Microstructure,porosity and mechanical properties of selective laser melted AlSi10Mg

Finite element modeling (FEM), microscopy, X-ray computed tomography (CT) and mechanical property tests were used to study the microstructure, porosity and mechanical properties of an AlSi10Mg alloy produced by selective laser melting (SLM). The simulation of the melt pool and thermal history under different energy densities produced an optimized result with an energy density of 44.5 J·mm⁻³. The high cooling rate during the SLM process significantly refined the previous α-Al dendrites. The growth direction of the network-like Al-Si eutectic structure at different orientations confirmed the anisotropic nature of the microstructure. Furthermore, the microhardness, tensile testing and fracture analysis results proved that there were no obvious distinctions in the strength between the transverse and longitudinal directions, and that the ductility was anisotropic, possibly due to the shape and distribution of the pores. The pores measured by X-ray CT at different energy densities confirmed that the sphericity of the pores was inversely related to pores volumes. With optimized processing conditions, the porosity of the selective laser melted sample decreased leading to the improved fabricated fuel system component via SLM.     

10cm氙离子推力器变推力特性研究

非重力阻尼的连续、快速、高精度补偿是实现重力梯度测量卫星精细重力场测量的关键技术之一,直接影响到整星工程任务的成败。针对重力梯度测量卫星在轨飞行期间对电推进系统宽范围连续变推力能力的应用需求,分析了10cm氙离子推力器推力调节响应特性。在此基础上,通过对阳极电流、励磁电流和阳极流率等推力高敏感响应参量的组合调节,开展了推力调节试验研究,验证了10cm氙离子推力器宽范围连续变推力调节能力,获得了1～20mN范围内的推力调节性能及其变化规律。试验结果表明：在采用地面供电、供气设备条件下,10cm氙离子推力器能够在100～597W的功率范围内实现0.98～20.29mN的推力宽范围调节,比冲175～3500s,推力分辨率优于50μN。研究为建立10cm氙离子电推进系统的推力控制数学模型及调节控制算法奠定基础。     

Zn含量对Mg-10Gd-4.8Y-0.6Zr合金组织和力学性能的影响

采用显微硬度和力学性能测试及金相显微镜、扫描电镜、透射电镜、X射线衍射等分析手段,研究了Zn含量对Mg-10Gd-4.8Y-0.6Zr合金挤压以及时效处理后合金组织和力学性能的影响。结果表明,在Mg-10Gd-4.8Y-0.6Zr合金中添加Zn元素,有利于细化合金晶粒,提高挤压态的强度。未添加Zn的合金T5态晶粒尺寸约为25μm,添加1%(质量分数,下同)Zn后,晶粒尺寸约为15μm,Zn含量为3%时,晶粒尺寸约为10μm。当Zn含量为1%时,合金挤压态和时效态的抗拉强度分别为337MPa,397MPa,屈服强度分别为128MPa,148MPa,伸长率分别为10.0%,5.0%,具有较好的综合性能。     

Missions to Mercury

Mercury is a very difficult planet to observe from the Earth, and space missions that target Mercury are essential for a comprehensive understanding of the planet. At the same time, it is also difficult to orbit because it is deep inside the Sun’s gravitational well. Only one mission has visited Mercury; that was Mariner 10 in the 1970s. This paper provides a brief history of Mariner 10 and the numerous imaginative but unsuccessful mission proposals since the 1970s for another Mercury mission. In the late 1990s, two missions—MESSENGER and BepiColombo—received the go-ahead; MESSENGER is on its way to its first encounter with Mercury in January 2008. The history, scientific objectives, mission designs, and payloads of both these missions are described in detail.     

表面处理对17-4PH不锈钢抗固体粒子冲蚀性能的影响

为对比研究表面处理对17-4PH不锈钢抗固体粒子冲蚀性能的影响,在17-4PH不锈钢表面进行了多弧离子镀陶瓷/金属多层膜制备、激光表面合金化(LSA)处理和超音速火焰喷涂(HVOF)硬质合金层处理,利用划痕仪、自组装的不锈钢抗固体粒子冲蚀(SPE)装置、多冲疲劳试验机对上述三种表面处理试样的小攻角和大攻角SPE失效行为和机理进行了研究。结果表明,微切削是17-4PH不锈钢及其表面改性试样小攻角下固体粒子冲蚀破坏的主要失效机制,多冲型疲劳破坏是17-4PH不锈钢及其表面改性试样大攻角下固体粒子冲蚀的主要失效机制。HVOF WC-17Co涂层可显著提高17-4PH不锈钢30°小攻角和90°大攻角下SPE抗力。激光表面合金化层能够改善17-4PH不锈钢抗30°小攻角和90°大攻角下SPE性能,但SPE性能改善效果弱于HVOF喷涂涂层。TiAl N/Ti多层膜不能显著提高17-4PH不锈钢抗30°小攻角和90°大攻角的SPE性能。     

基于CPSO的UAV编队集结路径规划

针对多无人机编队集结路径规划问题,提出了具有合作机制的分布式协同粒子群(CPSO)算法。为了满足无人机运动学约束,采用曲率连续的PH曲线作为备选路径。基于协同进化思想提出CPSO算法,为每架无人机规划出一条满足机间协同约束的最优安全可飞行路径。仿真结果表明,规划得到的多条路径能够满足无人机运动学约束、安全性及无人机之间的协同性要求;相比于协同进化遗传算法,CPSO算法搜索成功率更高,稳定性更好。     

不同冶炼工艺对1Cr18Ni10Ti钢夹杂物的影响

通过试验研究了1Cr18Ni10Ti不锈钢的4种冶炼工艺:真空感应+电渣重熔、真空感应(陶瓷过滤器)、真空感应(陶瓷过滤器)+电渣重熔、真空感应+真空自耗,得到钢锭中夹杂物的种类、大小以及数量的变化.对比试验结果可知,采用真空感应(陶瓷过滤器)冶炼工艺与真空感应+真空自耗之后的钢锭的夹杂物水平相当,D类夹杂物数量最少,大颗粒夹杂物占比也最小.     

Near-infrared study of open clusters Teutsch 10 and Teutsch 25

The astrophysical parameters have been estimated for two unstudied open star clusters Teutsch 10 and Teutsch 25 using the Two Micron All Sky Survey ($2\mathit{MASS}$) database. Radius is estimated as 4.5 arcmin for both clusters using radial density profiles. We have estimated proper motion values in both RA and DEC directions as $2.28\pm 0.3$ and $-0.38\pm 0.11$?mas?yr^?1 for Teutsch 10 and $0.48\pm 0.3$ and $3.35\pm 0.16$?mas?yr^?1 for Teutsch 25 using $\mathit{PPMXL}$¹ catalog. By estimating the stellar membership probabilities, we have identified 30 and 28 most likely members for Teutsch 10 and Teutsch 25 respectively. We have estimated the reddening as $E(B-V)=0.96\pm 0.3$?mag for Teutsch 10 and $0.58\pm 0.2$?mag for Teutsch 25, while the corresponding distances are $2.4\pm 0.2$ and $1.9\pm 0.1$?kpc. Ages of $70\pm 10$?Myr for Teutsch 10 and $900\pm 100$?Myr for Teutsch 25 are estimated using the theoretical isochrones of metallicity Z?=?0.019. The mass function slopes are derived as $1.23\pm 0.30$ and $1.09\pm 0.35$ for Teutsch 10 and Teutsch 25 respectively. Estimated mass function slope for both the clusters are close to the Salpeter value ($x=1.35$) within the errors. Estimated values of dynamical relaxation time are found to be less than cluster’s age for these objects. This concludes that both objects are dynamically relaxed. The possible reason for relaxation may be due to dynamical evolution or imprint of star formation or both.     

基于FPGA的RS232转429接口电路的设计与实现

介绍用于自动控制设备控制板卡的软硬件设计方法,采用混合输入（包括SCH和VHDL）实现该设计,重点阐述应用ISP开发软件采用VHDL语言实现整个软件接收、控制部分,测试表明设计方法合理有效。     

激波管中测量JP-10点火延时的吸附问题研究

在JP-10点火延时的激波管实验中,JP-10在激波管壁的吸附导致气相浓度的不确定是测量结果分散的主要原因之一.利用精确测定的吸附曲线确定了实验时JP-10真实的气相浓度,解决了高碳数碳氢燃料点火延时激波管实验时管壁吸附影响燃料气相浓度确定的困难.实验显示JP-10的吸附符合Langmuir吸附等温关系.