Articles | Volume 26, issue 7
https://doi.org/10.5194/acp-26-4669-2026
https://doi.org/10.5194/acp-26-4669-2026
Research article
 | 
09 Apr 2026
Research article |  | 09 Apr 2026

A new data set of nighttime chemical heating rates in the upper mesosphere and lower thermosphere derived from SCIAMACHY OH (9–6) emissions and SABER profiles

Xiaolin Wu, Yajun Zhu, Anne K. Smith, Martin Kaufmann, Guoying Jiang, Shuai Liu, and Jiyao Xu

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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-2025-5463', Anonymous Referee #1, 08 Jan 2026
    • AC1: 'Reply on RC1', Xiaolin Wu, 26 Feb 2026
    • AC2: 'Reply on RC1', Xiaolin Wu, 26 Feb 2026
  • RC2: 'Comment on egusphere-2025-5463', Anonymous Referee #2, 26 Jan 2026

Peer review completion

AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Xiaolin Wu on behalf of the Authors (26 Feb 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (06 Mar 2026) by John Plane
AR by Xiaolin Wu on behalf of the Authors (11 Mar 2026)  Manuscript 
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Short summary
Chemical reactions are key to the energy budget of the upper mesosphere–lower thermosphere, but this process remains poorly quantified. We derived a new dataset of nighttime chemical heating by combining observations from two different satellite instruments. The main exothermic reactions, hydrogen reacting with ozone and oxygen recombination, dominate at different altitudes and vary seasonally. The new results revise previous estimates and provide constraints on the mesopause energy budget.
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