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      The potential of gypsum speleothems for paleoclimatology: application to the Iberian Roman Human Period

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          Abstract

          Carbonate cave deposits (speleothems) have been used widely for paleoclimate reconstructions; however, few studies have examined the utility of other speleothem-forming minerals for this purpose. Here we demonstrate for the first time that stable isotopes (δ 17O, δ 18O and δD) of structurally-bound gypsum (CaSO 4·2H 2O) hydration water (GHW) can be used to infer paleoclimate. Specifically, we used a 63 cm-long gypsum stalactite from Sima Blanca Cave to reconstruct the climate history of SE Spain from ~ 800 BCE to ~ 800 CE. The gypsum stalactite indicates wet conditions in the cave and humid climate from ~ 200 BCE to 100 CE, at the time of the Roman Empire apogee in Hispania. From ~ 100 CE to ~ 600 CE, evaporation in the cave increased in response to regional aridification that peaked at ~ 500–600 CE, roughly coinciding with the transition between the Iberian Roman Humid Period and the Migration Period. Our record agrees with most Mediterranean and Iberian paleoclimate archives, demonstrating that stable isotopes of GHW in subaerial gypsum speleothems are a useful tool for paleoclimate reconstructions.

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          2500 years of European climate variability and human susceptibility.

          Climate variations influenced the agricultural productivity, health risk, and conflict level of preindustrial societies. Discrimination between environmental and anthropogenic impacts on past civilizations, however, remains difficult because of the paucity of high-resolution paleoclimatic evidence. We present tree ring-based reconstructions of central European summer precipitation and temperature variability over the past 2500 years. Recent warming is unprecedented, but modern hydroclimatic variations may have at times been exceeded in magnitude and duration. Wet and warm summers occurred during periods of Roman and medieval prosperity. Increased climate variability from ~250 to 600 C.E. coincided with the demise of the western Roman Empire and the turmoil of the Migration Period. Such historical data may provide a basis for counteracting the recent political and fiscal reluctance to mitigate projected climate change.
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            Total solar irradiance during the Holocene

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              Palaeo-climate reconstruction from stable isotope variations in speleothems: a review

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                Author and article information

                Contributors
                f.gazquez@ual.es
                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group UK (London )
                2045-2322
                9 September 2020
                9 September 2020
                2020
                : 10
                : 14705
                Affiliations
                [1 ]GRID grid.28020.38, ISNI 0000000101969356, Water Resources and Environmental Geology Research Group, Department of Biology and Geology, , University of Almería, ; Crta. Sacramento s/n, La Cañada de San Urbano, 04120 Almería, Spain
                [2 ]GRID grid.28020.38, ISNI 0000000101969356, Andalusian Centre for the Monitoring and Assessment of Global Change (CAESCG), , University of Almería, ; Crta. Sacramento s/n, La Cañada de San Urbano, 04120 Almería, Spain
                [3 ]GRID grid.5335.0, ISNI 0000000121885934, Godwin Laboratory for Palaeoclimate Research, Department of Earth Sciences, , University of Cambridge, ; Downing Street, Cambridge, CB2 3EQ UK
                [4 ]GRID grid.478592.5, ISNI 0000 0004 0598 3800, British Antarctic Survey, ; High Cross, Madingley Road, Cambridge, CB3 0ET UK
                [5 ]GRID grid.9435.b, ISNI 0000 0004 0457 9566, School of Archaeology, Geography & Environmental Sciences, , University of Reading, ; Whiteknights, Reading, Berkshire, RG6 6DR UK
                [6 ]GRID grid.14709.3b, ISNI 0000 0004 1936 8649, Centre de Recherche en Géochimie Et Géodynamique (GÉOTOP-UQAM)-McGill University, ; 201 ave. du Président-Kennedy 7e étage, local PK-7150, Montréal, QC H2X 3Y7 Canada
                Article
                71679
                10.1038/s41598-020-71679-3
                7481774
                32908198
                7358a065-dade-4969-b8ae-32014dc8ec2d
                © The Author(s) 2020

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 29 May 2020
                : 17 August 2020
                Funding
                Funded by: FundRef http://dx.doi.org/10.13039/501100000781, European Research Council;
                Award ID: 339694
                Award Recipient :
                Categories
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                © The Author(s) 2020

                Uncategorized
                geochemistry,palaeoclimate
                Uncategorized
                geochemistry, palaeoclimate

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