Spatial biases in oxygen-based Phanerozoic seawater temperature reconstructions

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Alexandre POHL , Thomas W. WONG  HEARING , Arnaud BRAYARD , Ethan GROSSMAN , Michael M. JOACHIMSKI , Guillaume LE  HIR , Thomas LETULLE , Daniel J. LUNT , Mathieu MARTINEZ , Emmanuelle PUCEAT , Guillaume SUAN , Paul VALDES , Yannick DONNADIEU
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Abstract

Stable oxygen isotopes (δ18O) are routinely used to reconstruct sea-surface temperatures (SSTs) in the geological past, with mineral δ18O values reflecting a combination of the temperature and oxygen isotope composition of seawater (δ18Osw). Temporal variation of mean-ocean δ18Osw is usually accounted for following estimates of land-ice volume. Spatial variations in δ18Osw, however, are often neglected or corrected using calibrations derived from the present-day or recent past. Geochemical methods for constraining δ18Osw and isotope-enabled general circulation model (GCM) simulations are still technically challenging. This lack of constraints on ancient δ18Osw is a substantial source of uncertainty for SST reconstructions. Here we use the co-variation of δ18Osw and seawater salinity, together with GCM simulations of ocean salinity, to propose estimations of spatial variability in δ18Osw over the Phanerozoic. Sensitivity tests of the δ18Osw-salinity relationship and climate model, and comparison with results of isotope-enabled GCMs, suggest that our calculations are robust at first order. We show that continental configuration exerts a primary control on δ18Osw spatial variability. Complex ocean basin geometries in periods younger than 66 Ma lead to strong inter-basinal contrasts in δ18Osw. Latitudinal SST gradients may be steeper than previously suggested during most of the Mesozoic and Cenozoic. This work has limitations, with δ18Osw-salinity relationships being less reliable in both low-latitude epicontinental settings and high-latitude regions of deep-water formation. Whilst our calculations are limited use in correcting δ18O measurements for local δ18Osw, they identify the time slices and paleogeographical regions that should be prioritized for future work using isotope-enabled GCMs.
氧基显生宙海水温度重建的空间偏差
稳定氧同位素(δ18O)通常用于重建地质历史的海表温度(SSTs),矿物δ18O值反映了海水温度和氧同位素组成(δ18Osw)的组合。平均海洋δ18Osw的时间变化通常由陆冰体积的估算来解释。然而,δ18Osw的空间变化通常被忽略或使用来自当前或最近过去的校准进行校正。约束δ18Osw的地球化学方法和同位素总环流模型(GCM)的模拟在技术上仍然具有挑战性。缺乏对古δ18Osw的约束是海温重建的主要不确定性来源。本文利用δ18Osw与海水盐度的共变,结合海洋盐度的GCM模拟,提出了显生宙δ18Osw的空间变异估计。δ 18osw -盐度关系和气候模型的敏感性测试,以及与同位素支持的GCMs结果的比较表明,我们的计算在一级是稳健的。研究表明,大陆构造对δ18Osw空间变异性起主要控制作用。在小于66 Ma的时期,复杂的洋盆几何结构导致了强烈的盆间δ18Osw对比。在中生代和新生代的大部分时间里,纬向海温梯度可能比以前认为的更陡。这项工作有局限性,δ 18osw -盐度关系在低纬度陆表环境和高纬度深水地层区域都不太可靠。虽然我们的计算在校正局部δ18Osw的δ18O测量中使用有限,但它们确定了应该优先使用同位素gcm进行未来工作的时间片和古地理区域。
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
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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