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221.
Aimed at the need of formation control of missile cooperative engagement, the adaptive sliding mode control theory is introduced to solve the controller design problem of formation based on the leader follower approach. Feedback precise linearization based on differential geometry theory is used to linearize the nonlinear motion model of missile and system model with follower track errors is formulated. In traditional leader follower approach, if the leader moves too fast due to the control saturated, the followers will not be able to track the desired position to keep formation. In order to overcome the disadvantage, an idea of speed control for the leader is introduced to guarantee formation keeping. Finally, an adaptive sliding mode controller is designed to overcome the problem of control input constraints. Theoretical analysis demonstrates that tracking error asymptotically converges to zero. Simulation results show that the leader is able to follow the desired path and the controller can help every missile configure desired formation. The simulation results verify stability and robustness of the formation controllers. 相似文献
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成对比较矩阵的一种逼近 总被引:2,自引:0,他引:2
本文证明了成对比较矩阵在相容性矩阵集合中的最佳逼近的存在性和不唯一性。再通过微分同胚,把原来的非线性逼近转化成一个线性逼近,用投影定理予以解决。并用一个例子说明该方法的简易可行。 相似文献
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介绍双发(Twin-engines)系统的战斗机的机载供电系统控制器的设计和实现。机载供电系统控制器是管理飞机的供电系统的航空电子设备,是飞机供电系统的核心设备,肩负飞机安全的使命。为了提高控制器的可靠性和灵活性,放弃传统的模拟方法,使用先进的数字化技术实现对飞机供电、配电系统的管理。在设计中为了提高可靠性,使用主动复制的容错技术,设计了双余度控制器,在发生单通道错误的情况下,整个系统能够正确工作。对机载供电系统控制器容错技术进行了研究,包括双余度系统的管理策略、同步控制机制、余度管理和故障综合、信号比较监控和通道切换逻辑。 相似文献
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文章研究了追踪航天器与失控旋转非合作目标航天器在椭圆轨道中的交会接近策略与控制。在接近策略方面,首先,根据目标航天器大致结构设定一个安全的停泊点,使追踪航天器交会至停泊点;其次,通过在停泊点对旋转目标航天器姿态的观测,分析和预测其运动并确定合适的抓捕点位置,设计安全的接近轨迹,使追踪航天器沿着该轨迹接近至理想的抓捕实施点位置。在控制方面,考虑实际系统中的不确定性,只利用两航天器之间相对位置的测量信息,设计基于特征模型的自适应控制方法实现交会接近。最后通过数学仿真模拟整个交会接近过程,验证了文中所提出的接近策略和控制方法。 相似文献
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Elías M. Lau Hiroyuki Iimura Scott E. Palo Susan K. Avery James P. Avery Chunmei Kang Nikolai A. Makarov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
A new meteor radar system was installed at the Amundsen–Scott station South Pole in 2001 to further the understanding of the dynamics of the Antarctic region. The antenna array consists of four yagis pointed along the 0°, 90°, 180°, and 270° meridians and five folded crossed dipoles arranged in a cross configuration and operating as an interferometer to provide position measurements for the detected radio meteors. The four yagis are time division multiplexed and used for both transmitting and receiving while the five folded crossed dipoles are only used for reception. The current arrangement of data acquisition (DAQ) systems at the South Pole allows the collection of meteors in a configuration similar to the previous meteor radar system that operated at the South Pole in the mid 1990s while also using an interferometer to accurately determine the meteor positions in the sky, which enables the determination of the vertical structure of the observed waves. This has been accomplished through the use of two DAQ and post-processing systems: COBRA (Colorado Obninsk radar) connected to the yagis and MEDAC (meteor echo detection and collection) connected to the folded crossed dipoles. With two separate DAQ systems operating in parallel we have the ability to directly compare the results and understand the inherent variability in the derived scientific results based on different system architectures and processing assumptions. The impact of operating a system without an interferometer on the amplitudes and phases of the observed wave components is considered. We find that the lack of altitude resolution of the COBRA DAQ system leads to an underestimation of the amplitude of the s = 1 component of the semidiurnal tide of ∼20% during the summer months. 相似文献