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ANGEO | Articles | Volume 37, issue 4
Ann. Geophys., 37, 525–533, 2019
https://doi.org/10.5194/angeo-37-525-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 37, 525–533, 2019
https://doi.org/10.5194/angeo-37-525-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 04 Jul 2019

Regular paper | 04 Jul 2019

Assessing the role of planetary and gravity waves in the vertical structure of ozone over midlatitudinal Europe

Peter Križan
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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
ED: Reconsider after major revisions (further review by editor and referees) (26 Mar 2019) by Andrew J. Kavanagh
AR by Peter Krizan on behalf of the Authors (26 Mar 2019)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (27 Mar 2019) by Andrew J. Kavanagh
RR by Anonymous Referee #1 (25 Apr 2019)
ED: Publish subject to revisions (further review by editor and referees) (26 Apr 2019) by Andrew J. Kavanagh
AR by Peter Krizan on behalf of the Authors (06 Jun 2019)  Author's response    Manuscript
ED: Publish as is (18 Jun 2019) by Andrew J. Kavanagh
AR by Peter Krizan on behalf of the Authors (19 Jun 2019)  Author's response    Manuscript
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Short summary
We observe the planetary and gravity wave activity in the vertical profile of ozone at the mid-European ozonosonde stations The performance of the used detection method is satisfactory. There are differences in the following characteristics of the structure caused by the planetary and gravity wave: the annual variation, the size, and the vertical distribution. The results are influenced by the ozonosonde vertical resolution only for small and medium structures.
We observe the planetary and gravity wave activity in the vertical profile of ozone at the...
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