Converged ensemble simulations of climate: possible trends in total solar irradiance cannot explain global warming alone

IF 2 3区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY
Gábor Drótos, Mátyás Herein, Tímea Haszpra, Imre M. Jánosi
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Abstract

We address the hypothetical question of whether an increasing total solar irradiance (TSI) trend, without anthropogenic contributions, could be sufficient to explain the ongoing global warming. To this end, the intermediate-complexity climate model PlaSim is used. To consider the total internal variability, we present a set of ensemble simulations, with different forcing histories in TSI and CO2 concentration, that have converged sufficiently tightly to the relevant probability distributions to provide a satisfactory bound on any spurious trend possibly arising from a sampling bias; similar bounds on any other unforced contributions to ensemble mean trends are also estimated. A key point is the consideration, among the forcing histories, the steepest increasing trend in TSI that is still consistent with observations according to a recent study; thereby, we essentially revisit corresponding TSI reconstructions, more than 20 years after their last modeling-based evaluation, by improving the analysis through taking care of all possible sources of error or uncertainty and incorporating data that have become available since then. Without any change in CO2 concentration, our TSI trend (i.e., and upper bound on actual TSI trends) is found to be insufficient to produce outcomes compatible with the observational record in global mean surface temperature (GMST) with a nonnegligible probability. We formalize our statement for quantifiers of GMST trends through evaluating their distributions over the ensemble, and we speculate that the hypothesis about the exclusive role of an increasing TSI remains implausible even beyond our particular model setup. At the same time, if we consider a constant TSI, and the observational record in CO2 concentration is applied as forcing, the simulation results and the recorded GMST match well. While we currently need to leave the question of a precise attribution open, we conclude by pointing out that an attribution of the ongoing global warming to an increasing TSI alone could be made plausible only if a bias in the set of land-based instrumental temperature measurements were increasing more rapidly than commonly estimated; an assessment of the latter possibility is out of the scope of our study, as well as addressing solar forcing mechanisms beyond the effect of TSI.
气候集合模拟:太阳总辐照度的可能趋势无法单独解释全球变暖问题
我们探讨的假设问题是,在没有人为因素的情况下,太阳总辐照度(TSI)的上升趋势是否足以解释当前的全球变暖现象。为此,我们使用了中等复杂程度的气候模式 PlaSim。为了考虑总的内部变率,我们提出了一组集合模拟,其中有不同的 TSI 和 CO2 浓度的强迫历史,它们与相关的概率分布收敛得足够紧密,从而为可能由采样偏差引起的任何虚假趋势提供了一个令人满意的边界;我们还估算了对集合平均趋势的任何其他非强迫贡献的类似边界。关键的一点是,根据最近的一项研究,在各种作用力历史中,考虑到了 TSI 最陡峭的上升趋势,而这一趋势与观测结果仍然是一致的;因此,在上一次基于建模的评估 20 多年后,我们基本上重新审视了相应的 TSI 重建,通过考虑所有可能的误差或不确定性来源,并纳入自那时以来可用的数据,改进了分析。我们发现,在二氧化碳浓度没有任何变化的情况下,我们的 TSI 趋势(即实际 TSI 趋势的上限)不足以以不可忽略的概率产生与全球平均表面温度(GMST)观测记录相一致的结果。我们通过评估全球平均表面温度趋势量化指标在集合中的分布,将我们的声明正式化,并推测关于 TSI 增加的唯一作用的假设即使超出我们特定的模型设置,仍然是不可信的。同时,如果我们考虑恒定的 TSI,并将观测到的 CO2 浓度记录用作强迫,模拟结果和记录的 GMST 非常吻合。虽然我们目前还需要对精确的归因问题保持开放态度,但我们最后指出,只有在陆基仪器温度测量的偏差比通常估计的增加得更快的情况下,将全球持续变暖仅仅归因于不断增加的 TSI 才是可信的;对后一种可能性的评估不在我们的研究范围之内,同时也不涉及 TSI 影响之外的太阳强迫机制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Frontiers in Earth Science
Frontiers in Earth Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
3.50
自引率
10.30%
发文量
2076
审稿时长
12 weeks
期刊介绍: Frontiers in Earth Science is an open-access journal that aims to bring together and publish on a single platform the best research dedicated to our planet. This platform hosts the rapidly growing and continuously expanding domains in Earth Science, involving the lithosphere (including the geosciences spectrum), the hydrosphere (including marine geosciences and hydrology, complementing the existing Frontiers journal on Marine Science) and the atmosphere (including meteorology and climatology). As such, Frontiers in Earth Science focuses on the countless processes operating within and among the major spheres constituting our planet. In turn, the understanding of these processes provides the theoretical background to better use the available resources and to face the major environmental challenges (including earthquakes, tsunamis, eruptions, floods, landslides, climate changes, extreme meteorological events): this is where interdependent processes meet, requiring a holistic view to better live on and with our planet. The journal welcomes outstanding contributions in any domain of Earth Science. The open-access model developed by Frontiers offers a fast, efficient, timely and dynamic alternative to traditional publication formats. The journal has 20 specialty sections at the first tier, each acting as an independent journal with a full editorial board. The traditional peer-review process is adapted to guarantee fairness and efficiency using a thorough paperless process, with real-time author-reviewer-editor interactions, collaborative reviewer mandates to maximize quality, and reviewer disclosure after article acceptance. While maintaining a rigorous peer-review, this system allows for a process whereby accepted articles are published online on average 90 days after submission. General Commentary articles as well as Book Reviews in Frontiers in Earth Science are only accepted upon invitation.
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