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221.
随着芯片设计向更高的频率发展,传统的时钟树综合策略是尽量减小时钟偏移,但是这样的时钟树综合策略已经逐渐不能满足时序收敛的需要,因此引入了有效时钟偏移的概念。文章通过一个在TSMC0.13μm工艺并流片成功的芯片BES7000作为设计实例,分析了有效时钟偏移引入之后对改进时序建立时间的效果。 相似文献
222.
We describe the results of determining the mass of the International Space Station using the data of MAMS accelerometer taken during correction of the station orbit on August 20, 2004. The correction was made by approach and attitude control engines (ACE) of the Progress transporting spacecraft. The engines were preliminary calibrated in an autonomous flight using the onboard device for measuring apparent velocity increment. The method of calibration is described and its results are presented. The error in station mass determination is about 1%. The same data of MAMS and similar data obtained during the orbit correction on August 26, 2004 were used for the analysis of high-frequency vibrations of the station mainframe caused by operation of the ACE of Progress. Natural frequencies of the ACE are determined. They lie in the frequency band 0.024–0.11 Hz. ACE operation is demonstrated to result in a substantial increase of microaccelerations onboard the station in the frequency range 0–1 Hz. The frequencies are indicated at which disturbances increase by more than an order of magnitude. The study described was carried out as a part of the Tensor technological experiment. 相似文献
223.
The results of reconstruction of uncontrolled attitude motion of the Foton M-2 satellite using measurements with the accelerometer TAS-3 are presented. The attitude motion of this satellite has been previously
determined by the measurement data of the Earth’s magnetic field and the angular velocity. The TAS-3 data for this purpose
are used for the first time. These data contain a well-pronounced additional component which made impossible their direct
employment for the reconstruction of the attitude motion and whose origin was unknown several years ago. Later it has become
known that the additional component is caused by the influence of the Earth’s magnetic field. The disclosure of this fact
allowed us to take into account a necessary correction in processing of TAS-3 data and to use them for the reconstruction
of the attitude motion of Foton M-2. Here, a modified method of processing TAS-3 data is described, as well as results of its testing and employing. The testing
consisted in the direct comparison of the motion reconstructed by the new method with the motion constructed by the magnetic
measurements. The new method allowed us to find the actual motion of Foton M-2 in the period June 9, 2005–June 14, 2005, when no magnetic measurements were carried out. 相似文献
224.
针对传统自适应控制在飞行器作动器具有幅值饱和与速率饱和的情况下难以实现良好飞行控制的问题,提出了一种基于神经网络与伪控制隔离的飞行器抗饱和自适应控制方法.首先根据模型参考自适应控制理论,结合动态逆与神经网络自适应方法,分析了系统的模型跟踪误差动力特征,并考虑飞行器具有参数不确定和未建模误差等动态逆误差,设计了在线神经网... 相似文献
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227.
基于自抗扰的直接力与气动力复合控制系统设计 总被引:2,自引:0,他引:2
针对直接力/气动力复合控制导弹的设计问题,提出了一种基于自抗扰控制技术的自动驾驶仪设计方法.首先分析了复合控制系统的特点和控制问题,建立了三通道的复合控制模型.然后针对俯仰通道和偏航通道提出了一种三环设计方法,内环和中环应用自抗扰控制器设计,主要考虑自抗扰控制器对对象参数变化和外部扰动的不敏感特性,外环采用PI控制器设计.最后针对滚转通道提出了一种双环设计方法,内环和外环均采用自抗扰控制器设计.仿真结果表明,所提出的控制方案对过载指令具有较好的跟踪效果,且控制器具有很强的鲁棒性,适用于直接力/气动力复合控制导弹的控制系统设计. 相似文献
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229.
The results of a preliminary analysis of microperturbations on the International Space Station during physical exercises of the crew are presented. The goal of this paper is to identify the parameters of perturbations when physical exercises are performed. The results of measurements by sensors of microaccelerations of both Russian and American segments during physical exercises in the service module of the Russian segment are analyzed. 相似文献
230.
A. V. Tavrov O. I. Korablev A. V. Rodin I. I. Vinogradov A. Yu. Trokhimovsky A. Yu. Ivanov L. V. Ksanfomaliti D. A. Orlov 《Cosmic Research》2011,49(2):99-109
In order to observe exoplanets we propose a space-based achromatic stellar coronagraph combined with a 0.8–1.5 m telescope. We develop an achromatic common path interferometer for observing an exoplanet (a faint off-axis source) on the background of a hoste star (bright axial source). An image of the star and its copy acquire an achromatic phase shift by 180° and interfere in antiphase. The achromatic phase shift is caused by geometric phase in the scheme of a three-dimensional interferometer. The interference process divides spatially the dark and light fields of the star image redirecting them to the opposite sides of a beam splitter. The interference process does not weaken the image of a planet, with equal intensities it is redirected to both sides of a beam splitter. The suggested scheme of common path interferometer ensures mechanical stability. The background signal is experimentally demonstrated to be reduced by six orders of magnitude. 相似文献