正相电离层骚扰研究

本文对我国五个电离层站月报资料中的正相电离层骚扰(f₀F₂增加)作了分析研究,获得了正相骚扰时空变化的规律性,地磁暴与正相电离层骚扰的关系.对正相电离层骚扰的机理也作了讨论.      

不确定非完整动力学系统的变结构指数镇定

链式系统是非完整运动学系统的一种标准形式. 通过坐标和输入变换,许多非完整运动学系统均可化为这种形式.当非完整运动学系统可化为链式系统时, 直接基于一类不确定非完整动力学系统, 利用变结构控制的方法设计了全局镇定控制律. 该控制律的特点是: 存在一个有限时间,使得在此时间后闭环系统的状态可以以任意速率指数收敛到零. 最后将该方法用于一类移动机器人的控制器设计,仿真结果验证了该方法的有效性.      

低纬地区夜间电离层底部电子浓度与磁扰的关系

本文利用100kHz的低频无线电波资料,计算分析了1986—1987年期间,几种不同磁扰情况下,低纬地区夜间电离层中100km以下区域积分电子浓度及其变化的起因.结果表明:该区域电子浓度的变化与地磁扰动关系密切.在磁静日期间,其值较小,且随磁扰而变化,但比磁扰滞后1到2天.在磁暴后,其值较大,会出现几次剧烈起伏.该区域积分电子浓度的起伏可大于一个量级.沉降电子产生的动致辐射可能是引起该区域电子浓度变化的主要原因之      

Large-scale traveling ionospheric disturbances of auroral origin according to the data of the GPS network and ionosondes

The intensity of large-scale traveling ionospheric disturbances (LS TIDs), registered using measurements of total electron content (TEC) during the magnetic storms on October 29–31, 2003, and on November 7–11, 2004, had been compared with that of local electron density disturbances. The data of TEC measurements at ground-based GPS receivers located near the ionospheric stations and the corresponding values of the critical frequency of the ionospheric F region f_oF2 were used for this purpose. The variations of TEC and f_oF2 were similar for all events mentioned above. The previous assumption that the ionospheric region with vertical extension from 150 to 200 km located near the F-layer maximum mainly contributes to the TEC variations was confirmed for the cases when the electron density disturbance at the F region maximum was not more than 50%. However, this region probably becomes vertically more extended when the electron density disturbance in the ionospheric F region is about 85%.     

一种基于串级线性自抗扰控制的四旋翼无人机控制方法

提出了一种基于串级线性自抗扰控制器的四旋翼无人机控制方法。根据建立的紊流模型形成了干扰风,在干扰风的环境下建立了四旋翼的运动学模型,并设计了一个串级的线性自抗扰控制器,其中外环采用位置控制,内环采用姿态控制。对比了该控制器与非线性自抗扰控制器和经典PID控制器在无风干扰和有风干扰下无人机的定点悬停的性能。仿真试验结果表明,无论是在无风干扰下还是在有风干扰下,该控制器的性能均好于非线性自抗扰控制器和PID控制器,具有较好的鲁棒性,能够运用到各种类型的旋翼无人机的工程控制中。     

力伺服系统的模糊自适应控制

位置扰动型施力系统存在着多余力的问题,同时由于系统的非线性及参数时变等因素的影响,给系统的校正和优化带来了困难,为了消除位置扰动型施力系统中存在的多余力以及非线性,参数时变等因素的影响,采用在非线性前馈校正基础上的模糊自适应控制策略,可以较好地消除系统的多余力,同时克服了系统的非线性及参数时变等因素的影响,改善系统的动态品质,仿真研究的结果验证上述结论。     

Geoeffectiveness of interplanetary shocks controlled by impact angles: A review

The high variability of the Sun’s magnetic field is responsible for the generation of perturbations that propagate throughout the heliosphere. Such disturbances often drive interplanetary shocks in front of their leading regions. Strong shocks transfer momentum and energy into the solar wind ahead of them which in turn enhance the solar wind interaction with magnetic fields in its way. Shocks then eventually strike the Earth’s magnetosphere and trigger a myriad of geomagnetic effects observed not only by spacecraft in space, but also by magnetometers on the ground. Recently, it has been revealed that shocks can show different geoeffectiveness depending closely on the angle of impact. Generally, frontal shocks are more geoeffective than inclined shocks, even if the former are comparatively weaker than the latter. This review is focused on results obtained from modeling and experimental efforts in the last 15?years. Some theoretical and observational background are also provided.     

Multi-scale nature of non-blade-order propagating flow disturbances in axial compressors

Non-blade-order flow disturbances, also referred to as pre-stall disturbances or tip flow unsteadiness, are closely related with compressor instabilities. The present work provides a comprehensive investigation on multi-scale nature of non-blade-order disturbances and the underlying flow physics in axial compressors. By applying full-annulus Unsteady Reynolds-Averaged Navier-Stokes (URANS) simulations, along with space–time correlation and spatial Fourier decomposition, to the disturbed pressure, the propagating feature of the non-blade-order disturbances is obtained. Further, a bridge between non-blade-order disturbances and the evolution of unsteady vortex has been set up. The results show that non-blade-order disturbances, featured as short-length-scale (35 modes across annulus), first appear as the occurrence of tip leakage vortex fluctuation, while the compressor still operates far from stall. Leading-edge radial vortex appears at near stall condition, and its movement induces a circumferential propagating disturbance overlaying on the one induced by oscillating tip leakage vortex. The interaction of the short-scale disturbances with a low-amplitude long-scale (of circumference) disturbance is observed, which results in disturbances with multiple scales of consecutive spatial modes, along with multiple frequency peaks in spectra. The compressor falls into stall as the circumferential nonuniform scattering of the leading-edge vortexes occurs. The densely- and sparsely-scattered leading-edge radial vortexes induce a high-amplitude long-scale (of circumference) disturbance, i.e. stall disturbance.