Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP

Abstract During solar storms, the Sun expels large amounts of energetic particles (SEP) that can react with the Earth’s atmospheric constituents and produce cosmogenic radionuclides such as 14 C, 10 Be and 36 Cl. Here we present 10 Be and 36 Cl data measured in ice cores from Greenland and Antarctic...

Full description

Bibliographic Details
Published in:Nature Communications
Main Authors: Paleari, Chiara I., Mekhaldi, Florian, Adolphi, Florian, Christl, Marcus, Vockenhuber, Christof, Gautschi, Philip, Beer, Jürg, Brehm, Nicolas, Erhardt, Tobias, Synal, Hans-Arno, Muscheler, Raimund
Format: Article in Journal/Newspaper
Language:English
Published: 2022
Subjects:
Greenland
Antarc*
Antarctica
Online Access:https://resolver.sub.uni-goettingen.de/purl?gro-2/105965
https://doi.org/10.1038/s41467-021-27891-4
Description
Summary:Abstract During solar storms, the Sun expels large amounts of energetic particles (SEP) that can react with the Earth’s atmospheric constituents and produce cosmogenic radionuclides such as 14 C, 10 Be and 36 Cl. Here we present 10 Be and 36 Cl data measured in ice cores from Greenland and Antarctica. The data consistently show one of the largest 10 Be and 36 Cl production peaks detected so far, most likely produced by an extreme SEP event that hit Earth 9125 years BP (before present, i.e., before 1950 CE), i.e., 7176 BCE. Using the 36 Cl/ 10 Be ratio, we demonstrate that this event was characterized by a very hard energy spectrum and was possibly up to two orders of magnitude larger than any SEP event during the instrumental period. Furthermore, we provide 10 Be-based evidence that, contrary to expectations, the SEP event occurred near a solar minimum.

Similar Items