HS—19型肖氏硬度计故障分析

从结构原理来分析故障的产生、发展、现象以及产生故障的排除方法。     

桥函数理论的研究进展

叙述了从研究沃尔什函数的复制理论和方块脉冲函数移位方法出发，推出桥函数的构造过程，桥函数把工程中常用的沃尔什函数和方块脉冲函数这两种似乎不相关的函数联系了起来，本文详细地给出了四种桥函数的构造过程和它们的波形。     

情感因素对语言学习的影响

情感因素对语言学习具有重大的影响。在学生智商水平相当的情况下,情感差异会导致学生学习成绩的高低之分。情感差异是由家庭、环境、情趣、学习方法等综合因素造成的。积极的情感会对学生的学习起到促进作用；反之,消极的情感则会阻碍学生的学习。教师在教学中应善于引导学生,促进学生积极情感的产生,减少消极情感的作用,以提高教学效果。     

A multi-aircraft conflict detection and resolution method for 4-dimensional trajectory-based operation

Conflict Detection and Resolution(CDR) is the key to ensure aviation safety based on Trajectory Prediction(TP). Uncertainties that affect aircraft motions cause difficulty in an accurate prediction of the trajectory, especially in the context of four-dimensional(4D) Trajectory-Based Operation(4DTBO), which brings the uncertainty of pilot intent. This study draws on the idea of time geography, and turns the research focus of CDR from TP to an analysis of the aircraft reachable space constrained by 4D waypoint constraints. The concepts of space–time reachability of aircraft and space–time potential conflict space are proposed. A novel pre-CDR scheme for multiple aircraft is established. A key advantage of the scheme is that the uncertainty of pilot intent is accounted for via a Space-Time Prism(STP) for aircraft. Conflict detection is performed by verifying whether the STPs of aircraft intersect or not, and conflict resolution is performed by planning a conflict-free space–time trajectory avoiding intersection. Numerical examples are presented to validate the efficiency of the proposed scheme.     

Statistical study of the time delay of ionospheric TEC storms to geomagnetic storms in Taoyuan,Taiwan

We have studied the time delay of ionospheric storms to geomagnetic storms at a low latitude station Taoyuan (25.02°N, 121.21°E), Taiwan using the Dst and TEC data during 126 geomagnetic storms from the year 2002 to 2014. In addition to the known local time dependence of the time delay, the statistics show that the time delay has significant seasonal characteristics, which can be explained within the framework of the seasonal characteristics of the ionospheric TEC. The data also show that there is no correlation between the time delay and the intensity of magnetic storms. As for the solar activity dependence of the time delay, the results show that there is no relationship between the time delay of positive storms and the solar activity, whereas the time delay of negative storms has weakly negative dependence on the solar activity, with correlation coefficient −0.41. Especially, there are two kinds of extreme events: pre-storm response events and long-time delay events. All of the pre-storm response events occurred during 15–20 LT, manifesting the Equator Ionospheric Anomaly (EIA) feature at Taoyuan. Moreover, the common features of the pre-storm response events suggest the storm sudden commencement (SSC) and weak geomagnetic disturbance before the main phase onset (MPO) of magnetic storms are two main possible causes of the pre-storm response events. By analyzing the geomagnetic indices during the events with long-time delay, we infer that this kind of events may not be caused by magnetic storms, and they might belong to ionospheric Q-disturbances.     

Mechanism of error propagation from the subdaily Universal Time model into the celestial pole offsets estimated by VLBI

Within the analysis of space geodetic observations, errors of the applied subdaily Earth rotation model can induce systematic effects in different estimated parameters. In this paper, we focus on the impact of the subdaily Universal Time (UT1) model on the celestial pole offsets (CPO) estimated from very long baseline interferometry (VLBI) observations. We provide a mechanism that describes the error propagation from the subdaily UT1 into the daily CPO.In typical 24-h VLBI sessions the observed quasars are well distributed over the sky. But the observations, if looked at from the Earth-fixed frame, are not homogeneously distributed. The amount of observations performed in different terrestrial directions shows an irregularity which can be roughly compared to the case where the observations are collected in only one Earth-fixed direction. This peculiarity leads to artefacts in VLBI solutions, producing a correlation between the subdaily variations in UT1 and the position of the celestial pole. As a result errors in diurnal terms of the subdaily UT1 model are partly compensated by the estimated CPO. We compute for each 24-h VLBI session from 1990 until 2011 the theoretical response of the CPO to an error in the subdaily UT1 by setting up a least-squares adjustment model and using as input the coordinates of the observed quasars and observation epochs. Then real observed response of the estimated CPO derived from the VLBI session solutions is compared to the predicted one. A very good agreement between the CPO values estimated from VLBI and the predicted values was achieved. The presented model of error propagation from the subdaily UT1 into the daily CPO allows to predict and explain the behaviour of CPO estimates of VLBI solutions computed with different subdaily Earth rotation models, what can be helpful for testing the accuracy of different subdaily tidal models.     

Passive localization by a single moving observer using TOA only with unknown SRI: Observability analysis and algorithm

Passive localization by a single moving observer using Time of Arrival (TOA) only with an unknown Signal Repetition Interval (SRI) is investigated in this paper. Observability analysis is performed first. The observability condition for uniquely determining the emitter position and SRI is derived. The conditional Cramer-Rao Lower Bound (CRLB) is also analyzed. It is found that the ambiguity of the SRI integer of the first TOA does not affect the theoretical estimation precision of the emitter position and SRI. A Reference-Fixed Differential TOA (RFDTOA)-based Iterative Maximum Likelihood Estimator (IMLE) is proposed, which only needs O(M) computational operations. Theoretical analysis and simulation results show that the Mean Square Error (MSE) of the proposed algorithm could attain the CRLB with moderate Gaussian measurement noise.     

一种基于随机优化算法的民用飞机突风动载荷重建方法

民用飞机突风载荷的准确重建对于飞行安全具有十分重要的意义。基于随机优化算法,提出一种突风动载荷重建方法。首先,基于频域气弹耦合方程,建立一个突风动载荷时域分析模型,其次,引入Hicks-Henne 型函数进行突风速度场的参数化建模,在此基础上,基于随机优化算法对各型函数参数进行迭代寻优,使得优化目标值与测量值一致,最终得到重建后的突风速度及对应的动态响应及载荷。最后,以GTA 模型经历1-cos 形状突风为例进行数值仿真。结果表明：本文提出的突风动载荷重建方法可有效实现突风速度场的识别,进而完成突风动载荷的重建;针对本文算例,过载最大误差为3.5%,载荷最大误差不超过1%。     

复杂构形的亚、跨、超音速定常及非定常气动力的Green函数算法综述

对亚、跨、超音速定常及非定常气动力的 Green函数算法作了简要回顾 ,包括该方法的基本原理、近年来在国内的发展及其在气动弹性和气动载荷计算中的应用等。算例表明该方法适用范围广、计算效率高且比较准确     

求解非定常空气动力系数主导极点的近似方法

在计算与风洞实验的基础上, 提出了机翼剪切翼梢气动布局, 对平面形状与翼型进行了 优化设计, 达到了巡航状态与爬升阶段较高的增升减阻要求。计算采用涡格面元法与涡升力展向 分布吸力比拟法相结合的方法, 既能考虑气动力的非线性因素, 又有较高的计算精度与速度。计 算结果与实验数据十分吻合。通过分析得到, 在矩形翼翼梢处增加具有较大前缘后掠角的梯形剪 切翼梢有不仅增加机翼展弦比, 且可改变展向环量分布, 使其接近椭圆分布; 剪切翼梢上的前缘 涡可抑制翼端涡的作用(使翼端涡强度变弱) , 并在剪切翼梢上产生附加升力。