Articles | Volume 18, issue 8
https://doi.org/10.5194/tc-18-3439-2024
https://doi.org/10.5194/tc-18-3439-2024
Research article
 | 
06 Aug 2024
Research article |  | 06 Aug 2024

The potential of in situ cosmogenic 14CO in ice cores as a proxy for galactic cosmic ray flux variations

Vasilii V. Petrenko, Segev BenZvi, Michael Dyonisius, Benjamin Hmiel, Andrew M. Smith, and Christo Buizert

Viewed

Total article views: 970 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
771 142 57 970 51 68
  • HTML: 771
  • PDF: 142
  • XML: 57
  • Total: 970
  • BibTeX: 51
  • EndNote: 68
Views and downloads (calculated since 03 Jan 2024)
Cumulative views and downloads (calculated since 03 Jan 2024)

Viewed (geographical distribution)

Total article views: 970 (including HTML, PDF, and XML) Thereof 947 with geography defined and 23 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 13 Nov 2024
Download
Short summary
This manuscript presents the concept for a new proxy for past variations in the galactic cosmic ray flux (GCR). Past variations in GCR flux are important to understand for interpretation of records of isotopes produced by cosmic rays; these records are used for reconstructing solar variations and past land ice extent. The proxy involves using measurements of 14CO in ice cores, which should provide an uncomplicated and precise estimate of past GCR flux variations for the past few thousand years.