2020Annales GeophysicaeOpen access

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, C. M. Denardini, L. C. A. Resende, R. P. Silva, Sony Su Chen, Giórgio Arlan da Silva Picanço, Z. Liu, Hui Li, Chunxiao Yan, Chi Wang, Nelson Jorge Schuch

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Abstract

In this work we analyze the ionograms obtained by the recent digisonde installed in Santa Maria (29.7 ∘ S, 53.7 ∘ W, dip angle = −37 ∘ ), Brazil, to calculate the monthly averages of the F2 layer critical frequency ( fo F2), its peak height ( hm F2), and the E-region critical frequency ( fo E) acquired during geomagnetically quiet days from September 2017 to August 2018. The monthly averages are compared to the 2016 version of the International Reference Ionosphere (IRI) model predictions in order to study its performance close to the center of the South America Magnetic Anomaly (SAMA), which is a region particularly important for high-frequency (HF) ground-to-satellite navigation signals. The fo F2 estimated with the Consultative Committee International Radio (CCIR) and International Union of Radio Science (URSI) options makes good predictions throughout the year, whereas, for hm F2, it is recommended to use the SHU-2015 option instead of the other available options (AMTB2013 and BSE-1979). The IRI-2016 model outputs for fo E and the observations presented very good agreement.

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What this paper is about

In this work we analyze the ionograms obtained by the recent digisonde installed in Santa Maria (29.7 ∘ S, 53.7 ∘ W, dip angle = −37 ∘ ), Brazil, to calculate the monthly averages of the F2 layer critical frequency ( fo F2), its peak height ( hm F2), and the E-region critical frequency ( fo E) acquired during geomagnetically quiet days from September 2017 to August 2018. The monthly averages are compared to the 2016 version of the International Reference Ionosphere (IRI) model predictions in order to study its performance close to the center of the South America Magnetic Anomaly (SAMA), which is a region particularly important for high-frequency (HF) ground-to-satellite navigation signals. The fo F2 estimated with the Consultative Committee International Radio (CCIR) and International Union of Radio Science (URSI) options makes good predictions throughout the year, whereas, for hm F2, it is recommended to use the SHU-2015 option instead of the other available options (AMTB2013 and BSE-1979). The IRI-2016 model outputs for fo E and the observations presented very good agreement.

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Available abstract

In this work we analyze the ionograms obtained by the recent digisonde installed in Santa Maria (29.7 ∘ S, 53.7 ∘ W, dip angle = −37 ∘ ), Brazil, to calculate the monthly averages of the F2 layer critical frequency ( fo F2), its peak height ( hm F2), and the E-region critical frequency ( fo E) acquired during geomagnetically quiet days from September 2017 to August 2018. The monthly averages are compared to the 2016 version of the International Reference Ionosphere (IRI) model predictions in order to study its performance close to the center of the South America Magnetic Anomaly (SAMA), which is a region particularly important for high-frequency (HF) ground-to-satellite navigation signals. The fo F2 estimated with the Consultative Committee International Radio (CCIR) and International Union of Radio Science (URSI) options makes good predictions throughout the year, whereas, for hm F2, it is recommended to use the SHU-2015 option instead of the other available options (AMTB2013 and BSE-1979). The IRI-2016 model outputs for fo E and the observations presented very good agreement.

Key concepts: International Reference Ionosphere, Radio Science, Critical frequency, Ionosphere, Anomaly (physics), Latitude, QUIET, High frequency

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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) — Research Paper | ScholarLens