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31.
娄淑慧 《南京航空航天大学学报》1990,(4)
本文介绍用于DGR-5A五自由度电动机器人关节伺服回路的脉宽调速系统。主要介绍脉宽调制型功率放大的工作原理及设计方法,同时简要介绍关节伺服回路的设计。 相似文献
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介绍了利用6个特征参数对7种数字调制方式进行调制方式的自动识别模型算法及仿真结果,表明所提出的自动识别算法能够很好的识别出各种数字调制信号,同时具备算法简单、速度快和准确率高的优点。 相似文献
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电磁干扰的产生及PCB设计中的抑制方案 总被引:1,自引:0,他引:1
电磁兼容性(EMC)常是制约设备间匹配性和正常性能实现的重要因素,因此电磁兼容性设计也是航天器设计中要考虑的关键因素。文章主要介绍了电磁干扰的产生原因,并从合理布局与布线、电容的设计、逻辑电路的使用等方面论述了如何在印制电路板(PCB)设计过程中减少电磁干扰。 相似文献
37.
残余载波调制是卫星测控中的常用调制体制。文章从理论上给出了该体制下信号的功率谱密度表达式,得到奇次谐波谱线展宽等结论,并通过仿真和实验进行了验证。利用所得结论讨论了遥测调制度测量方法,提出通过功率谱的2阶边带进行测量可以使结果得到改善。 相似文献
38.
H.S. Ahluwalia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u. 相似文献
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H. Krüger H. Moraal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
This paper is a follow-on of that of Krüger et al. [Krüger, H., Moraal, H., Bieber, J.W., Clem, J.M., Evenson, P.A., Pyle, K.R., Duldig, M.L., Humble, J.E. A calibration neutron monitor: energy response and instrumental temperature sensitivity. J. Geophys. Res. 113, A08101, doi:10.1029/2008JA013229, 2008], that describes the characteristics of a pair of calibration neutron monitors that were developed to intercalibrate the count rates of the world’s neutron monitors against each other. Such an intercalibration will allow the calculation of energy (rigidity) spectra, which will enhance the quality of the neutron monitor data. Krüger et al. (2008) investigated the energy and temperature response of the calibrators. This paper studies the statistical accuracy of the calibration procedure, its repeatability, and the sensitivity to its environment. The paper concludes with a calibration procedure that can minimise the uncertainties caused by these five effects, or at least correct for them. 相似文献
40.
H.S. Ahluwalia C. Lopate 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5. 相似文献