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arXiv 2310.05967physics.geo-phmath.DSnlin.CD
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非周期强迫下非自治混沌系统的演化:一个气候变化示例

The evolution of a non-autonomous chaotic system under non-periodic forcing: a climate change example

Francisco de Melo Viríssimo, David A. Stainforth, Jochen Bröcker

AI总结:

本文以低维类气候非线性系统研究非周期强迫下非自治混沌系统的中期气候行为,提出演化集与收敛时间概念,揭示初始条件不确定性和强迫速率的影响,为气候模型集合设计提供启示。

摘要:

复杂地球系统模型被广泛用于在未来大气温室气体浓度变化假设下对气候做出条件性陈述,这些陈述通常被称为气候预估。这些模型本身是高维非线性系统,人们常用吸引子和低维非线性系统(如经典的 Lorenz '63 系统)来讨论其行为。在非自治情形下,例如由人为气候变化引起的情形,相关对象有时被认为是拉回吸引子或快照吸引子。然而,拉回吸引子是给定时刻系统所有可能状态的集合,因此在做气候预估时并未考虑我们对地球系统当前状态的已有知识,因而对年际到多年代际气候预估的信息价值不高。本文通过使用一个具有三个变率时间尺度且受非周期强迫的低维、类气候非线性系统,来处理测量和解释模型中期气候的问题。我们引入了依赖于系统初始状态的“演化集”概念,并探讨其与不同类型初始条件不确定性以及外部强迫速率之间的联系。我们将“收敛时间”定义为某个因变量的分布失去其初始条件记忆所需的时间。我们推测收敛时间与经典混合时间概念之间存在联系,但这一联系的确切性质仍需进一步探索。这些结果对具有影响力的气候与地球系统模型集合的设计具有启示意义,并提出了一些具有数学意义的问题。

英文摘要:

Complex Earth System Models are widely utilised to make conditional statements about the future climate under some assumptions about changes in future atmospheric greenhouse gas concentrations; these statements are often referred to as climate projections. The models themselves are high-dimensional nonlinear systems and it is common to discuss their behaviour in terms of attractors and low-dimensional nonlinear systems such as the canonical Lorenz `63 system. In a non-autonomous situation, for instance due to anthropogenic climate change, the relevant object is sometimes considered to be the pullback or snapshot attractor. The pullback attractor, however, is a collection of {\em all} plausible states of the system at a given time and therefore does not take into consideration our knowledge of the current state of the Earth System when making climate projections, and are therefore not very informative regarding annual to multi-decadal climate projections. In this article, we approach the problem of measuring and interpreting the mid-term climate of a model by using a low-dimensional, climate-like, nonlinear system with three timescales of variability, and non-periodic forcing. We introduce the concept of an {\em evolution set} which is dependent on the starting state of the system, and explore its links to different types of initial condition uncertainty and the rate of external forcing. We define the {\em convergence time} as the time that it takes for the distribution of one of the dependent variables to lose memory of its initial conditions. We suspect a connection between convergence times and the classical concept of mixing times but the precise nature of this connection needs to be explored. These results have implications for the design of influential climate and Earth System Model ensembles, and raise a number of issues of mathematical interest.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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