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101.
V.B. Baranov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath. 相似文献
102.
提出了一种新的基于直接转化法的求解基于常微分方程(ODE)和微分代数方程(DAE)的最优控制问题的数值方法.该方法通过Legendre-Gauss拟谱法同时离散化状态变量和控制变量,把最优控制问题转化为一个非线性规划问题,并利用改进的多相处理方法避免优化无控段,同时基于稀疏矩阵探索其一阶导数信息.数值结果表明,与传统的直接转换法相比,该方法是一种通用高效的精度较高的ODE/DAE最优控制直接数值求解法.最后,从工程观点出发,应用该方法成功求解了终端自由有路径约束的奇异最优控制问题Goddard火箭问题. 相似文献
103.
通过摩擦补偿的分析提出了一种基于非线性摩擦模型参数观测器的自适应摩擦补偿方法,从工程实用角度出发采用的是库仑加粘滞的摩擦模型,设计了两个观测器实现对库仑摩擦系数和粘滞摩擦系数的估计,并用MATLAB软件对转台工作状态进行了仿真,结果表明此观测器有良好的自适应补偿性能。 相似文献
104.
Dong L. Wu Michael J. Schwartz Joe W. Waters Varavut Limpasuvan Qian Wu Timothy L. Killeen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
This paper describes a microwave limb technique for measuring Doppler wind in the Earth’s mesosphere. The research algorithm has been applied to Aura Microwave Limb Sounder (MLS) 118.75 GHz measurements where the O2 Zeeman lines are resolved by a digital autocorrelation spectrometer. A precision of ∼17 m/s for the line-of-sight (LOS) wind is achieved at 80–92 km, which corresponds to radiometric noise during 1/6 s integration time. The LOS winds from Aura MLS are mostly in the meridional direction at low- and mid-latitudes with vertical resolution of ∼8 km. This microwave Doppler technique has potential to obtain useful winds down to ∼40 km of the Earth’s atmosphere if measurements from other MLS frequencies (near H2O, O3, and CO lines) are used. Initial analyses show that the MLS winds from the 118.75 GHz measurements agree well with the TIDI (Thermosphere Ionosphere Mesosphere Energetics and Dynamics Doppler Interferometer) winds for the perturbations induced by a strong quasi 2-day wave (QTDW) in January 2005. Time series of MLS winds reveal many interesting climatological and planetary wave features, including the diurnal, semidiurnal tides, and the QTDW. Interactions between the tides and the QTDW are clearly evident, indicating possible large tidal structural changes after the QTDW events dissipate. 相似文献
105.
Katia Ferrière 《Space Science Reviews》2006,122(1-4):247-253
We present a theoretical overview of low-frequency waves and instabilities in collisionless, multi-component plasmas with
gyrotropic (
) thermal pressure. We show that the complete dispersion relation can be obtained in the framework of a mixed magnetohydrodynamic
(MHD)-kinetic formalism, which uses the MHD mass, momentum, and induction equations, together with the kinetically corrected
version of the double-adiabatic equations of state. The complete dispersion relation contains not only the three standard
modes (fast, slow, and Alfvén) from double-adiabatic MHD, but also the mirror mode from kinetic theory. We examine the stability
properties of these four modes, firstly in the case of a uniform medium, and secondly in the case of a stratified and rotating
medium. We also discuss the connections with the quasi-interchange modes (interchange and translation) often referred to in
the context of magnetospheric physics. 相似文献
106.
有输入未建模动态的非线性系统自适应逆设计 总被引:1,自引:1,他引:0
对于一类存在输人未建模动态的非线性系统,提出了一种基于RBF神经网络的自适应逆补偿器设计方法。首先用两个神经网络设计了补偿器,一个用来估计输入未建模动态,另一个用来作为未建模动态的自适应逆补偿器。该设计放宽了对未建模动态的一些苛刻的要求,如相对度为零,满足小增益条件等。文中仅要求D(u)逆稳和连续光滑。然后应用反演设计技术设计了控制器,并应用Lyapunov稳定性理论推导出神经网络权重向量的调节律,同时证明了闭环系统的渐近稳定性。最后给出的仿真研究证明了该设计方法的有效性。 相似文献
107.
逆向卸荷式气体减压阀的静态特性分析 总被引:2,自引:0,他引:2
对影响减压阀压力调节精度的非线性因素——摩擦力和流体稳态力进行了研究与讨论,建立了逆向卸荷式气体减压阀的静态特性数学模型,其中计算结果与实验结果相吻合。分析结果表明,摩擦力和流体稳态力对减压阀的静态特性偏差有着不同程度的影响,因此在设计过程中应该考虑摩擦力、流体稳态力对减压阀静态特性的影响。 相似文献
108.
基于L-M网络的涡扇发动机动态过程辨识 总被引:4,自引:0,他引:4
介绍了多层前馈网络的Levenberg-Marquardt (LM)算法,对涡扇发动机动态过程的数学模型进行了分析和简化,运用多层前馈网络L-M算法对涡扇发动机进行加力推力变换时的非线性MIMO动态过程的数学模型进行了辨识,辨识所用样本数据和测试数据均为试飞实测数据.辨识结果表明,这种方法收敛快精度高,非常适合于涡扇发动机非线性动态过程的建模. 相似文献
109.
110.
一种非线性末制导系统模型的精确线性化 总被引:1,自引:0,他引:1
针对未来高机动目标的拦截 ,运用非线性系统几何理论中的精确线性化方法 ,设计了一种空空导弹非线性末制导系统加速度指令。假设目标做逃逸机动 ,弹体 -自动驾驶仪响应用一个二阶环节描述 ,建立了导弹目标三维相对运动方程。根据终端约束直接选取系统输出阵 ,经动态反馈线性化 ,将非线性系统模型转化为线性方程 ,求得了目标任意机动时的非线性末制导系统的加速度指令。以纵向平面为例进行了仿真计算 ,结果表明该方法是行之有效的 ,得到的解可以用来改进导弹大离轴发射角时的进攻能力。 相似文献