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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Investigating dynamical complexity in the magnetosphere using various entropy measures
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Investigating dynamical complexity in the magnetosphere using various entropy measures

机译:调查的动态复杂性磁气圈使用各种熵措施

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The complex system of the Earth's magnetosphere corresponds to an open spatially extended nonequilibrium (input-output) dynamical system. The nonextensive Tsallis entropy has been recently introduced as an appropriate information measure to investigate dynamical complexity in the magnetosphere. The method has been employed for analyzing Dst time series and gave promising results, detecting the complexity dissimilarity among different physiological and pathological magnetospheric states (i.e., prestorm activity and intense magnetic storms, respectively). This paper explores the applicability and effectiveness of a variety of computable entropy measures (e.g., block entropy, Kolmogorov entropy, T complexity, and approximate entropy) to the investigation of dynamical complexity in the magnetosphere. We show that as the magnetic storm approaches there is clear evidence of significant lower complexity in the magnetosphere. The observed higher degree of organization of the system agrees with that inferred previously, from an independent linear fractal spectral analysis based on wavelet transforms. This convergence between nonlinear and linear analyses provides a more reliable detection of the transition from the quiet time to the storm time magnetosphere, thus showing evidence that the occurrence of an intense magnetic storm is imminent. More precisely, we claim that our results suggest an important principle: significant complexity decrease and accession of persistency in Dsttime series can be confirmed as the magnetic storm approaches, which can be used as diagnostic tools for the magnetospheric injury (global instability). Overall, approximate entropy and Tsallis entropy yield superior results for detecting dynamical complexity changes in the magnetosphere in comparison to the other entropy measures presented herein. Ultimately, the analysis tools developed in the course of this study for the treatment of Dst index can provide convenience for space weather applications.
机译:地球的磁气圈的复杂系统对应于一个开放的空间扩展非平衡态(输入输出)动力系统。的nonextensive Tsallis熵最近推出了一个适当的信息测量调查动态复杂性磁气圈。分析Dst时间序列,并承诺结果,检测不同的复杂性在不同的生理和病理磁性层的状态(例如,prestorm活动和强烈的磁性风暴,分别)。论文探讨了适用性各种各样的可计算的熵的有效性措施(例如,块熵,柯尔莫哥洛夫熵,T复杂度和近似熵)调查的动态复杂性磁气圈。风暴方法有明确的证据显著降低复杂性磁气圈。组织系统的同意推断出以前,从一个独立的线性基于小波的分形谱分析变换。和线性分析提供了一种更可靠检测过渡的安静的时间暴风雨时间磁气圈,从而显示发生一场激烈的证据磁暴迫在眉睫。声称,我们的结果显示一个重要原则:减少和很大的复杂性加入持久性Dsttime系列确认为磁暴的方法,可以用作诊断工具的吗磁性层的损伤(全球不稳定)。总的来说,近似熵和Tsallis熵为检测动态产生卓越的结果复杂的磁气圈的变化相比其他熵措施提出了。在本研究的课程开发Dst的治疗指数可以提供方便对空间天气应用程序。

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