论文标题
在磁性疟疾中非线性alfvén波动力学中的混乱和复杂性
Chaos and complexity in the dynamics of nonlinear Alfvén waves in a magnetoplasma
论文作者
论文摘要
在均匀的磁质体中研究了循环极化分散孔(AW)的非线性动力学。通过将波动力学限制为几个谐波模式,提出了一个低维动力学模型来描述非线性波浪波的相互作用。发现存在的两个调制$ k $ AW信封的浪潮数量的两个子间隙,即$(3/4)k_c <k <k_c $和$ 0 <k <(3/4)k_c $,其中$ k_c $是$ k $的关键值,下面是$ k $的关键值。在前者中,在MI生长速率较低的情况下,周期性和/或准周期性状态显示出发生,而后者的MI生长很高,则会带来混乱的状态。这些状态的存在是通过对Lyapunov指数光谱的分析以及动力学变量的分叉图和相空间肖像来确定的。此外,非线性运动中混沌相位空间的复杂性是通过相关维度(CD)的估计以及近似熵(APEN)来衡量的,并将其与已知的H {é}非MAP和LORENZ系统的相关性进行了比较。在低维模型中预测的混乱运动可能是在高维模型中观察到的Alfv {é} NIC波湍流的先决条件,该模型与地球的电离层和磁层相关。
The nonlinear dynamics of circularly polarized dispersive Alfv{é}n wave (AW) envelopes coupled to the driven ion sound waves of plasma slow response is studied in a uniform magnetoplasma. By restricting the wave dynamics to a few number of harmonic modes, a low-dimensional dynamical model is proposed to describe the nonlinear wave-wave interactions. It is found that two subintervals of the wave number of modulation $k$ of AW envelope exists, namely $(3/4)k_c<k<k_c$ and $0<k<(3/4)k_c$, where $k_c$ is the critical value of $k$ below which the modulational instability (MI) occurs. In the former, where the MI growth rate is low, the periodic and/or quasi-periodic states are shown to occur, whereas the latter, where the MI growth is high, brings about the chaotic states. The existence of these states is established by the analyses of Lyapunov exponent spectra together with the bifurcation diagram and phase-space portraits of dynamical variables. Furthermore, the complexities of chaotic phase spaces in the nonlinear motion are measured by the estimations of the correlation dimension (CD) as well as the approximate entropy (ApEn), and compared with those for the known H{é}non map and the Lorenz system in which a good qualitative agreement is noted. The chaotic motion thus predicted in a low-dimensional model can be a prerequisite for the onset of Alfv{é}nic wave turbulence to be observed in a higher dimensional model that and is relevant in the Earth's ionosphere and magnetosphere.