Large 14C excursion in 5480 BC indicates an abnormal sun in the mid-Holocene
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PNAS AUG 2016.pdf
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Accepted prepublication article
Author
Miyake, FusaJull, A. J. Timothy

Panyushkina, Irina P.
Wacker, Lukas
Salzer, Matthew
Baisan, Christopher H.
Lange, Todd
Cruz, Richard
Masuda, Kimiaki
Nakamura, Toshio
Affiliation
Department of Geosciences, University of ArizonaArizona Accelerator Mass Spectrometry Laboratory, University of Arizona
Laboratory of Tree Ring Research, University of Arizona
Issue Date
2017-01-31
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NATL ACAD SCIENCESCitation
Large 14C excursion in 5480 BC indicates an abnormal sun in the mid-Holocene 2017, 114 (5):881 Proceedings of the National Academy of SciencesRights
Copyright © 2016 The Authors. Published by National Academy of Sciences.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Radiocarbon content in tree-rings can be an excellent proxy of the past incoming cosmic ray intensities to the Earth. Although such past cosmic ray variations have been studied by measurements of 14C contents in tree rings with ≧10 year time resolution for the Holocene (1), there are few annual 14C data. There is a little understanding about annual 14C variations in the past with the exception of a few periods including the AD774-775 annual 14C excursion (2). Here, we report the result of 14C measurements using the bristlecone pine tree rings for the period from 5490 BC to 5411 BC with 1-2 year resolution, and a finding of an extraordinarily large 14C increase (20‰) from 5481 BC to 5471 BC (the 5480 BC event). The 14C increase rate of this event is much larger than that of the normal Grand Solar Minima. We propose the possible causes of this event are a special phase of grand solar minimum, or a combination of successive solar proton events and a normal grand solar minimum.Note
No embargo.ISSN
0027-84241091-6490
Version
Final accepted manuscriptSponsors
Japan Society for the Promotion of Science (JSPS) [26887019, 16H06005]; JSPS [G2602]; Toyoaki Scholarship FoundationAdditional Links
http://www.pnas.org/lookup/doi/10.1073/pnas.1613144114ae974a485f413a2113503eed53cd6c53
10.1073/pnas.1613144114