Articles | Volume 37, issue 4
https://doi.org/10.5194/angeo-37-471-2019
https://doi.org/10.5194/angeo-37-471-2019
Regular paper
 | 
02 Jul 2019
Regular paper |  | 02 Jul 2019

Ozone and temperature decadal solar-cycle responses, and their relation to diurnal variations in the stratosphere, mesosphere, and lower thermosphere, based on measurements from SABER on TIMED

Frank T. Huang and Hans G. Mayr

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Interactive discussion

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Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Reconsider after major revisions (further review by editor and referees) (13 May 2019) by Petr Pisoft
AR by Anna Mirena Feist-Polner on behalf of the Authors (15 May 2019)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (15 May 2019) by Petr Pisoft
RR by Anonymous Referee #1 (22 May 2019)
RR by Anonymous Referee #3 (31 May 2019)
ED: Publish subject to minor revisions (review by editor) (03 Jun 2019) by Petr Pisoft
AR by Svenja Lange on behalf of the Authors (04 Jun 2019)  Author's response
ED: Publish as is (05 Jun 2019) by Petr Pisoft
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Short summary
The sun’s radiation exhibits a cycle with a period of ~11 years. We need to understand how the atmospheric temperature and ozone react to this solar variation, as it can affect climate. The response depends on energy transfer, chemical reactions, and atmospheric motions. There is no consensus as to some details. For example, the responses depend on the local times of the variations. This study provides results of effects of local time on the responses, from 20 to 100 km, based on measurements.