Variations of 14-C around AD 775 and AD 1795 - due to solar activity
Ralph Neuhaeuser (U Jena), Dagmar Neuhaeuser (Jena)

TL;DR
This study compares 14-C variations around AD 775 and 1795 with other periods of solar activity, revealing patterns of rapid changes linked to solar activity fluctuations and proposing explanations for these anomalies.
Contribution
It identifies recurring patterns of 14-C variation linked to solar activity cycles and provides a detailed explanation of the causes behind the rapid increases around AD 775 and 1795.
Findings
Three periods of strong secular 14-C variation identified
Rapid 14-C increases explained by decreases in solar activity
Strong 14-C rises linked to specific solar cycle phases
Abstract
The motivation for our study is the disputed cause for the strong variation of 14-C around AD 775. Our method is to compare the 14-C variation around AD 775 with other periods of strong variability. Our results are: (a) We see three periods, where 14-C varied over 200 yr in a special way showing a certain pattern of strong secular variation: after a Grand Minimum with strongly increasing 14-C, there is a series of strong short-term drop(s), rise(s), and again drop(s) within 60 yr, ending up to 200 yr after the start of the Grand Minimum. These three periods include the strong rises around BC 671, AD 775, and AD 1795. (b) We show with several solar activity proxies (radioisotopes, sunspots, and aurorae) for the AD 770s and 1790s that such intense rapid 14-C increases can be explained by strong rapid decreases in solar activity and, hence, wind, so that the decrease in solar modulation…
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