Articles | Volume 38, issue 3
https://doi.org/10.5194/angeo-38-725-2020
https://doi.org/10.5194/angeo-38-725-2020
Regular paper
 | 
16 Jun 2020
Regular paper |  | 16 Jun 2020

Comparison of quiet-time ionospheric total electron content from the IRI-2016 model and from gridded and station-level GPS observations

Gizaw Mengistu Tsidu and Mulugeta Melaku Zegeye

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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
ED: Publish subject to revisions (further review by editor and referees) (17 Oct 2019) by Dalia Buresova
AR by Gizaw Mengistu Tsidu on behalf of the Authors (28 Nov 2019)
ED: Referee Nomination & Report Request started (23 Jan 2020) by Dalia Buresova
RR by Anonymous Referee #2 (23 Feb 2020)
RR by Anonymous Referee #3 (16 Apr 2020)
ED: Publish subject to minor revisions (review by editor) (21 Apr 2020) by Dalia Buresova
AR by Gizaw Mengistu Tsidu on behalf of the Authors (10 May 2020)  Author's response   Manuscript 
ED: Publish as is (14 May 2020) by Dalia Buresova
AR by Gizaw Mengistu Tsidu on behalf of the Authors (14 May 2020)  Manuscript 
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Short summary
The performance of the IRI-2016 model in simulating GPS-TEC is assessed based on various statistical tools during two distinct solar activity periods. In particular, the categorical metrics used in the study to assess the performance of the empirical and climatological IRI-2016 model at the margins of the TEC distribution reveal remarkable model skill in simulating the observed tails of the TEC distribution, which is much better than accurately simulating the observed climatology as designed.