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

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-3126', Anonymous Referee #1, 06 Feb 2024
  • RC2: 'Comment on egusphere-2023-3126', Ilya Usoskin, 06 Feb 2024

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to minor revisions (review by editor) (12 Apr 2024) by Hubertus Fischer
AR by Vasilii Petrenko on behalf of the Authors (15 May 2024)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (17 May 2024) by Hubertus Fischer
AR by Vasilii Petrenko on behalf of the Authors (25 May 2024)

Post-review adjustments

AA: Author's adjustment | EA: Editor approval
AA by Vasilii Petrenko on behalf of the Authors (10 Jul 2024)   Author's adjustment   Manuscript
EA: Adjustments approved (22 Jul 2024) by Hubertus Fischer
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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.