Acceleration of energetic particles by whistler waves in active space experiment with charged particle beams injection

In this paper the investigation of wave-particle interaction during simultaneous injection of electron and xenon ion beams from the satellite Intercosmos-25 (IK-25) carried out using the data of the double satellite system with subsatellite Magion-3 (APEX). Results of active space experiment devoted to the beam-plasma instability are partially presented in the paper Baranets et al. (2007). A specific feature of the experiment carried out in orbits 201, 202 was that charged particle flows were injected in the same direction along the magnetic field lines B₀ so the oblique beam-into-beam injection have been produced. Results of the beam-plasma interaction for this configuration were registered by scientific instruments mounted on the station IK-25 and Magion-3 subsatellite. Main attention is paid to study the electromagnetic and longitudinal waves excitation in different frequency ranges and the energetic electron fluxes disturbed due to wave-particle interaction with whistler waves. The whistler wave excitation on the 1st electron cyclotron harmonic via normal Doppler effect during electron beam injection in ionospheric plasma are considered.     

Planetary wave coupling of the atmosphere–ionosphere system during the Northern winter of 2008/2009

This paper presents the global spatial (latitude and altitude) structure and temporal variability of the ∼23-day ionospheric zonally symmetric (s = 0) planetary wave (PW) seen in the Northern winter of 2008/2009 (October 2008–March 2009). It is shown that these ∼23-day ionospheric oscillations are forced from PWs propagating from below. The COSMIC ionospheric parameters f_oF2 and h_mF2 and electron density at fixed altitudes and the SABER temperatures were utilized in order to define the waves which are present simultaneously in the atmosphere and ionosphere. The long-period PWs from the two data sets have been extracted through the same data analysis method. The similarity between the lower thermospheric ∼23-day (s = 0) temperature PW and its ionospheric electron density response provides valuable and strong experimental evidence for confirming the paradigm of atmosphere–ionosphere coupling.     

Response of low latitude D-region ionosphere to the total solar eclipse of 22 July 2009 deduced from ELF/VLF analysis

Response of the D-region of the ionosphere to the total solar eclipse of 22 July 2009 at low latitude, Varanasi (Geog. lat., 25.27° N; Geog. long., 82.98° E; Geomag. lat. = 14° 55’ N) was investigated using ELF/VLF radio signal. Tweeks, a naturally occurring VLF signal and radio signals from various VLF navigational transmitters are first time used simultaneously to study the effect of total solar eclipse (TSE). Tweeks occurrence is a nighttime phenomena but the obscuration of solar disc during TSE in early morning leads to tweek occurrence. The changes in D-region ionospheric VLF reflection heights (h) and electron density (n_e: 22.6–24.6 cm⁻³) during eclipse have been estimated from tweek analysis. The reflection height increased from ∼89 km from the first occurrence of tweek to about ∼93 km at the totality and then decreased to ∼88 km at the end of the eclipse, suggesting significant increase in tweek reflection height of about 5.5 km during the eclipse. The reflection heights at the time of totality during TSE are found to be less by 2–3 km as compared to the usual nighttime tweek reflection heights. This is due to partial nighttime condition created by TSE. A significant increase of 3 dB in the strength of the amplitude of VLF signal of 22.2 kHz transmitted from JJI-Japan is observed around the time of the total solar eclipse (TSE) as compared to a normal day. The modeled electron density height profile of the lower ionosphere depicts linear variation in the electron density with respect to solar radiation as observed by tweek analysis also. These low latitude ionospheric perturbations on the eclipse day are discussed and compared with other normal days.     

无人飞行器参数依赖鲁棒控制研究

研究了具有参数不确定性的无人飞行器参数依赖鲁棒控制器设计问题。采用误差四元数建立姿态运动方程,避免了欧拉角描述姿态运动存在奇异性的问题。通过引入附加的松弛矩阵使Lyapunov矩阵和系统矩阵分离,并利用平方和工具箱求解非线性矩阵不等式得到了系统的鲁棒控制器。仿真结果表明了所提出的控制器设计方法的可行性和有效性。     

直升机近地飞行时的配平和机动操纵分析

在单旋翼带涵道尾桨直升机的非线性全量飞行动力学模型的基础上,提出了求解配平和机动操纵问题的一种混合算法,研究了地面效应对配平和机动操纵的影响.以某直升机为算例,在近地飞行和考虑不同速度与高度时,分别进行了直升机稳定飞行时的配平计算,然后以侧向紧急转弯机动为例,对机动操纵规律的问题进行了计算分析,计算结果与地面效应的理论相符合,机动过载和操纵变化规律可以为飞行试验提供借鉴.所建立的理论方法可以为直升机近地飞行时的动力学和控制分析提供参考.      

超声速非平行边界层的非线性稳定性研究(英文)

用非线性抛物化稳定性方程(NPSE),研究超声速非平行边界层的扰动波的非线性演化过程。发展了高精度的数值方法,对NPSE进行有效求解和稳定推进。计算得到了各谐波的振幅增长曲线和不同的扰动剖面函数,特别是展示了谐波之间的非线性作用的物理特征,包括流向涡、展向涡和Λ结构的形成和演化等,以进行转捩过程的机理研究和分析。NPSE的计算结果显示了这个新方法是研究超声速边界层非线性稳定性的有效方法。     

变结构控制系统中的混沌现象

应用相轨迹、功率谱等方法,证实了一类变结构控制系统中存在混沌现象,分析了产生混沌现象的原因并给出不同条件下的混沌图形。     

基于不敏变换的GDOP计算

现有文献一般采用线性化的方法得到非线性系统的定位精度几何稀释(Geometrical Dilution of Precision,GDOP)。然而,当定位系统的非线性较强时,线性化方法得到的GDOP同系统实际定位误差存在较大的偏差。针对这种情况,提出采用不敏变换(Unscented Transformation,UT)计算GDOP的方法,并通过一个数值例子进行了验证。     

VCM-DDV建模与控制仿真

基于AMESim和Simulink的协同仿真环境,对新型音圈电机直接驱动伺服阀(VCM-DDV,Voice Coil Motor-Direct Drive Valve)进行了仿真研究.采用AMESim建立了VCM-DDV的非线性模型及虚拟液压测试系统,采用Simulink建立了数字控制器模型,通过接口组成了协同仿真环境.将VCM-DDV视为线性部分与非线性部分叠加,并将非线性部分视为线性系统状态空间的一个状态,建立了系统的状态空间模型.用全状态观测器得到非线性干扰项,设计了LQR(Linear Quadratic Regulator)全状态反馈和非线性补偿的复合控制方法.仿真结果表明:非线性补偿提高了系统的稳态控制精度,LQR状态反馈可以使系统达到需要的动态性能.     

基于半光程差的天线反射面型面精度检测

型面拟合最小量的选取是天线面板型面检测中的关键技术之一.天线表面各点半光程差的均方根是衡量天线型面精度的指标.根据圆锥曲面的几何定义及其光学性质,提出了圆锥曲面天线面板半光程差的直接计算方法,给出了基于半光程差的非线性最小二乘曲面拟合算法.以旋转抛物面天线面板为例,通过模拟和实际测量,对比分析了分别选取轴向误差和半光程差作为最小量拟合计算结果.试验验证了选取半光程差作为最小量拟合的算法具有更高的数值计算精度及稳定性.