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Estimation of chaotic nature of dynamical system through nonlinear analysis

机译:通过非线性分析估计动力系统的混沌性质

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Estimation of low-dimensional chaos from nonlinear time series is a very important but difficult task in scientific fields. Among the several techniques proposed for this aim are the rescaled range analysis and maximal Lyapunov exponent, which quantify the amount of a time series. These two techniques are applied to analyse the astronomical time series, which is non-stationary and nonlinear in nature. It is found that, (1) solar activity exhibits a complex and strongly chaotic behaviour and is governed by a low-dimensional chaotic attractor; (2) the predictability time of the chaotic motion in solar-activity indicator is up to 1.12 years. These results indicate that chaotic characteristics obviously exist in the solar time series, and thus techniques based on rescaled range analysis and maximal Lyapunov exponent can be used to analyse and predict solar activity. It should be pointed out that solar activity forecast should be done only for a short to medium term due to the initial value of the sensitive of the chaotic system.
机译:从非线性时间序列估计低维混沌是科学领域非常重要但艰巨的任务。为此目的提出的几种技术是重新定义的范围分析和最大Lyapunov指数,其量化了时间序列的量。应用这两种技术来分析天文时间序列,这是非静止和非线性的。发现(1)太阳能活动表现出复杂且强烈的混乱行为,并受低维混沌吸引子的管辖; (2)太阳能活动指标中混沌运动的可预测性时间高达1.12年。这些结果表明,太阳时间序列明显存在的混沌特性,因此基于重新分析和最大Lyapunov指数的技术可用于分析和预测太阳能活动。应该指出的是,由于混沌系统的敏感性的初始值,太阳能活动预测应该仅用于短到中期。

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