Journal
RADIOCARBON
Volume 59, Issue 2, Pages 293-302Publisher
UNIV ARIZONA DEPT GEOSCIENCES
DOI: 10.1017/RDC.2016.50
Keywords
Supernova; Miyake event; gamma flux
Categories
Funding
- Balliol Inter-disciplinary Institute
- Leverhulme Trust Early Career Fellowship
- Grants-in-Aid for Scientific Research [26887019, 16K13802] Funding Source: KAKEN
Ask authors/readers for more resources
Single-year spikes in radiocarbon production are caused by intense bursts of radiation from space. Supernovae emit both high-energy particle and electromagnetic radiation, but it is the latter that is most likely to strike the atmosphere all at once and cause a surge in C-14 production. In the 1990s, it was claimed that the supernova in 1006 CE produced exactly this effect. With the C-14 spikes in the years 775 and 994 CE now attributed to extreme solar events, attention has returned to the question of whether historical supernovae are indeed detectable using annual C-14 measurements. Here, we combine new and existing measurements over six documented and putative supernovae, and conclude that no such astrophysical event has yet left a distinct imprint on the past atmospheric C-14 record.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available