Research on modeling of heat source for electron beam welding fusion-solidification zone

In this paper, the common heat source model of point and linear heat source in the numerical simulation of electron beam welding (EBW) were summarized and introduced. The combined point-linear heat source model was brought forward and to simulate the welding temperature fields of EBW and predicting the weld shape. The model parameters were put forward and regulated in the combined model, which included the ratio of point heat source to linear heat source Qpr and the distribution of linear heat source Lr. Based on the combined model, the welding temperature fields of EBW were investigated. The results show that the predicted weld shapes are conformable to those of the actual, the temperature fields are reasonable and correct by simulating with combined point-linear heat source model and the typical weld shapes are gained.     

爆轰胞格尺寸的统计分析

爆轰胞格尺寸作为可燃系统的本征值,可用来确定爆轰传播时的临界尺寸,比如直管传播时的临界管径、管道突扩时的临界尺寸等.然而,该尺寸的测量具有较强的主观性.为了减少人工测量带来的不确定性,文章采用两种统计方法:概率密度函数法和自相关函数法,对数值模拟得到的不同规则程度的爆轰胞格进行了统计分析.爆轰胞格的不规则程度采用单步反...     

切向结构永磁同步电机极对数的选择

对于具有“聚磁”作用的切向结构永磁同步电机,增加极对数可以提高气隙磁密,使得电机体积减小、重量减轻,效率、转矩增大,但极对数的增加存在一个较为合理的值。本文定义了切向结构永磁同步电机“聚磁”的概念,并利用有限元分析软件讨论了极对数与气隙磁密、每极磁通、空载电势、转子导磁体磁密等物理量之间的关系。结论:(1)计及导磁材料饱和的情况下,气隙磁密和总磁通随极对数的增加存在一个最大值,即存在一个合理的极对数;(2)用气隙磁密Bδ与稀土永磁体的内磁感应强度BM之比来表示聚磁作用的程度时,极对数大于等于3时,电机具有聚磁能力;用Bδ与稀土永磁体的剩磁感应强度Br之比来表示聚磁作用的程度时,仅当极对数大于等于4时,切向结构永磁电机才显现出聚磁现象;(3)切向结构永磁电机极对数在3~6时较为合适。     

Influence of welding parameters on microstructure and mechanical properties of electron beam welded Ti60 to GH3128 joint with a Cu interlayer

Effects of welding parameters on the microstructure and mechanical properties of Ti/Cu/Ni joint welded by electron beam were investigated. High welding heat input increased the melting quantity of Ti60 titanium alloy and promoted the formation of Ti–Cu intermetallic compounds (IMC) such as Ti₂Cu and Ti₃Cu₄, increasing the brittleness of the joints. Low welding heat input was not conducive to the complete melting of the copper interlayer, and the unmelted copper reduced the performance of the joints. Under the optimal welding parameters, Ti–Ni IMCs in the weld would be replaced by (Cu, Ni) solid solutions ((Cu, Ni)_ss). However, Ti–Cu IMC layers cannot be eliminated entirely by changing the welding parameters. The maximum tensile strength of the joints was 201 MPa. The fracture of the joints occurred at the Ti–Cu IMC layer, which was a typical brittle fracture.     

用差分法处理相关性测量数据方法探讨

当测量参数（或称测量元素）具有强相关性时,运用测量求差法解算测量结果,能消除相关性误差因素的影响,获得高精度测量结果,如电影望远镜同帧画幅测量脱靶量.基于此,运用测量方法和数学手段构建一个虚拟的元素相关测量系统,以消除相关性误差因素的影响,同样能获得理想结果.用多台测速雷达组成的系统,可使火炮弹丸空间坐标的测量精度达到毫米量级,从而满足多种火炮立靶密集度的测量精度要求.     

扇形叶栅通道中密度比和流量比对叶片表面全气膜冷却特性的影响

为了研究扇形通道中真实三维弯扭导向叶片全气膜冷却特性,本文采用压敏漆(PSP)测试技术实验测量了叶片全气膜冷却效率,获得了不同密度比(1、1.5)和质量流量比(9.71%、11.64%、12.47%)对叶片全气膜冷却效率的影响规律,结果表明：低密度比条件下,随着出流比增加,叶片压力面侧气膜冷却效率逐渐增加,叶片吸力面侧靠近前缘区域气膜孔下游的冷却效率减小；密度比增加可以使叶片整体气膜冷却效率提高,其中压力面前侧靠近前缘区域的冷却效率提高最为明显,最多提高了182%；高密度比条件下,增加出流比仅会使得压力面侧-0.8< S/C <0气膜冷却效率小幅度增加。     

Statistical study of energetic electrons in Jupiter’s inner magnetosphere by Juno/JEDI

The Juno spacecraft made the first in-situ observations of energetic particles in the polar region of Jupiter’s magnetosphere. After Jupiter Orbit Insertion (JOI) in July 2016, data from ~20 Juno perijoves (PJs) obtained by Juno/JEDI are accumulated, providing an excellent opportunity to study the long term spatio-temporal distribution of energetic particles in Jupiter’s radiation belt. We transform Juno’s position from a Cartesian to a magnetic coordinate system by tracing magnetic field lines based on a fourth order Runge-Kutta method. Then the fluxes of energetic electrons from PJ1 to PJ14 sorted by different locations in magnetic coordinate space and the data are well organized by the L-shell parameter. The variation of electron flux increases with L-shell. The deviation (the ratio of the 75th percentile to the 25th percentile) of 0.51 MeV electron flux varies from a factor of 1.23 near L = 9.5 to 27.57 near L = 15.5. However, the mean flux decreases by about one order of magnitude in the same region. The electron spectra at larger L-shells are softer than that at smaller L-shells. On the other hand, the electron flux decreases more rapidly with increased L-shell when the location is off the equator. Along an L-shell, the electron flux decrease at first and then increase again from equator to mid-latitude region. In addition, we compare the statistical results with the widely used GIRE2 model. JEDI data correspond well with the GIRE2 model when the L-shell is > 14.75. GIRE2 underestimate the electron flux for L-shell smaller than 13.25. These results of this analysis are applicable to estimate the effects of the radiation environment in Jupiter’s magnetosphere.     

轮廓度约束下近净成形叶片余量优化方法

针对近净成形的叶片在自适应精加工中余量不均这一问题,提出了考虑叶型截面线轮廓度公差约束的余量优化方法。在设计基准与加工基准配准的条件下,改变工件做刚性位移的余量优化思路,建立一种新的叶身优化模型,避免优化后叶片检测处的截面线超出轮廓度公差,提升叶片余量优化阶段寻找到目标加工曲面的能力。最后以某压气机叶片为例进行验证,此方法不仅能够保证叶身加工余量,还能同时满足型面检测处的轮廓度公差,为近净成形的叶片在自适应加工中提供一种新的余量优化方法。     

A Partially Orthogonal EnKF approach to atmospheric density estimation using orbital debris

A key requirement for accurate trajectory prediction and space situational awareness is knowledge of how non-conservative forces affect space object motion. These forces vary temporally and spatially, and are driven by the underlying behavior of space weather particularly in Low Earth Orbit (LEO). Existing trajectory prediction algorithms adjust space weather models based on calibration satellite observations. However, lack of sufficient data and mismodeling of non-conservative forces cause inaccuracies in space object motion prediction, especially for uncontrolled debris objects. The uncontrolled nature of debris objects makes them particularly sensitive to the variations in space weather. Our research takes advantage of this behavior by utilizing observations of debris objects to infer the space environment parameters influencing their motion.The hypothesis of this research is that it is possible to utilize debris objects as passive, indirect sensors of the space environment. We focus on estimating atmospheric density and its spatial variability to allow for more precise prediction of LEO object motion. The estimated density is parameterized as a grid of values, distributed by latitude and local sidereal time over a spherical shell encompassing Earth at a fixed altitude of 400 km. The position and velocity of each debris object are also estimated. A Partially Orthogonal Ensemble Kalman Filter (POEnKF) is used for assimilation of space object measurements to estimate density.For performance comparison, the scenario characteristics (number of objects, measurement cadence, etc.) are based on a sensor tasking campaign executed for the High Accuracy Satellite Drag Model project. The POEnKF analysis details spatial comparisons between the true and estimated density fields, and quantifies the improved accuracy in debris object motion predictions due to more accurate drag force models from density estimates. It is shown that there is an advantage to utilizing multiple debris objects instead of just one object. Although the work presented here explores the POEnKF performance when using information from only 16 debris objects, the research vision is to utilize information from all routinely observed debris objects. Overall, the filter demonstrates the ability to estimate density to within a threshold of accuracy dependent on measurement/sensor error. In the case of a geomagnetic storm, the filter is able to track the storm and provide more accurate density estimates than would be achieved using a simple exponential atmospheric density model or MSIS Atmospheric Model (when calm conditions are assumed).     

Detection of the ionospheric disturbances on GPS-TEC using Differential Rate Of TEC (DROT) algorithm

The solar, geomagnetic, gravitational and seismic activities can cause spatial and temporal (hourly, diurnal, seasonal and annual) variabilities of the ionosphere. Main observable ionospheric parameters such as Total Electron Content (TEC) can be used to quantify these. TEC is the total number of electrons on a ray path crossing the atmosphere. The network of world-wide Global Positioning System (GPS) receivers provide a cost-effective solution in estimating TEC over a significant proportion of global land mass. This study is focused on the analysis of the variations of ionosphere over a midlatitude region using GPS-TEC estimates for three Sun Spot Numbers (SSN) periods. The investigation is based on a fast and automatic variability detection algorithm, Differential Rate Of TEC (DROT). The algorithm is tested using literature data on disturbances generated by a geomagnetic activity, a Solar Flare, a Medium Scale Travelling Ionospheric Disturbance (MSTID), a Large Scale TID (LSTID) and an earthquake. Very good agreement with the results in the literature is found. DROT is applied to IONOLAB-TEC estimates from nine Turkish National Permanent GPS Network (TNPGN Active) stations over Turkey to detect the any wave-like oscillations, sudden disturbances and other irregularities during December, March, June, September months for 2010, 2011, 2012 years. It is observed that DROT algorithm is capable of detecting both small and large scale variability due to climatic, gravitational, geomagnetic and solar activities in all layers of ionosphere. The highest DROT values are observed in 2010 during winter months. In higher solar activity years of 2011 and 2012, DROT is able to indicate both seasonal variability and severe changes in ionosphere due to increased number of geomagnetic storms and local seismic activities.