Articles | Volume 14, issue 1
https://doi.org/10.5194/amt-14-557-2021
https://doi.org/10.5194/amt-14-557-2021
Research article
 | 
26 Jan 2021
Research article |  | 26 Jan 2021

Accounting for the photochemical variation in stratospheric NO2 in the SAGE III/ISS solar occultation retrieval

Kimberlee Dubé, Adam Bourassa, Daniel Zawada, Douglas Degenstein, Robert Damadeo, David Flittner, and William Randel

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Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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AR: Author's response | RR: Referee report | ED: Editor decision
AR by Kimberlee Dubé on behalf of the Authors (26 Nov 2020)  Author's response   Manuscript 
ED: Publish subject to minor revisions (review by editor) (09 Dec 2020) by Michel Van Roozendael
AR by Kimberlee Dubé on behalf of the Authors (10 Dec 2020)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (11 Dec 2020) by Michel Van Roozendael
AR by Kimberlee Dubé on behalf of the Authors (11 Dec 2020)
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Short summary
SAGE III/ISS measures profiles of NO2; however the algorithm to convert raw measurements to NO2 concentration neglects variations caused by changes in chemistry over the course of a day. We devised a procedure to account for these diurnal variations and assess their impact on NO2 measurements from SAGE III/ISS. We find that the new NO2 concentration is more than 10 % lower than NO2 from the standard algorithm below 30 km, showing that this effect is important to consider at lower altitudes.