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@Article{MoroXDRSCPZLYWS:2019:PeIRBr,
               author = "Moro, Juliano and Xu, Jiyao and Denardin, Clezio Marcos and 
                         Resende, Laysa Cristina Ara{\'u}jo and Silva, R{\'e}gia Pereira 
                         da and Chen, Sony Su and Pican{\c{c}}o, Giorgio Arlan da Silva 
                         and Zhengkuan, Liu and Li, Hui and Yan, Chunxiao and Wang, Chi and 
                         Schuch, Nelson Jorge",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese 
                         Academy of Sciences (CAS)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {} and {} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and {Chinese Academy of Sciences (CAS)} and 
                         {Chinese Academy of Sciences (CAS)} and {Chinese Academy of 
                         Sciences (CAS)} and {Chinese Academy of Sciences (CAS)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Performance of the IRI-2016 at the Brazilian low-latitude 
                         ionosphere over the South America Magnetic Anomaly during solar 
                         minimum",
              journal = "Annales Geophysicae Discussions",
                 year = "2019",
               volume = "126",
                pages = "1--19",
             abstract = "In this work we analyse 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 (foF2), its peak height (hmF2), and the 
                         E-region critical frequency (foE) 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 15 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 foF2 
                         estimated with the Consultative Committee International Radio 
                         (CCIR) and International Union of Radio Science (URSI) options 
                         predicts well throughout the year. Whereas, for hmF2, 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 foE and the observations presented very good 
                         agreements.",
                  doi = "10.5194/angeo-2019-126",
                  url = "http://dx.doi.org/10.5194/angeo-2019-126",
                 issn = "0992-7689",
                label = "lattes: 3865836007446677 7 MoroXMCPSAZLYWJ:2019:PeIRBr",
             language = "en",
           targetfile = "moro_performance.pdf",
        urlaccessdate = "13 abr. 2021"
}


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