Prolonged production of ¹⁴C during the ~660 BCE solar proton event from Japanese tree rings

Annual rings record the intensity of cosmic rays (CRs) that had entered into the Earth's atmosphere. Several rapid ¹⁴C increases in the past, such as the 775 CE and 994CE ¹⁴C spikes, have been reported to originate from extreme solar proton events (SPEs). Another rapid ¹⁴C increase, also known as the ca. 660 BCE event in German oak tree rings as well as increases of ¹⁰Be and ³⁶Cl in ice cores, was presumed similar to the 775 CE event; however, as the ¹⁴C increase of approximately 10‰ in 660 BCE had taken a rather longer rise time of 3-4 years as compared to that of the 775 CE event, the occurrence could not be simply associated to an extreme SPE. In this study, to elucidate the rapid increase in ¹⁴C concentrations in tree rings around 660 BCE, we have precisely measured the ¹⁴C concentrations of earlywoods and latewoods inside the annual rings of Japanese cedar for the period 669-633 BCE. Based on the feature of ¹⁴C production rate calculated from the fine measured profile of the ¹⁴C concentrations, we found that the ¹⁴C rapid increase occurred within 665-663.5 BCE, and that duration of ¹⁴C production describing the event is distributed from one month to 41 months. The possibility of occurrence of consecutive SPEs over up to three years is offered.