Articles | Volume 21, issue 16
https://doi.org/10.5194/acp-21-12413-2021
https://doi.org/10.5194/acp-21-12413-2021
Research article
 | 
19 Aug 2021
Research article |  | 19 Aug 2021

Observation and modelling of ozone-destructive halogen chemistry in a passively degassing volcanic plume

Luke Surl, Tjarda Roberts, and Slimane Bekki

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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 acp-2021-145', Anonymous Referee #1, 31 Mar 2021
  • RC2: 'Comment on acp-2021-145', Anonymous Referee #2, 14 May 2021
  • AC1: 'Reply to both referees (acp-2021-145)', Luke Surl, 02 Jul 2021

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Luke Surl on behalf of the Authors (02 Jul 2021)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (15 Jul 2021) by Marc von Hobe
AR by Luke Surl on behalf of the Authors (16 Jul 2021)
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Short summary
Many different chemical reactions happen when the gases from a volcano mix with air, but what effects do they have? We present aircraft measurements which show that there is less ozone within the plume of Etna than outside it. We have also made a computer model of this chemistry. This model can reproduce the effects seen when halogens (bromine and chlorine) are included in the volcanic emissions. We look closely at the simulation to discover how complicated halogen reactions cause ozone loss.
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