Semidiurnal solar tide differences between fall and spring transition times in the Northern Hemisphere

Conte, J. Federico; Chau, Jorge L.; Laskar, Fazlul I.; Stober, Gunter; Schmidt, Hauke; Brown, Peter

doi:https://doi.org/10.5194/angeo-36-999-2018

Articles | Volume 36, issue 4

https://doi.org/10.5194/angeo-36-999-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Special issue:

Dynamics and interaction of processes in the Earth and its...

https://doi.org/10.5194/angeo-36-999-2018

© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 36, issue 4

Regular paper

|

13 Jul 2018

Regular paper |

| 13 Jul 2018

Semidiurnal solar tide differences between fall and spring transition times in the Northern Hemisphere

J. Federico Conte, Jorge L. Chau, Fazlul I. Laskar, Gunter Stober, Hauke Schmidt, and Peter Brown

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Final revised paper (published on 13 Jul 2018)
Preprint (discussion started on 03 Apr 2018)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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RC1: 'The review is attached as PDF file.', Anonymous Referee #1, 04 May 2018
- AC1: 'Response to referee #1 comments', Fede Conte, 14 May 2018
RC2: 'Reviewer comments on: "Semidiurnal solar tide differences between fall and spring transition times in the Northern Hemisphere"', Anonymous Referee #2, 08 May 2018
- AC2: 'Response to anonymous referee # 2', Fede Conte, 01 Jun 2018
- AC3: 'New version of the manuscript', Fede Conte, 01 Jun 2018

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

ED: Publish subject to minor revisions (review by editor) (09 Jun 2018) by Claudia Stolle

AR by Anna Wenzel on behalf of the Authors (28 Jun 2018) Author's response

ED: Publish as is (05 Jul 2018) by Claudia Stolle

Short summary

Based on comparisons of meteor radar measurements with HAMMONIA model simulations, we show that the differences exhibited by the semidiurnal solar tide (S2) observed at middle and high latitudes of the Northern Hemisphere between equinox times are mainly due to distinct behaviors of the migrating semidiurnal (SW2) and the non-migrating westward-propagating wave number 1 semidiurnal (SW1) tidal components.