Articles | Volume 37, issue 2
Ann. Geophys., 37, 171–182, 2019
https://doi.org/10.5194/angeo-37-171-2019
Ann. Geophys., 37, 171–182, 2019
https://doi.org/10.5194/angeo-37-171-2019

Regular paper 28 Mar 2019

Regular paper | 28 Mar 2019

Solar-eclipse-induced perturbations at mid-latitude during the 21 August 2017 event

Bolarinwa J. Adekoya et al.

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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) (10 Jul 2018) by Steve Milan
AR by Bolarinwa Adekoya on behalf of the Authors (11 Jul 2018)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (02 Aug 2018) by Steve Milan
RR by Anonymous Referee #2 (12 Sep 2018)
RR by Anonymous Referee #3 (13 Dec 2018)
ED: Publish subject to minor revisions (review by editor) (22 Jan 2019) by Steve Milan
AR by Bolarinwa Adekoya on behalf of the Authors (02 Feb 2019)  Author's response    Manuscript
ED: Publish as is (22 Feb 2019) by Steve Milan
AR by Bolarinwa Adekoya on behalf of the Authors (16 Mar 2019)  Author's response    Manuscript
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Short summary
We present the dynamics of perturbations during a solar eclipse using rare parameters for eclipse study. Reduction in solar radiation and natural gas heating are the cause of the observed changes. The use of the bottomside F-layer parameters to probe the topside ionosphere established their interrelationship. The implication is that eclipse-caused perturbation could be better explained using some ionosonde parameters.