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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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ACP | Articles | Volume 19, issue 7
Atmos. Chem. Phys., 19, 5209–5233, 2019
https://doi.org/10.5194/acp-19-5209-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Chem. Phys., 19, 5209–5233, 2019
https://doi.org/10.5194/acp-19-5209-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Research article 17 Apr 2019

Research article | 17 Apr 2019

Simulating the atmospheric response to the 11-year solar cycle forcing with the UM-UKCA model: the role of detection method and natural variability

Ewa M. Bednarz et al.

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Status: closed
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
AR by Ewa Bednarz on behalf of the Authors (29 Aug 2018)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (30 Aug 2018) by Martin Dameris
RR by Anonymous Referee #1 (11 Sep 2018)
ED: Reconsider after major revisions (24 Sep 2018) by Martin Dameris
AR by Ewa Bednarz on behalf of the Authors (27 Nov 2018)  Author's response    Manuscript
ED: Publish as is (03 Dec 2018) by Martin Dameris
Publications Copernicus
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Short summary
Following model improvements, the atmospheric response to the 11-year solar cycle forcing simulated in the UM-UKCA chemistry–climate model is discussed for the first time. In contrast to most previous studies in the literature, we compare the results diagnosed using both a composite and a MLR methodology, and we show that apparently different signals can be diagnosed in the troposphere. In addition, we look at the role of internal atmospheric variability for the detection of the solar response.
Following model improvements, the atmospheric response to the 11-year solar cycle forcing...
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