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941.
942.
为了在无刷直流电机发生轴承故障早期检测出轴承故障特征,本文就无刷直流电机轴承故障信息的提取提出了一种新的方法。该方法选择电机的母线电流和三相电流最大值作为轴承故障信息的提取对象,避免了相电流由于谐波含量过大及不连续带来的诊断效果不佳的后果。同时,本文选择小波包算法作为轴承故障信号提取的方法,能够更好地对轴承故障信息进行辨识。实验结果证明,通过对母线电流和三相电流最大值进行小波包分解能够很好地进行无刷直流电机轴承故障信息的提取。 相似文献
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944.
D. Kuang S. DesaiA. Sibthorpe X. Pi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We present a method to estimate the total neutral atmospheric density from precise orbit determination of Low Earth Orbit (LEO) satellites. We derive the total atmospheric density by determining the drag force acting on the LEOs through centimeter-level reduced-dynamic precise orbit determination (POD) using onboard Global Positioning System (GPS) tracking data. The precision of the estimated drag accelerations is assessed using various metrics, including differences between estimated along-track accelerations from consecutive 30-h POD solutions which overlap by 6 h, comparison of the resulting accelerations with accelerometer measurements, and comparison against an existing atmospheric density model, DTM-2000. We apply the method to GPS tracking data from CHAMP, GRACE, SAC-C, Jason-2, TerraSAR-X and COSMIC satellites, spanning 12 years (2001–2012) and covering orbital heights from 400 km to 1300 km. Errors in the estimates, including those introduced by deficiencies in other modeled forces (such as solar radiation pressure and Earth radiation pressure), are evaluated and the signal and noise levels for each satellite are analyzed. The estimated density data from CHAMP, GRACE, SAC-C and TerraSAR-X are identified as having high signal and low noise levels. These data all have high correlations with anominal atmospheric density model and show common features in relative residuals with respect to the nominal model in related parameter space. On the contrary, the estimated density data from COSMIC and Jason-2 show errors larger than the actual signal at corresponding altitudes thus having little practical value for this study. The results demonstrate that this method is applicable to data from a variety of missions and can provide useful total neutral density measurements for atmospheric study up to altitude as high as 715 km, with precision and resolution between those derived from traditional special orbital perturbation analysis and those obtained from onboard accelerometers. 相似文献
945.
自转旋翼机飞行性能理论建模技术 总被引:2,自引:0,他引:2
为研究自转旋翼机的飞行性能理论建模技术,基于基本分析法和配平分析法,对自转旋翼机整机需用功率的建模方法进行了研究,并研究了自转旋翼机的桨盘迎角特性、升阻特性以及自转旋翼桨叶剖面迎角分布特性等。研究表明:建立的基本分析法和配平分析法计算模型均可以准确计算自转旋翼机的整机需用功率和自转旋翼桨盘迎角,两种方法均可用于自转旋翼机飞行性能的分析;小速度时整机需用功率主要来自于自转旋翼功率,大速度时机身废阻功率成为整机需用功率的主要来源;适当增加总距可以提高自转旋翼和整机的升阻比;在自转旋翼设计时可以对桨叶剖面翼型的展向分布进行优化,在桨根处优先采用相对不易失速的翼型以推迟失速对最大飞行速度的限制。 相似文献
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947.
赵玉梅 《北华航天工业学院学报》2011,21(6):21-25
农业特色产业作为新的经济增长点,并且日益成为目前农村经济发展面临的新课题和拉动内需的新机遇。同时也应该看到,由于长期不合理的盲目开发等原因,农业生态环境恶化和自然资源紧缺的问题日益严峻,生态农业问题的提出是农业经济可持续发展的必然。本文结合河北省农业特色产业的发展现状,总结其存在的问题,分析河北省农业特色产业集群的可行... 相似文献
948.
刘建英 《中国民航学院学报》1998,16(5):22-28
介绍了自动控制领域内的一种新型控制方法——滑模变结构控制(SMVSS),并以8031单片机作控制器,在一台直流力矩电动机上实施了定位控制,从而证实了该算法对时变系统的有效性。 相似文献
949.
C.L. Stokely E.G. Stansbery R.M. Goldstein 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The continual monitoring of the low Earth orbit (LEO) debris environment using highly sensitive radars is essential for an accurate characterization of these dynamic populations. Debris populations are continually evolving since there are new debris sources, previously unrecognized debris sources, and debris loss mechanisms that are dependent on the dynamic space environment. Such radar data are used to supplement, update, and validate existing orbital debris models. NASA has been utilizing radar observations of the debris environment for over a decade from three complementary radars: the NASA JPL Goldstone radar, the MIT Lincoln Laboratory (MIT/LL) Long Range Imaging Radar (known as the Haystack radar), and the MIT/LL Haystack Auxiliary radar (HAX). All of these systems are highly sensitive radars that operate in a fixed staring mode to statistically sample orbital debris in the LEO environment. Each of these radars is ideally suited to measure debris within a specific size region. The Goldstone radar generally observes objects with sizes from 2 mm to 1 cm. The Haystack radar generally measures from 5 mm to several meters. The HAX radar generally measures from 2 cm to several meters. These overlapping size regions allow a continuous measurement of cumulative debris flux versus diameter from 2 mm to several meters for a given altitude window. This is demonstrated for all three radars by comparing the debris flux versus diameter over 200 km altitude windows for 3 nonconsecutive years from 1998 to 2003. These years correspond to periods before, during, and after the peak of the last solar cycle. Comparing the year to year flux from Haystack for each of these altitude regions indicate statistically significant changes in subsets of the debris populations. Potential causes of these changes are discussed. These analysis results include error bars that represent statistical sampling errors. 相似文献
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