电邮这篇文章 The Hallstatt solar cycle from radiocarbon data
- 作者: Ogurtsov M.G.1,2
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隶属关系:
- Ioffe Physical-Technical Institute
- Main (Pulkovo) Astronomic Observatory of the Russian Academy of Sciences
- 期: 卷 56, 编号 5 (2016)
- 页面: 641-644
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/155805
- DOI: https://doi.org/10.1134/S0016793216040150
- ID: 155805
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详细
The data on the 14C concentration in the Earth’s atmosphere are studied on a time span of 50000 years. It is shown that the Hallstatt cycle (a temporal variation with a period of 1500–2000 years) has been present in this series for at least 30000 years. However, this cycle is not purely of solar origin; nonsolar (supposedly climatic) factors contribute into it in certain epochs.
作者简介
M. Ogurtsov
Ioffe Physical-Technical Institute; Main (Pulkovo) Astronomic Observatory of the Russian Academy of Sciences
编辑信件的主要联系方式.
Email: maxim.ogurtsov@mail.ioffe.ru
俄罗斯联邦, St. Petersburg; St. Petersburg
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