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      Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE

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          Abstract

          The Sun sporadically produces eruptive events leading to intense fluxes of solar energetic particles (SEPs) that dramatically disrupt the near-Earth radiation environment. Such events have been directly studied for the last decades but little is known about the occurrence and magnitude of rare, extreme SEP events. Presently, a few events that produced measurable signals in cosmogenic radionuclides such as 14C, 10Be and 36Cl have been found. Analyzing annual 14C concentrations in tree-rings from Switzerland, Germany, Ireland, Russia, and the USA we discovered two spikes in atmospheric 14C occurring in 7176 and 5259 BCE. The ~2% increases of atmospheric 14C recorded for both events exceed all previously known 14C peaks but after correction for the geomagnetic field, they are comparable to the largest event of this type discovered so far at 775 CE. These strong events serve as accurate time markers for the synchronization with floating tree-ring and ice core records and provide critical information on the previous occurrence of extreme solar events which may threaten modern infrastructure.

          Abstract

          Two extreme solar energetic particle events have been found by carbon isotopes measured in ancient tree rings in 7176 and 5259 BCE. The recorded ~2% increases of atmospheric 14 C for both events exceeds in amplitude of all previously observed events.

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          THE INTCAL20 NORTHERN HEMISPHERE RADIOCARBON AGE CALIBRATION CURVE (0–55 CAL kBP)

          Radiocarbon ( 14 C) ages cannot provide absolutely dated chronologies for archaeological or paleoenvironmental studies directly but must be converted to calendar age equivalents using a calibration curve compensating for fluctuations in atmospheric 14 C concentration. Although calibration curves are constructed from independently dated archives, they invariably require revision as new data become available and our understanding of the Earth system improves. In this volume the international 14 C calibration curves for both the Northern and Southern Hemispheres, as well as for the ocean surface layer, have been updated to include a wealth of new data and extended to 55,000 cal BP. Based on tree rings, IntCal20 now extends as a fully atmospheric record to ca. 13,900 cal BP. For the older part of the timescale, IntCal20 comprises statistically integrated evidence from floating tree-ring chronologies, lacustrine and marine sediments, speleothems, and corals. We utilized improved evaluation of the timescales and location variable 14 C offsets from the atmosphere (reservoir age, dead carbon fraction) for each dataset. New statistical methods have refined the structure of the calibration curves while maintaining a robust treatment of uncertainties in the 14 C ages, the calendar ages and other corrections. The inclusion of modeled marine reservoir ages derived from a three-dimensional ocean circulation model has allowed us to apply more appropriate reservoir corrections to the marine 14 C data rather than the previous use of constant regional offsets from the atmosphere. Here we provide an overview of the new and revised datasets and the associated methods used for the construction of the IntCal20 curve and explore potential regional offsets for tree-ring data. We discuss the main differences with respect to the previous calibration curve, IntCal13, and some of the implications for archaeology and geosciences ranging from the recent past to the time of the extinction of the Neanderthals.
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            9,400 years of cosmic radiation and solar activity from ice cores and tree rings.

            Understanding the temporal variation of cosmic radiation and solar activity during the Holocene is essential for studies of the solar-terrestrial relationship. Cosmic-ray produced radionuclides, such as (10)Be and (14)C which are stored in polar ice cores and tree rings, offer the unique opportunity to reconstruct the history of cosmic radiation and solar activity over many millennia. Although records from different archives basically agree, they also show some deviations during certain periods. So far most reconstructions were based on only one single radionuclide record, which makes detection and correction of these deviations impossible. Here we combine different (10)Be ice core records from Greenland and Antarctica with the global (14)C tree ring record using principal component analysis. This approach is only possible due to a new high-resolution (10)Be record from Dronning Maud Land obtained within the European Project for Ice Coring in Antarctica in Antarctica. The new cosmic radiation record enables us to derive total solar irradiance, which is then used as a proxy of solar activity to identify the solar imprint in an Asian climate record. Though generally the agreement between solar forcing and Asian climate is good, there are also periods without any coherence, pointing to other forcings like volcanoes and greenhouse gases and their corresponding feedbacks. The newly derived records have the potential to improve our understanding of the solar dynamics and to quantify the solar influence on climate.
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              A signature of cosmic-ray increase in AD 774-775 from tree rings in Japan.

              Increases in (14)C concentrations in tree rings could be attributed to cosmic-ray events, as have increases in (10)Be and nitrate in ice cores. The record of the past 3,000 years in the IntCal09 data set, which is a time series at 5-year intervals describing the (14)C content of trees over a period of approximately 10,000 years, shows three periods during which (14)C increased at a rate greater than 3‰ over 10 years. Two of these periods have been measured at high time resolution, but neither showed increases on a timescale of about 1 year (refs 11 and 12). Here we report (14)C measurements in annual rings of Japanese cedar trees from ad 750 to ad 820 (the remaining period), with 1- and 2-year resolution. We find a rapid increase of about 12‰ in the (14)C content from ad 774 to 775, which is about 20 times larger than the change attributed to ordinary solar modulation. When averaged over 10 years, the data are consistent with the decadal IntCal (14)C data from North American and European trees. We argue that neither a solar flare nor a local supernova is likely to have been responsible.
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                Author and article information

                Contributors
                nbrehm@ethz.ch
                mchristl@phys.ethz.ch
                wacker@phys.ethz.ch
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                7 March 2022
                7 March 2022
                2022
                : 13
                : 1196
                Affiliations
                [1 ]GRID grid.5801.c, ISNI 0000 0001 2156 2780, Laboratory of Ion Beam Physics, ETHZ, ; Otto-Stern Weg 5 HPK, 8093 Zurich, Switzerland
                [2 ]GRID grid.5337.2, ISNI 0000 0004 1936 7603, Bristol Radiocarbon Accelerator Mass Spectrometry Facility, , Bristol University, ; Bristol, BS81TS UK
                [3 ]GRID grid.10894.34, ISNI 0000 0001 1033 7684, Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, ; 27568 Bremerhaven, Germany
                [4 ]GRID grid.4514.4, ISNI 0000 0001 0930 2361, Department of Geology – Quaternary Sciences, , Lund University, ; 22362 Lund, Sweden
                [5 ]GRID grid.478592.5, ISNI 0000 0004 0598 3800, British Antarctic Survey, Ice Dynamics and Paleoclimate, ; Cambridge, CB3 0ET UK
                [6 ]GRID grid.7450.6, ISNI 0000 0001 2364 4210, Albrecht von Haller Institute for Plant Sciences, Department of Palynology and Climate Dynamics, , Georg-August-University, ; Wilhelm-Weber-Str. 2a, 37073 Göttingen, Germany
                [7 ]GRID grid.484224.c, ISNI 0000 0004 5373 0664, Historic England, Cannon Bridge House, ; 25 Dowgate Hill, London, EC4R 2YA UK
                [8 ]GRID grid.5771.4, ISNI 0000 0001 2151 8122, Department of Geography, , Universität Innsbruck, ; Innrain 52, 6020 Innsbruck, Austria
                [9 ]GRID grid.5734.5, ISNI 0000 0001 0726 5157, Institute of Geological Sciences, , University of Bern, ; Baltzerstrasse 1+3, 3012 Bern, Switzerland
                [10 ]GRID grid.134563.6, ISNI 0000 0001 2168 186X, University of Arizona, the Laboratory for Tree-Ring Research, ; 1215 E. Lowell Street, Tucson, AZ 85721-0045 USA
                [11 ]GRID grid.419754.a, ISNI 0000 0001 2259 5533, Swiss Federal Research Institute WSL, ; Zürcherstrasse 111, 8903 Birmensdorf, Switzerland
                [12 ]GRID grid.482778.6, ISNI 0000 0001 2197 0186, Laboratory of Dendrochronology, Institute of Plant and Animal Ecology, Ural Branch of Russian Academy of Sciences, ; 8 Marta Street, 202, Ekaterinburg, 620144 Russia
                [13 ]GRID grid.412761.7, ISNI 0000 0004 0645 736X, Laboratory of Natural Science Methods in Humanities, , Ural Federal University, ; 19 Mira Street, Ekaterinburg, 620002 Russia
                [14 ]GRID grid.4777.3, ISNI 0000 0004 0374 7521, School of Natural and Built Environment, , The Queen’s University, ; Belfast, BT7 1NN UK
                [15 ]GRID grid.10858.34, ISNI 0000 0001 0941 4873, Sodankylä Geophysical Observatory and Space Physics and Astronomy Research Unit, University of Oulu, ; Oulu, FIN-90014 Finland
                [16 ]GRID grid.410350.3, ISNI 0000 0001 2174 9334, Present Address: UMR7209 Archéologie et Archéobotanique: Sociétés, Pratiques et Environnements, Muséum National d’Histoire Naturelle, ; CP56, 43 Rue Buffon, 75005 Paris, France
                Author information
                http://orcid.org/0000-0003-0248-7345
                http://orcid.org/0000-0002-3131-6652
                http://orcid.org/0000-0003-4871-5542
                http://orcid.org/0000-0003-1417-3060
                http://orcid.org/0000-0002-9483-2750
                http://orcid.org/0000-0003-0014-8753
                http://orcid.org/0000-0003-2772-3631
                http://orcid.org/0000-0001-8323-2955
                http://orcid.org/0000-0002-0007-5155
                http://orcid.org/0000-0003-2782-1979
                http://orcid.org/0000-0002-1737-4119
                http://orcid.org/0000-0002-6262-5554
                http://orcid.org/0000-0001-5353-7459
                http://orcid.org/0000-0002-7070-3292
                http://orcid.org/0000-0003-3033-8312
                http://orcid.org/0000-0001-8227-9081
                http://orcid.org/0000-0002-8215-2678
                Article
                28804
                10.1038/s41467-022-28804-9
                8901681
                35256613
                39ebd657-ab3e-4554-8c35-dddd81c11168
                © The Author(s) 2022

                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 license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license 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 license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 26 July 2021
                : 11 February 2022
                Funding
                Funded by: FundRef https://doi.org/10.13039/501100001711, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung (Swiss National Science Foundation);
                Award ID: SNF 197137
                Award Recipient :
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                solar physics

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