Articles | Volume 23, issue 8
https://doi.org/10.5194/acp-23-4849-2023
https://doi.org/10.5194/acp-23-4849-2023
Research article
 | 
24 Apr 2023
Research article |  | 24 Apr 2023

Atmospheric distribution of HCN from satellite observations and 3-D model simulations

Antonio G. Bruno, Jeremy J. Harrison, Martyn P. Chipperfield, David P. Moore, Richard J. Pope, Christopher Wilson, Emmanuel Mahieu, and Justus Notholt

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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-2022-1404', Hugh C. Pumphrey, 19 Dec 2022
  • RC2: 'Review of ‘Atmospheric distribution of HCN from satellite observations and 3-D model simulations’ by A. G. Bruno et al. (2022)', Anonymous Referee #2, 09 Jan 2023
  • AC1: 'Comment on egusphere-2022-1404', Antonio Giovanni Bruno, 24 Feb 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Antonio Giovanni Bruno on behalf of the Authors (24 Feb 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (08 Mar 2023) by Marc von Hobe
RR by Anonymous Referee #2 (09 Mar 2023)
ED: Publish as is (27 Mar 2023) by Marc von Hobe
AR by Antonio Giovanni Bruno on behalf of the Authors (28 Mar 2023)
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Short summary
A 3-D chemical transport model, TOMCAT; satellite data; and ground-based observations have been used to investigate hydrogen cyanide (HCN) variability. We found that the oxidation by O(1D) drives the HCN loss in the middle stratosphere and the currently JPL-recommended OH reaction rate overestimates HCN atmospheric loss. We also evaluated two different ocean uptake schemes. We found them to be unrealistic, and we need to scale these schemes to obtain good agreement with HCN observations.
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