A signature of cosmic-ray increase in AD 774-775 from tree rings in Japan
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作者:
Miyake, Fusa
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Nagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, JapanNagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
Miyake, Fusa
[1
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Nagaya, Kentaro
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Nagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, JapanNagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
Nagaya, Kentaro
[1
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Masuda, Kimiaki
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Nagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, JapanNagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
Masuda, Kimiaki
[1
]
Nakamura, Toshio
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Nagoya Univ, Ctr Chronol Res, Chikusa Ku, Nagoya, Aichi 4648601, JapanNagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
Nakamura, Toshio
[2
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机构:
[1] Nagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
[2] Nagoya Univ, Ctr Chronol Res, Chikusa Ku, Nagoya, Aichi 4648601, Japan
Increases in C-14 concentrations in tree rings could be attributed to cosmic-ray events(1-7), as have increases in Be-10 and nitrate in ice cores(8,9). The record of the past 3,000 years in the IntCal09 data set(10), which is a time series at 5-year intervals describing the C-14 content of trees over a period of approximately 10,000 years, shows three periods during which C-14 increased at a rate greater than 3 parts per thousand 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 C-14 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 parts per thousand in the C-14 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 C-14 data from North American and European trees(13). We argue that neither a solar flare nor a local supernova is likely to have been responsible.
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Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USAOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
Katsuda, Satoru
;
Tsunemi, Hiroshi
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Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, JapanOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
Tsunemi, Hiroshi
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Mori, Koji
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Miyazaki Univ, Fac Engn, Dept Appl Phys, Nishi Ku, Miyazaki 8892192, JapanOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
机构:
Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USAOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
Katsuda, Satoru
;
Tsunemi, Hiroshi
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Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, JapanOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan
Tsunemi, Hiroshi
;
Mori, Koji
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Miyazaki Univ, Fac Engn, Dept Appl Phys, Nishi Ku, Miyazaki 8892192, JapanOsaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan