Longitudinal parameter identification of a small unmanned aerial vehicle based on modified particle swarm optimization

This paper describes a longitudinal parameter identification procedure for a small unmanned aerial vehicle(UAV)through modified particle swam optimization(PSO).The procedure is demonstrated using a small UAV equipped with only an micro-electro-mechanical systems(MEMS)inertial measuring element and a global positioning system(GPS)receiver to provide test information.A small UAV longitudinal parameter mathematical model is derived and the modified method is proposed based on PSO with selective particle regeneration(SRPSO).Once modified PSO is applied to the mathematical model,the simulation results show that the mathematical model is correct,and aerodynamic parameters and coefficients of the propeller can be identified accurately.Results are compared with those of PSO and SRPSO and the comparison shows that the proposed method is more robust and faster than the other methods for the longitudinal parameter identification of the small UAV.Some parameter identification results are affected slightly by noise,but the identification results are very good overall.Eventually,experimental validation is employed to test the proposed method,which demonstrates the usefulness of this method.     

Radiation driven winds of hot stars: Theory of O-star atmospheres as a spectroscopic tool

The status of the continuing effort to construct radiation driven wind models for O-Stars atmospheres is reviewed. Emphasis is given to several problems relating to the fomation of UV line spectra the use of accurate atomic data, the inclusion of EUV radiation by shock heated matter, the simulation of photospheric line blocking.A new tool for O-star diagnostics is presented. This is based on the use of wind models to calculate synthetic high resolution spectra covering the observable UV region. A comparison with observed spectra then gives physical constraints on the properties of stellar winds and stellar parameters, additionally abundances can be determined.The astrophysical potential of this method is demonstrated by an application to two Of-stars, the galactic O4f-star -Puppis and the LMC O3f-star Melnick 42. With regard to effective temperatures and gravities, the results from the application of classical methods to the analysis of photospheric lines are only partially verified. Explanations for the shortcomings of classical NLTE methods are discussed.     

Spectral analyses of Wolf-Rayet stars: Theory,results, conclusions

Stratified Non-LTE models for expanding atmospheres became available in the recent years. They are based on the idealizing assumptions of spherical symmetry, stationarity and radiative equilibrium. From a critical discussion we conclude that this standard model is basically adequate for describing real Wolf-Rayet atmospheres and hence can be applied for quantitative spectral analyses of their spectra.By means of these models, the fundamental parameters have been determined meanwhile for the majority of the known Galactic WR stars. Most of them populate a vertical strip in the Herzsprung-Russell diagram at effective temperatures of 35 kK, the luminosities ranging from 10^4.5 to 10^5.9 L . Only early-type WN stars with strong lines and WC stars are hotter. The chemical composition of WR atmospheres corresponds to nuclear-processed material (WN: hydrogen burning in the CNO cycle; WC: helium burning). Hydrogen is depleted but still detectable in the cooler part of the WN subclass.Different scenarios for the evolutionary formation of the Wolf-Rayet stars are discussed in the light of the empirical data provided from the spectral analyses. Post-red-supergiant evolution can principally explain the basic observational properties, except the rather low luminosities of a considerable fraction of WN stars. Among the alternative scenarios, close-binary evolution can theoretically produce the least-luminous WN stars. However, final conclusions about the evolutionary formation of the WR stars are not yet possible.     

带有转轮的空间转轴起落架理论图设计原理

 <正> 1.前言 飞机采用空间转轴起落架一般有两种型式,其中之一为A型(图1(a)),支柱与机轮等构件相对位置保持不变,一起绕空间轴收入起落架舱;另一种为B型(图1(b)),它有两部分运动:一是支柱绕空间轴运动,一是机轮随支柱转动的同时,再相对支柱的转轮运动。     

曲线曲面的若干几何处理基础算法研究

给出了实用的曲线曲面的离散、投影、直线－圆环求交，空间直线距离计算等算法，曲线用密切圆逼近，采用差商计算离散点参数，算法速度快，根据几何性质构造了点的投影及曲线投影跟踪算法，用拟牛顿法加大收敛范围，利用相关性减少迭代次数，采用矢量方法和局部坐标系技巧，如空间直线间距离计算，直线－圈环求交等常用算法十分简洁。     

Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters

There are hundreds of satellites operating at the geosynchronous (GEO) orbit where relativistic electrons can cause severe damage. Thus, predicting relativistic electron fluxes is significant for spacecraft safety. In this study, using GOES satellite data during 2011–2020, we propose two neural network models with two hidden layers to predict geosynchronous relativistic electron fluxes at two energy channels (>0.8 MeV and > 2 MeV). The number of input neurons of the two channels (>0.8 MeV and > 2 MeV) are determined to be 36 and 44, respectively. The > 0.8 MeV model has 22 and 9 neurons in the hidden layers, while the > 2 MeV model has 25 and 15 neurons in the hidden layers. The input parameters include the north–south component of the interplanetary magnetic field, solar wind speed, solar wind dynamic pressure and solar wind proton density. Through the analysis of different time delays, we determine that the optimal time delays of two energy channels (>0.8 MeV and > 2 MeV) are 8 days and 10 days, respectively. The training set and validation set (Jan 2011-Dec 2018) are divided by the 10-fold cross-validation method, and the remaining data (Jan 2019-Feb 2020) is used to analyze the model performance as a test set. The prediction results of both energy channels show good agreement with satellite observations indicated by low RMSE (～0.3 cm^-2sr^-1s^?1), high PE (～0.8) and CC (～0.9). These results suggest that only using solar wind parameters is capable of obtaining reasonable predictions of geosynchronous relativistic electron fluxes.     

不同制式三相电机电参数的测量方法

介绍一种用单片机实现测量三相电机各种电参数的系统。无论对三相三线还是三相四线制电机,系统软件都能对被测量硬件进行扫描检测,然后自动地采用不同的测量方法进行电参数测量。     

返回式卫星回收片盒壳体成形与缺陷消除

文章介绍了返回式卫星回收片盒壳体拉伸成形过程中平板毛坯设计、工艺参数、中间工序热处理工艺规范及产生缺陷的消除方法。     

电磁脉冲弹对雷达“前门”损伤研究

分析了电磁脉冲弹从"前门"损伤雷达的机理,给出了雷达"前门"电磁损伤判断公式,并提出了一些雷达系统"前门"电磁加固措施.可作为电磁脉冲弹威胁下雷达系统生存性研究和战场抢修研究的理论参考.     

高原发射地空导弹二级发动机点火参数计算

建立了高原条件下地空导弹二级发动机点火参数的计算模型。对地空导弹Ａ型及其改进后的Ｂ型两种导弹进行了，并通过了部队高原条件下的实弹打靶试验。试验的圆满成功雇地研究其它地空导弹高原条件下二级发动机点火性能具有参考价值。