Articles | Volume 38, issue 2
https://doi.org/10.5194/angeo-38-457-2020
https://doi.org/10.5194/angeo-38-457-2020
Regular paper
 | 
06 Apr 2020
Regular paper |  | 06 Apr 2020

Performance of the IRI-2016 over Santa Maria, a Brazilian low-latitude station located in the central region of the South American Magnetic Anomaly (SAMA)

Juliano Moro, Jiyao Xu, Clezio Marcos Denardini, Laysa Cristina Araújo Resende, Régia Pereira Silva, Sony Su Chen, Giorgio Arlan da Silva Picanço, Liu Zhengkuan, Hui Li, Chunxiao Yan, Chi Wang, and Nelson Jorge Schuch

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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) (14 Feb 2020) by Fabiano Rodrigues
AR by Juliano Moro on behalf of the Authors (19 Feb 2020)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (19 Feb 2020) by Fabiano Rodrigues
RR by Anonymous Referee #2 (20 Feb 2020)
RR by Anonymous Referee #1 (27 Feb 2020)
ED: Publish subject to minor revisions (review by editor) (27 Feb 2020) by Fabiano Rodrigues
AR by Juliano Moro on behalf of the Authors (28 Feb 2020)  Author's response   Manuscript 
ED: Publish as is (10 Mar 2020) by Fabiano Rodrigues
AR by Juliano Moro on behalf of the Authors (10 Mar 2020)  Manuscript 
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Short summary
The monthly averages of the F2 critical frequency (foF2), its peak height (hmF2), and the E-region critical frequency (foE) acquired by the DPS4-D installed in Santa Maria, Brazil, is compared to the International Reference Ionosphere (IRI-2016) model predictions. It is important to test the performance of the IRI over Santa Maria because it is located in the SAMA, which is a region particularly important for high-frequency (HF) ground-to-satellite navigation signals.