during solidification. In this work, the solidification process of ternary Cu40Sn45Sb15 alloy was realized within intensive ultra-sonic field with a resonant frequency of 20 kHz and ultrasound power from 0 W to 1000 W. The ultrasound refines the size of the primary e(Cu3Sn) intermetallic compound by two orders of mag-nitudes. If the ultrasound power increases to 1000 W, g(Cu6Sn5) phase nucleates and grows directly from parent liquid phase without the occurrence of peri-eutectic reaction on the top of the alloy sam-ple where the ultrasound intensity is sufficiently high. These microstructural variations lead to the enhancement of compressive strength and elasticity modulus of ternary Cu40Sn45Sb15 alloy.     

开式整体叶盘四坐标插铣开槽粗加工刀位轨迹规划

提出在开式整体叶盘的粗加工阶段,采用插铣加工代替传统的五轴数控加工点铣和侧铣,实现高效加工.提出将自由曲面蜕变为直纹面,将复杂自由曲面粗加工问题转化为简单的直纹面粗加工问题.这种方法的加工效率比传统加工方法提高约60%以上.     

页轮干式磨削Ti6Al4V合金

进行了Ti6A14V合金锆刚玉页轮和碳化硅页轮的磨削性能试验研究,分析了磨削用量对磨削力、磨削温度和磨削表面完整性的影响。磨削力通过KISTLER9265B测力仪测定,磨削表面温度由NIUSB-621X信号采集系统测得,磨削表面形貌和金相组织由HiroxKH-7700型体视显微仪和Quanta200型扫描电镜（SEM）观察,表面粗糙度由Mahr Perthometer M1粗糙度仪测得,表层显微硬度通过HVS—1000硬度计测定。研究结果表明：页轮磨削钛合金工件表面没有发生烧伤现象,磨削热影响区厚度小于50μm,锆刚玉页轮比碳化硅页轮更适合干式磨削钛合金。     

基于宏程序的外球面粗精加工

目前,小内存的数控机床仍然是我国机床的主流,使加工程序变得简洁,对实际加工有着很重要的意义.宏程序的应用可以大大简化编程,本文通过实例介绍了数控铣削加工外球面的宏程序.     

数控电解加工整体叶轮的关键技术

以平行直纹型面的数控展成电解加工为例，对数控电解加工整体叶轮的主要关键技术，包括成形规律、展成运动、数控编程、阴极设计制造、机库及多轴联动数控系统、典型叶轮加工工艺逐一进行了介绍。     

飞机整体结构件加工变形的有限元模拟与试验研究

在模拟淬火、拉伸过程获得含有初始残余应力的预拉伸板材以及模拟单齿切削过程获得切削载荷的基础上,提出并采用接力算法,对一航空整体结构件的材料铣削过程进行有限元仿真,同时进行了试验研究.结果表明,有限元模拟的整体结构件的变形与试验具有一致性,从而证明提出的整体结构件加工仿真关键技术的可行性,避免了为研究加工变形而进行的繁琐的试错法.     

Intelligent NURBS Interpolator Based on the Adaptive Feedrate Control

首先分析了NURBS曲线的特点和NURBS曲线插补的参数值的求取方法;其次,在可控弓高误差算法的基础上,提出了一种简单而实用的NURBS曲线的自适应插补算法,该算法充分考虑到了机床的实际加工能力,对曲线段进行提前预插补,提前预插补减速所需的最大插补周期数,实现了进给速度提前减速,能使加工进给速度自适应地随着曲率半径和曲率半径的变化率的变化而变化,使得加工运动更平滑;并且该方法还避免了因加工曲线终点的判断而带来的复杂计算;最后给出了快速求取插补点的三次NURBS曲线动态矩阵表示和曲线曲率的快速计算方法。     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.     

Galactic Wind: Mass Fractionation and Cosmic Ray Acceleration

The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×10¹⁸ eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall Cosmic Ray spectrum.     

精密超精密加工技术在微机械制造中的应用

随着微机电系统的发展,微机械零件的材料应用领域不断扩大,结构形状也从二维、准三维提高到三维复杂结构,相应的微机械制造技术也随之发展,并在微机械零件制造中得到了应用。