Articles | Volume 17, issue 2
Research article
30 Jan 2017
Research article |  | 30 Jan 2017

Time-varying changes in the simulated structure of the Brewer–Dobson Circulation

Chaim I. Garfinkel, Valentina Aquila, Darryn W. Waugh, and Luke D. Oman


Interactive discussion

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 Chaim Garfinkel on behalf of the Authors (26 Oct 2016)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (11 Nov 2016) by Gabriele Stiller
RR by Anonymous Referee #5 (20 Dec 2016)
ED: Reconsider after minor revisions (Editor review) (22 Dec 2016) by Gabriele Stiller
AR by Chaim Garfinkel on behalf of the Authors (26 Dec 2016)  Author's response    Manuscript
ED: Publish as is (04 Jan 2017) by Gabriele Stiller
Short summary
Previous work has noted a discrepancy between models and observations in trends of the large-scale overturning circulation in the stratosphere. Here, we show that a model can simulate trends that are reminiscent of those observed, including space- and time-varying trends in different regions of the stratosphere. We therefore clarify that the statement that is often made that models simulate an accelerated circulation only applies over long time periods and is not true for the past 25 years.
Final-revised paper