Solar Activity from the Mid-Second Millennium B.C. to the First Millennium A.D. Based on Radiocarbon Data
- 作者: Dergachev V.A.1, Kudryavtsev I.V.1,2, Nagovitsyn Y.A.2,3
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隶属关系:
- Ioffe Institute, Russian Academy of Sciences
- Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences
- State University of Aerospace Instrumentation
- 期: 卷 59, 编号 7 (2019)
- 页面: 846-849
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157819
- DOI: https://doi.org/10.1134/S0016793219070119
- ID: 157819
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详细
The paper reports the results of reconstruction of the heliospheric modulation potential from radiocarbon data for the time interval from the mid-second millennium B.C. to the end of the first millennium A.D. It is known that significant climatic changes took place on the Earth during that time; specifically, the thickness of glaciers in Iceland and Norway were changing. Coincident changes are also observed in the radiocarbon data. The results of calculations show that the heliospheric modulation potential reaches a maximum (~590 MV) on this interval approximately in 1705 B.C. This suggests that solar activity at that moment was highest for the considered interval. Conversely, around 750 and 350 B.C., the smallest values of the modulation potential were observed and, consequently, solar activity could be lowest from the mid-second millennium B.C. to the end of the first millennium A.D.
作者简介
V. Dergachev
Ioffe Institute, Russian Academy of Sciences
Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021
I. Kudryavtsev
Ioffe Institute, Russian Academy of Sciences; Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences
编辑信件的主要联系方式.
Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021; St. Petersburg, 196140
Yu. Nagovitsyn
Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences; State University of Aerospace Instrumentation
Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 196140; St. Petersburg, 190000
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