3.9 Article

Solar Activity from the Mid-Second Millennium BC to the First Millennium AD Based on Radiocarbon Data

Journal

GEOMAGNETISM AND AERONOMY
Volume 59, Issue 7, Pages 846-849

Publisher

MAIK NAUKA/INTERPERIODICA/SPRINGER
DOI: 10.1134/S0016793219070119

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Funding

  1. Russian Foundation for Basic Research [18-02-0000583, 19-02-00088]

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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 (similar to 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.

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