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排序方式: 共有151条查询结果,搜索用时 640 毫秒
31.
为得到弹目交会过程中超宽带无线电引信接收机的时域输出信号,实现高速交会条件下引信接收机的性能优化,推导了取样积分微分电路的时域数学模型,提出了一种基于无载波信号时域多普勒效应的接收机输出信号时域仿真方法.弹目接近速度对接收机输出信号的影响研究表明,输出信号频率与弹目接近速度成正比;信号幅度与弹目接近速度关系曲线存在速度驻点.选择合理的积分、微分电容可设置恰当的速度驻点,提高引信的抗干扰性能. 相似文献
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测量中单输入单输出线性系统动态数学模型定阶方法的仿真研究 总被引:2,自引:0,他引:2
针对测量中单输入单输出线性系统的动态建模问题,通过计算机数字仿真,对现有的几种定阶方法进行了研究、分析,比较了它们在不同信噪比、不同数据长度、不同模型情况下模型定阶的可靠性、等价性和选择原则,并得到了一些重要的结论。 相似文献
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《中国航空学报》2016,(2):448-461
In a probe and drogue aerial refueling system, the bow wave of the receiver aircraft will produce a strong aerodynamic effect on the drogue once the receiver follows the drogue at a close distance. It is a major difficulty of docking control in the probe and drogue refueling. This paper analyses the bow wave effect and presents a simple method to model it. Firstly, the inviscid flow around the receiver is modeled based on the stream function defined by basic stream singularities.Secondly, a correction function is developed to eliminate the error caused by the absence of air viscosity. Then, the aerodynamic coefficients are used to calculate the induced aerodynamic force on the drogue. The obtained model is in an analytical form that can be easily applied to the controller design and the real-time simulations. In the verification part, computational fluid dynamics(CFD)simulation tests are conducted to validate the obtained flow fields and aerodynamic forces. Finally,the modeling method is applied to an F-16 receiver aircraft in a previously developed autonomous aerial refueling simulation system. The simulations results are analyzed and compared with the NASA flight-test data, which demonstrates the effectiveness of the proposed method. 相似文献
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Libo Liu Weixing WanBaiqi Ning Man-Lian ZhangMaosheng He Xinan Yue 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The electron density profiles in the bottomside F2-layer ionosphere are described by the thickness parameter B0 and the shape parameter B1 in the International Reference Ionosphere (IRI) model. We collected the ionospheric electron density (Ne) profiles from the FORMOSAT-3/COSMIC (F3/C) radio occultation measurements from DoY (day number of year) 194, 2006 to DoY 293, 2008 to investigate the daytime behaviors of IRI-B parameters (B0 and B1) in the equatorial regions. Our fittings confirm that the IRI bottomside profile function can well describe the averaged profiles in the bottomside ionosphere. Analysis of the equatorial electron density profile datasets provides unprecedented detail of the behaviors of B0 and B1 parameters in equatorial regions at low solar activity. The longitudinal averaged B1 has values comparable with IRI-2007 while it shows little seasonal variation. In contrast, the observed B0 presents semiannual variation with maxima in solstice months and minima in equinox months, which is not reproduced by IRI-2007. Moreover, there are complicated longitudinal variations of B0 with patterns varying with seasons. Peaks are distinct in the wave-like longitudinal structure of B0 in equinox months. An outstanding feature is that a stable peak appears around 100°E in four seasons. The significant longitudinal variation of B0 provides challenges for further improving the presentations of the bottomside ionosphere in IRI. 相似文献
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Olga Pirog Marat Deminov Galina Deminova Gelii Zherebtsov Nelya Polekh 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
An analysis of properties and peculiarities of the nighttime winter foF2 increases (NWI) in the East Siberia is made on data of ionospheric station Irkutsk in the periods 1958–1992 and 2002–2009 and the empirical model of the F2 layer critical frequency under the geomagnetic quiet conditions deduced from these data (model Q-F2). It is revealed, that the NWI is the stable regularity of the quiet ionosphere over Irkutsk. The amplitude of the NWI (the difference between maximum and minimum foF2 values at night hours) is the greatest in December–January and nearly the same at low and middle solar activity. It is a peculiarity of the quiet ionosphere in the East Siberia. Maximum in night foF2 under quiet geomagnetic conditions is observed mainly after midnight (02-04 LT) and is shifted to predawn hours as solar activity increases. At low solar activity the quiet ionosphere at ∼02–04 LT shows the following properties: (a) the fluctuations of foF2 and hmF2 are in the reverse correlation but this dependence is weak; (b) very strong fluctuations of foF2 (|δfoF2| > 30%) occur seldom (∼4% of events) and almost all of them are positive; an example of very strong fluctuations of foF2 up to 60% can be an extreme increase in the foF2 on 19.12.2008; (c) the very strong enhancements of foF2 in the NWI maximum can be observed at the low geomagnetic activity, they occur more often during substorms but very seldom during geomagnetic storms. Possible reasons of these properties of NWI are discussed. 相似文献