An adaptive turbo-shaft engine modeling method based on PS and MRR-LSSVR algorithms

In order to establish an adaptive turbo-shaft engine model with high accuracy, a new modeling method based on parameter selection (PS) algorithm and multi-input multi-output recursive reduced least square support vector regression (MRR-LSSVR) machine is proposed. Firstly, the PS algorithm is designed to choose the most reasonable inputs of the adaptive module. During this process, a wrapper criterion based on least square support vector regression (LSSVR) machine is adopted, which can not only reduce computational complexity but also enhance generalization performance. Secondly, with the input variables determined by the PS algorithm, a mapping model of engine parameter estimation is trained off-line using MRR-LSSVR, which has a satisfying accuracy within 5&. Finally, based on a numerical simulation platform of an integrated helicopter/ turbo-shaft engine system, an adaptive turbo-shaft engine model is developed and tested in a certain flight envelope. Under the condition of single or multiple engine components being degraded, many simulation experiments are carried out, and the simulation results show the effectiveness and validity of the proposed adaptive modeling method.     

一种转台角位置定位精度检测方法

角位置定位精度和速率精度是转台产品的最主要两项技术指标,转台产品均需检测。其中角位置精度检测方法的操作步骤多,影响因素多。本文从角位置精度的检测方法,检测步骤和检测技巧等方面进行初步的剖析,重点阐述用24面体进行位置精度检定中的过程与方法。     

Ionospheric electron density over Resolute Bay according to E-CHAIM model and RISR radar measurements

In this study, predictions of the E-CHAIM ionospheric model are compared with measurements by the incoherent scatter radars RISR at Resolute Bay, Canada, in the northern polar cap. Reasonable coverage was available for all seasons except winter for which no conclusions were drawn. It is shown that ratios of the model-to measured electron densities are close to unity in the central part of the F layer, around its peak. This is particularly evident for summer daytime. Distributions of the ratios are wider for other seasons indicating larger number of cases when the model underestimates or overestimates. E-CHAIM underestimates the electron density at ionospheric topside and bottomside by ～ 10–20 %. At the bottomside, the underestimations are strongest in summer and equinoctial nighttime. At the topside, the underestimations are strongest in autumn nighttime. Model overestimations are noticeable in the middle part of the F layer during dawn hours in autumn. Overall, the model tends to not predict highest-observed peak electron densities and the largest-observed heights of the peak.     

Testing the three-dimensional IRI-SIRMUP-P mapping of the ionosphere for disturbed periods

This paper describes the three-dimensional (3-D) electron density mapping of the ionosphere given as output by the assimilative IRI-SIRMUP-P (ISP) model for three different geomagnetic storms. Results of the 3-D model are shown by comparing the electron density profiles given by the model with the ones measured at two testing ionospheric stations: Roquetes (40.8°N, 0.5°E), Spain, and San Vito (40.6°N, 17.8°E), Italy. The reference ionospheric stations from which the autoscaled foF2 and M(3000)F2 data as well as the real-time vertical electron density profiles are assimilated by the ISP model are those of El Arenosillo (37.1°N, 353.3°E), Spain, Rome (41.8°N, 12.5°E), and Gibilmanna (37.9°N, 14.0°E), Italy. Overall, the representation of the ionosphere made by the ISP model is better than the climatological representation made by only the IRI-URSI and the IRI-CCIR models. However, there are few cases for which the assimilation of the autoscaled data from the reference stations causes either a strong underestimation or a strong overestimation of the real conditions of the ionosphere, which is in these cases better represented by only the IRI-URSI model. This ISP misrepresentation is mainly due to the fact that the reference ionospheric stations covering the region mapped by the model turn out to be few, especially for disturbed periods when the ionosphere is very variable both in time and in space and hence a larger number of stations would be required. The inclusion of new additional reference ionospheric stations could surely smooth out this concern.     

单轴台的大角度姿态快速机动联合控制方法

为验证小卫星大角度姿态快速机动与高精度稳定控制能力,基于单轴气浮台硬件仿真环境,提出了一种利用推力器与飞轮组合的联合控制策略.采用相平面控制技术与有限时间控制理论设计控制器,利用推力器实现无超调的快速机动控制,利用飞轮实现有限时间内的高精度稳定控制,使单轴台在有限时间内快速高精度稳定于目标姿态.物理仿真结果表明:该方法在有限时间内完成单轴台快速稳定控制的同时,可有效避免机动过程中的超调现象,且能有效规避推力器的频繁开关与飞轮的过快饱和等问题.     

体现主客方校准法的塔式垂准仪校准装置

介绍了基于顶杆原理的主客方校准法;叙述了以三轴重合为功能设计重点、以天顶天底和屋顶地面照准标融为一体为主线、可见光与激光校准项目有机结合的实现主客方校准法的校准装置设计思路与构建原则。最后,给出了装置复现的准铅垂线的准确度分析。     

在轨服务的相对运动耦合动力学建模与分析

研究在轨服务航天器逼近与捕获目标航天器的相对轨道姿态耦合动力学建模问题。考虑航天器姿态与对接位置的运动耦合,建立目标运行在任意轨道下的相对轨道姿态耦合动力学模型,并对模型中的运动耦合进行深入分析。设计一种非线性的输出反馈姿态控制律,将建立耦合动力学模型与CW方程进行仿真比较,验证轨道与姿态的运动耦合对两航天器对接点之间相对位置的运动影响。     

卫星遥感影像外方位元素的误差传播研究

高分辨率卫星遥感影像的几何定位精度与影像外方位元素精度密切相关.文章针对单景影像直接对地定位和立体影像前方交会定位两种典型情况,对影像各外方位元素在目标几何定位中的误差传播规律进行分析比较,相关结论可供卫星姿控及相机载荷设计方参考.     

基于刃边法的星载相机在轨MTF测量精度分析

调制传递函数(MTF)反映可见光对地遥感系统在对地物成像过程中信号的扩散与削弱程度,是表达系统辐射性能的重要指标.文章对星载可见光CCD相机在轨MTF主要测量方法进行比对分析,通过数据仿真,重点对随机噪声、边缘探测与拟合等主要影响刃边法精度的因素进行了分析.分析结果表明,计算所用刃边法能够较准确地计算可见光遥感系统的M...     

大功率舰船燃气轮机压气机增容模化设计研究

某重点项目的船用燃气轮机领域提出了更高等级功率燃气轮机的要求。为了在研制周期内快速设计一型压气机,以现有机型为母型机进行模化设计,在母型机特性图上合理选择模化点,确定模化比,得到增容后模化机的叶片和几何通流结构,划分网格时,充分考虑叶顶间隙、倒角、引气孔、梳齿密封等,以更接近于工程实际情况,对模化机进行全三维数值模拟计算,结果表明,模化机设计点性能指标达到要求,非设计工况喘振裕度基本与母型机相同,模化后叶顶相对间隙的降低会带来阻塞点流量的升高、失速点流量的降低,导致低转速下喘振裕度的升高和高转速下喘振裕度的降低。总体来说,模化增容设计继承了母型机优良的气动性能,为快速、高效研发新机型提供宝贵经验。